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etm.py
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etm.py
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# -*- coding: utf-8 -*-
u'''Classes L{ETMError} and L{Etm}, a pure Python implementation of
I{Charles Karney's} C++ class U{TransverseMercatorExact
<https://GeographicLib.SourceForge.io/html/classGeographicLib_1_1TransverseMercatorExact.html>},
abbreviated as C{TMExact} below.
Python class L{ExactTransverseMercator} implements the C{Exact Transverse
Mercator} (ETM) projection. Instances of class L{Etm} represent ETM
C{easting, nothing} locations.
Following is a copy of Karney's U{TransverseMercatorExact.hpp
<https://GeographicLib.SourceForge.io/html/TransverseMercatorExact_8hpp_source.html>}
file C{Header}.
Copyright (C) U{Charles Karney<mailto:Charles@Karney.com>} (2008-2017)
and licensed under the MIT/X11 License. For more information, see the
U{GeographicLib<https://GeographicLib.SourceForge.io>} documentation.
The method entails using the C{Thompson Transverse Mercator} as an
intermediate projection. The projections from the intermediate
coordinates to C{phi, lam} and C{x, y} are given by elliptic functions.
The inverse of these projections are found by Newton's method with a
suitable starting guess.
The relevant section of L.P. Lee's paper U{Conformal Projections Based On
Jacobian Elliptic Functions<https://DOI.org/10.3138/X687-1574-4325-WM62>}
is part V, pp 67--101. The C++ implementation and notation closely
follow Lee, with the following exceptions::
Lee here Description
x/a xi Northing (unit Earth)
y/a eta Easting (unit Earth)
s/a sigma xi + i * eta
y x Easting
x y Northing
k e Eccentricity
k^2 mu Elliptic function parameter
k'^2 mv Elliptic function complementary parameter
m k Scale
zeta zeta Complex longitude = Mercator = chi in paper
s sigma Complex GK = zeta in paper
Minor alterations have been made in some of Lee's expressions in an
attempt to control round-off. For example, C{atanh(sin(phi))} is
replaced by C{asinh(tan(phi))} which maintains accuracy near
C{phi = pi/2}. Such changes are noted in the code.
'''
# make sure int/int division yields float quotient
from __future__ import division
division = 1 / 2 # double check int division, see .datum.py, .utily.py
if not division:
raise ImportError('%s 1/2 == %d' % ('division', division))
del division
from pygeodesy.basics import EPS, PI_2, PI_4, property_doc_, \
property_RO, _xinstanceof
from pygeodesy.datum import Datum, Datums
from pygeodesy.elliptic import Elliptic, EllipticError, _TRIPS
from pygeodesy.errors import _incompatible
from pygeodesy.fmath import cbrt, Fsum, fsum_, hypot, hypot1, hypot2
from pygeodesy.interns import _COMMA_SPACE_, _convergence_, _easting_, \
_k0_, _lat_, _lon_, _lon0_, NN, _northing_, \
_no_convergence_, _scale_ # PYCHOK used!
from pygeodesy.karney import _diff182, _fix90, _norm180
from pygeodesy.lazily import _ALL_DOCS, _ALL_LAZY
from pygeodesy.named import _NamedBase, _NamedTuple, _xnamed
from pygeodesy.streprs import pairs, unstr
from pygeodesy.units import Lon, Scalar_
from pygeodesy.utily import sincos2
from pygeodesy.utm import _cmlon, _K0, _parseUTM5, Utm, UTMError, \
_toXtm8, _to7zBlldfn
from pygeodesy.utmupsBase import _LLEB
from math import asinh, atan, atan2, copysign, degrees, radians, \
sinh, sqrt, tan
__all__ = _ALL_LAZY.etm
__version__ = '20.07.17'
_OVERFLOW = 1.0 / EPS**2
_TOL = EPS
_TOL_10 = 0.1 * _TOL
_TAYTOL = pow(_TOL, 0.6)
_TAYTOL2 = 2.0 * _TAYTOL
class EasNorExact4Tuple(_NamedTuple):
'''4-Tuple C{(easting, northing, convergence, scale)} in
C{meter}, C{meter}, C{degrees} and C{scalar}.
'''
_Names_ = (_easting_, _northing_, _convergence_, _scale_)
class ETMError(UTMError):
'''Exact Transverse Mercator (ETM) parse, projection or other L{Etm} issue.
'''
pass
class Etm(Utm):
'''Exact Transverse Mercator (ETM) coordinate, a sub-class of
L{Utm}, a Universal Transverse Mercator (UTM) coordinate
using the L{ExactTransverseMercator} projection for highest
accuracy.
@note: Conversion of L{Etm} coordinates to and from (geodetic)
lat- and longitude is 3-4 times slower than L{Utm}.
