Coverage for pygeodesy/ellipsoids.py: 96%

2# -*- coding: utf-8 -*-

4u'''Ellipsoidal and spherical earth models.

6Classes L{a_f2Tuple}, L{Ellipsoid} and L{Ellipsoid2}, an L{Ellipsoids} registry and

72 dozen functions to convert I{equatorial} radius, I{polar} radius, I{eccentricities},

8I{flattenings} and I{inverse flattening}.

10See module L{datums} for L{Datum} and L{Transform} information and other details.

12Following is the list of predefined L{Ellipsoid}s, all instantiated lazily.

14@var Ellipsoids.Airy1830: Ellipsoid(name='Airy1830', a=6377563.396, f=0.00334085, f_=299.3249646, b=6356256.90923729)

15@var Ellipsoids.AiryModified: Ellipsoid(name='AiryModified', a=6377340.189, f=0.00334085, f_=299.3249646, b=6356034.44793853)

16@var Ellipsoids.ATS1977: Ellipsoid(name='ATS1977', a=6378135, f=0.00335281, f_=298.257, b=6356750.30492159)

17@var Ellipsoids.Australia1966: Ellipsoid(name='Australia1966', a=6378160, f=0.00335289, f_=298.25, b=6356774.71919531)

18@var Ellipsoids.Bessel1841: Ellipsoid(name='Bessel1841', a=6377397.155, f=0.00334277, f_=299.1528128, b=6356078.962818)

19@var Ellipsoids.BesselModified: Ellipsoid(name='BesselModified', a=6377492.018, f=0.00334277, f_=299.1528128, b=6356173.5087127)

20@var Ellipsoids.CGCS2000: Ellipsoid(name='CGCS2000', a=6378137, f=0.00335281, f_=298.2572221, b=6356752.31414036)

21@var Ellipsoids.Clarke1866: Ellipsoid(name='Clarke1866', a=6378206.4, f=0.00339008, f_=294.97869821, b=6356583.8)

22@var Ellipsoids.Clarke1880: Ellipsoid(name='Clarke1880', a=6378249.145, f=0.00340756, f_=293.465, b=6356514.86954978)

23@var Ellipsoids.Clarke1880IGN: Ellipsoid(name='Clarke1880IGN', a=6378249.2, f=0.00340755, f_=293.46602129, b=6356515)

24@var Ellipsoids.Clarke1880Mod: Ellipsoid(name='Clarke1880Mod', a=6378249.145, f=0.00340755, f_=293.46630766, b=6356514.96639549)

25@var Ellipsoids.CPM1799: Ellipsoid(name='CPM1799', a=6375738.7, f=0.00299052, f_=334.39, b=6356671.92557493)

26@var Ellipsoids.Delambre1810: Ellipsoid(name='Delambre1810', a=6376428, f=0.00321027, f_=311.5, b=6355957.92616372)

27@var Ellipsoids.Engelis1985: Ellipsoid(name='Engelis1985', a=6378136.05, f=0.00335282, f_=298.2566, b=6356751.32272154)

28@var Ellipsoids.Everest1969: Ellipsoid(name='Everest1969', a=6377295.664, f=0.00332445, f_=300.8017, b=6356094.667915)

29@var Ellipsoids.Everest1975: Ellipsoid(name='Everest1975', a=6377299.151, f=0.00332445, f_=300.8017255, b=6356098.14512013)

30@var Ellipsoids.Fisher1968: Ellipsoid(name='Fisher1968', a=6378150, f=0.00335233, f_=298.3, b=6356768.33724438)

31@var Ellipsoids.GEM10C: Ellipsoid(name='GEM10C', a=6378137, f=0.00335281, f_=298.2572236, b=6356752.31424783)

32@var Ellipsoids.GPES: Ellipsoid(name='GPES', a=6378135, f=0, f_=0, b=6378135)

33@var Ellipsoids.GRS67: Ellipsoid(name='GRS67', a=6378160, f=0.00335292, f_=298.24716743, b=6356774.51609071)

34@var Ellipsoids.GRS80: Ellipsoid(name='GRS80', a=6378137, f=0.00335281, f_=298.2572221, b=6356752.31414035)

35@var Ellipsoids.Helmert1906: Ellipsoid(name='Helmert1906', a=6378200, f=0.00335233, f_=298.3, b=6356818.16962789)

36@var Ellipsoids.IAU76: Ellipsoid(name='IAU76', a=6378140, f=0.00335281, f_=298.257, b=6356755.28815753)

37@var Ellipsoids.IERS1989: Ellipsoid(name='IERS1989', a=6378136, f=0.00335281, f_=298.257, b=6356751.30156878)

38@var Ellipsoids.IERS1992TOPEX: Ellipsoid(name='IERS1992TOPEX', a=6378136.3, f=0.00335281, f_=298.25722356, b=6356751.61659215)

39@var Ellipsoids.IERS2003: Ellipsoid(name='IERS2003', a=6378136.6, f=0.00335282, f_=298.25642, b=6356751.85797165)

40@var Ellipsoids.Intl1924: Ellipsoid(name='Intl1924', a=6378388, f=0.003367, f_=297, b=6356911.94612795)

41@var Ellipsoids.Intl1967: Ellipsoid(name='Intl1967', a=6378157.5, f=0.0033529, f_=298.24961539, b=6356772.2)

42@var Ellipsoids.Krassovski1940: Ellipsoid(name='Krassovski1940', a=6378245, f=0.00335233, f_=298.3, b=6356863.01877305)

43@var Ellipsoids.Krassowsky1940: Ellipsoid(name='Krassowsky1940', a=6378245, f=0.00335233, f_=298.3, b=6356863.01877305)

44@var Ellipsoids.Maupertuis1738: Ellipsoid(name='Maupertuis1738', a=6397300, f=0.0052356, f_=191, b=6363806.28272251)

45@var Ellipsoids.Mercury1960: Ellipsoid(name='Mercury1960', a=6378166, f=0.00335233, f_=298.3, b=6356784.28360711)

46@var Ellipsoids.Mercury1968Mod: Ellipsoid(name='Mercury1968Mod', a=6378150, f=0.00335233, f_=298.3, b=6356768.33724438)

47@var Ellipsoids.NWL1965: Ellipsoid(name='NWL1965', a=6378145, f=0.00335289, f_=298.25, b=6356759.76948868)

48@var Ellipsoids.OSU86F: Ellipsoid(name='OSU86F', a=6378136.2, f=0.00335281, f_=298.2572236, b=6356751.51693008)

49@var Ellipsoids.OSU91A: Ellipsoid(name='OSU91A', a=6378136.3, f=0.00335281, f_=298.2572236, b=6356751.6165948)

50@var Ellipsoids.Plessis1817: Ellipsoid(name='Plessis1817', a=6376523, f=0.00324002, f_=308.64, b=6355862.93325557)

51@var Ellipsoids.PZ90: Ellipsoid(name='PZ90', a=6378136, f=0.0033528, f_=298.2578393, b=6356751.36174571)

52@var Ellipsoids.SGS85: Ellipsoid(name='SGS85', a=6378136, f=0.00335281, f_=298.257, b=6356751.30156878)

53@var Ellipsoids.SoAmerican1969: Ellipsoid(name='SoAmerican1969', a=6378160, f=0.00335289, f_=298.25, b=6356774.71919531)

54@var Ellipsoids.Sphere: Ellipsoid(name='Sphere', a=6371008.771415, f=0, f_=0, b=6371008.771415)

55@var Ellipsoids.SphereAuthalic: Ellipsoid(name='SphereAuthalic', a=6371000, f=0, f_=0, b=6371000)

56@var Ellipsoids.SpherePopular: Ellipsoid(name='SpherePopular', a=6378137, f=0, f_=0, b=6378137)

57@var Ellipsoids.Struve1860: Ellipsoid(name='Struve1860', a=6378298.3, f=0.00339294, f_=294.73, b=6356657.14266956)

58@var Ellipsoids.WGS60: Ellipsoid(name='WGS60', a=6378165, f=0.00335233, f_=298.3, b=6356783.28695944)

59@var Ellipsoids.WGS66: Ellipsoid(name='WGS66', a=6378145, f=0.00335289, f_=298.25, b=6356759.76948868)

60@var Ellipsoids.WGS72: Ellipsoid(name='WGS72', a=6378135, f=0.00335278, f_=298.26, b=6356750.52001609)

61@var Ellipsoids.WGS84: Ellipsoid(name='WGS84', a=6378137, f=0.00335281, f_=298.25722356, b=6356752.31424518)

62@var Ellipsoids.WGS84_NGS: Ellipsoid(name='WGS84_NGS', a=6378137, f=0.00335281, f_=298.2572221, b=6356752.31414035)

63'''

64# make sure int/int division yields float quotient, see .basics

65from __future__ import division as _; del _ # noqa: E702 ;

67# from pygeodesy.albers import AlbersEqualAreaCylindrical # _MODS

68from pygeodesy.basics import copysign0, isbool, _isin, isint, typename

69from pygeodesy.constants import EPS, EPS_2, EPS0, EPS02, EPS1, INF, NINF, \

70 _EPSqrt, PI_2, PI_3, PI2, PI4, R_M, R_MA, R_FM, \

71 _EPStol as _TOL, _floatuple as _T, _isfinite, \

72 _over, _SQRT2, _0_0s, _0_0, _0_5, _1_0, _1_EPS, \

73 _2_0, _4_0, _90_0, _0_25, _3_0 # PYCHOK used!

74# from pygeodesy.ellipses import Ellipse # _MODS

75from pygeodesy.errors import _AssertionError, IntersectionError, _ValueError, _xattr, _xkwds_not

76from pygeodesy.fmath import cbrt, cbrt2, fdot, fmean_, Fhorner, fpowers, hypot, hypot_, \

77 hypot1, hypot2, sqrt3, Fsum

78# from pygeodesy.fsums import Fsum # from .fmath

79# from pygeodesy.internals import typename # from .basics

80from pygeodesy.interns import NN, _a_, _Airy1830_, _AiryModified_, _b_, _Bessel1841_, \

81 _Clarke1866_, _Clarke1880IGN_, _DMAIN_, _DOT_, _f_, _GRS80_, \

82 _Intl1924_, _incompatible_, _invalid_, _Krassovski1940_, \

83 _Krassowsky1940_, _lat_, _meridional_, _negative_, _not_finite_, \

84 _prime_vertical_, _Sphere_, _SPACE_, _vs_, _WGS72_, _WGS84_

85# from pygeodesy.lazily import _ALL_LAZY, _ALL_MODS as _MODS # from .named

86from pygeodesy.named import _lazyNamedEnumItem as _lazy, _name__, _NamedEnum, \

87 _NamedEnumItem, _NamedTuple, _Pass, _ALL_LAZY, _MODS

88from pygeodesy.namedTuples import Circle4Tuple, Distance2Tuple, Vector3Tuple, Vector4Tuple

89from pygeodesy.props import deprecated_Property_RO, Property_RO, property_doc_, \

90 deprecated_property_RO, property_RO, property_ROver

91from pygeodesy.streprs import Fmt, fstr, instr, strs, unstr

92# from pygeodesy.triaxials.triaxial5 import _hartzell3, _plumbTo3 # _MODS

93from pygeodesy.units import Azimuth, Bearing, Distance, Float, Float_, Lamd, Lat, _Lat0, \

94 Meter, Meter2, Meter3, Phi, Phid, Radius, Radius_, Scalar

95from pygeodesy.utily import atan1, atan1d, atan2b, degrees90, m2radians, radians2m, sincos2d

97from math import asinh, atan, atanh, cos, degrees, exp, fabs, radians, sin, sinh, sqrt, tan # as _tan

99__all__ = _ALL_LAZY.ellipsoids

100__version__ = '26.03.25'

101

102_f_0_0 = Float(f =_0_0) # zero flattening

103_f__0_0 = Float(f_=_0_0) # zero inverse flattening

104# see U{WGS84_f<https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Constants.html>}

105# _f_WGS84 = Float(f =_1_0 / (298257223563 / 1000000000)) # 0.003_352_810_664_747_480_5

106_f__WGS84 = Float(f_=_1_0 / (1000000000 / 298257223563)) # 298.257223562_999_97 vs 298.257223563

107

108

109def _aux(lat, inverse, auxLat, clip=90):

110 '''Return a named auxiliary latitude in C{degrees}.

111 '''

112 return Lat(lat, clip=clip, name=_lat_ if inverse else typename(auxLat))

113

114

115def _sin2cos2(rad):

116 '''(INTERNAL) Return 2-tuple C{(sin(B{phi})**2, cos(B{phi})**2)}.

117 '''

118 if rad:

119 s2 = sin(rad)**2

120 if s2 > EPS:

121 c2 = _1_0 - s2

122 if c2 > EPS:

123 if c2 < EPS1:

124 return s2, c2

125 else:

126 return _1_0, _0_0 # rad == PI_2

127 return _0_0, _1_0 # rad == 0

128

129

130class a_f2Tuple(_NamedTuple):

131 '''2-Tuple C{(a, f)} specifying an ellipsoid by I{equatorial}

132 radius C{a} in C{meter} and scalar I{flattening} C{f}.

133

134 @see: Class L{Ellipsoid2}.

135 '''

136 _Names_ = (_a_, _f_) # name 'f' not 'f_'

137 _Units_ = (_Pass, _Pass)

138

139 def __new__(cls, a, f, **name):

140 '''New L{a_f2Tuple} ellipsoid specification.

141

142 @arg a: Equatorial radius (C{scalar} > 0).

143 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

144 @kwarg name: Optional C{B{name}=NN} (C{str}).

145

146 @return: An L{a_f2Tuple}C{(a, f)}.

147

148 @raise UnitError: Invalid B{C{a}} or B{C{f}}.

149

150 @note: C{abs(B{f}) < }L{EPS<pygeodesy.constants.EPS>} is

151 forced to C{B{f}=0}, I{spherical}.

152

153 @note: Negative C{B{f}} produces a I{prolate} ellipsoid.

154 '''

155 a = Radius_(a=a) # low=EPS, high=None

156 f = Float_( f=f, low=None, high=EPS1)

157 if fabs(f) < EPS: # force spherical

158 f = _f_0_0

159 return _NamedTuple.__new__(cls, a, f, **name)

160

161 @Property_RO

162 def b(self):

163 '''Get the I{polar} radius (C{meter}), M{a * (1 - f)}.

164 '''

165 return a_f2b(self.a, self.f) # PYCHOK .a and .f

166

167 def ellipsoid(self, **name):

168 '''Return an L{Ellipsoid} for this 2-tuple C{(a, f)}.

169

170 @kwarg name: Optional C{B{name}=NN} (C{str}).

171

172 @raise NameError: A registered C{ellipsoid} with the

173 same B{C{name}} already exists.

174 '''

175 return Ellipsoid(self.a, f=self.f, name=self._name__(name)) # PYCHOK .a and .f

176

177 @Property_RO

178 def f_(self):

179 '''Get the I{inverse} flattening (C{scalar}), M{1 / f} == M{a / (a - b)}.

180 '''

181 return f2f_(self.f) # PYCHOK .f

182

183

184class Curvature2Tuple(_NamedTuple):

185 '''2-Tuple C{(meridional, prime_vertical)} of radii of curvature, both in

186 C{meter}, conventionally.

187 '''

188 _Names_ = (_meridional_, _prime_vertical_)

189 _Units_ = ( Meter, Meter)

190

191 @property_RO

192 def transverse(self):

193 '''Get this I{prime_vertical}, aka I{transverse} radius of curvature.

194 '''

195 return self.prime_vertical

196

197

198class Ellipsoid(_NamedEnumItem):

199 '''Ellipsoid with I{equatorial} and I{polar} radii, I{flattening}, I{inverse

200 flattening} and other, often used, I{cached} attributes, supporting

201 I{oblate} and I{prolate} ellipsoidal and I{spherical} earth models.

202 '''

203 _a = 0 # equatorial radius, semi-axis (C{meter})

204 _b = 0 # polar radius, semi-axis (C{meter}): a * (f - 1) / f

205 _f = 0 # (1st) flattening: (a - b) / a

206 _f_ = 0 # inverse flattening: 1 / f = a / (a - b)

207

208 _geodsolve = NN # means, use PYGEODESY_GEODSOLVE

209 _KsOrder = 8 # Krüger series order (4, 6 or 8)

210 _rhumbsolve = NN # means, use PYGEODESY_RHUMBSOLVE

211

212 def __init__(self, a, b=None, f_=None, f=None, **name):

213 '''New L{Ellipsoid} from the I{equatorial} radius I{and} either

214 the I{polar} radius or I{inverse flattening} or I{flattening}.

