Provided by: pdl_2.085-1ubuntu1_amd64 
NAME
PDL::Transform::Cartography - Useful cartographic projections
SYNOPSIS
# make a Mercator map of Earth
use PDL::Transform::Cartography;
$x = earth_coast();
$x = graticule(10,2)->glue(1,$x);
$t = t_mercator;
$w = pgwin(xs);
$w->lines($t->apply($x)->clean_lines());
DESCRIPTION
PDL::Transform::Cartography includes a variety of useful cartographic and observing projections (mappings
of the surface of a sphere), including reprojected observer coordinates. See PDL::Transform for more
information about image transforms in general.
Cartographic transformations are used for projecting not just terrestrial maps, but also any nearly
spherical surface including the Sun, the Celestial sphere, various moons and planets, distant stars, etc.
They also are useful for interpreting scientific images, which are themselves generally projections of a
sphere onto a flat focal plane (e.g. the "t_gnomonic" projection).
Unless otherwise noted, all the transformations in this file convert from (theta,phi) coordinates on the
unit sphere (e.g. (lon,lat) on a planet or (RA,dec) on the celestial sphere) into some sort of projected
coordinates, and have inverse transformations that convert back to (theta,phi). This is equivalent to
working from the equidistant cylindrical (or "plate carree") projection, if you are a cartography wonk.
The projected coordinates are generally in units of body radii (radians), so that multiplying the output
by the scale of the map yields physical units that are correct wherever the scale is correct for that
projection. For example, areas should be correct everywhere in the authalic projections; and linear
scales are correct along meridians in the equidistant projections and along the standard parallels in all
the projections.
The transformations that are authalic (equal-area), conformal (equal-angle), azimuthal (circularly
symmetric), or perspective (true perspective on a focal plane from some viewpoint) are marked. The first
two categories are mutually exclusive for all but the "unit sphere" 3-D projection.
Extra dimensions tacked on to each point to be transformed are, in general, ignored. That is so that you
can add on an extra index to keep track of pen color. For example, "earth_coast" returns a 3x<n> ndarray
containing (lon, lat, pen) at each list location. Transforming the vector list retains the pen value as
the first index after the dimensional directions.
GENERAL NOTES ON CARTOGRAPHY
Unless otherwise noted, the transformations and miscellaneous information in this section are taken from
Snyder & Voxland 1989: "An Album of Map Projections", US Geological Survey Professional Paper 1453, US
Printing Office (Denver); and from Snyder 1987: "Map Projections - A Working Manual", US Geological
Survey Professional Paper 1395, US Printing Office (Denver, USA). You can obtain your own copy of both
by contacting the U.S. Geological Survey, Federal Center, Box 25425, Denver, CO 80225 USA.
The mathematics of cartography have a long history, and the details are far trickier than the broad
overview. For terrestrial (and, in general, planetary) cartography, the best reference datum is not a
sphere but an oblate ellipsoid due to centrifugal force from the planet's rotation. Furthermore, because
all rocky planets, including Earth, have randomly placed mass concentrations that affect the
gravitational field, the reference gravitational isosurface (sea level on Earth) is even more complex
than an ellipsoid and, in general, different ellipsoids have been used for different locations at the
same time and for the same location at different times.
The transformations in this package use a spherical datum and hence include global distortion at about
the 0.5% level for terrestrial maps (Earth's oblateness is ~1/300). This is roughly equal to the
dimensional precision of physical maps printed on paper (due to stretching and warping of the paper) but
is significant at larger scales (e.g. for regional maps). If you need more precision than that, you will
want to implement and use the ellipsoidal transformations from Snyder 1987 or another reference work on
geodesy. A good name for that package would be "...::Cartography::Geodetic".
GENERAL NOTES ON PERSPECTIVE AND SCIENTIFIC IMAGES
Cartographic transformations are useful for interpretation of scientific images, as all cameras produce
projections of the celestial sphere onto the focal plane of the camera. A simple (single-element)
optical system with a planar focal plane generates gnomonic images -- that is to say, gnomonic
projections of a portion of the celestial sphere near the paraxial direction. This is the projection
that most consumer grade cameras produce.
