# Coverage for pygeodesy/ecef.py : 95%

## 447 statements 424 run 23 missing 46 excluded

Hot-keys on this page

r m x p toggle line displays

j k next/prev highlighted chunk

0 (zero) top of page

1 (one) first highlighted chunk

1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532 533 534 535 536 537 538 539 540 541 542 543 544 545 546 547 548 549 550 551 552 553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 596 597 598 599 600 601 602 603 604 605 606 607 608 609 610 611 612 613 614 615 616 617 618 619 620 621 622 623 624 625 626 627 628 629 630 631 632 633 634 635 636 637 638 639 640 641 642 643 644 645 646 647 648 649 650 651 652 653 654 655 656 657 658 659 660 661 662 663 664 665 666 667 668 669 670 671 672 673 674 675 676 677 678 679 680 681 682 683 684 685 686 687 688 689 690 691 692 693 694 695 696 697 698 699 700 701 702 703 704 705 706 707 708 709 710 711 712 713 714 715 716 717 718 719 720 721 722 723 724 725 726 727 728 729 730 731 732 733 734 735 736 737 738 739 740 741 742 743 744 745 746 747 748 749 750 751 752 753 754 755 756 757 758 759 760 761 762 763 764 765 766 767 768 769 770 771 772 773 774 775 776 777 778 779 780 781 782 783 784 785 786 787 788 789 790 791 792 793 794 795 796 797 798 799 800 801 802 803 804 805 806 807 808 809 810 811 812 813 814 815 816 817 818 819 820 821 822 823 824 825 826 827 828 829 830 831 832 833 834 835 836 837 838 839 840 841 842 843 844 845 846 847 848 849 850 851 852 853 854 855 856 857 858 859 860 861 862 863 864 865 866 867 868 869 870 871 872 873 874 875 876 877 878 879 880 881 882 883 884 885 886 887 888 889 890 891 892 893 894 895 896 897 898 899 900 901 902 903 904 905 906 907 908 909 910 911 912 913 914 915 916 917 918 919 920 921 922 923 924 925 926 927 928 929 930 931 932 933 934 935 936 937 938 939 940 941 942 943 944 945 946 947 948 949 950 951 952 953 954 955 956 957 958 959 960 961 962 963 964 965 966 967 968 969 970 971 972 973 974 975 976 977 978 979 980 981 982 983 984 985 986 987 988 989 990 991 992 993 994 995 996 997 998 999 1000 1001 1002 1003 1004 1005 1006 1007 1008 1009 1010 1011 1012 1013 1014 1015 1016 1017 1018 1019 1020 1021 1022 1023 1024 1025 1026 1027 1028 1029 1030 1031 1032 1033 1034 1035 1036 1037 1038 1039 1040 1041 1042 1043 1044 1045 1046 1047 1048 1049 1050 1051 1052 1053 1054 1055 1056 1057 1058 1059 1060 1061 1062 1063 1064 1065 1066 1067 1068 1069 1070 1071 1072 1073 1074 1075 1076 1077 1078 1079 1080 1081 1082 1083 1084 1085 1086 1087 1088 1089 1090 1091 1092 1093 1094 1095 1096 1097 1098 1099 1100 1101 1102 1103 1104 1105 1106 1107 1108 1109 1110 1111 1112 1113 1114 1115 1116 1117 1118 1119 1120 1121 1122 1123 1124 1125 1126 1127 1128 1129 1130 1131 1132 1133 1134 1135 1136 1137 1138 1139 1140 1141 1142 1143 1144 1145 1146 1147 1148 1149 1150 1151 1152 1153 1154 1155 1156 1157 1158 1159 1160 1161 1162 1163 1164 1165 1166 1167 1168 1169 1170 1171 1172 1173 1174 1175 1176 1177 1178 1179 1180 1181 1182 1183 1184 1185 1186 1187 1188 1189 1190 1191 1192 1193 1194 1195 1196 1197 1198 1199 1200 1201 1202 1203 1204 1205 1206 1207 1208 1209 1210 1211 1212 1213 1214 1215 1216 1217 1218 1219 1220 1221 1222 1223 1224 1225 1226 1227 1228 1229 1230 1231 1232 1233 1234 1235 1236 1237 1238 1239 1240 1241 1242 1243 1244 1245 1246 1247 1248 1249 1250 1251 1252 1253 1254 1255 1256 1257 1258 1259 1260 1261 1262 1263 1264 1265 1266 1267 1268 1269 1270 1271 1272 1273 1274 1275 1276 1277 1278 1279 1280 1281 1282 1283 1284 1285 1286 1287 1288 1289 1290 1291 1292 1293 1294 1295 1296 1297 1298 1299 1300 1301 1302 1303 1304 1305 1306 1307 1308 1309 1310 1311 1312 1313 1314 1315 1316 1317 1318 1319 | # -*- coding: utf-8 -*- u'''I{Geocentric} Earth-Centered, Earth-Fixed (ECEF) coordinates. Geocentric conversions transcoded from I{Charles Karney}'s C++ class U{Geocentric <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Geocentric.html>} into pure Python class L{EcefKarney}, class L{EcefSudano} based on I{John Sudano}'s U{paper<https://www.ResearchGate.net/publication/ 3709199_An_exact_conversion_from_an_Earth-centered_coordinate_system_to_latitude_longitude_and_altitude>}, class L{EcefVeness} transcoded from I{Chris Veness}' JavaScript classes U{LatLonEllipsoidal, Cartesian<https://www.Movable-Type.co.UK/scripts/geodesy/docs/latlon-ellipsoidal.js.html>}, class L{EcefYou} implementing I{Rey-Jer You}'s U{transformations <https://www.ResearchGate.net/publication/240359424>} and classes L{EcefFarrell22} and L{EcefFarrell22} from I{Jay A. Farrell}'s U{Table 2.1 and 2.2 <https://Books.Google.com/books?id=fW4foWASY6wC>}, page 29-30. Following is a copy of I{Karney}'s U{Detailed Description <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Geocentric.html>}. Convert between geodetic coordinates C{lat}-, C{lon}gitude and height C{h} (measured vertically from the surface of the ellipsoid) to geocentric C{x}, C{y} and C{z} coordinates, also known as I{Earth-Centered, Earth-Fixed} (U{ECEF<https://WikiPedia.org/wiki/ECEF>}). The origin of geocentric coordinates is at the center of the earth. The C{z} axis goes thru the North pole, C{lat} = 90°. The C{x} axis goes thru C{lat} = 0°, C{lon} = 0°. The I{local (cartesian) origin} is at (C{lat0}, C{lon0}, C{height0}). The I{local} C{x} axis points East, the I{local} C{y} axis points North and the I{local} C{z} axis is normal to the ellipsoid. The plane C{z = -height0} is tangent to the ellipsoid, hence the alternate name I{local tangent plane}. Forward conversion from geodetic to geocentric (ECEF) coordinates is straightforward. For the reverse transformation we use Hugues Vermeille's U{Direct transformation from geocentric coordinates to geodetic coordinates <https://DOI.org/10.1007/s00190-002-0273-6>}, J. Geodesy (2002) 76, 451-454. Several changes have been made to ensure that the method returns accurate results for all finite inputs (even if h is infinite). The changes are described in Appendix B of C. F. F. Karney U{Geodesics on an ellipsoid of