215

216 @arg a: Equatorial radius, semi-axis (C{meter}).

217 @arg b: Optional polar radius, semi-axis (C{meter}).

218 @arg f_: Inverse flattening: M{a / (a - b)} (C{float} >>> 1.0).

219 @arg f: Flattening: M{(a - b) / a} (C{scalar}, near zero for

220 spherical).

221 @kwarg name: Optional, unique C{B{name}=NN} (C{str}).

222

223 @raise NameError: Ellipsoid with the same B{C{name}} already exists.

224

225 @raise ValueError: Invalid B{C{a}}, B{C{b}}, B{C{f_}} or B{C{f}} or

226 B{C{f_}} and B{C{f}} are incompatible.

227

228 @note: M{abs(f_) > 1 / EPS} or M{abs(1 / f_) < EPS} is forced

229 to M{1 / f_ = 0}, spherical.

230 '''

231 ff_ = f, f_ # assertion below

232 n = _name__(**name) if name else NN

233 try:

234 a = Radius_(a=a) # low=EPS

235 if not _isfinite(a):

236 raise ValueError(_SPACE_(_a_, _not_finite_))

237

238 if b: # not _isin(b, None, _0_0)

239 b = Radius_(b=b) # low=EPS

240 f = a_b2f(a, b) if f is None else Float(f=f)

241 f_ = f2f_(f) if f_ is None else Float(f_=f_)

242 elif f is not None:

243 f = Float(f=f)

244 b = a_f2b(a, f)

245 f_ = f2f_(f) if f_ is None else Float(f_=f_)

246 elif f_:

247 f_ = Float(f_=f_)

248 b = a_f_2b(a, f_) # a * (f_ - 1) / f_

249 f = f_2f(f_)

250 else: # only a, spherical

251 f_ = f = 0

252 b = a # superfluous

253

254 if not (f < _1_0): # sanity check, see .ecef.Ecef.__init__

255 raise ValueError(_SPACE_(_f_, _invalid_))

256 if not _isfinite(b):

257 raise ValueError(_SPACE_(_b_, _not_finite_))

258

259 if fabs(f) < EPS or a == b or not f_: # spherical

260 b = a

261 f = _f_0_0

262 f_ = _f__0_0

263

264 except (TypeError, ValueError) as x:

265 d = _xkwds_not(None, b=b, f_=f_, f=f)

266 t = instr(self, a=a, name=n, **d)

267 raise _ValueError(t, cause=x)

268

269 self._a = a

270 self._b = b

271 self._f = f

272 self._f_ = f_

273

274 self._register(Ellipsoids, n)

275

276 if f and f_: # see test/testEllipsoidal

277 d = dict(eps=_TOL)

278 if None in ff_: # both f_ and f given

279 d.update(Error=_ValueError, txt=_incompatible_)

280 self._assert(_1_0 / f, f_=f_, **d)

281 self._assert(_1_0 / f_, f =f, **d)

282 self._assert(self.b2_a2, e21=self.e21, eps=EPS)

283

284 def __eq__(self, other):

285 '''Compare this and an other ellipsoid.

286

287 @arg other: The other ellipsoid (L{Ellipsoid} or L{Ellipsoid2}).

288

289 @return: C{True} if equal, C{False} otherwise.

290 '''

291 return self is other or (isinstance(other, Ellipsoid) and

292 self.a == other.a and

293 (self.f == other.f or self.b == other.b))

294

295 def __hash__(self):

296 return self._hash # memoized

297

298 @Property_RO

299 def a(self):

300 '''Get the I{equatorial} radius, semi-axis (C{meter}).

301 '''

302 return self._a

303

304 equatoradius = a # = Requatorial

305

306 @Property_RO

307 def a2(self):

308 '''Get the I{equatorial} radius I{squared} (C{meter} I{squared}), M{a**2}.

309 '''

310 return Meter2(a2=self.a**2)

311

312 @Property_RO

313 def a2_(self):

314 '''Get the inverse of the I{equatorial} radius I{squared} (C{meter} I{squared}), M{1 / a**2}.

315 '''

316 return Float(a2_=_1_0 / self.a2)

317

318 @Property_RO

319 def A(self):

320 '''Get the UTM I{meridional (or rectifying)} radius (C{meter}).

321

322 @note: C{A * PI / 2} ≈= L{L<Ellipsoid.L>}, the I{quarter meridian}.

323

324 @see: I{Meridian arc unit} U{Q<https://StudyLib.net/doc/7443565/>},

325 the mean, meridional length I{per radian}.

326 '''

327 A, n = self.a, self.n

328 if n:

329 d = (n + _1_0) * 1048576 / A

330 if d: # use 6 n**2 terms, half-way between the _KsOrder's 4, 6, 8

331 # <https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>

332 # <https://GeographicLib.SourceForge.io/C++/doc/transversemercator.html> and

333 # <https://www.MyGeodesy.id.AU/documents/Karney-Krueger%20equations.pdf> (3)

334 # A *= fhorner(n**2, 1048576, 262144, 16384, 4096, 1600, 784, 441) / 1048576) / (1 + n)

335 A = Radius(A=Fhorner(n**2, 1048576, 262144, 16384, 4096, 1600, 784, 441).fover(d))

336 return A

337# # Moritz, H. <https://Geodesy.Geology.Ohio-State.edu/course/refpapers/00740128.pdf>

338# # q = 4 / self.rocPolar

339# # Q = (1 - 3 / 4 * e'2 + 45 / 64 * e'4 - 175 / 256 * e'6 + 11025 / 16384 * e'8) * rocPolar

340# # = (4 + e'2 * (-3 + e'2 * (45 / 16 + e'2 * (-175 / 64 + e'2 * 11025 / 4096)))) / q

341# return Radius(Q=Fhorner(self.e22, 4, -3, 45 / 16, -175 / 64, 11025 / 4096).fover(q))

342

343 @Property_RO

344 def a_b(self):

345 '''Get the ratio I{equatorial} over I{polar} radius (C{float}), M{a / b} == M{1 / (1 - f)}.

346 '''

347 return Float(a_b=self.a / self.b if self.f else _1_0)

348

349 @Property_RO

350 def a2_b(self):

351 '''Get the I{polar} meridional (or polar) radius of curvature (C{meter}), M{a**2 / b}.

352

353 @see: U{Radii of Curvature

354 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}

355 and U{Moritz, H. (1980), Geodetic Reference System 1980

356 <https://WikiPedia.org/wiki/Earth_radius#cite_note-Moritz-2>}.

357

358 @note: Symbol C{c} is used by IUGG and IERS for the U{polar radius of curvature

359 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}, see L{c2}

360 and L{R2} or L{Rauthalic}.

361 '''

362 return Radius(a2_b=self.a2 / self.b if self.f else self.a) # = rocPolar

363

364 @Property_RO

365 def a2_b2(self):

366 '''Get the ratio I{equatorial} over I{polar} radius I{squared} (C{float}),

367 M{(a / b)**2} == M{1 / (1 - e**2)} == M{1 / (1 - e2)} == M{1 / e21}.

368 '''

369 return Float(a2_b2=self.a_b**2 if self.f else _1_0)

370

371 @Property_RO

372 def a_f(self):

373 '''Get the I{equatorial} radius and I{flattening} (L{a_f2Tuple}), see method C{toEllipsoid2}.

374 '''

375 return a_f2Tuple(self.a, self.f, name=self.name)

376

377 a_f2 = a_f # synonym

378

379 @Property_RO

380 def _albersCyl(self):

381 '''(INTERNAL) Helper for C{auxAuthalic}.

382 '''

383 return _MODS.albers.AlbersEqualAreaCylindrical(datum=self, name=self.name)

384

385 @Property_RO

386 def AlphaKs(self):

387 '''Get the I{Krüger} U{Alpha series coefficients<https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>} (C{KsOrder}C{-tuple}).

388 '''

389 return self._Kseries( # XXX int/int quotients may require from __future__ import division as _; del _ # noqa: E702 ;

390 # n n**2 n**3 n**4 n**5 n**6 n**7 n**8

391 _T(1/2, -2/3, 5/16, 41/180, -127/288, 7891/37800, 72161/387072, -18975107/50803200),

392 _T(13/48, -3/5, 557/1440, 281/630, -1983433/1935360, 13769/28800, 148003883/174182400), # PYCHOK unaligned

393 _T(61/240, -103/140, 15061/26880, 167603/181440, -67102379/29030400, 79682431/79833600), # PYCHOK unaligned

394 _T(49561/161280, -179/168, 6601661/7257600, 97445/49896, -40176129013/7664025600), # PYCHOK unaligned

395 _T(34729/80640, -3418889/1995840, 14644087/9123840, 2605413599/622702080), # PYCHOK unaligned

396 _T(212378941/319334400, -30705481/10378368, 175214326799/58118860800), # PYCHOK unaligned

397 _T(1522256789/1383782400, -16759934899/3113510400), # PYCHOK unaligned

398 _T(1424729850961/743921418240)) # PYCHOK unaligned

399

400 @Property_RO

401 def area(self):

402 '''Get the ellipsoid's surface area (C{meter} I{squared}), M{4 * PI * c2}.

403

404 @see: Properties L{areax}, L{c2} and L{R2} and functions

405 L{ellipsoidalExact.areaOf} and L{ellipsoidalKarney.areaOf}.

406 '''

407 return Meter2(area=self.c2 * PI4)

408

409 @Property_RO

410 def areax(self):

411 '''Get the ellipsoid's surface area (C{meter} I{squared}), M{4 * PI * c2x}, more

412 accurate for very I{oblate} ellipsoids.

413

414 @see: Properties L{area}, L{c2x} and L{R2x}, class L{GeodesicExact} and

415 functions L{ellipsoidalExact.areaOf} and L{ellipsoidalKarney.areaOf}.

416 '''

417 return Meter2(areax=self.c2x * PI4)

418

419 def _assert(self, val, eps=_TOL, f0=_0_0, Error=_AssertionError, txt=NN, **name_value):

420 '''(INTERNAL) Assert a C{name=value} vs C{val}.

421 '''

422 for n, v in name_value.items():

423 if fabs(v - val) > eps: # PYCHOK no cover

424 t = (v, _vs_, val)

425 t = _SPACE_.join(strs(t, prec=12, fmt=Fmt.g))

426 t = Fmt.EQUAL(self._DOT_(n), t)

427 raise Error(t, txt=txt or Fmt.exceeds_eps(eps))

428 return Float(v if self.f else f0, name=n)

429 raise Error(unstr(self._DOT_(typename(self._assert)), val,

430 eps=eps, f0=f0, **name_value))

431

432 def auxAuthalic(self, lat, inverse=False):

433 '''Compute the I{authalic} auxiliary latitude (Xi) or the I{inverse} thereof.

434

435 @arg lat: The geodetic (or I{authalic}) latitude (C{degrees90}).

436 @kwarg inverse: If C{True}, B{C{lat}} is the I{authalic} and

437 return the geodetic latitude (C{bool}).

438

439 @return: The I{authalic} (or geodetic) latitude in C{degrees90}.

440

441 @see: U{Inverse-/AuthalicLatitude<https://GeographicLib.SourceForge.io/

442 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Authalic latitude

443 <https://WikiPedia.org/wiki/Latitude#Authalic_latitude>}, and

444 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, p 16.

445 '''

446 if self.f:

447 _f = self._albersCyl._tanf if inverse else \

448 self._albersCyl._txif # PYCHOK attr

449 lat = atan1d(_f(tan(Phid(lat)))) # PYCHOK attr

450 return _aux(lat, inverse, Ellipsoid.auxAuthalic)

451

452 def auxConformal(self, lat, inverse=False):

453 '''Compute the I{conformal} auxiliary latitude (Chi) or the I{inverse} thereof.

454

455 @arg lat: The geodetic (or I{conformal}) latitude (C{degrees90}).

456 @kwarg inverse: If C{True}, B{C{lat}} is the I{conformal} and

457 return the geodetic latitude (C{bool}).

458

459 @return: The I{conformal} (or geodetic) latitude in C{degrees90}.

460

461 @see: U{Inverse-/ConformalLatitude<https://GeographicLib.SourceForge.io/

462 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Conformal latitude

463 <https://WikiPedia.org/wiki/Latitude#Conformal_latitude>}, and

464 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 15-16.

465 '''

466 if self.f:

467 _f = self.es_tauf if inverse else self.es_taupf # PYCHOK attr

468 lat = atan1d(_f(tan(Phid(lat)))) # PYCHOK attr

469 return _aux(lat, inverse, Ellipsoid.auxConformal)

470

471 def auxGeocentric(self, lat, inverse=False, height=_0_0):

472 '''Compute the I{geocentric} auxiliary latitude (Theta) or the I{inverse} thereof.

473

474 @arg lat: The geodetic (or I{geocentric}) latitude (C{degrees90}).

475 @kwarg inverse: If C{True}, B{C{lat}} is the geocentric and

476 return the I{geocentric} latitude (C{bool}).

477 @kwarg height: Optional, ellipsoidal height (C{meter}).

478

479 @return: The I{geocentric} (or geodetic) latitude in C{degrees90}.

480

481 @see: U{Inverse-/GeocentricLatitude<https://GeographicLib.SourceForge.io/

482 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Geocentric latitude

483 <https://WikiPedia.org/wiki/Latitude#Geocentric_latitude>}, and

484 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 17-18.

485 '''

486 if self.f: # and lat

487 t = tan(Phid(lat))

488 f = self.b2_a2

489 if height:

490 if inverse:

491 lat = atan1d(t * f) # geodetic n

492 d, f = f, _1_0

493 else:

494 d = _1_0

495 n = self.rocPrimeVertical(lat)

496 f = _over(n * f + height, n * d + height)

497 elif inverse:

498 f = self.a2_b2

499 lat = atan1d(t * f)

500 return _aux(lat, inverse, Ellipsoid.auxGeocentric)

501

502 def auxIsometric(self, lat, inverse=False):

503 '''Compute the I{isometric} auxiliary latitude (Psi) or the I{inverse} thereof.

504

505 @arg lat: The geodetic (or I{isometric}) latitude (C{degrees}).

506 @kwarg inverse: If C{True}, B{C{lat}} is the I{isometric} and

507 return the geodetic latitude (C{bool}).

508

509 @return: The I{isometric} (or geodetic) latitude in C{degrees}.

510

511 @note: The I{isometric} latitude for geodetic C{+/-90} is far

512 outside the C{[-90..+90]} range but the inverse thereof

513 is the original geodetic latitude.

514

515 @see: U{Inverse-/IsometricLatitude<https://GeographicLib.SourceForge.io/

516 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Isometric latitude

517 <https://WikiPedia.org/wiki/Latitude#Isometric_latitude>}, and

518 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 15-16.

519 '''

520 if self.f:

521 r = Phid(lat, clip=0)

522 lat = degrees(atan1(self.es_tauf(sinh(r))) if inverse else

523 asinh(self.es_taupf(tan(r))))

524 # clip=0, since auxIsometric(+/-90) is far outside [-90..+90]

525 return _aux(lat, inverse, Ellipsoid.auxIsometric, clip=0)

526

527 def auxParametric(self, lat, inverse=False):

528 '''Compute the I{parametric} auxiliary latitude (Beta) or the I{inverse} thereof.

529

530 @arg lat: The geodetic (or I{parametric}) latitude (C{degrees90}).

531 @kwarg inverse: If C{True}, B{C{lat}} is the I{parametric} and

532 return the geodetic latitude (C{bool}).

533

534 @return: The I{parametric} (or geodetic) latitude in C{degrees90}.