@see: Karney's U{Detailed Description<https://GeographicLib.SourceForge.io/
html/classGeographicLib_1_1TransverseMercatorExact.html#details>}.
'''
_Error = ETMError
_exactTM = None
def __init__(self, zone, hemisphere, easting, northing, band=NN, # PYCHOK expected
datum=Datums.WGS84, falsed=True,
convergence=None, scale=None, name=NN):
'''New L{Etm} coordinate.
@arg zone: Longitudinal UTM zone (C{int}, 1..60) or zone
with/-out (latitudinal) Band letter (C{str},
'01C'..'60X').
@arg hemisphere: Northern or southern hemisphere (C{str},
C{'N[orth]'} or C{'S[outh]'}).
@arg easting: Easting, see B{C{falsed}} (C{meter}).
@arg northing: Northing, see B{C{falsed}} (C{meter}).
@kwarg band: Optional, (latitudinal) band (C{str}, 'C'..'X').
@kwarg datum: Optional, this coordinate's datum (L{Datum}).
@kwarg falsed: Both B{C{easting}} and B{C{northing}} are
falsed (C{bool}).
@kwarg convergence: Optional meridian convergence, bearing
off grid North, clockwise from true North
(C{degrees}) or C{None}.
@kwarg scale: Optional grid scale factor (C{scalar}) or C{None}.
@kwarg name: Optional name (C{str}).
@raise ETMError: Invalid B{C{zone}}, B{C{hemishere}} or
B{C{band}}.
@example:
>>> import pygeodesy
>>> u = pygeodesy.Etm(31, 'N', 448251, 5411932)
'''
Utm.__init__(self, zone, hemisphere, easting, northing,
band=band, datum=datum, falsed=falsed,
convergence=convergence, scale=scale,
name=name)
self.exactTM = self.datum.exactTM # ExactTransverseMercator(datum=self.datum)
@property_doc_(''' the ETM projection (L{ExactTransverseMercator}).''')
def exactTM(self):
'''Get the ETM projection (L{ExactTransverseMercator}).
'''
return self._exactTM
@exactTM.setter # PYCHOK setter!
def exactTM(self, exactTM):
'''Set the ETM projection (L{ExactTransverseMercator}).
'''
_xinstanceof(ExactTransverseMercator, exactTM=exactTM)
E = self.datum.ellipsoid
if exactTM._E != E or exactTM.majoradius != E.a \
or exactTM.flattening != E.f:
raise ETMError(repr(exactTM), txt=_incompatible(repr(E)))
self._exactTM = exactTM
self._scale0 = exactTM.k0
def parseETM(self, strETM):
'''Parse a string to a ETM coordinate.
@return: The coordinate (L{Etm}).
@see: Function L{parseETM5} in this module L{etm}.
'''
return parseETM5(strETM, datum=self.datum, Etm=self.classof)
def toLatLon(self, LatLon=None, unfalse=True, **unused): # PYCHOK expected
'''Convert this ETM coordinate to an (ellipsoidal) geodetic point.
@kwarg LatLon: Optional, ellipsoidal class to return the
geodetic point (C{LatLon}) or C{None}.
@kwarg unfalse: Unfalse B{C{easting}} and B{C{northing}} if
falsed (C{bool}).
@return: This ETM coordinate as (B{C{LatLon}}) or a
L{LatLonDatum5Tuple}C{(lat, lon, datum,
convergence, scale)} if B{C{LatLon}} is C{None}.
@raise EllipticError: No convergence.
@raise TypeError: If B{C{LatLon}} is not ellipsoidal.
@example:
>>> from pygeodesy import ellipsoidalVincenty as eV, Etm
>>> u = Etm(31, 'N', 448251.795, 5411932.678)
>>> ll = u.toLatLon(eV.LatLon) # 48°51′29.52″N, 002°17′40.20″E
'''
xTM, d = self.exactTM, self.datum
# double check that this and exactTM's ellipsoids stil match
if xTM._E != d.ellipsoid:
t = repr(d.ellipsoid)
raise ETMError(repr(xTM._E), txt=_incompatible(t))
if self._latlon and self._latlon_args == (xTM, unfalse):
return self._latlon5(LatLon)
f = not unfalse
e, n = self.to2en(falsed=f)
# f = unfalse == self.falsed
# == unfalse and self.falsed or (not unfalse and not self.falsed)
# == unfalse if self.falsed else not unfalse
# == unfalse if self.falsed else f
if self.falsed:
f = unfalse
lon0 = _cmlon(self.zone) if f else None
lat, lon, g, k = xTM.reverse(e, n, lon0=lon0)
ll = _LLEB(lat, lon, datum=d, name=self.name)
ll._convergence = g
ll._scale = k
self._latlon_to(ll, xTM, unfalse)
return self._latlon5(LatLon)
def _latlon_to(self, ll, xTM, unfalse):
'''(INTERNAL) See C{.toLatLon}, C{toEtm8}, C{_toXtm8}.