revolution<https://ArXiv.org/abs/1102.1215v1>}, Feb. 2011, 85, 105-117 (U{preprint<https://ArXiv.org/abs/1102.1215v1>}). Vermeille similarly updated his method in U{An analytical method to transform geocentric into geodetic coordinates <https://DOI.org/10.1007/s00190-010-0419-x>}, J. Geodesy (2011) 85, 105-117. See U{Geocentric coordinates <https://GeographicLib.SourceForge.io/C++/doc/geocentric.html>} for more information. The errors in these routines are close to round-off. Specifically, for points within 5,000 km of the surface of the ellipsoid (either inside or outside the ellipsoid), the error is bounded by 7 nm (7 nanometers) for the WGS84 ellipsoid. See U{Geocentric coordinates <https://GeographicLib.SourceForge.io/C++/doc/geocentric.html>} for further information on the errors. @see: Module L{ltp} and class L{LocalCartesian}, a transcription of I{Charles Karney}'s C++ class U{LocalCartesian <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1LocalCartesian.html>}, providing conversion to and from I{local} cartesian cordinates in a I{local tangent plane} as opposed to I{geocentric} (ECEF) ones. ''' from pygeodesy.basics import copysign0, isscalar, issubclassof, neg, map1, \ _xinstanceof, _xsubclassof from pygeodesy.constants import EPS, EPS0, EPS02, EPS1, EPS2, EPS_2, PI, PI_2, \ _0_0, _0_0001, _0_01, _0_5, _1_0, _1_0_1T, _2_0, _3_0, _4_0, \ _6_0, _60_0, _90_0, _100_0, isnon0, \ _N_2_0 # PYCHOK used! from pygeodesy.datums import a_f2Tuple, _ellipsoidal_datum # from pygeodesy.ellipsoids import a_f2Tuple # from .datums from pygeodesy.errors import _IndexError, LenError, _ValueError, _TypesError, \ _xdatum, _xkwds from pygeodesy.fmath import cbrt, fdot, hypot, hypot1, hypot2_ from pygeodesy.fsums import Fsum, fsum_ from pygeodesy.interns import NN, _a_, _C_, _datum_, _ellipsoid_, _f_, _h_, \ _height_, _lat_, _lon_, _M_, _name_, _singular_, \ _SPACE_, _x_, _xyz_, _y_, _z_, _tolerance_ # PYCHOK used! from pygeodesy.lazily import _ALL_DOCS, _ALL_LAZY, _ALL_MODS as _MODS from pygeodesy.named import _NamedBase, _NamedTuple, notOverloaded, _Pass, _xnamed from pygeodesy.namedTuples import LatLon2Tuple, LatLon3Tuple, \ PhiLam2Tuple, Vector3Tuple, Vector4Tuple from pygeodesy.props import deprecated_method, Property_RO, property_RO, property_doc_ from pygeodesy.streprs import Fmt, unstr from pygeodesy.units import Height, Int, Lam, Lat, Lon, Meter, Phi, Scalar, Scalar_ from pygeodesy.utily import atan2d, degrees90, degrees180, sincos2, sincos2_, \ sincos2d_ from math import asin, atan2, cos, degrees, radians, sqrt __all__ = _ALL_LAZY.ecef __version__ = '22.09.26' _Ecef_ = 'Ecef' _prolate_ = 'prolate' _TRIPS = 17 # 8..9 sufficient, EcefSudano.reverse _xyz_y_z = _xyz_, _y_, _z_ # _xargs_names(_xyzn4)[:3] class EcefError(_ValueError): '''An ECEF or C{Ecef*} related issue. ''' pass def _llhn4(latlonh, lon, height, suffix=NN, Error=EcefError, name=NN): # in .ltp.LocalCartesian.forward and -.reset '''(INTERNAL) Get C{lat, lon, h, name} as C{4-tuple}. ''' try: lat, lon = latlonh.lat, latlonh.lon h = getattr(latlonh, _height_, getattr(latlonh, _h_, height)) n = getattr(latlonh, _name_, NN) except AttributeError: lat, h, n = latlonh, height, NN try: llhn = Lat(lat), Lon(lon), Height(h), (name or n) except (TypeError, ValueError) as x: t = _lat_, _lon_, _height_ if suffix: t = (_ + suffix for _ in t) d = dict(zip(t, (lat, lon, h))) raise Error(cause=x, **d) return llhn def _xyzn4(xyz, y, z, Types, Error=EcefError, name=NN, # in .ltp _xyz_y_z_names=_xyz_y_z): '''(INTERNAL) Get an C{(x, y, z, name)} 4-tuple. ''' try: try: t = xyz.x, xyz.y, xyz.z, getattr(xyz, _name_, name) if not isinstance(xyz, Types): raise _TypesError(_xyz_y_z_names[0], xyz, *Types) except AttributeError: t = map1(float, xyz, y, z) + (name,) except (TypeError, ValueError) as x: d = dict(zip(_xyz_y_z_names, (xyz, y, z))) raise Error(cause=x, **d) return t # assert _xyz_y_z == _xargs_names(_xyzn4)[:3] class _EcefBase(_NamedBase): '''(INTERNAL) Base class for L{EcefKarney}, L{EcefVeness} and L{EcefYou}. ''' _datum = None _E = None def __init__(self, a_ellipsoid, f=None, name=NN): '''New C{Ecef*} converter. @arg a_ellipsoid: A (non-prolate) ellipsoid (L{Ellipsoid}, L{Ellipsoid2}, L{Datum} or L{a_f2Tuple}) or C{scalar} ellipsoid's equatorial radius (C{meter}). @kwarg f: C{None} or the ellipsoid flattening (C{scalar}), required for C{scalar} B{C{a_ellipsoid}}, C{B{f}=0} represents a sphere, negative B{C{f}} a prolate ellipsoid. @kwarg name: Optional name (C{str}). @raise EcefError: If B{C{a_ellipsoid}} not L{Ellipsoid}, L{Ellipsoid2}, L{Datum} or L{a_f2Tuple} or C{scalar} or B{C{f}} not C{scalar} or if C{scalar} B{C{a_ellipsoid}} not positive or B{C{f}} not less than 1.0. ''' if name: self.name = name try: E = a_ellipsoid if f is None: pass elif isscalar(E) and isscalar(f): E = a_f2Tuple(E, f) else: raise ValueError # _invalid_ d = _ellipsoidal_datum(E, name=name) E = d.ellipsoid if E.a < EPS or E.f > EPS1: raise ValueError # _invalid_ except (TypeError, ValueError) as x: t = unstr(self.classname, a=a_ellipsoid, f=f) raise EcefError(_SPACE_(t, _ellipsoid_), cause=x) self._datum = d self._E = E def __eq__(self, other): '''Compare this and an other Ecef. @arg other: The other ecef (C{Ecef*}). @return: C{True} if equal, C{False} otherwise. ''' return other is self or (isinstance(other, self.