535

536 @see: U{Inverse-/ParametricLatitude<https://GeographicLib.SourceForge.io/

537 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Parametric latitude

538 <https://WikiPedia.org/wiki/Latitude#Parametric_(or_reduced)_latitude>},

539 and U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, p 18.

540 '''

541 if self.f:

542 lat = self._Betad(Lat(lat), inverse=inverse)

543 return _aux(lat, inverse, Ellipsoid.auxParametric)

544

545 auxReduced = auxParametric # synonymous

546

547 def auxRectifying(self, lat, inverse=False):

548 '''Compute the I{rectifying} auxiliary latitude (Mu) or the I{inverse} thereof.

549

550 @arg lat: The geodetic (or I{rectifying}) latitude (C{degrees90}).

551 @kwarg inverse: If C{True}, B{C{lat}} is the I{rectifying} and

552 return the geodetic latitude (C{bool}).

553

554 @return: The I{rectifying} (or geodetic) latitude in C{degrees90}.

555

556 @see: U{Inverse-/RectifyingLatitude<https://GeographicLib.SourceForge.io/

557 C++/doc/classGeographicLib_1_1Ellipsoid.html>}, U{Rectifying latitude

558 <https://WikiPedia.org/wiki/Latitude#Rectifying_latitude>}, and

559 U{Snyder<https://Pubs.USGS.gov/pp/1395/report.pdf>}, pp 16-17.

560 '''

561 if self.f:

562 lat = Lat(lat)

563 if 0 < fabs(lat) < _90_0:

564 if inverse:

565 e = self._elliptic_e22

566 d = degrees90(e.fEinv(e.cE * lat / _90_0))

567 lat = self.auxParametric(d, inverse=True)

568 else:

569 lat = _over(self.Llat(lat), self.L) * _90_0

570 return _aux(lat, inverse, Ellipsoid.auxRectifying)

571

572 @Property_RO

573 def b(self):

574 '''Get the I{polar} radius, semi-axis (C{meter}).

575 '''

576 return self._b

577

578 polaradius = b # = Rpolar

579

580 @Property_RO

581 def b_a(self):

582 '''Get the ratio I{polar} over I{equatorial} radius (C{float}), M{b / a == f1 == 1 - f}.

583

584 @see: Property L{f1}.

585 '''

586 return self._assert(self.b / self.a, b_a=self.f1, f0=_1_0)

587

588 @Property_RO

589 def b2(self):

590 '''Get the I{polar} radius I{squared} (C{float}), M{b**2}.

591 '''

592 return Meter2(b2=self.b**2)

593

594 @Property_RO

595 def b2_a(self):

596 '''Get the I{equatorial} meridional radius of curvature (C{meter}), M{b**2 / a}, see C{rocMeridional}C{(0)}.

597

598 @see: U{Radii of Curvature<https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}.

599 '''

600 return Radius(b2_a=_over(self.b2, self.a) if self.f else self.b)

601

602 @Property_RO

603 def b2_a2(self):

604 '''Get the ratio I{polar} over I{equatorial} radius I{squared} (C{float}), M{(b / a)**2}

605 == M{(1 - f)**2} == M{1 - e**2} == C{e21}.

606 '''

607 return Float(b2_a2=self.b_a**2 if self.f else _1_0)

608

609 def _Betad(self, lat, inverse=False):

610 '''(INTERNAL) Get the I{parametric (or reduced) auxiliary latitude} or inverse thereof.

611 '''

612 s, c = sincos2d(lat) # like Karney's tand(lat)

613 s *= self.a_b if inverse else self.b_a

614 return atan1d(s, c) # (s * a, c * b) if inverse else (s * b, c * a)

615

616 @Property_RO

617 def BetaKs(self):

618 '''Get the I{Krüger} U{Beta series coefficients<https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>} (C{KsOrder}C{-tuple}).

619 '''

620 return self._Kseries( # XXX int/int quotients may require from __future__ import division as _; del _ # noqa: E702 ;

621 # n n**2 n**3 n**4 n**5 n**6 n**7 n**8

622 _T(1/2, -2/3, 37/96, -1/360, -81/512, 96199/604800, -5406467/38707200, 7944359/67737600),

623 _T(1/48, 1/15, -437/1440, 46/105, -1118711/3870720, 51841/1209600, 24749483/348364800), # PYCHOK unaligned

624 _T(17/480, -37/840, -209/4480, 5569/90720, 9261899/58060800, -6457463/17740800), # PYCHOK unaligned

625 _T(4397/161280, -11/504, -830251/7257600, 466511/2494800, 324154477/7664025600), # PYCHOK unaligned

626 _T(4583/161280, -108847/3991680, -8005831/63866880, 22894433/124540416), # PYCHOK unaligned

627 _T(20648693/638668800, -16363163/518918400, -2204645983/12915302400), # PYCHOK unaligne

628 _T(219941297/5535129600, -497323811/12454041600), # PYCHOK unaligned

629 _T(191773887257/3719607091200)) # PYCHOK unaligned

630

631 @deprecated_Property_RO

632 def c(self): # PYCHOK no cover

633 '''DEPRECATED, use property C{R2} or C{Rauthalic}.'''

634 return self.R2

635

636 @Property_RO

637 def c2(self):

638 '''Get the I{authalic} earth radius I{squared} (C{meter} I{squared}).

639

640 @see: Properties L{c2x}, L{area}, L{R2}, L{Rauthalic}, I{Karney's} U{equation (60)

641 <https://Link.Springer.com/article/10.1007%2Fs00190-012-0578-z>} and C++ U{Ellipsoid.Area

642 <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Ellipsoid.html>},

643 U{Authalic radius<https://WikiPedia.org/wiki/Earth_radius#Authalic_radius>}, U{Surface area

644 <https://WikiPedia.org/wiki/Ellipsoid>} and U{surface area

645 <https://www.Numericana.com/answer/geometry.htm#oblate>}.

646 '''

647 return self._c2f(False)

648

649 @Property_RO

650 def c2x(self):

651 '''Get the I{authalic} earth radius I{squared} (C{meter} I{squared}), more accurate for very I{oblate}

652 ellipsoids.

653

654 @see: Properties L{c2}, L{areax}, L{R2x}, L{Rauthalicx}, class L{GeodesicExact} and I{Karney}'s comments at C++

655 attribute U{GeodesicExact._c2<https://GeographicLib.SourceForge.io/C++/doc/GeodesicExact_8cpp_source.html>}.

656 '''

657 return self._c2f(True)

658

659 def _c2f(self, c2x):

660 '''(INTERNAL) Helper for C{.c2} and C{.c2x}.

661 '''

662 f, c2 = self.f, self.b2

663 if f:

664 e = self.e

665 if e > EPS0:

666 if f > 0: # .isOblate

667 c2 *= (asinh(sqrt(self.e22abs)) if c2x else atanh(e)) / e

668 elif f < 0: # .isProlate

669 c2 *= atan1(e) / e # XXX asin?

670 c2 = Meter2(c2=(self.a2 + c2) * _0_5)

671 return c2

672

673 def circle4(self, lat):

674 '''Get the equatorial or a parallel I{circle of latitude}.

675

676 @arg lat: Geodetic latitude (C{degrees90} or C{str}).

677

678 @return: A L{Circle4Tuple}C{(radius, height, lat, beta)}.

679

680 @raise RangeError: Latitude B{C{lat}} outside valid range, only if

681 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

682

683 @raise TypeError: Invalid B{C{lat}}.

684

685 @raise ValueError: Invalid B{C{lat}}.

686

687 @see: Definition of U{I{p} and I{z} under B{Parametric (or reduced) latitude}

688 <https://WikiPedia.org/wiki/Latitude>}, I{Karney's} C++ U{CircleRadius and CircleHeight

689 <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Ellipsoid.html>}

690 and method C{Triaxial.ellipse5}.

691 '''

692 lat = _Lat0(lat)

693 if lat:

694 B = lat # beta

695 if fabs(lat) < _90_0:

696 if self.f:

697 B = self._Betad(lat)

698 z, r = sincos2d(B)

699 r *= self.a

700 z *= self.b

701 else: # near-polar

702 r, z = _0_0, copysign0(self.b, lat)

703 else: # equatorial

704 r = self.a

705 z = lat = B = _0_0

706 return Circle4Tuple(r, z, lat, B)

707

708 def degrees2m(self, deg, lat=0):

709 '''Convert an arc in degrees to a distance along the equator or

710 along a parallel of (geodetic) latitude.

711

712 @arg deg: The angle (C{degrees}).

713 @kwarg lat: Parallel latitude (C{degrees90}, C{str}).

714

715 @return: Distance (C{meter}, same units as the equatorial

716 and polar radii) or C{0} for near-polar B{C{lat}}.

717

718 @raise RangeError: Latitude B{C{lat}} outside valid range and

719 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

720

721 @raise ValueError: Invalid B{C{deg}} or B{C{lat}}.

722 '''

723 return self.radians2m(radians(deg), lat=lat)

724

725 def distance2(self, lat0, lon0, lat1, lon1):

726 '''I{Approximate} the distance and (initial) bearing between

727 two points based on the U{local, flat earth approximation

728 <https://www.EdWilliams.org/avform.htm#flat>} aka U{Hubeny

729 <https://www.OVG.AT/de/vgi/files/pdf/3781/>} formula.

730

731 I{Suitable only for distances of several hundred Km or Miles

732 and only between points not near-polar}.

733

734 @arg lat0: From latitude (C{degrees}).

735 @arg lon0: From longitude (C{degrees}).

736 @arg lat1: To latitude (C{degrees}).

737 @arg lon1: To longitude (C{degrees}).

738

739 @return: A L{Distance2Tuple}C{(distance, initial)} with C{distance}

740 in same units as this ellipsoid's axes.

741

742 @note: The meridional and prime_vertical radii of curvature are

743 taken and scaled I{at the initial latitude}, see C{roc2}.

744

745 @see: Function L{pygeodesy.flatLocal}/L{pygeodesy.hubeny}.

746 '''

747 phi0 = Phid(lat0=lat0)

748 m, n = self.roc2_(phi0, scaled=True)

749 m *= Phid(lat1=lat1) - phi0

750 n *= Lamd(lon1=lon1) - Lamd(lon0=lon0)

751 return Distance2Tuple(hypot(m, n), atan2b(n, m))

752

753 @Property_RO

754 def e(self):

755 '''Get the I{unsigned, (1st) eccentricity} (C{float}), M{sqrt(1 - (b / a)**2))}, see C{a_b2e}.

756

757 @see: Property L{es}.

758 '''

759 return Float(e=sqrt(self.e2abs) if self.e2 else _0_0)

760

761 @deprecated_Property_RO

762 def e12(self): # see property ._e12

763 '''DEPRECATED, use property C{e21}.'''

764 return self.e21

765

766# @Property_RO

767# def _e12(self): # see property ._elliptic_e12

768# # (INTERNAL) until e12 above can be replaced with e21.

769# return self.e2 / (_1_0 - self.e2) # see I{Karney}'s Ellipsoid._e12 = e2 / (1 - e2)

770

771 @Property_RO

772 def e2(self):

773 '''Get the I{signed, (1st) eccentricity squared} (C{float}), M{f * (2 - f)

774 == 1 - (b / a)**2}, see C{a_b2e2}.

775 '''

776 return self._assert(a_b2e2(self.a, self.b), e2=f2e2(self.f))

777

778 @Property_RO

779 def e2abs(self):

780 '''Get the I{unsigned, (1st) eccentricity squared} (C{float}).

781 '''

782 return fabs(self.e2)

783

784 @Property_RO

785 def e21(self):

786 '''Get 1 less I{1st eccentricity squared} (C{float}), M{1 - e**2}

787 == M{1 - e2} == M{(1 - f)**2} == M{b**2 / a**2}, see C{b2_a2}.

788 '''

789 return self._assert((_1_0 - self.f)**2, e21=_1_0 - self.e2, f0=_1_0)

790

791# _e2m = e21 # see I{Karney}'s Ellipsoid._e2m = 1 - _e2

792 _1_e21 = a2_b2 # == M{1 / e21} == M{1 / (1 - e**2)}

793

794 @Property_RO

795 def e22(self):

796 '''Get the I{signed, 2nd eccentricity squared} (C{float}), M{e2 / (1 - e2)

797 == e2 / (1 - f)**2 == (a / b)**2 - 1}, see C{a_b2e22}.

798 '''

799 return self._assert(a_b2e22(self.a, self.b), e22=f2e22(self.f))

800

801 @Property_RO

802 def e22abs(self):

803 '''Get the I{unsigned, 2nd eccentricity squared} (C{float}).

804 '''

805 return fabs(self.e22)

806

807 @Property_RO

808 def e32(self):

809 '''Get the I{signed, 3rd eccentricity squared} (C{float}), M{e2 / (2 - e2)

810 == (a**2 - b**2) / (a**2 + b**2)}, see C{a_b2e32}.

811 '''

812 return self._assert(a_b2e32(self.a, self.b), e32=f2e32(self.f))

813

814 @Property_RO

815 def e32abs(self):

816 '''Get the I{unsigned, 3rd eccentricity squared} (C{float}).

817 '''

818 return fabs(self.e32)

819

820 @Property_RO

821 def e4(self):

822 '''Get the I{unsignd, (1st) eccentricity} to 4th power (C{float}), M{e**4 == e2**2}.

823 '''

824 return Float(e4=self.e2**2 if self.e2 else _0_0)

825

826 eccentricity = e # eccentricity

827# eccentricity2 = e2 # eccentricity squared

828 eccentricity1st2 = e2 # first eccentricity squared, signed

829 eccentricity2nd2 = e22 # second eccentricity squared, signed

830 eccentricity3rd2 = e32 # third eccentricity squared, signed

831

832 def ecef(self, Ecef=None):

833 '''Return U{ECEF<https://WikiPedia.org/wiki/ECEF>} converter.

834

835 @kwarg Ecef: ECEF class to use, default L{EcefKarney}.

836

837 @return: An ECEF converter for this C{ellipsoid}.

838

839 @raise TypeError: Invalid B{C{Ecef}}.

840

841 @see: Module L{pygeodesy.ecef}.

842 '''

843 return _MODS.ecef._4Ecef(self, Ecef)

844

845 @Property_RO

846 def _elliptic_e12(self): # see I{Karney}'s Ellipsoid._e12

847 '''(INTERNAL) Elliptic helper for C{Rhumb}.

848 '''

849 e12 = _over(self.e2, self.e2 - _1_0) # NOT DEPRECATED .e12!

850 return _MODS.elliptic.Elliptic(e12)

851

852 @Property_RO

853 def _elliptic_e22(self): # aka ._elliptic_ep2

854 '''(INTERNAL) Elliptic helper for C{auxRectifying}, C{L}, C{Llat}.

855 '''

856 return _MODS.elliptic.Elliptic(-self.e22abs) # complex

857

858 equatoradius = a # Requatorial

859

860 @Property_RO

861 def equatorimeter(self):

862 '''Get the ellipsoid's I{equatorial} perimeter (C{meter}).

863 '''

864 return Meter(equatorimeter=self.a * PI2)

865

866 def e2s(self, s):

867 '''Compute norm M{sqrt(1 - e2 * s**2)}.

868

869 @arg s: Sine value (C{scalar}).

870

871 @return: Norm (C{float}).

872

873 @raise ValueError: Invalid B{C{s}}.

874 '''

875 return sqrt(self.e2s2(s)) if self.e2 else _1_0

876

877 def e2s2(self, s):

878 '''Compute M{1 - e2 * s**2}.

879

880 @arg s: Sine value (C{scalar}).

881

882 @return: Result (C{float}).

883

884 @raise ValueError: Invalid B{C{s}}.

885 '''

886 r, e2 = _1_0, self.e2

887 if e2: # and s

888 try:

889 r -= e2 * Scalar(s=s)**2

890 if r < 0:

891 raise ValueError(_negative_)

892 except (TypeError, ValueError) as x:

893 t = self._DOT_(typename(Ellipsoid.e2s2))

894 raise _ValueError(t, s, cause=x)

895 return r

896

897 @Property_RO

898 def es(self):

899 '''Get the I{signed (1st) eccentricity} (C{float}).