'''
self._latlon, self._latlon_args = ll, (xTM, unfalse)
def toUtm(self): # PYCHOK signature
'''Coopy this ETM to a UTM coordinate.
@return: The UTM coordinate (L{Utm}).
'''
return self._xnamed(self._xcopy2(Utm))
class ExactTransverseMercator(_NamedBase):
'''A Python version of Karney's U{TransverseMercatorExact
<https://GeographicLib.SourceForge.io/html/TransverseMercatorExact_8cpp_source.html>}
C++ class, a numerically exact transverse mercator projection,
referred to as C{TMExact} here.
@see: C{TMExact(real a, real f, real k0, bool extendp)}.
'''
_a = 0 # major radius
_datum = None # Datum
_e = 0 # eccentricity
_E = None # Ellipsoid
_extendp = True
_f = 0 # flattening
_k0 = 1 # central scale factor
_k0_a = 0
_lon0 = 0 # central meridian
_trips_ = _TRIPS
# see ._reset() below:
# _e_PI_2 = _e * PI_2
# _e_PI_4 = _e * PI_4
# _e_TAYTOL = _e * _TAYTOL
# _1_e_90 = (1 - _e) * 90
# _1_e_PI_2 = (1 - _e) * PI_2
# _1_e2_PI_2 = (1 - _e * 2) * PI_2
# _mu = _e**2
# _mu_2_1 = (_e**2 + 2) * 0.5
# _Eu = Elliptic(_mu)
# _Eu_cE_1_4 = _Eu.cE * 0.25
# _Eu_cK_cE = _Eu.cK / _Eu.cE
# _Eu_cK_PI_2 = _Eu.cK / PI_2
# _mv = 1 - _mu
# _3_mv = 3.0 / _mv
# _3_mv_e = _3_mv / _e
# _Ev = Elliptic(_mv)
# _Ev_cKE_3_4 = _Ev.cKE * 0.75
# _Ev_cKE_5_4 = _Ev.cKE * 1.25
def __init__(self, datum=Datums.WGS84, lon0=0, k0=_K0, extendp=True, name=NN):
'''New L{ExactTransverseMercator} projection.
@kwarg datum: The datum and ellipsoid to use (C{Datum}).
@kwarg lon0: The central meridian (C{degrees180}).
@kwarg k0: The central scale factor (C{float}).
@kwarg extendp: Use the extended domain (C{bool}).
@kwarg name: Optional name for the projection (C{str}).
@raise EllipticError: No convergence.
@raise ETMError: Invalid B{C{k0}}.
@raise TypeError: Invalid B{C{datum}}.
@raise ValueError: Invalid B{C{lon0}} or B{C{k0}}.
@note: The maximum error for all 255.5K U{TMcoords.dat
<https://Zenodo.org/record/32470>} tests (with
C{0 <= lat <= 84} and C{0 <= lon}) is C{5.2e-08
.forward} or 52 nano-meter easting and northing
and C{3.8e-13 .reverse} or 0.38 pico-degrees lat-
and longitude (with Python 3.7.3, 2.7.16, PyPy6
3.5.3 and PyPy6 2.7.13, all in 64-bit on macOS
10.13.6 High Sierra).
'''
if not extendp:
self._extendp = False
if name:
self.name = name
self.datum = datum
self.lon0 = lon0
self.k0 = k0
@property_doc_(''' the datum (L{Datum}).''')
def datum(self):
'''Get the datum (L{Datum}) or C{None}.
'''
return self._datum
@datum.setter # PYCHOK setter!
def datum(self, datum):
'''Set the datum and ellipsoid (L{Datum}).
@raise EllipticError: No convergence.
@raise TypeError: Invalid B{C{datum}}.
'''
_xinstanceof(Datum, datum=datum)
E = datum.ellipsoid
self._reset(E.e, E.e2)
self._a = E.a
self._f = E.f # flattening = (a - b) / a
self._datum = datum
self._E = E
@property_RO
def equatoradius(self):
'''Get the equatorial (major) radius, semi-axis (C{meter}).
'''
return self._a
majoradius = equatoradius # for backward compatibility
@property_RO
def extendp(self):
'''Get using the extended domain (C{bool}).
'''
return self._extendp
@property_RO
def flattening(self):
'''Get the flattening (C{float}).
'''
return self._f
def forward(self, lat, lon, lon0=None): # MCCABE 13
'''Forward projection, from geographic to transverse Mercator.
@arg lat: Latitude of point (C{degrees}).
@arg lon: Longitude of point (C{degrees}).
@kwarg lon0: Central meridian of the projection (C{degrees}).
@return: L{EasNorExact4Tuple}C{(easting, northing,
convergence, scale)} in C{meter}, C{meter},
C{degrees} and C{scalar}.
