def intersection(start1,
end1,
start2,
end2,
height=None,
wrap=False,
LatLon=LatLon):
'''Compute the intersection point of two paths both defined
by two points or a start point and bearing from North.
@param start1: Start point of the first path (L{LatLon}).
@param end1: End point ofthe first path (L{LatLon}) or
the initial bearing at the first start point
(compass C{degrees360}).
@param start2: Start point of the second path (L{LatLon}).
@param end2: End point of the second path (L{LatLon}) or
the initial bearing at the second start point
(compass C{degrees360}).
@keyword height: Optional height for the intersection point,
overriding the mean height (C{meter}).
@keyword wrap: Wrap and unroll longitudes (C{bool}).
@keyword LatLon: Optional (sub-)class to return the intersection
point (L{LatLon}) or C{None}.
@return: The intersection point (B{C{LatLon}}) or a
L{LatLon3Tuple}C{(lat, lon, height)} if B{C{LatLon}}
is C{None}. An alternate intersection point might
be the L{antipode} to the returned result.
@raise TypeError: A B{C{start}} or B{C{end}} point not L{LatLon}.
@raise ValueError: Intersection is ambiguous or infinite or
the paths are parallel, coincident or null.
@example:
>>> p = LatLon(51.8853, 0.2545)
>>> s = LatLon(49.0034, 2.5735)
>>> i = intersection(p, 108.547, s, 32.435) # '50.9078°N, 004.5084°E'
'''
_Trll.others(start1, name='start1')
_Trll.others(start2, name='start2')
hs = [start1.height, start2.height]
a1, b1 = start1.to2ab()
a2, b2 = start2.to2ab()
db, b2 = unrollPI(b1, b2, wrap=wrap)
r12 = haversine_(a2, a1, db)
if abs(r12) < EPS: # [nearly] coincident points
a, b = map1(degrees, favg(a1, a2), favg(b1, b2))
# see <https://www.EdWilliams.org/avform.htm#Intersection>
elif isscalar(end1) and isscalar(end2): # both bearings
sa1, ca1, sa2, ca2, sr12, cr12 = sincos2(a1, a2, r12)
x1, x2 = (sr12 * ca1), (sr12 * ca2)
if abs(x1) < EPS or abs(x2) < EPS:
raise ValueError('intersection %s: %r vs %r' % ('parallel',
(start1, end1),
(start2, end2)))
# handle domain error for equivalent longitudes,
# see also functions asin_safe and acos_safe at
# <https://www.EdWilliams.org/avform.htm#Math>
t1, t2 = map1(acos1, (sa2 - sa1 * cr12) / x1, (sa1 - sa2 * cr12) / x2)
if sin(db) > 0:
t12, t21 = t1, PI2 - t2
else:
t12, t21 = PI2 - t1, t2
t13, t23 = map1(radiansPI2, end1, end2)
x1, x2 = map1(
wrapPI,
t13 - t12, # angle 2-1-3
t21 - t23) # angle 1-2-3
sx1, cx1, sx2, cx2 = sincos2(x1, x2)
if sx1 == 0 and sx2 == 0: # max(abs(sx1), abs(sx2)) < EPS
raise ValueError('intersection %s: %r vs %r' % ('infinite',
(start1, end1),
(start2, end2)))
sx3 = sx1 * sx2
# if sx3 < 0:
# raise ValueError('intersection %s: %r vs %r' % ('ambiguous',
# (start1, end1), (start2, end2)))
x3 = acos1(cr12 * sx3 - cx2 * cx1)
r13 = atan2(sr12 * sx3, cx2 + cx1 * cos(x3))
a, b = _destination2(a1, b1, r13, t13)
# choose antipode for opposing bearings
if _xb(a1, b1, end1, a, b, wrap) < 0 or \
_xb(a2, b2, end2, a, b, wrap) < 0:
a, b = antipode(a, b)
else: # end point(s) or bearing(s)
x1, d1 = _x3d2(start1, end1, wrap, '1', hs)
x2, d2 = _x3d2(start2, end2, wrap, '2', hs)
x = x1.cross(x2)
if x.length < EPS: # [nearly] colinear or parallel paths
raise ValueError('intersection %s: %r vs %r' % ('colinear',
(start1, end1),
(start2, end2)))
a, b = x.to2ll()
# choose intersection similar to sphericalNvector
d1 = _xdot(d1, a1, b1, a, b, wrap)
d2 = _xdot(d2, a2, b2, a, b, wrap)
if (d1 < 0 and d2 > 0) or (d1 > 0 and d2 < 0):
a, b = antipode(a, b)
h = fmean(hs) if height is None else height
r = LatLon3Tuple(a, b, h) if LatLon is None else \
LatLon(a, b, height=h)
return _xnamed(r, intersection.__name__)
def _mdef(self, lat):
'''(INTERNAL) Compute m(lat).