900

901 @see: Property L{e}.

902 '''

903 # note, self.e is always non-negative

904 return Float(es=copysign0(self.e, self.f)) # see .ups

905

906 def es_atanh(self, x):

907 '''Compute M{es * atanh(es * x)} or M{-es * atan(es * x)}

908 for I{oblate} respectively I{prolate} ellipsoids where

909 I{es} is the I{signed} (1st) eccentricity.

910

911 @raise ValueError: Invalid B{C{x}}.

912

913 @see: Function U{Math::eatanhe<https://GeographicLib.SourceForge.io/

914 C++/doc/classGeographicLib_1_1Math.html>}.

915 '''

916 return self._es_atanh(Scalar(x=x)) if self.f else _0_0

917

918 def _es_atanh(self, x): # see .albers._atanhee, .AuxLat._atanhee

919 '''(INTERNAL) Helper for .es_atanh, ._es_taupf2 and ._exp_es_atanh.

920 '''

921 es = self.es # signOf(es) == signOf(f)

922 return es * (atanh(es * x) if es > 0 else # .isOblate

923 (-atan(es * x) if es < 0 else # .isProlate

924 _0_0)) # .isSpherical

925

926 @Property_RO

927 def es_c(self):

928 '''Get M{(1 - f) * exp(es_atanh(1))} (C{float}), M{b_a * exp(es_atanh(1))}.

929 '''

930 return Float(es_c=(self._exp_es_atanh_1 * self.b_a) if self.f else _1_0)

931

932 def es_tauf(self, taup):

933 '''Compute I{Karney}'s U{equations (19), (20) and (21)

934 <https://ArXiv.org/abs/1002.1417>}.

935

936 @see: I{Karney}'s C++ method U{Math::tauf<https://GeographicLib.

937 SourceForge.io/C++/doc/classGeographicLib_1_1Math.html>} and

938 and I{Veness}' JavaScript method U{toLatLon<https://www.

939 Movable-Type.co.UK/scripts/latlong-utm-mgrs.html>}.

940 '''

941 t = Scalar(taup=taup)

942 if self.f: # .isEllipsoidal

943 a = fabs(t)

944 T = (self._exp_es_atanh_1 if a > 70 else self._1_e21) * t

945 if fabs(T * _EPSqrt) < _2_0: # handles +/- INF and NAN

946 s = (a * _TOL) if a > _1_0 else _TOL

947 for T, _, d in self._es_tauf3(t, T): # max 2

948 if fabs(d) < s:

949 break

950 t = Scalar(tauf=T)

951 return t

952

953 def _es_tauf3(self, taup, T, N=9): # in .utm.Utm._toLLEB

954 '''(INTERNAL) Yield a 3-tuple C{(τi, iteration, delta)} for at most

955 B{C{N}} Newton iterations, converging rapidly except when C{delta}

956 toggles on +/-1.12e-16 or +/-4.47e-16, see C{.utm.Utm._toLLEB}.

957 '''

958 e = self._1_e21

959 _F2_ = Fsum(T).fsum2f_ # τ0

960 _tf2 = self._es_taupf2

961 for i in range(1, N + 1):

962 a, h = _tf2(T)

963 # = (taup - a) / hypot1(a) / ((e + T**2) / h)

964 d = _over((taup - a) * (T**2 + e), hypot1(a) * h)

965 T, d = _F2_(d) # τi, (τi - τi-1)

966 yield T, i, d

967

968 def es_taupf(self, tau):

969 '''Compute I{Karney}'s U{equations (7), (8) and (9)

970 <https://ArXiv.org/abs/1002.1417>}.

971

972 @see: I{Karney}'s C++ method U{Math::taupf<https://GeographicLib.

973 SourceForge.io/C++/doc/classGeographicLib_1_1Math.html>}.

974 '''

975 t = Scalar(tau=tau)

976 if self.f: # .isEllipsoidal

977 t, _ = self._es_taupf2(t)

978 t = Scalar(taupf=t)

979 return t

980

981 def _es_taupf2(self, tau):

982 '''(INTERNAL) Return 2-tuple C{(es_taupf(tau), hypot1(tau))}.

983 '''

984 if _isfinite(tau):

985 h = hypot1(tau)

986 s = sinh(self._es_atanh(tau / h))

987 a = hypot1(s) * tau - h * s

988 else:

989 a, h = tau, INF

990 return a, h

991

992 @Property_RO

993 def _exp_es_atanh_1(self):

994 '''(INTERNAL) Helper for .es_c and .es_tauf.

995 '''

996 return exp(self._es_atanh(_1_0)) if self.es else _1_0

997

998 @Property_RO

999 def f(self):

1000 '''Get the I{flattening} (C{scalar}), M{(a - b) / a}, C{0} for spherical, negative for prolate.

1001 '''

1002 return self._f

1003

1004 @Property_RO

1005 def f_(self):

1006 '''Get the I{inverse flattening} (C{scalar}), M{1 / f} == M{a / (a - b)}, C{0} for spherical, see C{a_b2f_}.

1007 '''

1008 return self._f_

1009

1010 @Property_RO

1011 def f1(self):

1012 '''Get the I{1 - flattening} (C{float}), M{f1 == 1 - f == b / a}.

1013

1014 @see: Property L{b_a}.

1015 '''

1016 return Float(f1=_1_0 - self.f)

1017

1018 @Property_RO

1019 def f2(self):

1020 '''Get the I{2nd flattening} (C{float}), M{(a - b) / b == f / (1 - f)}, C{0} for spherical, see C{a_b2f2}.

1021 '''

1022 return self._assert(self.a_b - _1_0, f2=f2f2(self.f))

1023

1024 @deprecated_Property_RO

1025 def geodesic(self):

1026 '''DEPRECATED, use property C{geodesicw}.'''

1027 return self.geodesicw

1028

1029 def geodesic_(self, exact=True):

1030 '''Get the an I{exact} C{Geodesic...} instance for this ellipsoid.

1031

1032 @kwarg exact: If C{bool} return L{GeodesicExact}C{(exact=B{exact}, ...)},

1033 otherwise a L{Geodesic}, L{GeodesicExact} or L{GeodesicSolve}

1034 instance for I{this} ellipsoid.

1035

1036 @return: The C{exact} geodesic (C{Geodesic...}).

1037

1038 @raise TypeError: Invalid B{C{exact}}.

1039

1040 @raise ValueError: Incompatible B{C{exact}} ellipsoid.

1041 '''

1042 if isbool(exact): # for consistenccy with C{.rhumb_}

1043 g = _MODS.geodesicx.GeodesicExact(self, C4order=30 if exact else 24,

1044 name=self.name)

1045 else:

1046 g = exact

1047 E = _xattr(g, ellipsoid=None)

1048 if not (E is self and isinstance(g, self._Geodesics)):

1049 raise _ValueError(exact=g, ellipsoid=E, txt_not_=self.name)

1050 return g

1051

1052 @property_ROver

1053 def _Geodesics(self):

1054 '''(INTERNAL) Get all C{Geodesic...} classes, I{once}.

1055 '''

1056 t = (_MODS.geodesicx.GeodesicExact,

1057 _MODS.geodsolve.GeodesicSolve)

1058 try:

1059 t += (_MODS.geodesicw.Geodesic,

1060 _MODS.geodesicw._wrapped.Geodesic)

1061 except ImportError:

1062 pass

1063 return t # overwrite property_ROver

1064

1065 @property_RO

1066 def geodesicw(self):

1067 '''Get this ellipsoid's I{wrapped} U{geodesicw.Geodesic

1068 <https://GeographicLib.SourceForge.io/Python/doc/code.html>}, provided

1069 I{Karney}'s U{geographiclib<https://PyPI.org/project/geographiclib>}

1070 package is installed.

1071 '''

1072 # if not self.isEllipsoidal:

1073 # raise _IsnotError(_ellipsoidal_, ellipsoid=self)

1074 return _MODS.geodesicw.Geodesic(self)

1075

1076 @property_RO

1077 def geodesicx(self):

1078 '''Get this ellipsoid's I{exact} L{GeodesicExact}.

1079 '''

1080 # if not self.isEllipsoidal:

1081 # raise _IsnotError(_ellipsoidal_, ellipsoid=self)

1082 return _MODS.geodesicx.GeodesicExact(self, name=self.name)

1083

1084 @property

1085 def geodsolve(self):

1086 '''Get this ellipsoid's L{GeodesicSolve}, the I{wrapper} around utility

1087 U{GeodSolve<https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>},

1088 provided the path to the C{GeodSolve} executable is specified with env

1089 variable C{PYGEODESY_GEODSOLVE} or re-/set with this property..

1090 '''

1091 # if not self.isEllipsoidal:

1092 # raise _IsnotError(_ellipsoidal_, ellipsoid=self)

1093 return _MODS.geodsolve.GeodesicSolve(self, path=self._geodsolve, name=self.name)

1094

1095 @geodsolve.setter # PYCHOK setter!

1096 def geodsolve(self, path):

1097 '''Re-/set the (fully qualified) path to the U{GeodSolve

1098 <https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>} executable,

1099 overriding env variable C{PYGEODESY_GEODSOLVE} (C{str}).

1100 '''

1101 self._geodsolve = path

1102

1103 def hartzell4(self, pov, los=None):

1104 '''Compute the intersection of this ellipsoid's surface and a Line-Of-Sight

1105 from a Point-Of-View in space.

1106

1107 @arg pov: Point-Of-View outside this ellipsoid (C{Cartesian}, L{Ecef9Tuple}

1108 or L{Vector3d}).

1109 @kwarg los: Line-Of-Sight, I{direction} to this ellipsoid (L{Los}, L{Vector3d})

1110 or C{True} for the I{normal, perpendicular, plumb} to the surface

1111 of this ellipsoid or C{False} or C{None} to point to its center.

1112

1113 @return: L{Vector4Tuple}C{(x, y, z, h)} with the cartesian coordinates C{x},

1114 C{y} and C{z} of the projection on or the intersection with this

1115 ellipsoid and the I{distance} C{h} from B{C{pov}} to C{(x, y, z)}

1116 along B{C{los}}, all in C{meter}, conventionally.

1117

1118 @raise IntersectionError: Null B{C{pov}} or B{C{los}} vector, or B{C{pov}}

1119 is inside this ellipsoid or B{C{los}} points

1120 outside this ellipsoid or in opposite direction.

1121

1122 @raise TypeError: Invalid B{C{pov}} or B{C{los}}.

1123

1124 @see: U{I{Satellite Line-of-Sight Intersection with Earth}<https://StephenHartzell.

1125 Medium.com/satellite-line-of-sight-intersection-with-earth-d786b4a6a9b6>} and

1126 methods L{Ellipsoid.height4} and L{Triaxial.hartzell4}.

1127 '''

1128 try:

1129 m = _MODS._triaxials_triaxial5

1130 v, d, i = m._hartzell3(pov, los, self._triaxial)

1131 except Exception as x:

1132 raise IntersectionError(pov=pov, los=los, cause=x)

1133 return Vector4Tuple(v.x, v.y, v.z, d, iteration=i, name__=self.hartzell4)

1134

1135 @Property_RO

1136 def _hash(self):

1137 return hash((self.a, self.f))

1138

1139 def height4(self, xyz, normal=True):

1140 '''Compute the projection on and the height of a cartesian above or below

1141 this ellipsoid's surface.

1142

1143 @arg xyz: The cartesian (C{Cartesian}, L{Ecef9Tuple}, L{Vector3d},

1144 L{Vector3Tuple} or L{Vector4Tuple}).

1145 @kwarg normal: If C{True}, the projection is perpendicular to (the nearest

1146 point on) this ellipsoid's surface, otherwise the C{radial}

1147 line to this ellipsoid's center (C{bool}).

1148

1149 @return: L{Vector4Tuple}C{(x, y, z, h)} with the cartesian coordinates C{x},

1150 C{y} and C{z} of the projection on and the height C{h} above or

1151 below this ellipsoid's surface, all in C{meter}, conventionally.

1152

1153 @raise ValueError: Null B{C{xyz}}.

1154

1155 @raise TypeError: Non-cartesian B{C{xyz}}.

1156

1157 @see: U{Distance to<https://StackOverflow.com/questions/22959698/distance-from-given-point-to-given-ellipse>}

1158 and U{intersection with<https://MathWorld.Wolfram.com/Ellipse-LineIntersection.html>} an ellipse and

1159 methods L{Ellipsoid.hartzell4} and L{Triaxial.height4}.

1160 '''

1161 v = _MODS.vector3d._otherV3d(xyz=xyz)

1162 r = v.length

1163

1164 a, b, i = self.a, self.b, None

1165 if r < EPS0: # EPS

1166 v = v.times(_0_0)

1167 h = -a

1168

1169 elif self.isSpherical:

1170 v = v.times(a / r)

1171 h = r - a

1172

1173 elif normal: # perpendicular to ellipsoid

1174 x, y = hypot(v.x, v.y), fabs(v.z)

1175 if x < EPS0: # PYCHOK no cover

1176 z = copysign0(b, v.z)

1177 v = Vector3Tuple(v.x, v.y, z)

1178 h = y - b # polar

1179 elif y < EPS0: # PYCHOK no cover

1180 t = a / r

1181 v = v.times_(t, t, 0) # force z=0.0

1182 h = x - a # equatorial

1183 else: # normal in 1st quadrant

1184 m = _MODS._triaxials_triaxial5

1185 x, y, i = m._plumbTo3(x, y, self)

1186 t, v = v, v.times_(x, x, y)

1187 h = t.minus(v).length

1188

1189 else: # radial to ellipsoid's center

1190 h = hypot_(a * v.z, b * v.x, b * v.y)

1191 t = (a * b / h) if h > EPS0 else _0_0 # EPS

1192 v = v.times(t)

1193 h = r * (_1_0 - t)

1194

1195 return Vector4Tuple(v.x, v.y, v.z, h, iteration=i, name__=self.height4)

1196

1197 def _heightB(self, sa, ca, z, p): # in ecef.EcefSudano, ecec.EcefVeness

1198 '''(INTERNAL) Height above ellipsoid (Bowring eqn 7) at C{lat}.

1199 '''

1200 # sa, ca = sincos2d(lat)

1201 # p = hypot(x, y) # distance to polar axis

1202

1203 # r = a / self.e2s(sa) # length of normal terminated by polar axis

1204 # h = p * ca + z * sa - (a * a / r)

1205 return (p * ca + fabs(z * sa) - self.a * self.e2s(sa)) if sa else (p - self.a)

1206

1207 @Property_RO

1208 def _heightMax(self):

1209 '''(INTERNAL) Get the height limit (C{meter}, conventionally).

1210 '''

1211 return self.a / EPS_2 # self.a * _2_EPS, about 12M lightyears

1212

1213 def _hubeny_2(self, phi2, phi1, lam21, scaled=True, squared=True):

1214 '''(INTERNAL) like function C{pygeodesy.flatLocal_}/C{pygeodesy.hubeny_},

1215 returning the I{angular} distance in C{radians squared} or C{radians}

1216 '''

1217 m, n = self.roc2_((phi2 + phi1) * _0_5, scaled=scaled)

1218 h, r = (hypot2, self.a2_) if squared else (hypot, _1_0 / self.a)

1219 return h(m * (phi2 - phi1), n * lam21) * r

1220

1221 @Property_RO

1222 def isEllipsoidal(self):

1223 '''Is this model I{ellipsoidal} (C{bool})?

1224 '''

1225 return self.f != 0

1226

1227 @Property_RO

1228 def isOblate(self):

1229 '''Is this ellipsoid I{oblate} (C{bool})? I{Prolate} or

1230 spherical otherwise.

1231 '''

1232 return self.f > 0

1233

1234 @Property_RO

1235 def isProlate(self):

1236 '''Is this ellipsoid I{prolate} (C{bool})? I{Oblate} or

1237 spherical otherwise.

1238 '''

1239 return self.f < 0

1240

1241 @Property_RO

1242 def isSpherical(self):

1243 '''Is this ellipsoid I{spherical} (C{bool})?