@see: C{void TMExact::Forward(real lon0, real lat, real lon,
real &x, real &y,
real &gamma, real &k)}.
@raise EllipticError: No convergence.
'''
lat = _fix90(lat)
lon, _ = _diff182((self._lon0 if lon0 is None else lon0), lon)
# Explicitly enforce the parity
backside = _lat = _lon = False
if not self.extendp:
if lat < 0:
_lat, lat = True, -lat
if lon < 0:
_lon, lon = True, -lon
if lon > 90:
backside = True
if lat == 0:
_lat = True
lon = 180 - lon
# u,v = coordinates for the Thompson TM, Lee 54
if lat == 90:
u, v = self._Eu.cK, 0
elif lat == 0 and lon == self._1_e_90:
u, v = 0, self._Ev.cK
else: # tau = tan(phi), taup = sinh(psi)
tau, lam = tan(radians(lat)), radians(lon)
u, v = self._zetaInv(self._E.es_taupf(tau), lam)
sncndn6 = self._sncndn6(u, v)
xi, eta, _ = self._sigma3(v, *sncndn6)
if backside:
xi = 2 * self._Eu.cE - xi
y = xi * self._k0_a
x = eta * self._k0_a
if lat == 90:
g, k = lon, self._k0
else:
g, k = self._zetaScaled(sncndn6, ll=False)
if backside:
g = 180 - g
if _lat:
y, g = -y, -g
if _lon:
x, g = -x, -g
return EasNorExact4Tuple(x, y, g, k)
@property_doc_(''' the central scale factor (C{float}).''')
def k0(self):
'''Get the central scale factor (C{float}), aka I{C{scale0}}.
'''
return self._k0 # aka scale0
@k0.setter # PYCHOK setter!
def k0(self, k0):
'''Set the central scale factor (C{float}), aka I{C{scale0}}.
@raise ETMError: Invalid B{C{k0}}.
'''
self._k0 = Scalar_(k0, name=_k0_, Error=ETMError, low=_TOL_10, high=1.0)
# if not self._k0 > 0:
# raise Scalar_.Error_(Scalar_, k0, name=_k0_, Error=ETMError)
self._k0_a = self._k0 * self._a
@property_doc_(''' the central meridian (C{degrees180}).''')
def lon0(self):
'''Get the central meridian (C{degrees180}).
'''
return self._lon0
@lon0.setter # PYCHOK setter!
def lon0(self, lon0):
'''Set the central meridian (C{degrees180}).
@raise ValueError: Invalid B{C{lon0}}.
'''
self._lon0 = _norm180(Lon(lon0, name=_lon0_))
def _reset(self, e, e2):
'''(INTERNAL) Get elliptic functions and pre-compute some
frequently used values.
@arg e: Eccentricity (C{float}).
@arg e2: Eccentricity squared (C{float}).
@raise EllipticError: No convergence.
'''
# assert e2 == e**2
self._e = e
self._e_PI_2 = e * PI_2
self._e_PI_4 = e * PI_4
self._e_TAYTOL = e * _TAYTOL
self._1_e_90 = (1 - e) * 90
self._1_e_PI_2 = (1 - e) * PI_2
self._1_e2_PI_2 = (1 - e * 2) * PI_2
self._mu = e2
self._mu_2_1 = (e2 + 2) * 0.5
self._Eu = Elliptic(self._mu)
self._Eu_cE_1_4 = self._Eu.cE * 0.25
self._Eu_cK_cE = self._Eu.cK / self._Eu.cE
self._Eu_cK_PI_2 = self._Eu.cK / PI_2
self._mv = 1 - e2
self._3_mv = 3.0 / self._mv
self._3_mv_e = self._3_mv / e
self._Ev = Elliptic(self._mv)
self._Ev_cKE_3_4 = self._Ev.cKE * 0.75
self._Ev_cKE_5_4 = self._Ev.cKE * 1.25
def reverse(self, x, y, lon0=None):
'''Reverse projection, from Transverse Mercator to geographic.
@arg x: Easting of point (C{meters}).
@arg y: Northing of point (C{meters}).
@kwarg lon0: Central meridian of the projection (C{degrees}).
@return: L{LatLonExact4Tuple}C{(lat, lon, convergence, scale)}
in C{degrees}, C{degrees180}, C{degrees} and C{scalar}.
@see: C{void TMExact::Reverse(real lon0, real x, real y,
real &lat, real &lon,
real &gamma, real &k)}
@raise EllipticError: No convergence.