'''
s, c = sincos2(lat)
s *= self._e
return c / sqrt(1 - s**2)
def reverse(self, xyz, y=None, z=None, **no_M): # PYCHOK unused M
'''Convert from geocentric C{(x, y, z)} to geodetic C{(lat, lon, height)}
transcribed 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.
@param xyz: Either an L{Ecef9Tuple}, an C{(x, y, z)} 3-tuple or C{scalar}
ECEF C{x} coordinate in C{meter}.
@keyword y: ECEF C{y} coordinate in C{meter} for C{scalar} B{C{xyz}}
and B{C{z}}.
@keyword z: ECEF C{z} coordinate in C{meter} for C{scalar} B{C{xyz}}
and B{C{y}}.
@keyword no_M: Rotation matrix C{M} not available.
@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}, L{EcefMatrix} C{M}
always C{None} and C{datum} if available.
@raise EcefError: If B{C{xyz}} not L{Ecef9Tuple} 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).
'''
x, y, z, name = _xyzn4(xyz, y, z, Error=EcefError)
E = self.ellipsoid
p = hypot(x, y) # distance from minor axis
r = hypot(p, z) # polar radius
if min(p, r) > EPS:
# parametric latitude (Bowring eqn 17, replaced)
t = (E.b * z) / (E.a * p) * (1 + E.e22 * E.b / r)
c = 1 / 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)
b = atan2(y, x) # ... and longitude
# 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), degrees180(b)
# see <https://GIS.StackExchange.com/questions/28446>
elif p > EPS: # lat arbitrarily zero
C, lat, lon, h = 2, 0.0, degrees180(atan2(y, x)), p - E.a
else: # polar lat, lon arbitrarily zero
C, lat, lon, h = 3, copysign(90.0, z), 0.0, abs(z) - E.b
r = Ecef9Tuple(x, y, z, lat, lon, h, C, None, self.datum)
return self._xnamed(r, name)
def _inverse(self, other, azis, wrap):
'''(INTERNAL) Inverse Vincenty method.
@raise TypeError: The B{C{other}} point is not L{LatLon}.
@raise ValueError: If this and the B{C{other}} point's L{Datum}
ellipsoids are not compatible.
@raise VincentyError: Vincenty fails to converge for the current
L{LatLon.epsilon} and L{LatLon.iterations}
limit and/or if this and the B{C{other}}
point are coincident or near-antipodal.
'''
E = self.ellipsoids(other)
c1, s1, _ = _r3(self.lat, E.f)
c2, s2, _ = _r3(other.lat, E.f)
c1c2, s1c2 = c1 * c2, s1 * c2
c1s2, s1s2 = c1 * s2, s1 * s2
dl, _ = unroll180(self.lon, other.lon, wrap=wrap)
ll = dl = radians(dl)
for _ in range(self._iterations):
ll_ = ll
sll, cll = sincos2(ll)
ss = hypot(c2 * sll, c1s2 - s1c2 * cll)
if ss < EPS: # coincident or antipodal, ...
if self.isantipodeTo(other, eps=self._epsilon):
raise VincentyError('%s, %r %sto %r' % ('ambiguous',
self, 'antipodal ', other))
d = 0.0 # like Karney, ...