1244 '''

1245 return self.f == 0

1246

1247 def _Kseries(self, *AB8Ks):

1248 '''(INTERNAL) Compute the 4-, 6- or 8-th order I{Krüger} Alpha

1249 or Beta series coefficients per I{Karney}'s U{equations (35)

1250 and (36)<https://ArXiv.org/pdf/1002.1417v3.pdf>}.

1251

1252 @arg AB8Ks: 8-Tuple of 8-th order I{Krüger} Alpha or Beta series

1253 coefficient tuples.

1254

1255 @return: I{Krüger} series coefficients (L{KsOrder}C{-tuple}).

1256

1257 @see: I{Karney}'s 30-th order U{TMseries30

1258 <https://GeographicLib.SourceForge.io/C++/doc/tmseries30.html>}.

1259 '''

1260 k = self.KsOrder

1261 if self.n:

1262 ns = fpowers(self.n, k)

1263 ks = tuple(fdot(AB8Ks[i][:k-i], *ns[i:]) for i in range(k))

1264 else:

1265 ks = _0_0s(k)

1266 return ks

1267

1268 @property_doc_(''' the I{Krüger} series' order (C{int}), see properties C{AlphaKs}, C{BetaKs}.''')

1269 def KsOrder(self):

1270 '''Get the I{Krüger} series' order (C{int} 4, 6 or 8).

1271 '''

1272 return self._KsOrder

1273

1274 @KsOrder.setter # PYCHOK setter!

1275 def KsOrder(self, order):

1276 '''Set the I{Krüger} series' order (C{int} 4, 6 or 8).

1277

1278 @raise ValueError: Invalid B{C{order}}.

1279 '''

1280 if not (isint(order) and _isin(order, 4, 6, 8)):

1281 raise _ValueError(order=order)

1282 if self._KsOrder != order:

1283 Ellipsoid.AlphaKs._update(self)

1284 Ellipsoid.BetaKs._update(self)

1285 self._KsOrder = order

1286

1287 @Property_RO

1288 def L(self):

1289 '''Get the I{quarter meridian} C{L}, aka the C{polar distance}

1290 along a meridian between the equator and a pole (C{meter}),

1291 M{b * Elliptic(-e2 / (1 - e2)).cE} or M{b * PI / 2}.

1292 '''

1293 r = self._elliptic_e22.cE if self.f else PI_2

1294 return Distance(L=self.b * r)

1295

1296 def Llat(self, lat):

1297 '''Return the I{meridional length}, the distance along a meridian

1298 between the equator and a (geodetic) latitude, see C{L}.

1299

1300 @arg lat: Geodetic latitude (C{degrees90}).

1301

1302 @return: The meridional length at B{C{lat}}, negative on southern

1303 hemisphere (C{meter}).

1304 '''

1305 r = self._elliptic_e22.fEd(self.auxParametric(lat)) if self.f else Phid(lat)

1306 return Distance(Llat=self.b * r)

1307

1308 Lmeridian = Llat # meridional distance

1309

1310 @property_RO

1311 def _Lpd(self):

1312 '''Get the I{quarter meridian} per degree (C{meter}), M{self.L / 90}.

1313 '''

1314 return Meter(_Lpd=self.L / _90_0)

1315

1316 @property_RO

1317 def _Lpr(self):

1318 '''Get the I{quarter meridian} per radian (C{meter}), M{self.L / PI_2}.

1319 '''

1320 return Meter(_Lpr=self.L / PI_2)

1321

1322 @deprecated_Property_RO

1323 def majoradius(self): # PYCHOK no cover

1324 '''DEPRECATED, use property C{a} or C{Requatorial}.'''

1325 return self.a

1326

1327 def m2degrees(self, distance, lat=0):

1328 '''Convert a distance to an arc in degrees along the equator or

1329 along a parallel of (geodetic) latitude.

1330

1331 @arg distance: Distance (C{meter}).

1332 @kwarg lat: Parallel latitude (C{degrees90}, C{str}).

1333

1334 @return: Angle (C{degrees}) or C{0} for near-polar B{C{lat}}.

1335

1336 @raise RangeError: Latitude B{C{lat}} outside valid range and

1337 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

1338

1339 @raise ValueError: Invalid B{C{distance}} or B{C{lat}}.

1340 '''

1341 return degrees(self.m2radians(distance, lat=lat))

1342

1343 def m2radians(self, distance, lat=0):

1344 '''Convert a distance to an angle along the equator or along

1345 a parallel of (geodetic) latitude.

1346

1347 @arg distance: Distance (C{meter}).

1348 @kwarg lat: Parallel latitude (C{degrees90}, C{str}).

1349

1350 @return: Angle (C{radians}) or C{INF} for near-polar B{C{lat}}.

1351

1352 @raise RangeError: Latitude B{C{lat}} outside valid range and

1353 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

1354

1355 @raise ValueError: Invalid B{C{distance}} or B{C{lat}}.

1356 '''

1357 r = self.circle4(lat).radius if lat else self.a

1358 return m2radians(distance, radius=r, lat=0)

1359

1360 @deprecated_Property_RO

1361 def minoradius(self): # PYCHOK no cover

1362 '''DEPRECATED, use property C{b}, C{polaradius} or C{Rpolar}.'''

1363 return self.b

1364

1365 @Property_RO

1366 def n(self):

1367 '''Get the I{3rd flattening} (C{float}), M{f / (2 - f) == (a - b) / (a + b)}, see C{a_b2n}.

1368 '''

1369 return self._assert(a_b2n(self.a, self.b), n=f2n(self.f))

1370

1371 flattening = f

1372 flattening1st = f

1373 flattening2nd = f2

1374 flattening3rd = n

1375

1376 polaradius = b # Rpolar

1377

1378 @property_RO

1379 def polarimeter(self):

1380 '''Get the ellipsoid's I{polar}, meridional perimeter (C{meter}).

1381 '''

1382 return Meter(polarimeter=self.L * _4_0)

1383

1384# Q = A # I{meridian arc unit} C{Q}, the mean, meridional length I{per radian}

1385

1386 @deprecated_Property_RO

1387 def quarteradius(self): # PYCHOK no cover

1388 '''DEPRECATED, use property C{L} or method C{Llat}.'''

1389 return self.L

1390

1391 @Property_RO

1392 def R1(self):

1393 '''Get the I{mean} earth radius per I{IUGG} (C{meter}), M{(2 * a + b) / 3 == a * (1 - f / 3)}.

1394

1395 @see: U{Earth radius<https://WikiPedia.org/wiki/Earth_radius>}

1396 and method C{Rgeometric}.

1397 '''

1398 return Radius(R1=fmean_(self.a, self.a, self.b) if self.f else self.a)

1399

1400 Rmean = R1

1401

1402 @Property_RO

1403 def R2(self):

1404 '''Get the I{authalic} earth radius (C{meter}), M{sqrt(c2)}.

1405

1406 @see: C{R2x}, C{c2}, C{area} and U{Earth radius

1407 <https://WikiPedia.org/wiki/Earth_radius>}.

1408 '''

1409 return Radius(R2=sqrt(self.c2) if self.f else self.a)

1410# # Moritz, H. <https://Geodesy.Geology.Ohio-State.edu/course/refpapers/00740128.pdf>

1411# # R2 = (1 - 2/3 * e'2 + 26/45 * e'4 - 100/189 * e'6 + 7034/14175 * e'8) * rocPolar

1412# # = (3 + e'2 * (-2 + e'2 * (26/15 + e'2 * (-100/63 + e'2 * 7034/4725)))) * rocPolar / 3

1413# return Fhorner(self.e22, 3, -2, 26 / 15, -100 / 63, 7034 / 4725).fover(3 / self.rocPolar)

1414

1415 Rauthalic = R2

1416

1417 @Property_RO

1418 def R2x(self):

1419 '''Get the I{authalic} earth radius (C{meter}), M{sqrt(c2x)}.

1420

1421 @see: C{R2}, C{c2x} and C{areax}.

1422 '''

1423 return Radius(R2x=sqrt(self.c2x) if self.f else self.a)

1424

1425 Rauthalicx = R2x

1426

1427 @Property_RO

1428 def R3(self):

1429 '''Get the I{volumetric} earth radius (C{meter}), M{(a * a * b)**(1/3)}.

1430

1431 @see: U{Earth radius<https://WikiPedia.org/wiki/Earth_radius>} and C{volume}.

1432 '''

1433 r = (cbrt(self.b_a) * self.a) if self.f else self.a

1434 return Radius(R3=r)

1435

1436 Rvolumetric = R3

1437

1438 def radians2m(self, rad, lat=0):

1439 '''Convert an angle to the distance along the equator or along

1440 a parallel of (geodetic) latitude.

1441

1442 @arg rad: The angle (C{radians}).

1443 @kwarg lat: Parallel latitude (C{degrees90}, C{str}).

1444

1445 @return: Distance (C{meter}, same units as the equatorial

1446 and polar radii) or C{0} for near-polar B{C{lat}}.

1447

1448 @raise RangeError: Latitude B{C{lat}} outside valid range and

1449 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

1450

1451 @raise ValueError: Invalid B{C{rad}} or B{C{lat}}.

1452 '''

1453 r = self.circle4(lat).radius if lat else self.a

1454 return radians2m(rad, radius=r, lat=0)

1455

1456 @Property_RO

1457 def Rbiaxial(self):

1458 '''Get the I{biaxial, quadratic} mean earth radius (C{meter}), M{sqrt((a**2 + b**2) / 2)}.

1459

1460 @see: C{Rtriaxial}

1461 '''

1462 a, b = self.a, self.b

1463 if b != a:

1464 b = hypot(a, b) / _SQRT2

1465 return Radius(Rbiaxial=b)

1466

1467 Requatorial = a # for consistent naming

1468

1469 def Rgeocentric(self, lat):

1470 '''Compute the I{geocentric} earth radius of (geodetic) latitude.

1471

1472 @arg lat: Latitude (C{degrees90}).

1473

1474 @return: Geocentric earth radius (C{meter}).

1475

1476 @raise ValueError: Invalid B{C{lat}}.

1477

1478 @see: U{Geocentric Radius

1479 <https://WikiPedia.org/wiki/Earth_radius#Geocentric_radius>}

1480 '''

1481 r, p = self.a, Phid(lat)

1482 if p and self.f:

1483 if fabs(p) < PI_2:

1484 s2, c2 = _sin2cos2(p)

1485 # R == sqrt((a2**2 * c2 + b2**2 * s2) / (a2 * c2 + b2 * s2))

1486 # == sqrt(a2**2 * (c2 + (b2 / a2)**2 * s2) / (a2 * (c2 + b2 / a2 * s2)))

1487 # == sqrt(a2 * (c2 + (b2 / a2)**2 * s2) / (c2 + (b2 / a2) * s2))

1488 # == a * sqrt((c2 + b2_a2 * b2_a2 * s2) / (c2 + b2_a2 * s2))

1489 s2 *= self.b2_a2

1490 r *= sqrt((c2 + self.b2_a2 * s2) / (c2 + s2))

1491 else:

1492 r = self.b

1493 return Radius(Rgeocentric=r)

1494

1495 @Property_RO

1496 def Rgeometric(self):

1497 '''Get the I{geometric} mean earth radius (C{meter}), M{sqrt(a * b)}.

1498

1499 @see: C{R1}.

1500 '''

1501 g = sqrt(self.a * self.b) if self.f else self.a

1502 return Radius(Rgeometric=g)

1503

1504 def rhumb_(self, exact=True):

1505 '''Get the an I{exact} C{Rhumb...} instance for this ellipsoid.

1506

1507 @kwarg exact: If C{bool} or C{None} return L{Rhumb}C{(exact=B{exact}, ...)},

1508 otherwise a L{Rhumb}, L{RhumbAux} or L{RhumbSolve} instance

1509 for I{this} ellipsoid.

1510

1511 @return: The C{exact} rhumb (C{Rhumb...}).

1512

1513 @raise TypeError: Invalid B{C{exact}}.

1514

1515 @raise ValueError: Incompatible B{C{exact}} ellipsoid.

1516 '''

1517 if isbool(exact): # use Rhumb for backward compatibility

1518 r = _MODS.rhumb.ekx.Rhumb(self, exact=exact, name=self.name)

1519 else:

1520 r = exact

1521 E = _xattr(r, ellipsoid=None)

1522 if not (E is self and isinstance(r, self._Rhumbs)):

1523 raise _ValueError(exact=r, ellipsosid=E, txt_not_=self.name)

1524 return r

1525

1526 @property_RO

1527 def rhumbaux(self):

1528 '''Get this ellipsoid's I{Auxiliary} C{rhumb.RhumbAux}.

1529 '''

1530 # if not self.isEllipsoidal:

1531 # raise _IsnotError(_ellipsoidal_, ellipsoid=self)

1532 return _MODS.rhumb.aux_.RhumbAux(self, name=self.name)

1533

1534 @property_RO

1535 def rhumbekx(self):

1536 '''Get this ellipsoid's I{Elliptic, Krüger} C{rhumb.Rhumb}.

1537 '''

1538 # if not self.isEllipsoidal:

1539 # raise _IsnotError(_ellipsoidal_, ellipsoid=self)

1540 return _MODS.rhumb.ekx.Rhumb(self, name=self.name)

1541

1542 @property_ROver

1543 def _Rhumbs(self):

1544 '''(INTERNAL) Get all C{Rhumb...} classes, I{once}.

1545 '''

1546 r = _MODS.rhumb

1547 return (r.aux_.RhumbAux, # overwrite property_ROver

1548 r.ekx.Rhumb, r.solve.RhumbSolve)

1549

1550 @property

1551 def rhumbsolve(self):

1552 '''Get this ellipsoid's L{RhumbSolve}, the I{wrapper} around utility

1553 U{RhumbSolve<https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>},

1554 provided the path to the C{RhumbSolve} executable is specified with env

1555 variable C{PYGEODESY_RHUMBSOLVE} or re-/set with this property.

1556 '''

1557 # if not self.isEllipsoidal:

1558 # raise _IsnotError(_ellipsoidal_, ellipsoid=self)

1559 return _MODS.rhumb.solve.RhumbSolve(self, path=self._rhumbsolve, name=self.name)

1560

1561 @rhumbsolve.setter # PYCHOK setter!

1562 def rhumbsolve(self, path):

1563 '''Re-/set the (fully qualified) path to the U{RhumbSolve

1564 <https://GeographicLib.SourceForge.io/C++/doc/GeodSolve.1.html>} executable,

1565 overriding env variable C{PYGEODESY_RHUMBSOLVE} (C{str}).

1566 '''

1567 self._rhumbsolve = path

1568

1569 @deprecated_property_RO

1570 def rhumbx(self):

1571 '''DEPRECATED on 2023.11.28, use property C{rhumbekx}.'''

1572 return self.rhumbekx

1573

1574 def Rlat(self, lat):

1575 '''I{Average} the earth radius between C{equatoradius} at C{0} and

1576 C{polaradius} at C{+/-90} degrees latitude.

1577

1578 @arg lat: Latitude (C{degrees90}, C{str} or C{Ang}).

1579

1580 @return: Averaged earth radius (C{meter}).

1581

1582 @raise RangeError: Latitude B{C{lat}} outside valid range, only if

1583 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

1584

1585 @raise TypeError: Invalid B{C{lat}}.

1586

1587 @raise ValueError: Invalid B{C{lat}}.

1588 '''

1589 # r = a - (a - b) * |lat| / 90

1590 r = self.a

1591 if self.f: # .isEllipsoidal

1592 lat = _Lat0(lat)

1593 if lat:

1594 r -= (r - self.b) * fabs(lat) / _90_0

1595 r = Radius(Rlat=r)

1596 return r

1597

1598 Rpolar = b # for consistent naming

1599

1600 def roc1_(self, sa, ca=None):

1601 '''Compute the I{prime-vertical}, I{normal} radius of curvature

1602 of (geodetic) latitude, I{unscaled}.

1603

1604 @arg sa: Sine of the latitude (C{float}, [-1.0..+1.0]).

1605 @kwarg ca: Optional cosine of the latitude (C{float}, [-1.0..+1.0])

1606 to use an alternate formula.

1607

1608 @return: The prime-vertical radius of curvature (C{float}).