__class__) and other.ellipsoid == self.ellipsoid) @Property_RO def equatoradius(self): '''Get the I{equatorial} radius, semi-axis (C{meter}). ''' return self.ellipsoid.a a = equatorialRadius = equatoradius # Karney property @Property_RO def datum(self): '''Get the datum (L{Datum}). ''' return self._datum @Property_RO def ellipsoid(self): '''Get the ellipsoid (L{Ellipsoid} or L{Ellipsoid2}). ''' return self._E @Property_RO def flattening(self): # Karney property '''Get the I{flattening} (C{float}), M{(a - b) / a}, positive for I{oblate}, negative for I{prolate} or C{0} for I{near-spherical}. ''' return self.ellipsoid.f f = flattening def _forward(self, lat, lon, h, name, M=False, _philam=False): # in .ltp.LocalCartesian.forward and -.reset '''(INTERNAL) Common for all C{Ecef*}. ''' E = self.ellipsoid if _philam: sa, ca, sb, cb = sincos2_(lat, lon) lat = Lat(degrees90( lat)) lon = Lon(degrees180(lon)) else: sa, ca, sb, cb = sincos2d_(lat, lon) n = E.roc1_(sa, ca) if self._isYou else E.roc1_(sa) z = (h + n * E.e21) * sa x = (h + n) * ca m = self._Matrix(sa, ca, sb, cb) if M else None return Ecef9Tuple(x * cb, x * sb, z, lat, lon, h, 0, m, self.datum, name=name or self.name) def forward(self, latlonh, lon=None, height=0, M=False, name=NN): '''Convert from geodetic C{(lat, lon, height)} to geocentric C{(x, y, z)}. @arg latlonh: Either a C{LatLon}, an L{Ecef9Tuple} or C{scalar} latitude (C{degrees}). @kwarg lon: Optional C{scalar} longitude for C{scalar} B{C{latlonh}} (C{degrees}). @kwarg height: Optional height (C{meter}), vertically above (or below) the surface of the ellipsoid. @kwarg M: Optionally, return the rotation L{EcefMatrix} (C{bool}). @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geocentric C{(x, y, z)} coordinates for the given geodetic ones C{(lat, lon, height)}, case C{C} 0, optional C{M} (L{EcefMatrix}) and C{datum} if available. @raise EcefError: If B{C{latlonh}} not C{LatLon}, L{Ecef9Tuple} or C{scalar} or B{C{lon}} not C{scalar} for C{scalar} B{C{latlonh}} or C{abs(lat)} exceeds 90°. @note: Use method C{.forward_} to specify C{lat} and C{lon} in C{radians} and avoid double angle conversions. ''' llhn = _llhn4(latlonh, lon, height, name=name) return _EcefBase._forward(self, *llhn, M=M) def forward_(self, phi, lam, height=0, M=False, name=NN): '''Like method C{.forward} except with geodetic lat- and longitude given in I{radians}. @arg phi: Latitude in I{radians} (C{scalar}). @arg lam: Longitude in I{radians} (C{scalar}). @kwarg height: Optional height (C{meter}), vertically above (or below) the surface of the ellipsoid. @kwarg M: Optionally, return the rotation L{EcefMatrix} (C{bool}). @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with C{lat} set to C{degrees90(B{phi})} and C{lon} to C{degrees180(B{lam})}. @raise EcefError: If B{C{phi}} or B{C{lam}} invalid or not C{scalar}. ''' try: # like function C{_llhn4} above plhn = Phi(phi), Lam(lam), Height(height), name except (TypeError, ValueError) as x: raise EcefError(phi=phi, lam=lam, height=height, cause=x) return self._forward(*plhn, M=M, _philam=True) @property_RO def _Geocentrics(self): '''(INTERNAL) Valid geocentric classes. ''' t = Ecef9Tuple, _MODS.cartesianBase.CartesianBase _EcefBase._Geocentrics = t # overwrite the property return t @Property_RO def _isYou(self): '''(INTERNAL) Is this an C{EcefYou}?. ''' return isinstance(self, EcefYou) def _Matrix(self, sa, ca, sb, cb): '''Creation a rotation matrix. @arg sa: C{sin(phi)} (C{float}). @arg ca: C{cos(phi)} (C{float}). @arg sb: C{sin(lambda)} (C{float}). @arg cb: C{cos(lambda)} (C{float}). @return: An L{EcefMatrix}. ''' return self._xnamed(EcefMatrix(sa, ca, sb, cb)) def reverse(self, xyz, y=None, z=None, M=False, name=NN): # PYCHOK no cover '''(INTERNAL) I{Must be overloaded}, see function C{notOverloaded}. ''' notOverloaded(self, xyz, y=y, z=z, M=M, name=name) def toStr(self, prec=9, **unused): # PYCHOK signature '''Return this C{Ecef*} as a string. @kwarg prec: Precision, number of decimal digits (0..9). @return: This C{Ecef*} representation (C{str}). ''' return self.attrs(_a_, _f_, _datum_, _name_, prec=prec) # _ellipsoid_ class EcefFarrell21(_EcefBase): '''Conversion between geodetic and geocentric, aka I{Earth-Centered, Earth-Fixed} (ECEF) coordinates based on I{Jay A. Farrell}'s U{Table 2.1<https://Books.Google.com/books?id=fW4foWASY6wC>}, page 29. ''' def reverse(self, xyz, y=None, z=None, M=None, name=NN): # PYCHOK unused M '''Convert from geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)} using I{Farrell}'s U{Table 2.1<https://Books.Google.com/books?id=fW4foWASY6wC>}, page 29. @arg xyz: A geocentric (C{Cartesian}, L{Ecef9Tuple}) or C{scalar} ECEF C{x} coordinate (C{meter}). @kwarg y: ECEF C{y} coordinate for C{scalar} B{C{xyz}} and B{C{z}} (C{meter}). @kwarg z: ECEF C{z} coordinate for C{scalar} B{C{xyz}} and B{C{y}} (C{meter}). @kwarg M: I{Ignored}, rotation matrix C{M} not available. @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geodetic coordinates C{(lat, lon, height)} for the given geocentric ones C{(x, y, z)}, case C{C=1}, C{M=None} always and C{datum} if available. @raise EcefError: Invalid B{C{xyz}} or C{scalar} C{x} or B{C{y}} and/or B{C{z}} not C{scalar} for C{scalar} B{C{xyz}} or C{sqrt} domain or zero division error. @see: L{EcefFarrell22} and L{EcefVeness}. ''' x, y, z, name = _xyzn4(xyz, y, z, self._Geocentrics, name=name) E = self.ellipsoid a = E.a a2 = E.a2 b2 = E.b2 e_ = E.a_b * E.e # 0.0820944... WGS84 e2 = E.e2 e4 = E.e4 try: # names as page 29 z2 = z**2 ez = (_1_0 - e2) * z2 # E.e2s2(z) p = hypot(x, y) p2 = p**2 G = p2 + ez - e2 * (a2 - b2) # p2 + ez - e4 * a2 F = b2 * z2 * 54 c = e4 * p2 * F / G**3 s = cbrt(_1_0 + c + sqrt(c**2 + c * 2)) P = F / (_3_0 * (fsum_(_1_0, s, _1_0 / s) * G)**2) Q = sqrt(_1_0 + _2_0 * e4 * P) Q1 = Q + _1_0 r0 = P * e2 * p / Q1 - sqrt(fsum_(a2 * (Q1 / Q) * _0_5, -P * ez / (Q * Q1), -P * p2 * _0_5)) r = p + e2 * r0 v = b2 / (a * sqrt(r**2 + ez)) h = hypot(r, z) * (_1_0 - v) t = atan2(z + e_**2 * v * z, p) # note, phi and lam are swapped on page 29 except (ValueError, ZeroDivisionError) as e: raise EcefError(x=x, y=y, z=z, cause=e) return Ecef9Tuple(x, y, z, degrees90(t), atan2d(y, x), h, 1, None, self.datum, name=name or self.name) class EcefFarrell22(_EcefBase): '''Conversion between geodetic and geocentric, aka I{Earth-Centered, Earth-Fixed} (ECEF) coordinates based on I{Jay A. Farrell}'s U{Table 2.2<https://Books.Google.com/books?id=fW4foWASY6wC>}, page 30. ''' def reverse(self, xyz, y=None, z=None, M=None, name=NN): # PYCHOK unused M '''Convert from geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)} using I{Farrell}'s