'''
# undoes the steps in .forward.
xi = y / self._k0_a
eta = x / self._k0_a
backside = _lat = _lon = False
if not self.extendp: # enforce the parity
if y < 0:
_lat, xi = True, -xi
if x < 0:
_lon, eta = True, -eta
if xi > self._Eu.cE:
xi = 2 * self._Eu.cE - xi
backside = True
# u,v = coordinates for the Thompson TM, Lee 54
if xi != 0 or eta != self._Ev.cKE:
u, v = self._sigmaInv(xi, eta)
else:
u, v = 0, self._Ev.cK
if v != 0 or u != self._Eu.cK:
g, k, lat, lon = self._zetaScaled(self._sncndn6(u, v))
else:
g, k, lat, lon = 0, self._k0, 90, 0
if backside:
lon, g = (180 - lon), (180 - g)
if _lat:
lat, g = -lat, -g
if _lon:
lon, g = -lon, -g
lon += self._lon0 if lon0 is None else _norm180(lon0)
return LatLonExact4Tuple(_norm180(lat), _norm180(lon), g, k)
def _scaled(self, tau, d2, snu, cnu, dnu, snv, cnv, dnv):
'''(INTERNAL) C{scaled}.
@note: Argument B{C{d2}} is C{_mu * cnu**2 + _mv * cnv**2}
from C{._sigma3} or C{._zeta3}.
@return: 2-Tuple C{(convergence, scale)}.
@see: C{void TMExact::Scale(real tau, real /*lam*/,
real snu, real cnu, real dnu,
real snv, real cnv, real dnv,
real &gamma, real &k)}.
'''
mu, mv = self._mu, self._mv
cnudnv = cnu * dnv
# Lee 55.12 -- negated for our sign convention. g gives
# the bearing (clockwise from true north) of grid north
g = atan2(mv * cnv * snv * snu, cnudnv * dnu)
# Lee 55.13 with nu given by Lee 9.1 -- in sqrt change
# the numerator from
#
# (1 - snu^2 * dnv^2) to (_mv * snv^2 + cnu^2 * dnv^2)
#
# to maintain accuracy near phi = 90 and change the
# denomintor from
# (dnu^2 + dnv^2 - 1) to (_mu * cnu^2 + _mv * cnv^2)
#
# to maintain accuracy near phi = 0, lam = 90 * (1 - e).
# Similarly rewrite sqrt term in 9.1 as
#
# _mv + _mu * c^2 instead of 1 - _mu * sin(phi)^2
q2 = (mv * snv**2 + cnudnv**2) / d2
# originally: sec2 = 1 + tau**2 # sec(phi)^2
# k = sqrt(mv + mu / sec2) * sqrt(sec2) * sqrt(q2)
# = sqrt(mv + mv * tau**2 + mu) * sqrt(q2)
k = sqrt(fsum_(mu, mv, mv * tau**2)) * sqrt(q2)
return degrees(g), k * self._k0
def _sigma3(self, v, snu, cnu, dnu, snv, cnv, dnv): # PYCHOK unused
'''(INTERNAL) C{sigma}.
@return: 3-Tuple C{(xi, eta, d2)}.
@see: C{void TMExact::sigma(real /*u*/, real snu, real cnu, real dnu,
real v, real snv, real cnv, real dnv,
real &xi, real &eta)}.
@raise EllipticError: No convergence.
'''
# Lee 55.4 writing
# dnu^2 + dnv^2 - 1 = _mu * cnu^2 + _mv * cnv^2
d2 = self._mu * cnu**2 + self._mv * cnv**2
xi = self._Eu.fE(snu, cnu, dnu) - self._mu * snu * cnu * dnu / d2
eta = v - self._Ev.fE(snv, cnv, dnv) + self._mv * snv * cnv * dnv / d2
return xi, eta, d2
def _sigmaDwd(self, snu, cnu, dnu, snv, cnv, dnv):
'''(INTERNAL) C{sigmaDwd}.
@return: 2-Tuple C{(du, dv)}.
@see: C{void TMExact::dwdsigma(real /*u*/, real snu, real cnu, real dnu,
real /*v*/, real snv, real cnv, real dnv,
real &du, real &dv)}.
'''
snuv = snu * snv
# Reciprocal of 55.9: dw / ds = dn(w)^2/_mv,
# expanding complex dn(w) using A+S 16.21.4
d = self._mv * (cnv**2 + self._mu * snuv**2)**2
r = cnv * dnu * dnv
i = -cnu * snuv * self._mu
du = (r**2 - i**2) / d
dv = 2 * r * i / d
return du, dv
def _sigmaInv(self, xi, eta):
'''(INTERNAL) Invert C{sigma} using Newton's method.
@return: 2-Tuple C{(u, v)}.
@see: C{void TMExact::sigmainv(real xi, real eta,
real &u, real &v)}.
@raise EllipticError: No convergence.