1609

1610 @note: The delta between both formulae with C{Ellipsoids.WGS84}

1611 is less than 2 nanometer over the entire latitude range.

1612

1613 @see: Method L{roc2_} and class L{EcefYou}.

1614 '''

1615 if sa and self.f: # .isEllipsoidal

1616 if ca is None:

1617 r = self.e2s2(sa) # see .roc2_ and _EcefBase._forward

1618 n = sqrt(self.a2 / r) if r > EPS02 else _0_0

1619 elif ca: # derived from EcefYou.forward

1620 h = hypot(ca, self.b_a * sa)

1621 n = self.a / h

1622 else:

1623 n = self.a2_b / fabs(sa)

1624 else:

1625 n = self.a

1626 return n

1627

1628 def roc2(self, lat, scaled=False):

1629 '''Compute the I{meridional} and I{prime-vertical}, I{normal}

1630 radii of curvature of (geodetic) latitude.

1631

1632 @arg lat: Latitude (C{degrees90}).

1633 @kwarg scaled: Scale prime_vertical by C{cos(radians(B{lat}))} (C{bool}).

1634

1635 @return: An L{Curvature2Tuple}C{(meridional, prime_vertical)} with

1636 the radii of curvature.

1637

1638 @raise ValueError: Invalid B{C{lat}}.

1639

1640 @see: Methods L{roc2_} and L{roc1_}, U{Local, flat earth approximation

1641 <https://www.EdWilliams.org/avform.htm#flat>} and meridional and

1642 prime vertical U{Radii of Curvature<https://WikiPedia.org/wiki/

1643 Earth_radius#Radii_of_curvature>}.

1644 '''

1645 return self.roc2_(Phid(lat), scaled=scaled)

1646

1647 def roc2_(self, phi, scaled=False):

1648 '''Compute the I{meridional} and I{prime-vertical}, I{normal} radii of

1649 curvature of (geodetic) latitude.

1650

1651 @arg phi: Latitude (C{radians}).

1652 @kwarg scaled: Scale prime_vertical by C{cos(B{phi})} (C{bool}).

1653

1654 @return: An L{Curvature2Tuple}C{(meridional, prime_vertical)} with the

1655 radii of curvature.

1656

1657 @raise ValueError: Invalid B{C{phi}}.

1658

1659 @see: Methods L{roc2} and L{roc1_}, property L{rocEquatorial2}, U{Local,

1660 flat earth approximation<https://www.EdWilliams.org/avform.htm#flat>}

1661 and the meridional and prime vertical U{Radii of Curvature

1662 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}.

1663 '''

1664 p = fabs(Phi(phi))

1665 if self.f:

1666 r = self.e2s2(sin(p))

1667 if r > EPS02:

1668 n = sqrt(self.a2 / r)

1669 m = n * self.e21 / r

1670 else:

1671 m = n = _0_0

1672 else:

1673 m = n = self.a

1674 if scaled and p:

1675 n *= cos(p) if p < PI_2 else _0_0

1676 return Curvature2Tuple(m, n)

1677

1678 def rocAzimuth(self, lat, azimuth):

1679 '''Compute the I{directional} radius of curvature of (geodetic) latitude

1680 and C{azimuth} compass direction.

1681

1682 @see: Method L{rocBearing<Ellipsoid.rocBearing>} for details, using C{azimuth} for C{bearing}.

1683 '''

1684 return Radius(rocAzimuth=self._rocDirectional(lat, Azimuth(azimuth)))

1685

1686 def rocBearing(self, lat, bearing):

1687 '''Compute the I{directional} radius of curvature of (geodetic) latitude

1688 and C{bearing} compass direction.

1689

1690 @arg lat: Latitude (C{degrees90}).

1691 @arg bearing: Direction (compass C{degrees360}).

1692

1693 @return: Directional radius of curvature (C{meter}).

1694

1695 @raise RangeError: Latitude B{C{lat}} outside valid range and

1696 L{rangerrors<pygeodesy.rangerrors>} is C{True}.

1697

1698 @raise ValueError: Invalid B{C{lat}} or B{C{bearing}}.

1699

1700 @see: U{Radii of Curvature<https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}

1701 '''

1702 return Radius(rocBearing=self._rocDirectional(lat, Bearing(bearing)))

1703

1704 def _rocDirectional(self, lat, deg):

1705 '''(INTERNAL) Helper for C{rocAzimuth} and C{rocBearing}.

1706 '''

1707 if self.f:

1708 s2, c2 = _sin2cos2(radians(deg))

1709 m, n = self.roc2_(Phid(lat))

1710 if n < m: # == n / (c2 * n / m + s2)

1711 c2 *= n / m

1712 elif m < n: # == m / (c2 + s2 * m / n)

1713 s2 *= m / n

1714 n = m

1715 r = _over(n, c2 + s2) # == 1 / (c2 / m + s2 / n)

1716 else:

1717 r = self.b # == self.a

1718 return r

1719

1720 @Property_RO

1721 def rocEquatorial2(self):

1722 '''Get the I{meridional} and I{prime-vertical}, I{normal} radii of curvature

1723 at the equator as L{Curvature2Tuple}C{(meridional, prime_vertical)}.

1724

1725 @see: Methods L{rocMeridional} and L{rocPrimeVertical}, properties L{b2_a},

1726 L{a2_b}, C{rocPolar} and polar and equatorial U{Radii of Curvature

1727 <https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}.

1728 '''

1729 m = self.b2_a if self.f else self.a

1730 return Curvature2Tuple(m, self.a)

1731

1732 def rocGauss(self, lat):

1733 '''Compute the I{Gaussian} radius of curvature of (geodetic) latitude.

1734

1735 @arg lat: Latitude (C{degrees90}).

1736

1737 @return: Gaussian radius of curvature (C{meter}).

1738

1739 @raise ValueError: Invalid B{C{lat}}.

1740

1741 @see: Non-directional U{Radii of Curvature<https://WikiPedia.org/wiki/

1742 Earth_radius#Radii_of_curvature>}

1743 '''

1744 # using ...

1745 # m, n = self.roc2_(Phid(lat))

1746 # return sqrt(m * n)

1747 # ... requires 1 or 2 sqrt

1748 g = self.b

1749 if self.f:

1750 s2, c2 = _sin2cos2(Phid(lat))

1751 g = _over(g, c2 + self.b2_a2 * s2)

1752 return Radius(rocGauss=g)

1753

1754 def rocMean(self, lat):

1755 '''Compute the I{mean} radius of curvature of (geodetic) latitude.

1756

1757 @arg lat: Latitude (C{degrees90}).

1758

1759 @return: Mean radius of curvature (C{meter}).

1760

1761 @raise ValueError: Invalid B{C{lat}}.

1762

1763 @see: Non-directional U{Radii of Curvature<https://WikiPedia.org/wiki/

1764 Earth_radius#Radii_of_curvature>}

1765 '''

1766 if self.f:

1767 m, n = self.roc2_(Phid(lat))

1768 m *= _over(n * _2_0, m + n) # == 2 / (1 / m + 1 / n)

1769 else:

1770 m = self.a

1771 return Radius(rocMean=m)

1772

1773 def rocMeridional(self, lat):

1774 '''Compute the I{meridional} radius of curvature of (geodetic) latitude.

1775

1776 @arg lat: Latitude (C{degrees90}).

1777

1778 @return: Meridional radius of curvature (C{meter}).

1779

1780 @raise ValueError: Invalid B{C{lat}}.

1781

1782 @see: Methods L{roc2} and L{roc2_}, U{Local, flat earth approximation

1783 <https://www.EdWilliams.org/avform.htm#flat>} and U{Radii of

1784 Curvature<https://WikiPedia.org/wiki/Earth_radius#Radii_of_curvature>}.

1785 '''

1786 r = self.roc2_(Phid(lat)) if lat else self.rocEquatorial2

1787 return Radius(rocMeridional=r.meridional)

1788

1789 rocPolar = a2_b # synonymous

1790

1791 def rocPrimeVertical(self, lat):

1792 '''Compute the I{prime-vertical}, I{normal} radius of curvature of

1793 (geodetic) latitude, aka the I{transverse} radius of curvature.

1794

1795 @arg lat: Latitude (C{degrees90}).

1796

1797 @return: Prime-vertical radius of curvature (C{meter}).

1798

1799 @raise ValueError: Invalid B{C{lat}}.

1800

1801 @see: Methods L{roc2}, L{roc2_} and L{roc1_}, U{Local, flat earth

1802 approximation<https://www.EdWilliams.org/avform.htm#flat>} and

1803 U{Radii of Curvature<https://WikiPedia.org/wiki/

1804 Earth_radius#Radii_of_curvature>}.

1805 '''

1806 r = self.roc1_(sin(Phid(lat))) if lat else self.a

1807 return Radius(rocPrimeVertical=r)

1808

1809 rocTransverse = rocPrimeVertical # synonymous

1810

1811 @deprecated_Property_RO

1812 def Rquadratic(self): # PYCHOK no cover

1813 '''DEPRECATED, use property C{Rbiaxial} or C{Rtriaxial}.'''

1814 return self.Rbiaxial

1815

1816 @deprecated_Property_RO

1817 def Rr(self): # PYCHOK no cover

1818 '''DEPRECATED, use property C{Rrectifying}.'''

1819 return self.Rrectifying

1820

1821 @Property_RO

1822 def Rrectifying(self):

1823 '''Get the I{rectifying} earth radius (C{meter}), M{((a**(3/2) + b**(3/2)) / 2)**(2/3)}.

1824

1825 @see: U{Earth radius<https://WikiPedia.org/wiki/Earth_radius>}.

1826 '''

1827 r = self.a

1828 if self.f:

1829 r *= cbrt2((sqrt3(self.b_a) + _1_0) * _0_5)

1830 return Radius(Rrectifying=r)

1831

1832 @deprecated_Property_RO

1833 def Rs(self): # PYCHOK no cover

1834 '''DEPRECATED, use property C{Rgeometric}.'''

1835 return self.Rgeometric

1836

1837 @Property_RO

1838 def Rtriaxial(self):

1839 '''Get the I{triaxial, quadratic} mean earth radius (C{meter}), M{sqrt((3 * a**2 + b**2) / 4)}.

1840

1841 @see: C{Rbiaxial}

1842 '''

1843 q, b = self.a, self.b

1844 if b < q:

1845 q *= sqrt((self.b2_a2 + _3_0) * _0_25)

1846 elif b > q:

1847 q = sqrt((self.a2_b2 * _3_0 + _1_0) * _0_25) * b

1848 return Radius(Rtriaxial=q)

1849

1850 def toEllipse(self, **name):

1851 '''Get this ellipsoid's meridional ellipse L{Ellipse<pygeodesy.Ellipse>}.

1852

1853 @kwarg name: Optional, unique C{B{name}=NN} (C{str}).

1854 '''

1855 return _MODS.ellipses.Ellipse(self.a, self.b, **name)

1856

1857 def toEllipsoid2(self, **name):

1858 '''Get a copy of this ellipsoid as an L{Ellipsoid2}.

1859

1860 @kwarg name: Optional, unique C{B{name}=NN} (C{str}).

1861

1862 @see: Property C{a_f}.

1863 '''

1864 return Ellipsoid2(self, None, **name)

1865

1866 def toStr(self, prec=8, terse=4, **sep_name): # PYCHOK expected

1867 '''Return this ellipsoid as a text string.

1868

1869 @kwarg prec: Number of decimal digits, unstripped (C{int}).

1870 @kwarg terse: Limit the number of items (C{int}, 0...18),

1871 use C{B{terse}=0} or C{=None} for all.

1872 @kwarg sep_name: Optional C{B{name}=NN} (C{str}) or C{None}

1873 to exclude this ellipsoid's name and separator

1874 C{B{sep}=", "} to join the items (C{str}).

1875

1876 @return: This C{Ellipsoid}'s attributes (C{str}).

1877 '''

1878 E = Ellipsoid

1879 t = (E.a, E.f, E.f_, E.b, E.f2, E.n, E.e,

1880 E.e2, E.e21, E.e22, E.e32,

1881 E.A, E.L, E.R1, E.R2, E.R3,

1882 E.Rbiaxial, E.Rtriaxial)

1883 if terse:

1884 t = t[:terse]

1885 return self._instr(prec=prec, props=t, **sep_name)

1886

1887 def toTriaxial(self, **name):

1888 '''Convert this ellipsoid to a L{Triaxial_}.

1889

1890 @kwarg name: Optional C{B{name}=NN} (C{str}).

1891

1892 @return: A L{Triaxial_} or L{Triaxial} with the C{X} axis

1893 pointing east and C{Z} pointing north.

1894

1895 @see: Method L{Triaxial_.toEllipsoid}.

1896 '''

1897 T = self._triaxial

1898 return T.copy(**name) if name else T

1899

1900 @property_RO

1901 def _triaxial(self):

1902 '''(INTERNAL) Get this ellipsoid's un-/ordered C{Triaxial/_}.

1903 '''

1904 a, b, t = self.a, self.b, _MODS.triaxials

1905 T = t.Triaxial if a > b else t.Triaxial_

1906 return T(a, a, b, name=self.name)

1907

1908 @Property_RO

1909 def volume(self):

1910 '''Get the ellipsoid's I{volume} (C{meter**3}), M{4 / 3 * PI * R3**3}.

1911

1912 @see: C{R3}.

1913 '''

1914 return Meter3(volume=self.a2 * self.b * PI_3 * _4_0)

1915

1916

1917class Ellipsoid2(Ellipsoid):

1918 '''An L{Ellipsoid} specified by I{equatorial} radius and I{flattening}.

1919 '''

1920 def __init__(self, a, f=None, **name):

1921 '''New L{Ellipsoid2}.

1922

1923 @arg a: Equatorial radius, semi-axis (C{meter}) or a previous

1924 L{Ellipsoid} instance.

1925 @arg f: Flattening: (C{float} < 1.0, negative for I{prolate}),

1926 if B{C{a}} is in C{meter}.

1927 @kwarg name: Optional, unique C{B{name}=NN} (C{str}).

1928

1929 @raise NameError: Ellipsoid with that B{C{name}} already exists.

1930

1931 @raise ValueError: Invalid B{C{a}} or B{C{f}}.

1932

1933 @note: C{abs(B{f}) < EPS} is forced to C{B{f}=0}, I{spherical}.

1934 Negative C{B{f}} produces a I{prolate} ellipsoid.

1935 '''

1936 if f is None and isinstance(a, Ellipsoid):

1937 Ellipsoid.__init__(self, a.a, f =a.f,

1938 b=a.b, f_=a.f_, **name)

1939 else:

1940 Ellipsoid.__init__(self, a, f=f, **name)

1941

1942

1943def _ispherical_a_b(a, b):

1944 '''(INTERNAL) C{True} for spherical or invalid C{a} or C{b}.

1945 '''

1946 return a < EPS0 or b < EPS0 or fabs(a - b) < EPS0

1947

1948

1949def _ispherical_f(f):

1950 '''(INTERNAL) C{True} for spherical or invalid C{f}.

1951 '''

1952 return f > EPS1 or fabs(f) < EPS

1953

1954

1955def _ispherical_f_(f_):

1956 '''(INTERNAL) C{True} for spherical or invalid C{f_}.

1957 '''

1958 f_ = fabs(f_)

1959 return f_ < EPS or f_ > _1_EPS

1960

1961

1962def a_b2e(a, b):

1963 '''Return C{e}, the I{1st eccentricity} for a given I{equatorial} and I{polar} radius.

1964

1965 @arg a: Equatorial radius (C{scalar} > 0).

1966 @arg b: Polar radius (C{scalar} > 0).

1967

1968 @return: The I{unsigned}, (1st) eccentricity (C{float} or C{0}), M{sqrt(1 - (b / a)**2)}.

1969

1970 @note: The result is always I{non-negative} and C{0} for I{near-spherical} ellipsoids.

1971 '''

1972 e2 = _a2b2e2(a, b, b2=False)

1973 return Float(e=sqrt(fabs(e2)) if e2 else _0_0) # == sqrt(fabs((a - b) * (a + b))) / a

1974

1975

1976def a_b2e2(a, b):

1977 '''Return C{e2}, the I{1st eccentricity squared} for a given I{equatorial} and I{polar} radius.