U{Table 2.2<https://Books.Google.com/books?id=fW4foWASY6wC>}, page 30. @arg xyz: A geocentric (C{Cartesian}, L{Ecef9Tuple}) or C{scalar} ECEF C{x} coordinate (C{meter}). @kwarg y: ECEF C{y} coordinate for C{scalar} B{C{xyz}} and B{C{z}} (C{meter}). @kwarg z: ECEF C{z} coordinate for C{scalar} B{C{xyz}} and B{C{y}} (C{meter}). @kwarg M: I{Ignored}, rotation matrix C{M} not available. @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geodetic coordinates C{(lat, lon, height)} for the given geocentric ones C{(x, y, z)}, case C{C=1}, C{M=None} always and C{datum} if available. @raise EcefError: Invalid B{C{xyz}} or C{scalar} C{x} or B{C{y}} and/or B{C{z}} not C{scalar} for C{scalar} B{C{xyz}} or C{sqrt} domain or zero division error. @see: L{EcefFarrell21} and L{EcefVeness}. ''' x, y, z, name = _xyzn4(xyz, y, z, self._Geocentrics, name=name) E = self.ellipsoid a = E.a b = E.b try: # see EcefVeness.reverse p = hypot(x, y) s, c = sincos2(atan2(z * a, p * b)) t = atan2(z + E.e22 * b * s**3, p - E.e2 * a * c**3) s, c = sincos2(t) if c: # E.roc1_(s) = E.a / sqrt(1 - E.e2 * s**2) h = p / c - (E.roc1_(s) if s else a) else: # polar h = abs(z) - b # note, phi and lam are swapped on page 30 except (ValueError, ZeroDivisionError) as e: raise EcefError(x=x, y=y, z=z, cause=e) return Ecef9Tuple(x, y, z, degrees90(t), atan2d(y, x), h, 1, None, self.datum, name=name or self.name) class EcefKarney(_EcefBase): '''Conversion between geodetic and geocentric, aka I{Earth-Centered, Earth-Fixed} (ECEF) coordinates transcoded from I{Karney}'s C++ U{Geocentric <https://GeographicLib.SourceForge.io/C++/doc/classGeographicLib_1_1Geocentric.html>} methods. @note: On methods C{.forward} and C{.forwar_}, let C{v} be a unit vector located at C{(lat, lon, h)}. We can express C{v} as column vectors in one of two ways, C{v1} in east, north, up coordinates (where the components are relative to a local coordinate system at C{C(lat0, lon0, h0)}) or as C{v0} in geocentric C{x, y, z} coordinates. Then, M{v0 = M ⋅ v1} where C{M} is the rotation matrix. ''' @Property_RO def hmax(self): '''Get the distance or height limit (C{meter}, conventionally). ''' return self.equatoradius / EPS_2 # self.equatoradius * _2_EPS, 12M lighyears def reverse(self, xyz, y=None, z=None, M=False, name=NN): '''Convert from geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)}. @arg xyz: A geocentric (C{Cartesian}, L{Ecef9Tuple}) or C{scalar} ECEF C{x} coordinate (C{meter}). @kwarg y: ECEF C{y} coordinate for C{scalar} B{C{xyz}} and B{C{z}} (C{meter}). @kwarg z: ECEF C{z} coordinate for C{scalar} B{C{xyz}} and B{C{y}} (C{meter}). @kwarg M: Optionally, return the rotation L{EcefMatrix} (C{bool}). @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geodetic coordinates C{(lat, lon, height)} for the given geocentric ones C{(x, y, z)}, case C{C}, optional C{M} (L{EcefMatrix}) and C{datum} if available. @raise EcefError: Invalid B{C{xyz}} or C{scalar} C{x} or B{C{y}} and/or B{C{z}} not C{scalar} for C{scalar} B{C{xyz}}. @note: In general, there are multiple solutions and the result which minimizes C{height} is returned, i.e., C{(lat, lon)} corresponds to the closest point on the ellipsoid. If there are still multiple solutions with different latitudes (applies only if C{z} = 0), then the solution with C{lat} > 0 is returned. If there are still multiple solutions with different longitudes (applies only if C{x} = C{y} = 0) then C{lon} = 0 is returned. The returned C{height} value is not below M{−E.a * (1 − E.e2) / sqrt(1 − E.e2 * sin(lat)**2)}. The returned C{lon} is in the range [−180°, 180°]. Like C{forward} above, M{v1 = Transpose(M) ⋅ v0}. ''' def norm3(y, x): h = hypot(y, x) # EPS0, EPS_2 return (y / h, x / h, h) if h > 0 else (_0_0, _1_0, h) x, y, z, name = _xyzn4(xyz, y, z, self._Geocentrics, name=name) E = self.ellipsoid sb, cb, R = norm3(y, x) h = hypot(R, z) # distance to earth center if h > self.hmax: # PYCHOK no cover # We are really far away (> 12M light years). Treat the earth # as a point and h, above as an acceptable approximation to the # height. This avoids overflow, e.g., in the computation of disc # below. It's possible that h has overflowed to INF, that's OK. # Treat finite x, y, but R overflows to +INF by scaling by 2. sb, cb, R = norm3(y * _0_5, x * _0_5) sa, ca, _ = norm3(z * _0_5, R) C = 1 elif E.e4: # E.isEllipsoidal # Treat prolate spheroids by swapping R and Z here and by # switching the arguments to phi = atan2(...) at the end. p = (R / E.a)**2 q = E.e21 * (z / E.a)**2 if E.isProlate: p, q = q, p r = p + q - E.e4 e = E.e4 * q if e or r > 0: # Avoid possible division by zero when r = 0 by multiplying # equations for s and t by r^3 and r, respectively. s = e * p / _4_0 # s = r^3 * s u = r = r / _6_0 r2 = r**2 r3 = r * r2 t3 = s + r3 disc = s * (r3 + t3) if disc < 0: # t is complex, but the way u is defined, the result is real. # There are three possible cube roots. We choose the root # which avoids cancellation. Note, disc < 0 implies r < 0. u += _2_0 * r * cos(atan2(sqrt(-disc), -t3) / _3_0) else: # Pick the sign on the sqrt to maximize abs(T3). This # minimizes loss of precision due to cancellation. The # result is unchanged because of the way the t is used # in definition of u. if disc > 0: t3 += copysign0(sqrt(disc), t3) # t3 = (r * t)^3 # N.B. cbrt always returns the real root, cbrt(-8) = -2. t = cbrt(t3) # t = r * t # t can be zero; but then r2 / t -> 0. if t: u = fsum_(u, t, r2 / t) v = sqrt(e + u**2) # guaranteed positive # Avoid loss of accuracy when u < 0. Underflow doesn't occur in # E.e4 * q / (v - u) because u ~ e^4 when q is small and u < 0. uv = (e / (v - u)) if u < 0 else (u + v) # u+v, guaranteed positive # Need to guard against w going negative due to roundoff in uv - q. w = max(_0_0, E.e2abs * (uv - q) / (_2_0 * v)) # Rearrange expression for k to avoid loss of accuracy due to # subtraction. Division by 0 not possible because uv > 0, w >= 0. k1 = k2 = uv / (sqrt(uv + w**2) + w) if E.isProlate: k1 -= E.e2 else: k2 += E.e2 sa, ca, h = norm3(z / k1, R / k2) h *= k1 - E.e21 C = 2 else: # e = E.e4 * q == 0 and r <= 0 # This leads to k = 0 (oblate, equatorial plane) and k + E.e^2 = 0 # (prolate, rotation axis) and the generation of 0/0 in the general # formulas for phi and h, using the general formula and division # by 0 in formula for h. Handle this case by taking the limits: # f > 0: z -> 0, k -> E.e2 * sqrt(q) / sqrt(E.e4 - p) # f < 0: r -> 0, k + E.e2 -> -E.e2 * sqrt(q) / sqrt(E.e4 - p) q = E.e4 - p if E.isProlate: p, q = q, p e = E.a else: e = E.b2_a sa, ca, h = norm3(sqrt(q * E._1_e21), sqrt(p)) if z < 0: sa = neg(sa) # for tiny negative z, not for prolate h *= neg(e / E.e2abs) C = 3 else: # E.e4 == 0, spherical case # Dealing with underflow in the general case with E.e2 = 0 is # difficult. Origin maps to North pole, same as with ellipsoid. sa, ca, _ = norm3((z if h else _1_0), R) h -= E.a C = 4 m = self._Matrix(sa, ca, sb, cb) if M else None return Ecef9Tuple(x, y, z, atan2d(sa, ca), atan2d(sb, cb), h, C, m, self.datum, name=name or self.name) class EcefSudano(_EcefBase): '''Conversion between geodetic and geocentric, aka I{Earth-Centered, Earth-Fixed} (ECEF) coordinates based on I{John J. Sudano}'s U{paper <https://www.ResearchGate.net/publication/ 3709199_An_exact_conversion_from_an_Earth-centered_coordinate_system_to_latitude_longitude_and_altitude>}. ''' _tol = EPS2 @property_doc_(''' the convergence tolerance (C{float}).''') def tolerance(self): '''Get the convergence tolerance (C{float}). ''' return self._tol @tolerance.setter # PYCHOK setter! def tolerance(self, tol): '''Set the convergence tolerance (C{scalar}). @raise TypeError: Non-scalar B{C{tol}}. @raise ValueError: Out-of-bounds B{C{tol}}. ''' self._tol = Scalar_(tol, low=EPS, name=_tolerance_) def reverse(self, xyz, y=None, z=None, M=None, name=NN): # PYCHOK unused M '''Convert from geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)} using I{Sudano}'s U{iterative method<https://www.ResearchGate.net/publication/ 3709199_An_exact_conversion_from_an_Earth-centered_coordinate_system_to_latitude_longitude_and_altitude>}. @arg xyz: A geocentric (C{Cartesian}, L{Ecef9Tuple}) or C{scalar} ECEF C{x} coordinate (C{meter}). @kwarg y: ECEF C{y} coordinate for C{scalar} B{C{xyz}} and B{C{z}} (C{meter}). @kwarg z: ECEF C{z} coordinate for C{scalar} B{C{xyz}} and B{C{y}} (C{meter}). @kwarg M: I{Ignored}, rotation matrix C{M} not available. @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geodetic coordinates C{(lat, lon, height)} for the given geocentric ones C{(x, y, z)}, iteration C{C}, C{M=None} always and C{datum} if available. @raise EcefError: Invalid B{C{xyz}} or C{scalar} C{x} or B{C{y}} and/or B{C{z}} not C{scalar} for C{scalar} B{C{xyz}} or no convergence. ''' x, y, z, name = _xyzn4(xyz, y, z, self._Geocentrics, name=name) E = self.ellipsoid e = E.e2 * E.a h = hypot(x, y) # Rh d = e - h a = atan2(z, h * E.e21) sa, ca = sincos2(abs(a)) # Sudano's Eq (A-6) and (A-7) refactored/reduced, # replacing Rn from Eq (A-4) with n = E.a / ca: # N = ca**2 * ((z + E.e2 * n * sa) * ca - h * sa) # = ca**2 * (z * ca + E.e2 * E.a * sa - h * sa) # = ca**2 * (z * ca + (E.e2 * E.a - h) * sa) # D = ca**3 * (E.e2 * n / E.e2s2(sa)) - h # = ca**2 * (E.e2 * E.a / E.e2s2(sa) - h / ca**2) # N / D = (z * ca + (E.e2 * E.a - h) * sa) / # (E.e2 * E.a / E.e2s2(sa) - h / ca**2) tol = self.tolerance _S2_ = Fsum(sa).fsum2_ for C in range(1, _TRIPS): ca2 = _1_0 - sa**2 if ca2 < EPS_2: # PYCHOK no cover ca = _0_0 break ca = sqrt(ca2) r = e / E.e2s2(sa) - h / ca2 if abs(r) < EPS_2: break a = None sa, r = _S2_(-z * ca / r, -d * sa / r) if abs(r) < tol: break else: t = unstr(self.reverse.__name__, x=x, y=y, z=z) raise EcefError(Fmt.no_convergence(r, tol), txt=t) if a is None: a = copysign0(asin(sa), z) h = fsum_(h * ca, abs(z * sa), -E.a * E.e2s(sa)) # use Veness', # since Sudano's Eq (7) doesn't provide the correct height # h = (abs(z) + h - E.a * cos(a + E.e21) * sa / ca) / (ca + sa) r = Ecef9Tuple(x, y, z, degrees90(a), atan2d(y, x), h, C, None, self.datum, name=name or self.name) r._iteration = C return r class EcefVeness(_EcefBase): '''Conversion between geodetic and geocentric, aka I{Earth-Centered, Earth-Fixed} (ECEF) coordinates transcoded from I{Chris Veness}' JavaScript classes U{LatLonEllipsoidal, Cartesian <https://www.Movable-Type.co.UK/scripts/geodesy/docs/latlon-ellipsoidal.js.html>}. @see: U{A Guide to Coordinate Systems in Great Britain <https://www.OrdnanceSurvey.co.UK/documents/resources/guide-coordinate-systems-great-britain.pdf>}, section I{B) Converting between 3D Cartesian and ellipsoidal latitude, longitude and height coordinates}. ''' def reverse(self, xyz, y=None, z=None, M=None, name=NN): # PYCHOK unused M '''Convert from geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)} transcoded from I{Chris Veness}' U{JavaScript <https://www.Movable-Type.co.UK/scripts/geodesy/docs/latlon-ellipsoidal.js.html>}. Uses B. R. Bowring’s formulation for μm precision in concise form: U{'The accuracy of geodetic latitude and height equations' <https://www.ResearchGate.net/publication/ 233668213_The_Accuracy_of_Geodetic_Latitude_and_Height_Equations>}, Survey Review, Vol 28, 218, Oct 1985. @arg xyz: A geocentric (C{Cartesian}, L{Ecef9Tuple}) or C{scalar} ECEF C{x} coordinate (C{meter}). @kwarg y: ECEF C{y} coordinate for C{scalar} B{C{xyz}} and B{C{z}} (C{meter}). @kwarg z: ECEF C{z} coordinate for C{scalar} B{C{xyz}} and B{C{y}} (C{meter}). @kwarg M: I{Ignored}, rotation matrix C{M} not available. @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geodetic coordinates C{(lat, lon, height)} for the given geocentric ones C{(x, y, z)}, case C{C}, C{M=None} always and C{datum} if available. @raise EcefError: Invalid B{C{xyz}} or C{scalar} C{x} or B{C{y}} and/or B{C{z}} not C{scalar} for C{scalar} B{C{xyz}}. @see: Ralph M. Toms U{'An Efficient Algorithm for Geocentric to Geodetic Coordinate Conversion'<https://www.OSTI.gov/scitech/biblio/110235>}, Sept 