if azis: # return zeros
d = d, 0, 0
return d
cs = s1s2 + c1c2 * cll
s = atan2(ss, cs)
sa = c1c2 * sll / ss
c2a = 1 - sa**2
if abs(c2a) < EPS:
c2a = 0 # equatorial line
ll = dl + E.f * sa * s
else:
c2sm = cs - 2 * s1s2 / c2a
ll = dl + _dl(E.f, c2a, sa, s, cs, ss, c2sm)
if abs(ll - ll_) < self._epsilon:
break
# # omitted and applied only after failure to converge below, see footnote
# # under Inverse at <https://WikiPedia.org/wiki/Vincenty's_formulae>
# # <https://GitHub.com/ChrisVeness/geodesy/blob/master/latlon-vincenty.js>
# elif abs(ll) > PI and self.isantipodeTo(other, eps=self._epsilon):
# raise VincentyError('%s, %r %sto %r' % ('ambiguous', self,
# 'antipodal ', other))
else:
t = 'antipodal ' if self.isantipodeTo(other, eps=self._epsilon) else ''
raise VincentyError('%s, %r %sto %r' % ('no convergence', self, t, other))
if c2a: # e22 == (a / b)**2 - 1
A, B = _p2(c2a * E.e22)
s = A * (s - _ds(B, cs, ss, c2sm))
b = E.b
# if self.height or other.height:
# b += self._havg(other)
d = b * s
if azis: # forward and reverse azimuth
sll, cll = sincos2(ll)
f = degrees360(atan2(c2 * sll, c1s2 - s1c2 * cll))
r = degrees360(atan2(c1 * sll, -s1c2 + c1s2 * cll))
d = d, f, r
return d
def toUtm8(latlon,
lon=None,
datum=None,
Utm=Utm,
falsed=True,
name=NN,
zone=None,
**cmoff):
'''Convert a lat-/longitude point to a UTM 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 UTM coordinate,
overriding B{C{latlon}}'s datum (L{Datum},
L{Ellipsoid}, L{Ellipsoid2} or L{a_f2Tuple}).
@kwarg Utm: Optional class to return the UTM coordinate
(L{Utm}) 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 UTM coordinate (B{C{Utm}}) or if B{C{Utm}} is
C{None} or not B{C{falsed}}, a L{UtmUps8Tuple}C{(zone,
hemipole, easting, northing, band, datum, convergence,
scale)}. The C{hemipole} is the C{'N'|'S'} hemisphere.
@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 TypeError: Invalid B{C{datum}} or B{C{latlon}} not ellipsoidal.
@raise UTMError: Invalid B{C{zone}}.
@raise ValueError: If B{C{lon}} value is missing or if
B{C{latlon}} is invalid.
@note: Implements Karney’s method, using 8-th order Krüger series,
giving results accurate to 5 nm (or better) for distances
up to 3900 km from the central meridian.
@example:
>>> p = LatLon(48.8582, 2.2945) # 31 N 448251.8 5411932.7
>>> u = toUtm(p) # 31 N 448252 5411933
>>> p = LatLon(13.4125, 103.8667) # 48 N 377302.4 1483034.8
>>> u = toUtm(p) # 48 N 377302 1483035
'''
z, B, lat, lon, d, f, name = _to7zBlldfn(latlon, lon, datum, falsed, name,
zone, UTMError, **cmoff)
d = _ellipsoidal_datum(d, name=name)
E = d.ellipsoid
a, b = radians(lat), radians(lon)
# easting, northing: Karney 2011 Eq 7-14, 29, 35
sb, cb = sincos2(b)
T = tan(a)
T12 = hypot1(T)
S = sinh(E.e * atanh(E.e * T / T12))
T_ = T * hypot1(S) - S * T12
H = hypot(T_, cb)
y = atan2(T_, cb) # ξ' ksi
x = asinh(sb / H) # η' eta
A0 = E.A * getattr(Utm, '_scale0', _K0) # Utm is class or None
K = _Kseries(E.AlphaKs, x, y) # Krüger series
y = K.ys(y) * A0 # ξ
x = K.xs(x) * A0 # η
# convergence: Karney 2011 Eq 23, 24
p_ = K.ps(1)
q_ = K.qs(0)
c = degrees(atan(T_ / hypot1(T_) * tan(b)) + atan2(q_, p_))
# scale: Karney 2011 Eq 25
k = E.e2s(sin(a)) * T12 / H * (A0 / E.a * hypot(p_, q_))
return _toXtm8(Utm, z, lat, x, y, B, d, c, k, f, name, latlon, EPS)
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 toLatLon(self, LatLon=None, eps=EPS, unfalse=True, **LatLon_kwds):
'''Convert this UTM coordinate to an (ellipsoidal) geodetic point.