1978

1979 @arg a: Equatorial radius (C{scalar} > 0).

1980 @arg b: Polar radius (C{scalar} > 0).

1981

1982 @return: The I{signed}, (1st) eccentricity I{squared} (C{float} or C{0}), M{1 - (b / a)**2}.

1983

1984 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

1985 for I{near-spherical} ellipsoids.

1986 '''

1987 return Float(e2=_a2b2e2(a, b, b2=False))

1988

1989

1990def a_b2e22(a, b):

1991 '''Return C{e22}, the I{2nd eccentricity squared} for a given I{equatorial} and I{polar} radius.

1992

1993 @arg a: Equatorial radius (C{scalar} > 0).

1994 @arg b: Polar radius (C{scalar} > 0).

1995

1996 @return: The I{signed}, 2nd eccentricity I{squared} (C{float} or C{0}), M{(a / b)**2 - 1}.

1997

1998 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

1999 for I{near-spherical} ellipsoids.

2000 '''

2001 return Float(e22=_a2b2e2(a, b, a2=False))

2002

2003

2004def a_b2e32(a, b):

2005 '''Return C{e32}, the I{3rd eccentricity squared} for a given I{equatorial} and I{polar} radius.

2006

2007 @arg a: Equatorial radius (C{scalar} > 0).

2008 @arg b: Polar radius (C{scalar} > 0).

2009

2010 @return: The I{signed}, 3rd eccentricity I{squared} (C{float} or C{0}),

2011 M{(a**2 - b**2) / (a**2 + b**2)}.

2012

2013 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2014 for I{near-spherical} ellipsoids.

2015 '''

2016 return Float(e32=_a2b2e2(a, b))

2017

2018

2019def _a2b2e2(a, b, a2=True, b2=True):

2020 '''(INTERNAL) Helper for C{a_b2e}, C{a_b2e2}, C{a_b2e22} and C{a_b2e32}.

2021 '''

2022 if _ispherical_a_b(a, b):

2023 e2 = _0_0

2024 else: # a > 0, b > 0

2025 a, b = (_1_0, b / a) if a > b else (a / b, _1_0)

2026 a2b2 = float(a - b) * (a + b)

2027 e2 = _over(a2b2, (a**2 if a2 else _0_0) +

2028 (b**2 if b2 else _0_0)) if a2b2 else _0_0

2029 return e2

2030

2031

2032def a_b2f(a, b):

2033 '''Return C{f}, the I{flattening} for a given I{equatorial} and I{polar} radius.

2034

2035 @arg a: Equatorial radius (C{scalar} > 0).

2036 @arg b: Polar radius (C{scalar} > 0).

2037

2038 @return: The flattening (C{scalar} or C{0}), M{(a - b) / a}.

2039

2040 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2041 for I{near-spherical} ellipsoids.

2042 '''

2043 f = 0 if _ispherical_a_b(a, b) else _over(float(a - b), a)

2044 return _f_0_0 if _ispherical_f(f) else Float(f=f)

2045

2046

2047def a_b2f_(a, b):

2048 '''Return C{f_}, the I{inverse flattening} for a given I{equatorial} and I{polar} radius.

2049

2050 @arg a: Equatorial radius (C{scalar} > 0).

2051 @arg b: Polar radius (C{scalar} > 0).

2052

2053 @return: The inverse flattening (C{scalar} or C{0}), M{a / (a - b)}.

2054

2055 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2056 for I{near-spherical} ellipsoids.

2057 '''

2058 f_ = 0 if _ispherical_a_b(a, b) else _over(a, float(a - b))

2059 return _f__0_0 if _ispherical_f_(f_) else Float(f_=f_)

2060

2061

2062def a_b2f2(a, b):

2063 '''Return C{f2}, the I{2nd flattening} for a given I{equatorial} and I{polar} radius.

2064

2065 @arg a: Equatorial radius (C{scalar} > 0).

2066 @arg b: Polar radius (C{scalar} > 0).

2067

2068 @return: The I{signed}, 2nd flattening (C{scalar} or C{0}), M{(a - b) / b}.

2069

2070 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2071 for I{near-spherical} ellipsoids.

2072 '''

2073 t = 0 if _ispherical_a_b(a, b) else float(a - b)

2074 return Float(f2=_0_0 if fabs(t) < EPS0 else _over(t, b))

2075

2076

2077def a_b2n(a, b):

2078 '''Return C{n}, the I{3rd flattening} for a given I{equatorial} and I{polar} radius.

2079

2080 @arg a: Equatorial radius (C{scalar} > 0).

2081 @arg b: Polar radius (C{scalar} > 0).

2082

2083 @return: The I{signed}, 3rd flattening (C{scalar} or C{0}), M{(a - b) / (a + b)}.

2084

2085 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2086 for I{near-spherical} ellipsoids.

2087 '''

2088 t = 0 if _ispherical_a_b(a, b) else float(a - b)

2089 return Float(n=_0_0 if fabs(t) < EPS0 else _over(t, a + b))

2090

2091

2092def a_f2b(a, f):

2093 '''Return C{b}, the I{polar} radius for a given I{equatorial} radius and I{flattening}.

2094

2095 @arg a: Equatorial radius (C{scalar} > 0).

2096 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2097

2098 @return: The polar radius (C{float}), M{a * (1 - f)}.

2099 '''

2100 b = a if _ispherical_f(f) else (a * (_1_0 - f))

2101 return Radius_(b=a if _ispherical_a_b(a, b) else b)

2102

2103

2104def a_f_2b(a, f_):

2105 '''Return C{b}, the I{polar} radius for a given I{equatorial} radius and I{inverse flattening}.

2106

2107 @arg a: Equatorial radius (C{scalar} > 0).

2108 @arg f_: Inverse flattening (C{scalar} >>> 1).

2109

2110 @return: The polar radius (C{float}), M{a * (f_ - 1) / f_}.

2111 '''

2112 b = a if _ispherical_f_(f_) else _over(a * (f_ - _1_0), f_)

2113 return Radius_(b=a if _ispherical_a_b(a, b) else b)

2114

2115

2116def b_f2a(b, f):

2117 '''Return C{a}, the I{equatorial} radius for a given I{polar} radius and I{flattening}.

2118

2119 @arg b: Polar radius (C{scalar} > 0).

2120 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2121

2122 @return: The equatorial radius (C{float}), M{b / (1 - f)}.

2123 '''

2124 t = _1_0 - f

2125 a = b if fabs(t) < EPS0 else _over(b, t)

2126 return Radius_(a=b if _ispherical_a_b(a, b) else a)

2127

2128

2129def b_f_2a(b, f_):

2130 '''Return C{a}, the I{equatorial} radius for a given I{polar} radius and I{inverse flattening}.

2131

2132 @arg b: Polar radius (C{scalar} > 0).

2133 @arg f_: Inverse flattening (C{scalar} >>> 1).

2134

2135 @return: The equatorial radius (C{float}), M{b * f_ / (f_ - 1)}.

2136 '''

2137 t = f_ - _1_0

2138 a = b if _ispherical_f_(f_) or fabs(t) < EPS0 \

2139 or fabs(t - f_) < EPS0 else _over(b * f_, t)

2140 return Radius_(a=b if _ispherical_a_b(a, b) else a)

2141

2142

2143def e2f(e):

2144 '''Return C{f}, the I{flattening} for a given I{1st eccentricity}.

2145

2146 @arg e: The (1st) eccentricity (0 <= C{float} < 1)

2147

2148 @return: The flattening (C{scalar} or C{0}).

2149

2150 @see: Function L{e22f}.

2151 '''

2152 return e22f(e**2)

2153

2154

2155def e22f(e2):

2156 '''Return C{f}, the I{flattening} for a given I{1st eccentricity squared}.

2157

2158 @arg e2: The (1st) eccentricity I{squared}, I{signed} (L{NINF} < C{float} < 1)

2159

2160 @return: The flattening (C{float} or C{0}), M{e2 / (sqrt(1 - e2) + 1)}.

2161 '''

2162 return Float(f=_over(e2, sqrt(_1_0 - e2) + _1_0)) if e2 and e2 < _1_0 else _f_0_0

2163

2164

2165def f2e2(f):

2166 '''Return C{e2}, the I{1st eccentricity squared} for a given I{flattening}.

2167

2168 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2169

2170 @return: The I{signed}, (1st) eccentricity I{squared} (C{float} < 1), M{f * (2 - f)}.

2171

2172 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2173 for I{near-spherical} ellipsoids.

2174

2175 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/

2176 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening

2177 <https://WikiPedia.org/wiki/Flattening>}.

2178 '''

2179 return Float(e2=_0_0 if _ispherical_f(f) else (f * (_2_0 - f)))

2180

2181

2182def f2e22(f):

2183 '''Return C{e22}, the I{2nd eccentricity squared} for a given I{flattening}.

2184

2185 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2186

2187 @return: The I{signed}, 2nd eccentricity I{squared} (C{float} > -1 or C{INF}),

2188 M{f * (2 - f) / (1 - f)**2}.

2189

2190 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2191 for near-spherical ellipsoids.

2192

2193 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/

2194 C++/doc/classGeographicLib_1_1Ellipsoid.html>}.

2195 '''

2196 # e2 / (1 - e2) == f * (2 - f) / (1 - f)**2

2197 t = (_1_0 - f)**2

2198 return Float(e22=INF if t < EPS0 else _over(f2e2(f), t)) # PYCHOK type

2199

2200

2201def f2e32(f):

2202 '''Return C{e32}, the I{3rd eccentricity squared} for a given I{flattening}.

2203

2204 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2205

2206 @return: The I{signed}, 3rd eccentricity I{squared} (C{float}),

2207 M{f * (2 - f) / (1 + (1 - f)**2)}.

2208

2209 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2210 for I{near-spherical} ellipsoids.

2211

2212 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/

2213 C++/doc/classGeographicLib_1_1Ellipsoid.html>}.

2214 '''

2215 # e2 / (2 - e2) == f * (2 - f) / (1 + (1 - f)**2)

2216 e2 = f2e2(f)

2217 return Float(e32=_over(e2, _2_0 - e2))

2218

2219

2220def f_2f(f_):

2221 '''Return C{f}, the I{flattening} for a given I{inverse flattening}.

2222

2223 @arg f_: Inverse flattening (C{scalar} >>> 1).

2224

2225 @return: The flattening (C{scalar} or C{0}), M{1 / f_}.

2226

2227 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2228 for I{near-spherical} ellipsoids.

2229 '''

2230 f = 0 if _ispherical_f_(f_) else _over(_1_0, f_)

2231 return _f_0_0 if _ispherical_f(f) else Float(f=f) # PYCHOK type

2232

2233

2234def f2f_(f):

2235 '''Return C{f_}, the I{inverse flattening} for a given I{flattening}.

2236

2237 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2238

2239 @return: The inverse flattening (C{scalar} or C{0}), M{1 / f}.

2240

2241 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2242 for I{near-spherical} ellipsoids.

2243 '''

2244 f_ = 0 if _ispherical_f(f) else _over(_1_0, f)

2245 return _f__0_0 if _ispherical_f_(f_) else Float(f_=f_) # PYCHOK type

2246

2247

2248def f2f2(f):

2249 '''Return C{f2}, the I{2nd flattening} for a given I{flattening}.

2250

2251 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2252

2253 @return: The I{signed}, 2nd flattening (C{scalar} or C{INF}), M{f / (1 - f)}.

2254

2255 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2256 for I{near-spherical} ellipsoids.

2257

2258 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/

2259 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening

2260 <https://WikiPedia.org/wiki/Flattening>}.

2261 '''

2262 t = _1_0 - f

2263 return Float(f2=_0_0 if _ispherical_f(f) else

2264 (INF if fabs(t) < EPS else _over(f, t))) # PYCHOK type

2265

2266

2267def f2n(f):

2268 '''Return C{n}, the I{3rd flattening} for a given I{flattening}.

2269

2270 @arg f: Flattening (C{scalar} < 1, negative for I{prolate}).

2271

2272 @return: The I{signed}, 3rd flattening (-1 <= C{float} < 1),

2273 M{f / (2 - f)}.

2274

2275 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2276 for I{near-spherical} ellipsoids.

2277

2278 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/

2279 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening

2280 <https://WikiPedia.org/wiki/Flattening>}.

2281 '''

2282 return Float(n=_0_0 if _ispherical_f(f) else _over(f, float(_2_0 - f)))

2283

2284

2285def n2e2(n):

2286 '''Return C{e2}, the I{1st eccentricity squared} for a given I{3rd flattening}.

2287

2288 @arg n: The 3rd flattening (-1 <= C{scalar} < 1).

2289

2290 @return: The I{signed}, (1st) eccentricity I{squared} (C{float} or NINF),

2291 M{4 * n / (1 + n)**2}.

2292

2293 @note: The result is positive for I{oblate}, negative for I{prolate} or C{0}

2294 for I{near-spherical} ellipsoids.

2295

2296 @see: U{Flattening<https://WikiPedia.org/wiki/Flattening>}.

2297 '''

2298 t = (n + _1_0)**2

2299 return Float(e2=_0_0 if fabs(n) < EPS0 else

2300 (NINF if t < EPS0 else _over(_4_0 * n, t)))

2301

2302

2303def n2f(n):

2304 '''Return C{f}, the I{flattening} for a given I{3rd flattening}.

2305

2306 @arg n: The 3rd flattening (-1 <= C{scalar} < 1).

2307

2308 @return: The flattening (C{scalar} or NINF), M{2 * n / (1 + n)}.

2309

2310 @see: U{Eccentricity conversions<https://GeographicLib.SourceForge.io/

2311 C++/doc/classGeographicLib_1_1Ellipsoid.html>} and U{Flattening

2312 <https://WikiPedia.org/wiki/Flattening>}.

2313 '''

2314 t = n + _1_0

2315 f = 0 if fabs(n) < EPS0 else (NINF if t < EPS0 else _over(_2_0 * n, t))

2316 return _f_0_0 if _ispherical_f(f) else Float(f=f)

2317

2318

2319def n2f_(n):

2320 '''Return C{f_}, the I{inverse flattening} for a given I{3rd flattening}.

2321

2322 @arg n: The 3rd flattening (-1 <= C{scalar} < 1).

2323

2324 @return: The inverse flattening (C{scalar} or C{0}), M{1 / f}.

2325

2326 @see: L{n2f} and L{f2f_}.

2327 '''

2328 return f2f_(n2f(n))

2329

2330

2331class Ellipsoids(_NamedEnum):

2332 '''(INTERNAL) L{Ellipsoid} registry, I{must} be a sub-class

2333 to accommodate the L{_LazyNamedEnumItem} properties.

2334 '''

2335 def _Lazy(self, a, b, f_, **kwds):

2336 '''(INTERNAL) Instantiate the L{Ellipsoid}.

2337 '''

2338 return Ellipsoid(a, b=b, f_=f_, **kwds)

2339

2340Ellipsoids = Ellipsoids(Ellipsoid) # PYCHOK singleton

2341'''Some pre-defined L{Ellipsoid}s, all I{lazily} instantiated.'''

