%GEODPROJ Geodesic projections for an ellipsoid
% This package implements four projections based on geodesics:
% * the azimuthal equidistant projection (eqdazim)
% * the Cassini-Soldner projection (cassini)
% * the transverse Mercator projection (tranmerc)
% * the ellipsoidal gnomonic projection (gnomonic)
% The package implements the forward projection (from geographic to
% projected coordinates) and inverse projection (from projected to
% geographic coordinates) with abbreviated function names (listed in
% parentheses in the list above) suffixed by _FWD and _INV. In addition,
% implementations of the UTM projection are provided with UTM_FWD and
% UTM_INV. For each function, metric properties of the projection are
% also returned.
% This package requires the availability of MATLAB File Exchange package
% "Geodesics on an ellipsoid of revolution" for performing the necessary
% geodesic computations:
% The azimuthal equidistant inverse projection is a geodesic projection
% defined by
% [S,AZI0] = GEODDISTANCE(LAT0,LON0,LAT,LON)
% X = S.*SIND(AZI0), Y = S.*COSD(AZI0)
% Thus all distances and azimuths relative to the center point are
% The Cassini-Solder projection is a rectangular geodesic projection
% whose inverse is specified by
% [LAT1,LON1,AZI1] = GEODRECKON(LAT0,LON0,Y,0)
% [LAT,LON] = GEODRECKON(LAT1,LON1,X,AZI1+90)
% Cassini-Soldner is a transverse cylindrical projection where the
% meridian LON0 maps to a straight line with constant scale and distances
% perpendicular to the central meridian are true. Cassini-Soldner was
% widely used for large scale maps until about 1930 (when it was
% supplanted by various conformal projections, in particular, by the
% transverse Mercator projection).
% The transverse Mercator projection is also a cylindrical projection
% which maps the central meridian to a straight line at constant scale.
% However the behavior either side of the central meridian is determined
% by the condition of conformality. The implementation used in this
% package is based on the series method described in
% C. F. F. Karney, Transverse Mercator with an accuracy of a few
% nanometers, J. Geodesy 85(8), 475-485 (Aug. 2011);
% Addenda: http://geographiclib.sf.net/tm-addenda.html
% The ellipsoidal gnomonic projection is defined by
% [~,AZI0,~,~,m,M] = GEODDISTANCE(LAT0,LON0,LAT,LON)
% RHO = m./M, X = RHO.*SIND(AZI0), Y = RHO.*COSD(AZI0)
% Obviously this is an azimuthal projection. It also enjoys approximately
% the property of the spherical gnomonic projection, that geodesics map
% to straight lines. The projection is derived in Section 8 of
% C. F. F. Karney, Algorithms for geodesics,
% J. Geodesy 87, 43-55 (2013);
% Addenda: http://geographiclib.sf.net/geod-addenda.html
% The parameters of the ellipsoid are specified by the optional ELLIPSOID
% argument to the routines. This is a two-element vector of the form
% [a,e], where a is the equatorial radius, e is the eccentricity e =
% sqrt(a^2-b^2)/a, and b is the polar semi-axis. Typically, a and b are
% measured in meters and the linear and area quantities returned by the
% routines are then in meters and meters^2. However, other units can be
% employed. If ELLIPSOID is omitted, then the WGS84 ellipsoid (more
% precisely, the value returned by DEFAULTELLIPSOID) is assumed [6378137,
% 0.0818191908426215] corresponding to a = 6378137 meters and a
% flattening f = (a-b)/a = 1/298.257223563. The flattening and
% eccentricity are related by
% e = sqrt(f * (2 - f))
% f = e^2 / (1 + sqrt(1 - e^2))
% (The functions ECC2FLAT and FLAT2ECC implement these conversions.) For
% a sphere, set e = 0; for a prolate ellipsoid (b > a), specify e as a
% pure imaginary number.
% All angles (latitude, longitude, azimuth) are measured in degrees with
% latitudes increasing northwards, longitudes increasing eastwards, and
% azimuths measured clockwise from north. For a point at a pole, the
% azimuth is defined by keeping the longitude fixed, writing lat =
% +/-(90-eps), and taking the limit eps -> 0+.
% Restrictions on the inputs:
% * All latitudes must lie in [-90, 90].
% * All longitudes and azimuths must lie in [-540, 540). On output,
% these quantities lie in [-180, 180).
% * The equatorial radius, a, must be positive.
% * The eccentricity, e, should be satisfy abs(e) < 0.2 in order to
% retain full accuracy (this corresponds to flattenings satisfying
% abs(f) <= 1/50, approximately). This condition holds for most
% applications in geodesy.
% These routines are fully vectorized so that their speed is competitive
% with the compiled C++ code. These MATLAB versions are transcriptions
% of several C++ classes provided by GeographicLib which is available at
% The routines duplicate some of the functionality of the EQDAZIM,
% CASSINISTD, TRANMERC, and GNOMONIC projections in the the MATLAB
% mapping toolbox. The major improvements offered by this package are
% * The azimuthal equidistant and gnomonic projections are defined
% for the ellipsoid (instead of just for the sphere).
% * The Cassini-Soldner projection is essentially exact (instead of
% being defined in terms of an approximate series).
% * The transverse Mercator projection uses a much more accurate
% series which greatly extends its domain of applicability.
% The primary importance of the two azimuthal projections is that they
% offer a convenient way of solving various geometrical problems on the
% ellipsoid. In particular the azimuthal equidistant projection allows
% problems associated with determining maritime boundaries to be solved
% easily. Similarly the gnomonic projection allows the intersection of
% two geodesics to be determined quickly.
% See also EQDAZIM_FWD, EQDAZIM_INV, CASSINI_FWD, CASSINI_INV,
% TRANMERC_FWD, TRANMERC_INV, GNOMONIC_FWD, GNOMONIC_INV, UTM_FWD,
% UTM_INV, DEFAULTELLIPSOID, ECC2FLAT, FLAT2ECC, GEODDISTANCE,
% Copyright (c) Charles Karney (2012) <firstname.lastname@example.org>.
% This file was distributed with GeographicLib 1.29.