@kwarg LatLon: Optional, ellipsoidal class to return the
geodetic point (C{LatLon}) or C{None}.
@kwarg eps: Optional convergence limit, L{EPS} or above
(C{float}).
@kwarg unfalse: Unfalse B{C{easting}} and B{C{northing}}
if falsed (C{bool}).
@kwarg LatLon_kwds: Optional, additional B{C{LatLon}} keyword
arguments, ignored if C{B{LatLon}=None}.
@return: This UTM coordinate (B{C{LatLon}}) or if B{C{LatLon}}
is C{None}, a L{LatLonDatum5Tuple}C{(lat, lon, datum,
convergence, scale)}.
@raise TypeError: If B{C{LatLon}} is not ellipsoidal.
@raise UTMError: Invalid meridional radius or H-value.
@example:
>>> u = Utm(31, 'N', 448251.795, 5411932.678)
>>> from pygeodesy import ellipsoidalVincenty as eV
>>> ll = u.toLatLon(eV.LatLon) # 48°51′29.52″N, 002°17′40.20″E
'''
if eps < EPS:
eps = EPS # less doesn't converge
if self._latlon and self._latlon_args == (eps, unfalse):
return self._latlon5(LatLon)
E = self.datum.ellipsoid # XXX vs LatLon.datum.ellipsoid
x, y = self.eastingnorthing2(falsed=not unfalse)
# from Karney 2011 Eq 15-22, 36
A0 = self.scale0 * E.A
if A0 < EPS:
raise self._Error(meridional=A0)
x /= A0 # η eta
y /= A0 # ξ ksi
K = _Kseries(E.BetaKs, x, y) # Krüger series
y = neg(K.ys(-y)) # ξ'
x = neg(K.xs(-x)) # η'
shx = sinh(x)
sy, cy = sincos2(y)
H = hypot(shx, cy)
if H < EPS:
raise self._Error(H=H)
T = t0 = sy / H # τʹ
S = Fsum(T)
q = _1_0 / E.e12
P = 7 # -/+ toggle trips
d = _1_0 + eps
while abs(d) > eps and P > 0:
p = -d # previous d, toggled
h = hypot1(T)
s = sinh(E.e * atanh(E.e * T / h))
t = T * hypot1(s) - s * h
d = (t0 - t) / hypot1(t) * ((q + T**2) / h)
T, d = S.fsum2_(d) # τi, (τi - τi-1)
if d == p: # catch -/+ toggling of d
P -= 1
# else:
# P = 0
a = atan(T) # lat
b = atan2(shx, cy)
if unfalse and self.falsed:
b += radians(_cmlon(self.zone))
ll = _LLEB(degrees90(a),
degrees180(b),
datum=self.datum,
name=self.name)
# convergence: Karney 2011 Eq 26, 27
p = neg(K.ps(-1))
q = K.qs(0)
ll._convergence = degrees(atan(tan(y) * tanh(x)) + atan2(q, p))
# scale: Karney 2011 Eq 28
ll._scale = E.e2s(sin(a)) * hypot1(T) * H * (A0 / E.a / hypot(p, q))
self._latlon_to(ll, eps, unfalse)
return self._latlon5(LatLon, **LatLon_kwds)
def _sncndn3(self, phi):
'''(INTERNAL) Helper for C{.fEinv} and C{._fXf}.