2342# <https://www.GNU.org/software/gama/manual/html_node/Supported-ellipsoids.html>

2343# <https://GSSC.ESA.int/navipedia/index.php/Reference_Frames_in_GNSS>

2344# <https://kb.OSU.edu/dspace/handle/1811/77986>

2345# <https://www.IBM.com/docs/en/db2/11.5?topic=systems-supported-spheroids>

2346# <https://w3.Energistics.org/archive/Epicentre/Epicentre_v3.0/DataModel/LogicalDictionary/StandardValues/ellipsoid.html>

2347# <https://GitHub.com/locationtech/proj4j/blob/master/src/main/java/org/locationtech/proj4j/datum/Ellipsoid.java>

2348Ellipsoids._assert( # <https://WikiPedia.org/wiki/Earth_ellipsoid>

2349 Airy1830 = _lazy(_Airy1830_, *_T(6377563.396, _0_0, 299.3249646)), # b=6356256.909

2350 AiryModified = _lazy(_AiryModified_, *_T(6377340.189, _0_0, 299.3249646)), # b=6356034.448

2351# APL4_9 = _lazy('APL4_9', *_T(6378137.0, _0_0, 298.24985392)), # Appl. Phys. Lab. 1965

2352# ANS = _lazy('ANS', *_T(6378160.0, _0_0, 298.25)), # Australian Nat. Spheroid

2353# AN_SA96 = _lazy('AN_SA96', *_T(6378160.0, _0_0, 298.24985392)), # Australian Nat. South America

2354 Australia1966 = _lazy('Australia1966', *_T(6378160.0, _0_0, 298.25)), # b=6356774.7192

2355 ATS1977 = _lazy('ATS1977', *_T(6378135.0, _0_0, 298.257)), # "Average Terrestrial System"

2356 Bessel1841 = _lazy(_Bessel1841_, *_T(6377397.155, 6356078.962818, 299.152812797)),

2357 BesselModified = _lazy('BesselModified', *_T(6377492.018, _0_0, 299.1528128)),

2358# BesselNamibia = _lazy('BesselNamibia', *_T(6377483.865, _0_0, 299.1528128)),

2359 CGCS2000 = _lazy('CGCS2000', *_T(R_MA, _0_0, 298.257222101)), # BeiDou Coord System (BDC)

2360# Clarke1858 = _lazy('Clarke1858', *_T(6378293.639, _0_0, 294.260676369)),

2361 Clarke1866 = _lazy(_Clarke1866_, *_T(6378206.4, 6356583.8, 294.978698214)),

2362 Clarke1880 = _lazy('Clarke1880', *_T(6378249.145, 6356514.86954978, 293.465)),

2363 Clarke1880IGN = _lazy(_Clarke1880IGN_, *_T(6378249.2, 6356515.0, 293.466021294)),

2364 Clarke1880Mod = _lazy('Clarke1880Mod', *_T(6378249.145, 6356514.96639549, 293.466307656)), # aka Clarke1880Arc

2365 CPM1799 = _lazy('CPM1799', *_T(6375738.7, 6356671.92557493, 334.39)), # Comm. des Poids et Mesures

2366 Delambre1810 = _lazy('Delambre1810', *_T(6376428.0, 6355957.92616372, 311.5)), # Belgium

2367 Engelis1985 = _lazy('Engelis1985', *_T(6378136.05, 6356751.32272154, 298.2566)),

2368# Everest1830 = _lazy('Everest1830', *_T(6377276.345, _0_0, 300.801699997)),

2369# Everest1948 = _lazy('Everest1948', *_T(6377304.063, _0_0, 300.801699997)),

2370# Everest1956 = _lazy('Everest1956', *_T(6377301.243, _0_0, 300.801699997)),

2371 Everest1969 = _lazy('Everest1969', *_T(6377295.664, 6356094.667915, 300.801699997)),

2372 Everest1975 = _lazy('Everest1975', *_T(6377299.151, 6356098.14512013, 300.8017255)),

2373 Fisher1968 = _lazy('Fisher1968', *_T(6378150.0, 6356768.33724438, 298.3)),

2374# Fisher1968Mod = _lazy('Fisher1968Mod', *_T(6378155.0, _0_0, 298.3)),

2375 GEM10C = _lazy('GEM10C', *_T(R_MA, 6356752.31424783, 298.2572236)),

2376 GPES = _lazy('GPES', *_T(6378135.0, 6356750.0, _0_0)), # "Gen. Purpose Earth Spheroid"

2377 GRS67 = _lazy('GRS67', *_T(6378160.0, _0_0, 298.247167427)), # Lucerne b=6356774.516

2378# GRS67Truncated = _lazy('GRS67Truncated', *_T(6378160.0, _0_0, 298.25)),

2379 GRS80 = _lazy(_GRS80_, *_T(R_MA, 6356752.314140347, 298.25722210088)), # IUGG, ITRS, ETRS89

2380# Hayford1924 = _lazy('Hayford1924', *_T(6378388.0, 6356911.94612795, None)), # aka Intl1924 f_=297

2381 Helmert1906 = _lazy('Helmert1906', *_T(6378200.0, 6356818.16962789, 298.3)),

2382# Hough1960 = _lazy('Hough1960', *_T(6378270.0, _0_0, 297.0)),

2383 IAU76 = _lazy('IAU76', *_T(6378140.0, _0_0, 298.257)), # Int'l Astronomical Union

2384 IERS1989 = _lazy('IERS1989', *_T(6378136.0, _0_0, 298.257)), # b=6356751.302

2385 IERS1992TOPEX = _lazy('IERS1992TOPEX', *_T(6378136.3, 6356751.61659215, 298.257223563)), # IERS/TOPEX/Poseidon/McCarthy

2386 IERS2003 = _lazy('IERS2003', *_T(6378136.6, 6356751.85797165, 298.25642)),

2387 Intl1924 = _lazy(_Intl1924_, *_T(6378388.0, _0_0, 297.0)), # aka Hayford b=6356911.9462795

2388 Intl1967 = _lazy('Intl1967', *_T(6378157.5, 6356772.2, 298.24961539)), # New Int'l

2389 Krassovski1940 = _lazy(_Krassovski1940_, *_T(6378245.0, 6356863.01877305, 298.3)), # spelling

2390 Krassowsky1940 = _lazy(_Krassowsky1940_, *_T(6378245.0, 6356863.01877305, 298.3)), # spelling

2391# Kaula = _lazy('Kaula', *_T(6378163.0, _0_0, 298.24)), # Kaula 1961

2392# Lerch = _lazy('Lerch', *_T(6378139.0, _0_0, 298.257)), # Lerch 1979

2393 Maupertuis1738 = _lazy('Maupertuis1738', *_T(6397300.0, 6363806.28272251, 191.0)), # France

2394 Mercury1960 = _lazy('Mercury1960', *_T(6378166.0, 6356784.28360711, 298.3)),

2395 Mercury1968Mod = _lazy('Mercury1968Mod', *_T(6378150.0, 6356768.33724438, 298.3)),

2396# MERIT = _lazy('MERIT', *_T(6378137.0, _0_0, 298.257)), # MERIT 1983

2397# NWL10D = _lazy('NWL10D', *_T(6378135.0, _0_0, 298.26)), # Naval Weapons Lab.

2398 NWL1965 = _lazy('NWL1965', *_T(6378145.0, 6356759.76948868, 298.25)), # Naval Weapons Lab.

2399# NWL9D = _lazy('NWL9D', *_T(6378145.0, 6356759.76948868, 298.25)), # NWL1965

2400 OSU86F = _lazy('OSU86F', *_T(6378136.2, 6356751.51693008, 298.2572236)),

2401 OSU91A = _lazy('OSU91A', *_T(6378136.3, 6356751.6165948, 298.2572236)),

2402# Plessis1817 = _lazy('Plessis1817', *_T(6397523.0, 6355863.0, 153.56512242)), # XXX incorrect?

2403 Plessis1817 = _lazy('Plessis1817', *_T(6376523.0, 6355862.93325557, 308.64)), # XXX IGN France 1972

2404# Prolate = _lazy('Prolate', *_T(6356752.3, R_MA, _0_0)),

2405 PZ90 = _lazy('PZ90', *_T(6378136.0, _0_0, 298.257839303)), # GLOSNASS PZ-90 and PZ-90.11

2406# SEAsia = _lazy('SEAsia', *_T(6378155.0, _0_0, 298.3)), # SouthEast Asia

2407 SGS85 = _lazy('SGS85', *_T(6378136.0, 6356751.30156878, 298.257)), # Soviet Geodetic System

2408 SoAmerican1969 = _lazy('SoAmerican1969', *_T(6378160.0, 6356774.71919531, 298.25)), # South American

2409 Sphere = _lazy(_Sphere_, *_T(R_M, R_M, _0_0)), # pseudo

2410 SphereAuthalic = _lazy('SphereAuthalic', *_T(R_FM, R_FM, _0_0)), # pseudo

2411 SpherePopular = _lazy('SpherePopular', *_T(R_MA, R_MA, _0_0)), # EPSG:3857 Spheroid

2412 Struve1860 = _lazy('Struve1860', *_T(6378298.3, 6356657.14266956, 294.73)),

2413# Walbeck = _lazy('Walbeck', *_T(6376896.0, _0_0, 302.78)),

2414# WarOffice = _lazy('WarOffice', *_T(6378300.0, _0_0, 296.0)),

2415 WGS60 = _lazy('WGS60', *_T(6378165.0, 6356783.28695944, 298.3)),

2416 WGS66 = _lazy('WGS66', *_T(6378145.0, 6356759.76948868, 298.25)),

2417 WGS72 = _lazy(_WGS72_, *_T(6378135.0, _0_0, 298.26)), # b=6356750.52

2418 WGS84 = _lazy(_WGS84_, *_T(R_MA, _0_0, _f__WGS84)), # b=6356752.3142451793

2419# U{NOAA/NOS/NGS/inverse<https://GitHub.com/noaa-ngs/inverse/blob/main/invers3d.f>}

2420 WGS84_NGS = _lazy('WGS84_NGS', *_T(R_MA, _0_0, 298.257222100882711243162836600094))

2421)

2422

2423_EWGS84 = Ellipsoids.WGS84 # (INTERNAL) shared

2424

2425if __name__ == _DMAIN_:

2426

2427 from pygeodesy import nameof, printf

2428

2429 for E in (_EWGS84, Ellipsoids.GRS80, # NAD83,

2430 Ellipsoids.Sphere, Ellipsoids.SpherePopular,

2431 Ellipsoid(_EWGS84.b, _EWGS84.a, name='_Prolate')):

2432 e = f2n(E.f) - E.n

2433 printf('# %s: %s', _DOT_('Ellipsoids', E.name), E.toStr(prec=10, terse=0), nl=1)

2434 printf('# e=%s, f_=%s, f=%s, n=%s (%s)', fstr(E.e, prec=13, fmt=Fmt.e),

2435 fstr(E.f_, prec=13, fmt=Fmt.e),

2436 fstr(E.f, prec=13, fmt=Fmt.e),

2437 fstr(E.n, prec=13, fmt=Fmt.e),

2438 fstr(e, prec=9, fmt=Fmt.e))

2439 printf('# %s %s', Ellipsoid.AlphaKs.name, fstr(E.AlphaKs, prec=20))

2440 printf('# %s %s', Ellipsoid.BetaKs.name, fstr(E.BetaKs, prec=20))

2441 printf('# %s %s', nameof(Ellipsoid.KsOrder), E.KsOrder) # property

2442

2443 from pygeodesy.internals import _pregistry

2444 # __doc__ of this file, force all into registry

2445 _pregistry(Ellipsoids)

2446

2447# % python3.13 -m pygeodesy.ellipsoids

2448

2449# Ellipsoids.WGS84: name='WGS84', a=6378137, f=0.0033528107, f_=298.257223563, b=6356752.3142451793, f2=0.0033640898, n=0.0016792204, e=0.0818191908, e2=0.00669438, e21=0.99330562, e22=0.0067394967, e32=0.0033584313, A=6367449.1458234144, L=10001965.7293127235, R1=6371008.7714150595, R2=6371007.1809184738, R3=6371000.7900091587, Rbiaxial=6367453.6345163295, Rtriaxial=6372797.5559594007

2450# e=8.1819190842622e-02, f_=2.98257223563e+02, f=3.3528106647475e-03, n=1.6792203863837e-03 (0.0e+00)

2451# AlphaKs 0.00083773182062446994, 0.00000076085277735725, 0.00000000119764550324, 0.00000000000242917068, 0.00000000000000571182, 0.0000000000000000148, 0.00000000000000000004, 0.0

2452# BetaKs 0.00083773216405794875, 0.0000000590587015222, 0.00000000016734826653, 0.00000000000021647981, 0.00000000000000037879, 0.00000000000000000072, 0.0, 0.0

2453# KsOrder 8

2454

2455# Ellipsoids.GRS80: name='GRS80', a=6378137, f=0.0033528107, f_=298.2572221009, b=6356752.3141403468, f2=0.0033640898, n=0.0016792204, e=0.081819191, e2=0.00669438, e21=0.99330562, e22=0.0067394968, e32=0.0033584313, A=6367449.1457710434, L=10001965.7292304561, R1=6371008.7713801153, R2=6371007.1808835147, R3=6371000.7899741363, Rbiaxial=6367453.6344640013, Rtriaxial=6372797.5559332585

2456# e=8.1819191042833e-02, f_=2.9825722210088e+02, f=3.3528106811837e-03, n=1.6792203946295e-03 (0.0e+00)

2457# AlphaKs 0.00083773182472890429, 0.00000076085278481561, 0.00000000119764552086, 0.00000000000242917073, 0.00000000000000571182, 0.0000000000000000148, 0.00000000000000000004, 0.0

2458# BetaKs 0.0008377321681623882, 0.00000005905870210374, 0.000000000167348269, 0.00000000000021647982, 0.00000000000000037879, 0.00000000000000000072, 0.0, 0.0

2459# KsOrder 8

2460

2461# Ellipsoids.Sphere: name='Sphere', a=6371008.7714149999, f=0, f_=0, b=6371008.7714149999, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6371008.7714149999, L=10007557.1761167478, R1=6371008.7714149999, R2=6371008.7714149999, R3=6371008.7714149999, Rbiaxial=6371008.7714149999, Rtriaxial=6371008.7714149999

2462# e=0.0e+00, f_=0.0e+00, f=0.0e+00, n=0.0e+00 (0.0e+00)

2463# AlphaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0

2464# BetaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0

2465# KsOrder 8

2466

2467# Ellipsoids.SpherePopular: name='SpherePopular', a=6378137, f=0, f_=0, b=6378137, f2=0, n=0, e=0, e2=0, e21=1, e22=0, e32=0, A=6378137, L=10018754.171394622, R1=6378137, R2=6378137, R3=6378137, Rbiaxial=6378137, Rtriaxial=6378137

2468# e=0.0e+00, f_=0.0e+00, f=0.0e+00, n=0.0e+00 (0.0e+00)

2469# AlphaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0

2470# BetaKs 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0, 0.0

2471# KsOrder 8

2472

2473# Ellipsoids._Prolate: name='_Prolate', a=6356752.3142451793, f=-0.0033640898, f_=-297.257223563, b=6378137, f2=-0.0033528107, n=-0.0016792204, e=0.0820944379, e2=-0.0067394967, e21=1.0067394967, e22=-0.00669438, e32=-0.0033584313, A=6367449.1458234144, L=10035500.5204500332, R1=6363880.5428301189, R2=6363878.9413582645, R3=6363872.5644020075, Rbiaxial=6367453.6345163295, Rtriaxial=6362105.2243882557

2474# e=8.2094437949696e-02, f_=-2.97257223563e+02, f=-3.3640898209765e-03, n=-1.6792203863837e-03 (0.0e+00)

2475# AlphaKs -0.00084149152514366627, 0.00000076653480614871, -0.00000000120934503389, 0.0000000000024576225, -0.00000000000000578863, 0.00000000000000001502, -0.00000000000000000004, 0.0

2476# BetaKs -0.00084149187224351817, 0.00000005842735196773, -0.0000000001680487236, 0.00000000000021706261, -0.00000000000000038002, 0.00000000000000000073, -0.0, 0.0

2477# KsOrder 8

2478

2479# **) MIT License

2480#

2482#

2483# Permission is hereby granted, free of charge, to any person obtaining a

2484# copy of this software and associated documentation files (the "Software"),

2485# to deal in the Software without restriction, including without limitation

2486# the rights to use, copy, modify, merge, publish, distribute, sublicense,

2487# and/or sell copies of the Software, and to permit persons to whom the

2488# Software is furnished to do so, subject to the following conditions:

2489#

2490# The above copyright notice and this permission notice shall be included

2491# in all copies or substantial portions of the Software.

2492#

2493# THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS

2494# OR IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY,

2495# FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL

2496# THE AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR

2497# OTHER LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE,

2498# ARISING FROM, OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR

2499# OTHER DEALINGS IN THE SOFTWARE.