'''
u, v, trip = self._sigmaInv0(xi, eta)
if not trip:
U, V = Fsum(u), Fsum(v)
# min iterations = 2, max = 7, mean = 3.9
for _ in range(self._trips_): # GEOGRAPHICLIB_PANIC
sncndn6 = self._sncndn6(u, v)
X, E, _ = self._sigma3(v, *sncndn6)
dw, dv = self._sigmaDwd( *sncndn6)
X = xi - X
E -= eta
u, du = U.fsum2_(X * dw, E * dv)
v, dv = V.fsum2_(X * dv, -E * dw)
if trip:
break
trip = hypot2(du, dv) < _TOL_10
else:
t = unstr(self._sigmaInv.__name__, xi, eta)
raise EllipticError(_no_convergence_, txt=t)
return u, v
def _sigmaInv0(self, xi, eta):
'''(INTERNAL) Starting point for C{sigmaInv}.
@return: 3-Tuple C{(u, v, trip)}.
@see: C{bool TMExact::sigmainv0(real xi, real eta,
real &u, real &v)}.
'''
trip = False
if eta > self._Ev_cKE_5_4 or xi < min(- self._Eu_cE_1_4,
eta - self._Ev.cKE):
# sigma as a simple pole at
# w = w0 = Eu.K() + i * Ev.K()
# and sigma is approximated by
# sigma = (Eu.E() + i * Ev.KE()) + 1 / (w - w0)
x = xi - self._Eu.cE
y = eta - self._Ev.cKE
d = hypot2(x, y)
u = self._Eu.cK + x / d
v = self._Ev.cK - y / d
elif eta > self._Ev.cKE or (xi < self._Eu_cE_1_4 and
eta > self._Ev_cKE_3_4):
# At w = w0 = i * Ev.K(), we have
# sigma = sigma0 = i * Ev.KE()
# sigma' = sigma'' = 0
#
# including the next term in the Taylor series gives:
# sigma = sigma0 - _mv / 3 * (w - w0)^3
#
# When inverting this, we map arg(w - w0) = [-pi/2, -pi/6]
# to arg(sigma - sigma0) = [-pi/2, pi/2]
# mapping arg = [-pi/2, -pi/6] to [-pi/2, pi/2]
d = eta - self._Ev.cKE
r = hypot(xi, d)
# Error using this guess is about 0.068 * rad^(5/3)
trip = r < _TAYTOL2
# Map the range [-90, 180] in sigma space to [-90, 0] in
# w space. See discussion in zetainv0 on the cut for ang.
r = cbrt(r * self._3_mv)
a = atan2(d - xi, xi + d) / 3.0 - PI_4
s, c = sincos2(a)
u = r * c
v = r * s + self._Ev.cK
else: # use w = sigma * Eu.K/Eu.E (correct in the limit _e -> 0)
u = xi * self._Eu_cK_cE
v = eta * self._Eu_cK_cE
return u, v, trip
def _sncndn6(self, u, v):
'''(INTERNAL) Get 6-tuple C{(snu, cnu, dnu, snv, cnv, dnv)}.
'''
# snu, cnu, dnu = self._Eu.sncndn(u)
# snv, cnv, dnv = self._Ev.sncndn(v)
return self._Eu.sncndn(u) + self._Ev.sncndn(v)
def toStr(self, **kwds):
'''Return a C{str} representation.
@arg kwds: Optional, overriding keyword arguments.
'''
d = dict(name=self.name) if self.name else {}
d = dict(datum=self.datum.name, lon0=self.lon0,
k0=self.k0, extendp=self.extendp, **d)
return _COMMA_SPACE_.join(pairs(d, **kwds))
def _zeta3(self, snu, cnu, dnu, snv, cnv, dnv):
'''(INTERNAL) C{zeta}.
@return: 3-Tuple C{(taup, lambda, d2)}.
@see: C{void TMExact::zeta(real /*u*/, real snu, real cnu, real dnu,
real /*v*/, real snv, real cnv, real dnv,
real &taup, real &lam)}
'''
e = self._e
# Lee 54.17 but write
# atanh(snu * dnv) = asinh(snu * dnv / sqrt(cnu^2 + _mv * snu^2 * snv^2))
# atanh(_e * snu / dnv) = asinh(_e * snu / sqrt(_mu * cnu^2 + _mv * cnv^2))
d1 = cnu**2 + self._mv * (snu * snv)**2
d2 = self._mu * cnu**2 + self._mv * cnv**2
# Overflow value s.t. atan(overflow) = pi/2
t1 = t2 = copysign(_OVERFLOW, snu)
if d1 > 0:
t1 = snu * dnv / sqrt(d1)
lam = 0
if d2 > 0:
t2 = sinh(e * asinh(e * snu / sqrt(d2)))
if d1 > 0:
lam = atan2(dnu * snv , cnu * cnv) - \
atan2(cnu * snv * e, dnu * cnv) * e
# psi = asinh(t1) - asinh(t2)
# taup = sinh(psi)
taup = t1 * hypot1(t2) - t2 * hypot1(t1)
return taup, lam, d2
def _zetaDwd(self, snu, cnu, dnu, snv, cnv, dnv):
'''(INTERNAL) C{zetaDwd}.