1995 and U{'An Improved Algorithm for Geocentric to Geodetic Coordinate Conversion'<https://www.OSTI.gov/scitech/servlets/purl/231228>}, Apr 1996, both from Lawrence Livermore National Laboratory (LLNL) and John J. Sudano U{An exact conversion from an Earth-centered coordinate system to latitude longitude and altitude<https://www.ResearchGate.net/ publication/3709199_An_exact_conversion_from_an_Earth-centered_coordinate_system_to_latitude_longitude_and_altitude>}. ''' x, y, z, name = _xyzn4(xyz, y, z, self._Geocentrics, name=name) E = self.ellipsoid p = hypot(x, y) # distance from minor axis r = hypot(p, z) # polar radius if min(p, r) > EPS0: # parametric latitude (Bowring eqn 17, replaced) t = (E.b * z) / (E.a * p) * (_1_0 + E.e22 * E.b / r) c = _1_0 / hypot1(t) s = t * c # geodetic latitude (Bowring eqn 18) a = atan2(z + E.e22 * E.b * s**3, p - E.e2 * E.a * c**3) # height above ellipsoid (Bowring eqn 7) sa, ca = sincos2(a) # r = E.a / E.e2s(sa) # length of normal terminated by minor axis # h = p * ca + z * sa - (E.a * E.a / r) h = fsum_(p * ca, z * sa, -E.a * E.e2s(sa)) C, lat, lon = 1, degrees90(a), atan2d(y, x) # see <https://GIS.StackExchange.com/questions/28446> elif p > EPS: # lat arbitrarily zero C, lat, lon, h = 2, _0_0, atan2d(y, x), p - E.a else: # polar lat, lon arbitrarily zero C, lat, lon, h = 3, copysign0(_90_0, z), _0_0, abs(z) - E.b return Ecef9Tuple(x, y, z, lat, lon, h, C, None, # M=None self.datum, name=name or self.name) class EcefYou(_EcefBase): '''Conversion between geodetic and geocentric, aka I{Earth-Centered, Earth-Fixed} (ECEF) coordinates using I{Rey-Jer You}'s U{transformation <https://www.ResearchGate.net/publication/240359424>}. @see: W.E. Featherstone, S.J. (Sten) Claessens U{Closed-form transformation between geodetic and ellipsoidal coordinates <https://Espace.Curtin.edu.AU/bitstream/handle/20.500.11937/11589/115114_9021_geod2ellip_final.pdf>} Studia Geophysica et Geodaetica, 2008, 52, 1-18 and U{PyMap3D <https://PyPI.org/project/pymap3d>}. ''' def __init__(self, a_ellipsoid, f=None, name=NN): _EcefBase.__init__(self, a_ellipsoid, f=f, name=name) # inherited documentation E = self.ellipsoid if E.isProlate or (E.a2 - E.b2) < 0: raise EcefError(ellipsoid=E, txt=_prolate_) def reverse(self, xyz, y=None, z=None, M=None, name=NN): # PYCHOK unused M '''Convert geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)} using I{Rey-Jer You}'s transformation. @arg xyz: A geocentric (C{Cartesian}, L{Ecef9Tuple}) or C{scalar} ECEF C{x} coordinate (C{meter}). @kwarg y: ECEF C{y} coordinate for C{scalar} B{C{xyz}} and B{C{z}} (C{meter}). @kwarg z: ECEF C{z} coordinate for C{scalar} B{C{xyz}} and B{C{y}} (C{meter}). @kwarg M: I{Ignored}, rotation matrix C{M} not available. @kwarg name: Optional name (C{str}). @return: An L{Ecef9Tuple}C{(x, y, z, lat, lon, height, C, M, datum)} with geodetic coordinates C{(lat, lon, height)} for the given geocentric ones C{(x, y, z)}, case C{C=1}, C{M=None} always and C{datum} if available. @raise EcefError: Invalid B{C{xyz}} or C{scalar} C{x} or B{C{y}} and/or B{C{z}} not C{scalar} for C{scalar} B{C{xyz}}. ''' x, y, z, name = _xyzn4(xyz, y, z, self._Geocentrics, name=name) r2 = hypot2_(x, y, z) E = self.ellipsoid e2 = E.a2 - E.b2 # == E.e2 * E.a2 if e2 < 0: raise EcefError(ellipsoid=E, txt=_prolate_) e = sqrt(e2) # XXX sqrt0(e2)? q = hypot(x, y) u = fsum_(r2, -e2, hypot(r2 - e2, 2 * e * z)) * _0_5 if u > EPS02: u = sqrt(u) p = hypot(u, e) B = atan2(p * z, u * q) # beta0 = atan(p / u * z / q) sB, cB = sincos2(B) if cB and sB: p *= E.a d = (p / cB - e2 * cB) / sB if isnon0(d): B += fsum_(u * E.b, -p, e2) / d sB, cB = sincos2(B) elif u < 0: raise EcefError(x=x, y=y, z=z, txt=_singular_) else: sB, cB = copysign0(_1_0, z), _0_0 h = hypot(z - E.b * sB, q - E.a * cB) if hypot2_(x, y, z * E.a_b) < E.a2: h = neg(h) # inside ellipsoid return Ecef9Tuple(x, y, z, atan2d(E.a * sB, E.b * cB), # atan(E.a_b * tan(B)) atan2d(y, x), h, 1, None, # C=1, M=None self.datum, name=name or self.name) class EcefMatrix(_NamedTuple): '''A rotation matrix. ''' _Names_ = ('_0_0_', '_0_1_', '_0_2_', # row-order '_1_0_', '_1_1_', '_1_2_', '_2_0_', '_2_1_', '_2_2_') _Units_ = (Scalar,) * len(_Names_) def _validate(self, **_OK): # PYCHOK unused '''(INTERNAL) Allow C{_Names_} with leading underscore. ''' _NamedTuple._validate(self, _OK=True) def __new__(cls, sa, ca, sb, cb, *_more): '''New L{EcefMatrix} matrix. @arg sa: C{sin(phi)} (C{float}). @arg ca: C{cos(phi)} (C{float}). @arg sb: C{sin(lambda)} (C{float}). @arg cb: C{cos(lambda)} (C{float}). @arg _more: (INTERNAL) from C{.multiply}. @raise EcefError: If B{C{sa}}, B{C{ca}}, B{C{sb}} or B{C{cb}} outside M{[-1.0, +1.0]}. ''' t = sa, ca, sb, cb if _more: # all 9 matrix elements ... t += _more # ... from .multiply elif max(map(abs, t)) > _1_0: raise EcefError(unstr(EcefMatrix.__name__, *t)) else: # build matrix from the following quaternion operations # qrot(lam, [0,0,1]) * qrot(phi, [0,-1,0]) * [1,1,1,1]/2 # or # qrot(pi/2 + lam, [0,0,1]) * qrot(-pi/2 + phi, [-1,0,0]) # where # qrot(t,v) = [cos(t/2), sin(t/2)*v[1], sin(t/2)*v[2], sin(t/2)*v[3]] # Local X axis (east) in geocentric coords # M[0] = -slam; M[3] = clam; M[6] = 0; # Local Y axis (north) in geocentric coords # M[1] = -clam * sphi; M[4] = -slam * sphi; M[7] = cphi; # Local Z axis (up) in geocentric coords # M[2] = clam * cphi; M[5] = slam * cphi; M[8] = sphi; t = (-sb, -cb * sa, cb * ca, cb, -sb * sa, sb * ca, _0_0, ca, sa) return _NamedTuple.