'''
sn, cn = sincos2(phi)
return sn, cn, self.fDelta(sn, cn)
def toOsgr(latlon, lon=None, datum=Datums.WGS84, Osgr=Osgr, name=''):
'''Convert a lat-/longitude point to an OSGR coordinate.
@param latlon: Latitude (C{degrees}) or an (ellipsoidal)
geodetic C{LatLon} point.
@keyword lon: Optional longitude in degrees (scalar or C{None}).
@keyword datum: Optional datum to convert (C{Datum}).
@keyword Osgr: Optional (sub-)class to return the OSGR
coordinate (L{Osgr}) or C{None}.
@keyword name: Optional B{C{Osgr}} name (C{str}).
@return: The OSGR coordinate (B{C{Osgr}}) or an
L{EasNor2Tuple}C{(easting, northing)} if B{C{Osgr}}
is C{None}.
@raise TypeError: Non-ellipsoidal B{C{latlon}} or B{C{datum}}
conversion failed.
@raise OSGRError: Invalid B{C{latlon}} or B{C{lon}}.
@example:
>>> p = LatLon(52.65798, 1.71605)
>>> r = toOsgr(p) # TG 51409 13177
>>> # for conversion of (historical) OSGB36 lat-/longitude:
>>> r = toOsgr(52.65757, 1.71791, datum=Datums.OSGB36)
'''
if not isinstance(latlon, _LLEB):
# XXX fix failing _LLEB.convertDatum()
latlon = _LLEB(*parseDMS2(latlon, lon), datum=datum)
elif lon is not None:
raise OSGRError('%s not %s: %r' % ('lon', None, lon))
elif not name: # use latlon.name
name = nameof(latlon)
E = _OSGB36.ellipsoid
ll = _ll2datum(latlon, _OSGB36, 'latlon')
a, b = map1(radians, ll.lat, ll.lon)
sa, ca = sincos2(a)
s = E.e2s2(sa) # r, v = E.roc2_(sa, _F0); r = v / r
v = E.a * _F0 / sqrt(s) # nu
r = s / E.e12 # nu / rho == v / (v * E.e12 / s) == s / E.e12
x2 = r - 1 # η2
ta = tan(a)
ca3, ca5 = fpowers(ca, 5, 3) # PYCHOK false!
ta2, ta4 = fpowers(ta, 4, 2) # PYCHOK false!
vsa = v * sa
I4 = (E.b * _F0 * _M(E.Mabcd, a) + _N0, (vsa / 2) * ca,
(vsa / 24) * ca3 * fsum_(5, -ta2, 9 * x2),
(vsa / 720) * ca5 * fsum_(61, ta4, -58 * ta2))
V4 = (_E0, (v * ca), (v / 6) * ca3 * (r - ta2), (v / 120) * ca5 * fdot(
(-18, 1, 14, -58), ta2, 5 + ta4, x2, ta2 * x2))
d, d2, d3, d4, d5, d6 = fpowers(b - _B0, 6) # PYCHOK false!
n = fdot(I4, 1, d2, d4, d6)
e = fdot(V4, 1, d, d3, d5)
if Osgr is None:
r = EasNor2Tuple(e, n)
else:
r = Osgr(e, n)
if lon is None and isinstance(latlon, _LLEB):
r._latlon = latlon # XXX weakref(latlon)?
return _xnamed(r, name)
def toLatLon(self, LatLon=None, datum=Datums.WGS84):
'''Convert this OSGR coordinate to an (ellipsoidal) geodetic
point.
I{Note formulation implemented here due to Thomas, Redfearn,
etc. is as published by OS, but is inferior to Krüger as
used by e.g. Karney 2011.}
@keyword LatLon: Optional ellipsoidal (sub-)class to return
the point (C{LatLon}) or C{None}.
@keyword datum: Optional datum to use (C{Datum}).