@return: 2-Tuple C{(du, dv)}.
@see: C{void TMExact::dwdzeta(real /*u*/, real snu, real cnu, real dnu,
real /*v*/, real snv, real cnv, real dnv,
real &du, real &dv)}.
'''
cnu2 = cnu**2 * self._mu
cnv2 = cnv**2
dnuv = dnu * dnv
dnuv2 = dnuv**2
snuv = snu * snv
snuv2 = snuv**2 * self._mu
# Lee 54.21 but write
# (1 - dnu^2 * snv^2) = (cnv^2 + _mu * snu^2 * snv^2)
# (see A+S 16.21.4)
d = self._mv * (cnv2 + snuv2)**2
du = cnu * dnuv * (cnv2 - snuv2) / d
dv = -cnv * snuv * (cnu2 + dnuv2) / d
return du, dv
def _zetaInv(self, taup, lam):
'''(INTERNAL) Invert C{zeta} using Newton's method.
@return: 2-Tuple C{(u, v)}.
@see: C{void TMExact::zetainv(real taup, real lam,
real &u, real &v)}.
@raise EllipticError: No convergence.
'''
psi = asinh(taup)
sca = 1.0 / hypot1(taup)
u, v, trip = self._zetaInv0(psi, lam)
if not trip:
stol2 = _TOL_10 / max(psi**2, 1.0)
U, V = Fsum(u), Fsum(v)
# min iterations = 2, max = 6, mean = 4.0
for _ in range(self._trips_): # GEOGRAPHICLIB_PANIC
sncndn6 = self._sncndn6(u, v)
T, L, _ = self._zeta3( *sncndn6)
dw, dv = self._zetaDwd(*sncndn6)
T = (taup - T) * sca
L -= lam
u, du = U.fsum2_(T * dw, L * dv)
v, dv = V.fsum2_(T * dv, -L * dw)
if trip:
break
trip = hypot2(du, dv) < stol2
else:
t = unstr(self._zetaInv.__name__, taup, lam)
raise EllipticError(_no_convergence_, txt=t)
return u, v
def _zetaInv0(self, psi, lam):
'''(INTERNAL) Starting point for C{zetaInv}.
@return: 3-Tuple C{(u, v, trip)}.
@see: C{bool TMExact::zetainv0(real psi, real lam, # radians
real &u, real &v)}.
'''
trip = False
if psi < -self._e_PI_4 and lam > self._1_e2_PI_2 \
and psi < (lam - self._1_e_PI_2):
# N.B. this branch is normally not taken because psi < 0
# is converted psi > 0 by Forward.
#
# There's a log singularity at w = w0 = Eu.K() + i * Ev.K(),
# corresponding to the south pole, where we have, approximately
#
# psi = _e + i * pi/2 - _e * atanh(cos(i * (w - w0)/(1 + _mu/2)))
#
# Inverting this gives:
h = sinh(1 - psi / self._e)
a = (PI_2 - lam) / self._e
s, c = sincos2(a)
u = self._Eu.cK - asinh(s / hypot(c, h)) * self._mu_2_1
v = self._Ev.cK - atan2(c, h) * self._mu_2_1
elif psi < self._e_PI_2 and lam > self._1_e2_PI_2:
# At w = w0 = i * Ev.K(), we have
#
# zeta = zeta0 = i * (1 - _e) * pi/2
# zeta' = zeta'' = 0
#
# including the next term in the Taylor series gives:
#
# zeta = zeta0 - (_mv * _e) / 3 * (w - w0)^3
#
# When inverting this, we map arg(w - w0) = [-90, 0] to
# arg(zeta - zeta0) = [-90, 180]
d = lam - self._1_e_PI_2
r = hypot(psi, d)
# Error using this guess is about 0.21 * (rad/e)^(5/3)
trip = r < self._e_TAYTOL
# atan2(dlam-psi, psi+dlam) + 45d gives arg(zeta - zeta0)
# in range [-135, 225). Subtracting 180 (since multiplier
# is negative) makes range [-315, 45). Multiplying by 1/3
# (for cube root) gives range [-105, 15). In particular
# the range [-90, 180] in zeta space maps to [-90, 0] in
# w space as required.
r = cbrt(r * self._3_mv_e)
a = atan2(d - psi, psi + d) / 3.0 - PI_4
s, c = sincos2(a)
u = r * c
v = r * s + self._Ev.cK
else:
# Use spherical TM, Lee 12.6 -- writing C{atanh(sin(lam) /
# cosh(psi)) = asinh(sin(lam) / hypot(cos(lam), sinh(psi)))}.
# This takes care of the log singularity at C{zeta = Eu.K()},
# corresponding to the north pole.
s, c = sincos2(lam)
h, r = sinh(psi), self._Eu_cK_PI_2
# But scale to put 90, 0 on the right place
u = r * atan2(h, c)
v = r * asinh(s / hypot(c, h))
return u, v, trip
def _zetaScaled(self, sncndn6, ll=True):
'''(INTERNAL) Recompute (T, L) from (u, v) to improve accuracy of Scale.