__new__(cls, *t) def column(self, column): '''Get matrix B{C{column}} as 3-tuple. ''' if 0 <= column < 3: return self[column::3] raise _IndexError(column=column) @Property_RO def _column_0(self): return self.column(0) @Property_RO def _column_1(self): return self.column(1) @Property_RO def _column_2(self): return self.column(2) def copy(self, **unused): # PYCHOK signature '''Make a shallow or deep copy of this instance. @return: The copy (C{This class} or subclass thereof). ''' return self.classof(*self) __copy__ = __deepcopy__ = copy def multiply(self, other): '''Matrix multiply M{M0' ⋅ M} this matrix transposed with an other matrix. @arg other: The other matrix (L{EcefMatrix}). @return: The matrix product (L{EcefMatrix}). @raise TypeError: If B{C{other}} is not L{EcefMatrix}. ''' _xinstanceof(EcefMatrix, other=other) # like LocalCartesian.MatrixMultiply, transposed(self) X other # <https://GeographicLib.SourceForge.io/C++/doc/LocalCartesian_8cpp_source.html> M = (fdot(self[r::3], *other[c::3]) for r in range(3) for c in range(3)) return _xnamed(EcefMatrix(*M), EcefMatrix.multiply.__name__) def rotate(self, xyz, *xyz0): '''Forward rotation M{M0' ⋅ ([x, y, z] - [x0, y0, z0])'}. @arg xyz: Local C{(x, y, z)} coordinates (C{3-tuple}). @arg xyz0: Optional, local C{(x0, y0, z0)} origin (C{3-tuple}). @return: Rotated C{(x, y, z)} location (C{3-tuple}). @raise LenError: Unequal C{len(B{xyz})} and C{len(B{xyz0})}. ''' if xyz0: if len(xyz0) != len(xyz): raise LenError(self.rotate, xyz0=len(xyz0), xyz=len(xyz)) xyz = tuple(c - c0 for c, c0 in zip(xyz, xyz0)) # x' = M[0] * x + M[3] * y + M[6] * z # y' = M[1] * x + M[4] * y + M[7] * z # z' = M[2] * x + M[5] * y + M[8] * z return (fdot(xyz, *self._column_0), fdot(xyz, *self._column_1), fdot(xyz, *self._column_2)) def row(self, row): '''Get matrix B{C{row}} as 3-tuple. ''' if 0 <= row < 3: r = row * 3 return self[r: r+3] raise _IndexError(row=row) @Property_RO def _row_0(self): return self.row(0) @Property_RO def _row_1(self): return self.row(1) @Property_RO def _row_2(self): return self.row(2) def unrotate(self, xyz, *xyz0): '''Inverse rotation M{[x0, y0, z0] + M0 ⋅ [x,y,z]'}. @arg xyz: Local C{(x, y, z)} coordinates (C{3-tuple}). @arg xyz0: Optional, local C{(x0, y0, z0)} origin (C{3-tuple}). @return: Unrotated C{(x, y, z)} location (C{3-tuple}). @raise LenError: Unequal C{len(B{xyz})} and C{len(B{xyz0})}. ''' if xyz0: if len(xyz0) != len(xyz): raise LenError(self.unrotate, xyz0=len(xyz0), xyz=len(xyz)) _xyz = _1_0_1T + xyz # x' = x0 + M[0] * x + M[1] * y + M[2] * z # y' = y0 + M[3] * x + M[4] * y + M[5] * z # z' = z0 + M[6] * x + M[7] * y + M[8] * z xyz_ = (fdot(_xyz, xyz0[0], *self._row_0), fdot(_xyz, xyz0[1], *self._row_1), fdot(_xyz, xyz0[2], *self._row_2)) else: # x' = M[0] * x + M[1] * y + M[2] * z # y' = M[3] * x + M[4] * y + M[5] * z # z' = M[6] * x + M[7] * y + M[8] * z xyz_ = (fdot(xyz, *self._row_0), fdot(xyz, *self._row_1), fdot(xyz, *self._row_2)) return xyz_ class Ecef9Tuple(_NamedTuple): '''9-Tuple C{(x, y, z, lat, lon, height, C, M, datum)} with I{geocentric} C{x}, C{y} and C{z} plus I{geodetic} C{lat}, C{lon} and C{height}, case C{C} (see the C{Ecef*.reverse} methods) and optionally, the rotation matrix C{M} (L{EcefMatrix}) and C{datum}, with C{lat} and C{lon} in C{degrees} and C{x}, C{y}, C{z} and C{height} in C{meter}, conventionally. ''' _Names_ = (_x_, _y_, _z_, _lat_, _lon_, _height_, _C_, _M_, _datum_) _Units_ = ( Meter, Meter, Meter, Lat, Lon, Height, Int, _Pass, _Pass) _IndexM = _Names_.index(_M_) # for ._M_x_M @property_RO def _CartesianBase(self): '''(INTERNAL) Get/cache class C{CartesianBase}. ''' Ecef9Tuple._CartesianBase = C = _MODS.cartesianBase.CartesianBase # overwrite property return C @deprecated_method def convertDatum(self, datum2): # for backward compatibility '''DEPRECATED, use method L{toDatum}.''' return self.toDatum(datum2) @Property_RO def lam(self): '''Get the longitude in C{radians} (C{float}). ''' return self.philam.lam @Property_RO def lamVermeille(self): '''Get the longitude in C{radians [-PI*3/2..+PI*3/2]} after U{Vermeille <https://Search.ProQuest.com/docview/639493848>} (2004), p 95. @see: U{Karney<https://GeographicLib.SourceForge.io/C++/doc/geocentric.html>}, U{Vermeille<https://Search.ProQuest.com/docview/847292978>} 2011, pp 112-113, 116 and U{Featherstone, et.al.<https://Search.ProQuest.com/docview/872827242>}, p 7. ''' x, y = self.x, self.y if y > EPS0: r = _N_2_0 * atan2(x, hypot(y, x) + y) + PI_2 elif y < -EPS0: r = _2_0 * atan2(x, hypot(y, x) - y) - PI_2 else: # y == 0 r = PI if x < 0 else _0_0 return Lam(Vermeille=r) @Property_RO def latlon(self): '''Get the lat-, longitude in C{degrees} (L{LatLon2Tuple}C{(lat, lon)}). ''' return LatLon2Tuple(self.lat, self.lon, name=self.name) @Property_RO def latlonheight(self): '''Get the lat-, longitude in C{degrees} and height (L{LatLon3Tuple}C{(lat, lon, height)}). ''' return self.latlon.to3Tuple(self.height) @Property_RO def latlonheightdatum(self): '''Get the lat-, longitude in C{degrees} with height and datum (L{LatLon4Tuple}C{(lat, lon, height, datum)}). ''' return self.latlonheight.to4Tuple(self.datum) @Property_RO def latlonVermeille(self): '''Get the latitude and I{Vermeille} longitude in C{degrees [-225..+225]} (L{LatLon2Tuple}C{(lat, lon)}). @see: Property C{lonVermeille}. ''' return LatLon2Tuple(self.lat, self.lonVermeille, name=self.name) @Property_RO def lonVermeille(self): '''Get the longitude in C{degrees [-225..+225]} after U{Vermeille <https://Search.ProQuest.com/docview/639493848>} (2004), p 95. @see: Property C{lamVermeille}. ''' return Lon(Vermeille=degrees(self.lamVermeille)) def _T_x_M(self, T): '''(INTERNAL) Update M{self.M = T.multiply(self.M)}. ''' t = list(self) M = self._IndexM t[M] = T.multiply(t[M]) return self.classof(*t) @Property_RO def phi(self): '''Get the latitude in C{radians} (C{float}). ''' return self.philam.phi @Property_RO def philam(self): '''Get the lat-, longitude in C{radians} (L{PhiLam2Tuple}C{(phi, lam)}). ''' return PhiLam2Tuple(radians(self.lat), radians(self.lon), name=self.name) @Property_RO def philamheight(self): '''Get the lat-, longitude in C{radians} and height (L{PhiLam3Tuple}C{(phi, lam, height)}). ''' return self.philam.to3Tuple(self.height) @Property_RO def philamheightdatum(self): '''Get the lat-, longitude in C{radians} with height and datum (L{PhiLam4Tuple}C{(phi, lam, height, datum)}). ''' return self.philamheight.to4Tuple(self.datum) @Property_RO def philamVermeille(self): '''Get the latitude and I{Vermeille} longitude in C{radians [-PI*3/2..