@return: The geodetic point (B{C{LatLon}}) or a
L{LatLonDatum3Tuple}C{(lat, lon, datum)}
if B{C{LatLon}} is C{None}.
@raise OSGRError: No convergence.
@raise TypeError: If B{C{LatLon}} is not ellipsoidal or if
B{C{datum}} conversion failed.
@example:
>>> from pygeodesy import ellipsoidalVincenty as eV
>>> g = Osgr(651409.903, 313177.270)
>>> p = g.toLatLon(eV.LatLon) # 52°39′28.723″N, 001°42′57.787″E
>>> # to obtain (historical) OSGB36 lat-/longitude point
>>> p = g.toLatLon(eV.LatLon, datum=Datums.OSGB36) # 52°39′27.253″N, 001°43′04.518″E
'''
if self._latlon:
return self._latlon3(LatLon, datum)
E = self.datum.ellipsoid # _OSGB36.ellipsoid, Airy130
a_F0 = E.a * _F0
b_F0 = E.b * _F0
e, n = self.easting, self.northing
n_N0 = n - _N0
a, m = _A0, n_N0
sa = Fsum(a)
for _ in range(_TRIPS):
a = sa.fsum_(m / a_F0)
m = n_N0 - b_F0 * _M(E.Mabcd, a) # meridional arc
if abs(m) < _10um:
break
else:
t = self.classname, self.toStr(prec=-3), 'toLatLon'
raise OSGRError('no convergence %s(%s).%s' % t)
sa, ca = sincos2(a)
s = E.e2s2(sa) # r, v = E.roc2_(sa, _F0)
v = a_F0 / sqrt(s) # nu
r = v * E.e12 / s # rho = a_F0 * E.e12 / pow(s, 1.5) == a_F0 * E.e12 / (s * sqrt(s))
vr = v / r # == s / E.e12
x2 = vr - 1 # η2
ta = tan(a)
v3, v5, v7 = fpowers(v, 7, 3) # PYCHOK false!
ta2, ta4, ta6 = fpowers(ta**2, 3) # PYCHOK false!
tar = ta / r
V4 = (a, tar / (2 * v), tar / (24 * v3) * fdot(
(1, 3, -9), 5 + x2, ta2, ta2 * x2), tar / (720 * v5) * fdot(
(61, 90, 45), 1, ta2, ta4))
csa = 1.0 / ca
X5 = (_B0, csa / v, csa / (6 * v3) * fsum_(vr, ta, ta),
csa / (120 * v5) * fdot(
(5, 28, 24), 1, ta2, ta4), csa / (5040 * v7) * fdot(
(61, 662, 1320, 720), 1, ta2, ta4, ta6))
d, d2, d3, d4, d5, d6, d7 = fpowers(e - _E0, 7) # PYCHOK false!
a = fdot(V4, 1, -d2, d4, -d6)
b = fdot(X5, 1, d, -d3, d5, -d7)
self._latlon = _LLEB(degrees90(a),
degrees180(b),
datum=self.datum,
name=self.name)
return self._latlon3(LatLon, datum)
def intersection(start1, end1, start2, end2, height=None, wrap=False,
LatLon=LatLon, **LatLon_kwds):
'''Compute the intersection point of two paths both defined
by two points or a start point and bearing from North.
@arg start1: Start point of the first path (L{LatLon}).
@arg end1: End point ofthe first path (L{LatLon}) or
the initial bearing at the first start point
(compass C{degrees360}).
@arg start2: Start point of the second path (L{LatLon}).
@arg end2: End point of the second path (L{LatLon}) or
the initial bearing at the second start point
(compass C{degrees360}).
@kwarg height: Optional height for the intersection point,
overriding the mean height (C{meter}).
@kwarg wrap: Wrap and unroll longitudes (C{bool}).
@kwarg LatLon: Optional class to return the intersection
point (L{LatLon}) or C{None}.
@kwarg LatLon_kwds: Optional, additional B{C{LatLon}} keyword
arguments, ignored if B{C{LatLon=None}}.