@arg sncndn6: 6-Tuple C{(snu, cnu, dnu, snv, cnv, dnv)}.
@return: 2-Tuple C{(g, k)} if B{C{ll}} is C{False} else
4-tuple C{(g, k, lat, lon)}.
'''
t, lam, d2 = self._zeta3( *sncndn6)
tau = self._E.es_tauf(t)
r = self._scaled(tau, d2, *sncndn6)
if ll:
r += degrees(atan(tau)), degrees(lam)
return r
class LatLonExact4Tuple(_NamedTuple):
'''4-Tuple C{(lat, lon, convergence, scale)} in C{degrees180},
C{degrees}, C{degrees} and C{scalar}.
'''
_Names_ = (_lat_, _lon_, _convergence_, _scale_)
def parseETM5(strUTM, datum=Datums.WGS84, Etm=Etm, falsed=True, name=NN):
'''Parse a string representing a UTM coordinate, consisting
of C{"zone[band] hemisphere easting northing"}.
@arg strUTM: A UTM coordinate (C{str}).
@kwarg datum: Optional datum to use (L{Datum}).
@kwarg Etm: Optional class to return the UTM coordinate
(L{Etm}) or C{None}.
@kwarg falsed: Both easting and northing are falsed (C{bool}).
@kwarg name: Optional B{C{Etm}} name (C{str}).
@return: The UTM coordinate (B{C{Etm}}) or if B{C{Etm}} is
C{None}, a L{UtmUps5Tuple}C{(zone, hemipole, easting,
northing, band)}. The C{hemipole} is the hemisphere
C{'N'|'S'}.
@raise ETMError: Invalid B{C{strUTM}}.
@example:
>>> u = parseETM5('31 N 448251 5411932')
>>> u.toStr2() # [Z:31, H:N, E:448251, N:5411932]
>>> u = parseETM5('31 N 448251.8 5411932.7')
>>> u.toStr() # 31 N 448252 5411933
'''
r = _parseUTM5(strUTM, datum, Etm, falsed, Error=ETMError)
return _xnamed(r, name)
def toEtm8(latlon, lon=None, datum=None, Etm=Etm, falsed=True, name=NN,
zone=None, **cmoff):
'''Convert a lat-/longitude point to an ETM coordinate.
@arg latlon: Latitude (C{degrees}) or an (ellipsoidal)
geodetic C{LatLon} point.
@kwarg lon: Optional longitude (C{degrees}) or C{None}.
@kwarg datum: Optional datum for this ETM coordinate,
overriding B{C{latlon}}'s datum (C{Datum}).
@kwarg Etm: Optional class to return the ETM coordinate
(L{Etm}) or C{None}.
@kwarg falsed: False both easting and northing (C{bool}).
@kwarg name: Optional B{C{Utm}} name (C{str}).
@kwarg zone: Optional UTM zone to enforce (C{int} or C{str}).
@kwarg cmoff: DEPRECATED, use B{C{falsed}}. Offset longitude
from the zone's central meridian (C{bool}).
@return: The ETM coordinate (B{C{Etm}}) or a
L{UtmUps8Tuple}C{(zone, hemipole, easting, northing,
band, datum, convergence, scale)} if B{C{Etm}} is
C{None} or not B{C{falsed}}. The C{hemipole} is the
C{'N'|'S'} hemisphere.
@raise EllipticError: No convergence.
@raise ETMError: Invalid B{C{zone}}.
@raise TypeError: If B{C{latlon}} is not ellipsoidal.
@raise RangeError: If B{C{lat}} outside the valid UTM bands or
if B{C{lat}} or B{C{lon}} outside the valid
range and L{rangerrors} set to C{True}.
@raise ValueError: If B{C{lon}} value is missing or if
B{C{latlon}} is invalid.
'''
z, B, lat, lon, d, f, name = _to7zBlldfn(latlon, lon, datum,
falsed, name, zone,
ETMError, **cmoff)
lon0 = _cmlon(z) if f else None
x, y, g, k = d.exactTM.forward(lat, lon, lon0=lon0)
return _toXtm8(Etm, z, lat, x, y, B, d, g, k, f,
name, latlon, d.exactTM, Error=ETMError)
__all__ += _ALL_DOCS(EasNorExact4Tuple, LatLonExact4Tuple)
# **) MIT License
#
# Copyright (C) 2016-2020 -- 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,