+PI*3/2]} (L{PhiLam2Tuple}C{(phi, lam)}). @see: Property C{lamVermeille}. ''' return PhiLam2Tuple(radians(self.lat), self.lamVermeille, name=self.name) def toCartesian(self, Cartesian=None, **Cartesian_kwds): '''Return the geocentric C{(x, y, z)} coordinates as an ellipsoidal or spherical C{Cartesian}. @kwarg Cartesian: Optional class to return C{(x, y, z)} (L{ellipsoidalKarney.Cartesian}, L{ellipsoidalNvector.Cartesian}, L{ellipsoidalVincenty.Cartesian}, L{sphericalNvector.Cartesian} or L{sphericalTrigonometry.Cartesian}) or C{None}. @kwarg Cartesian_kwds: Optional, additional B{C{Cartesian}} keyword arguments, ignored if C{B{Cartesian} is None}. @return: A C{B{Cartesian}(x, y, z, **B{Cartesian_kwds})} instance or a L{Vector4Tuple}C{(x, y, z, h)} if C{B{Cartesian} is None}. @raise TypeError: Invalid B{C{Cartesian}} or B{C{Cartesian_kwds}}. ''' if Cartesian in (None, Vector4Tuple): r = self.xyzh elif Cartesian is Vector3Tuple: r = self.xyz else: _xsubclassof(self._CartesianBase, Cartesian=Cartesian) r = Cartesian(self, **_xkwds(Cartesian_kwds, name=self.name)) return r def toDatum(self, datum2): '''Convert this C{Ecef9Tuple} to an other datum. @arg datum2: Datum to convert I{to} (L{Datum}). @return: The converted 9-Tuple (C{Ecef9Tuple}). @raise TypeError: The B{C{datum2}} is not a L{Datum}. ''' if self.datum in (None, datum2): # PYCHOK _Names_ r = self.copy() else: c = self._CartesianBase(self, datum=self.datum, name=self.name) # PYCHOK _Names_ # c.toLatLon converts datum, x, y, z, lat, lon, etc. # and returns another Ecef9Tuple iff LatLon is None r = c.toLatLon(datum=datum2, LatLon=None) return r def toLatLon(self, LatLon=None, **LatLon_kwds): '''Return the geodetic C{(lat, lon, height[, datum])} coordinates. @kwarg LatLon: Optional class to return C{(lat, lon, height[, datum])} or C{None}. @kwarg LatLon_kwds: Optional B{C{height}}, B{C{datum}} and other B{C{LatLon}} keyword arguments. @return: An instance of C{B{LatLon}(lat, lon, **B{LatLon_kwds})} or if B{C{LatLon}} is C{None}, a L{LatLon3Tuple}C{(lat, lon, height)} respectively L{LatLon4Tuple}C{(lat, lon, height, datum)} depending on whether C{datum} is un-/specified. @raise TypeError: Invalid B{C{LatLon}} or B{C{LatLon_kwds}}. ''' kwds = _xkwds(LatLon_kwds, height=self.height, datum=self.datum, name=self.name) # PYCHOK Ecef9Tuple d = kwds[_datum_] if LatLon is None: r = LatLon3Tuple(self.lat, self.lon, kwds[_height_], name=kwds[_name_]) # PYCHOK Ecef9Tuple if d: r = r.to4Tuple(d) # checks type(d) else: if d is None: # remove None datum _ = kwds.pop[_datum_] r = LatLon(self.lat, self.lon, **kwds) # PYCHOK Ecef9Tuple _xdatum(getattr(r, _datum_, self.datum), self.datum) # PYCHOK Ecef9Tuple return r def toLocal(self, ltp, Xyz=None, **Xyz_kwds): '''Convert this geocentric to I{local} C{x}, C{y} and C{z}. @kwarg ltp: The I{local tangent plane} (LTP) to use (L{Ltp}). @kwarg Xyz: Optional class to return C{x}, C{y} and C{z} (L{XyzLocal}, L{Enu}, L{Ned}) or C{None}. @kwarg Xyz_kwds: Optional, additional B{C{Xyz}} keyword arguments, ignored if C{B{Xyz} is None}. @return: An B{C{Xyz}} instance or if C{B{Xyz} is None}, a L{Local9Tuple}C{(x, y, z, lat, lon, height, ltp, ecef, M)} with C{M=None}, always. @raise TypeError: Invalid B{C{ltp}}. ''' return _MODS.ltp._xLtp(ltp)._ecef2local(self, Xyz, Xyz_kwds) def toVector(self, Vector=None, **Vector_kwds): '''Return the geocentric C{(x, y, z)} coordinates as vector. @kwarg Vector: Optional vector class to return C{(x, y, z)} or C{None}. @kwarg Vector_kwds: Optional, additional B{C{Vector}} keyword arguments, ignored if C{B{Vector} is None}. @return: A C{Vector}C{(x, y, z, **Vector_kwds)} instance or a L{Vector3Tuple}C{(x, y, z)} if B{C{Vector}} is C{None}. @see: Propertes C{xyz} and C{xyzh} ''' return self.xyz if Vector is None else self._xnamed( Vector(self.x, self.y, self.z, **Vector_kwds)) # PYCHOK Ecef9Tuple @Property_RO def xyz(self): '''Get the geocentric C{(x, y, z)} coordinates (L{Vector3Tuple}C{(x, y, z)}). ''' return Vector3Tuple(self.x, self.y, self.z, name=self.name) @Property_RO def xyzh(self): '''Get the geocentric C{(x, y, z)} coordinates and C{height} (L{Vector4Tuple}C{(x, y, z, h)}) ''' return self.xyz.to4Tuple(self.height) def _4Ecef(this, Ecef): # in .datums.Datum.ecef, .ellipsoids.Ellipsoid.ecef '''Return an ECEF converter for C{this} L{Datum} or L{Ellipsoid}. ''' if Ecef is None: Ecef = EcefKarney else: _xinstanceof(*_Ecefs, Ecef=Ecef) return Ecef(this, name=this.name) def _xEcef(Ecef): # PYCHOK .latlonBase.py '''(INTERNAL) Validate B{C{Ecef}} I{class}. ''' if issubclassof(Ecef, _EcefBase): return Ecef raise _TypesError(_Ecef_, Ecef, *_Ecefs) _Ecefs = (EcefKarney, EcefSudano, EcefVeness, EcefYou, EcefFarrell21, EcefFarrell22) __all__ += _ALL_DOCS(_EcefBase) # **) MIT License # # Copyright (C) 2016-2022 -- mrJean1 at Gmail -- All Rights Reserved. # # Permission is hereby granted, free of charge, to any person obtaining a # copy of this software and associated documentation files (the "Software"), # to deal in the Software without restriction, including without limitation # the rights to use, copy, modify, merge, publish, distribute, sublicense, # and/or sell copies of the Software, and to permit persons to whom the # Software is furnished to do so, subject to the following conditions: # # The above copyright notice and this permission notice shall be included # in all copies or substantial portions of the Software. # # THE SOFTWARE IS PROVIDED "AS IS", WITHOUT WARRANTY OF ANY KIND, EXPRESS # OR IMPLIED, INCLUDING BUT NOT LIMITED TO THE WARRANTIES OF MERCHANTABILITY, # FITNESS FOR A PARTICULAR PURPOSE AND NONINFRINGEMENT. IN NO EVENT SHALL # THE AUTHORS OR COPYRIGHT HOLDERS BE LIABLE FOR ANY CLAIM, DAMAGES OR # OTHER LIABILITY, WHETHER IN AN ACTION OF CONTRACT, TORT OR OTHERWISE, # ARISING FROM, OUT OF OR IN CONNECTION WITH THE SOFTWARE OR THE USE OR # OTHER DEALINGS IN THE SOFTWARE.