@return: The intersection point (B{C{LatLon}}) or a
L{LatLon3Tuple}C{(lat, lon, height)} if B{C{LatLon}}
is C{None}. An alternate intersection point might
be the L{antipode} to the returned result.
@raise IntersectionError: Intersection is ambiguous or infinite
or the paths are coincident, colinear
or parallel.
@raise TypeError: A B{C{start}} or B{C{end}} point not L{LatLon}.
@raise ValueError: Invalid B{C{height}}.
@example:
>>> p = LatLon(51.8853, 0.2545)
>>> s = LatLon(49.0034, 2.5735)
>>> i = intersection(p, 108.547, s, 32.435) # '50.9078°N, 004.5084°E'
'''
_T00.others(start1, name=_start1_)
_T00.others(start2, name=_start2_)
hs = [start1.height, start2.height]
a1, b1 = start1.philam
a2, b2 = start2.philam
db, b2 = unrollPI(b1, b2, wrap=wrap)
r12 = vincentys_(a2, a1, db)
if abs(r12) < EPS: # [nearly] coincident points
a, b = favg(a1, a2), favg(b1, b2)
# see <https://www.EdWilliams.org/avform.htm#Intersection>
elif isscalar(end1) and isscalar(end2): # both bearings
sa1, ca1, sa2, ca2, sr12, cr12 = sincos2(a1, a2, r12)
x1, x2 = (sr12 * ca1), (sr12 * ca2)
if abs(x1) < EPS or abs(x2) < EPS:
raise IntersectionError(start1=start1, end1=end1,
start2=start2, end2=end2, txt='parallel')
# handle domain error for equivalent longitudes,
# see also functions asin_safe and acos_safe at
# <https://www.EdWilliams.org/avform.htm#Math>
t1, t2 = map1(acos1, (sa2 - sa1 * cr12) / x1,
(sa1 - sa2 * cr12) / x2)
if sin(db) > 0:
t12, t21 = t1, PI2 - t2
else:
t12, t21 = PI2 - t1, t2
t13, t23 = map1(radiansPI2, end1, end2)
x1, x2 = map1(wrapPI, t13 - t12, # angle 2-1-3
t21 - t23) # angle 1-2-3
sx1, cx1, sx2, cx2 = sincos2(x1, x2)
if sx1 == 0 and sx2 == 0: # max(abs(sx1), abs(sx2)) < EPS
raise IntersectionError(start1=start1, end1=end1,
start2=start2, end2=end2, txt='infinite')
sx3 = sx1 * sx2
# if sx3 < 0:
# raise IntersectionError(start1=start1, end1=end1,
# start2=start2, end2=end2, txt=_ambiguous_)
x3 = acos1(cr12 * sx3 - cx2 * cx1)
r13 = atan2(sr12 * sx3, cx2 + cx1 * cos(x3))
a, b = _destination2(a1, b1, r13, t13)
# choose antipode for opposing bearings
if _xb(a1, b1, end1, a, b, wrap) < 0 or \
_xb(a2, b2, end2, a, b, wrap) < 0:
a, b = antipode_(a, b) # PYCHOK PhiLam2Tuple
else: # end point(s) or bearing(s)
x1, d1 = _x3d2(start1, end1, wrap, _1_, hs)
x2, d2 = _x3d2(start2, end2, wrap, _2_, hs)
x = x1.cross(x2)
if x.length < EPS: # [nearly] colinear or parallel paths
raise IntersectionError(start1=start1, end1=end1,
start2=start2, end2=end2, txt=_colinear_)
a, b = x.philam
# choose intersection similar to sphericalNvector
d1 = _xdot(d1, a1, b1, a, b, wrap)
if d1:
d2 = _xdot(d2, a2, b2, a, b, wrap)
if (d2 < 0 and d1 > 0) or (d2 > 0 and d1 < 0):
a, b = antipode_(a, b) # PYCHOK PhiLam2Tuple
h = fmean(hs) if height is None else Height(height)
return _latlon3(degrees90(a), degrees180(b), h,
intersection, LatLon, **LatLon_kwds)