Magnification in an optical system changes the angle of incidence of the rays on the focal plane for a
given angle of incidence at the aperture. For example, a 10x telescope with a 2 degree field of view
exhibits the same gnomonic distortion as a simple optical system with a 20 degree field of view. Wide-
angle optics typically have magnification less than 1 ('fisheye lenses'), reducing the gnomonic
distortion considerably but introducing "equidistant azimuthal" distortion -- there's no such thing as a
free lunch!
Because many solar-system objects are spherical, PDL::Transform::Cartography includes perspective
projections for producing maps of spherical bodies from perspective views. Those projections are
"t_vertical" and "t_perspective". They map between (lat,lon) on the spherical body and planar projected
coordinates at the viewpoint. "t_vertical" is the vertical perspective projection given by Snyder, but
"t_perspective" is a fully general perspective projection that also handles magnification correction.
TRANSVERSE & OBLIQUE PROJECTIONS; STANDARD OPTIONS
Oblique projections rotate the sphere (and graticule) to an arbitrary angle before generating the
projection; transverse projections rotate the sphere exactly 90 degrees before generating the projection.
Most of the projections accept the following standard options, useful for making transverse and oblique
projection maps.
o, origin, Origin [default (0,0,0)]
The origin of the oblique map coordinate system, in (old-theta, old-phi) coordinates.
r, roll, Roll [default 0.0]
The roll angle of the sphere about the origin, measured CW from (N = up) for reasonable values of phi
and CW from (S = up) for unreasonable values of phi. This is equivalent to observer roll angle CCW
from the same direction.
u, unit, Unit [default 'degree']
This is the name of the angular unit to use in the lon/lat coordinate system.
b, B
The "B" angle of the body -- used for extraterrestrial maps. Setting this parameter is exactly
equivalent to setting the phi component of the origin, and in fact overrides it.
l,L
The longitude of the central meridian as observed -- used for extraterrestrial maps. Setting this
parameter is exactly equivalent to setting the theta component of the origin, and in fact overrides
it.
p,P
The "P" (or position) angle of the body -- used for extraterrestrial maps. This parameter is a
synonym for the roll angle, above.
bad, Bad, missing, Missing [default nan]
This is the value that missing points get. Mainly useful for the inverse transforms. (This should
work fine if set to BAD, if you have bad-value support compiled in). The default nan is asin(1.2),
calculated at load time.
EXAMPLES
Draw a Mercator map of the world on-screen:
$w = pgwin(xs);
$w->lines(earth_coast->apply(t_mercator)->clean_lines);
Here, earth_coast() returns a 3xn ndarray containing (lon, lat, pen) values for the included world
coastal outline; "t_mercator" converts the values to projected Mercator coordinates, and "clean_lines"
breaks lines that cross the 180th meridian.
Draw a Mercator map of the world, with lon/lat at 10 degree intervals:
$w = pgwin(xs)
$x = earth_coast()->glue(1,graticule(10,1));
$w->lines($x->apply(t_mercator)->clean_lines);
This works just the same as the first example, except that a map graticule has been applied with
interline spacing of 10 degrees lon/lat and inter-vertex spacing of 1 degree (so that each meridian
contains 181 points, and each parallel contains 361 points).
NOTES
Currently angular conversions are rather simpleminded. A list of common conversions is present in the
main constructor, which inserts a conversion constant to radians into the {params} field of the new
transform. Something like Math::Convert::Units should be used instead to generate the conversion
constant.
A cleaner higher-level interface is probably needed (see the examples); for example, earth_coast could
return a graticule if asked, instead of needing one to be glued on.
The class structure is somewhat messy because of the varying needs of the different transformations.
PDL::Transform::Cartography is a base class that interprets the origin options and sets up the basic
machinery of the Transform. The conic projections have their own subclass, PDL::Transform::Conic, that
interprets the standard parallels. Since the cylindrical and azimuthal projections are pretty simple,
they are not subclassed.
The perl 5.6.1 compiler is quite slow at adding new classes to the structure, so it does not makes sense
to subclass new transformations merely for the sake of pedantry.
AUTHOR
Copyright 2002, Craig DeForest (deforest@boulder.swri.edu). This module may be modified and distributed
under the same terms as PDL itself. The module comes with NO WARRANTY.
The included digital world map is derived from the 1987 CIA World Map, translated to ASCII in 1988 by Joe
Dellinger (geojoe@freeusp.org) and simplified in 1995 by Kirk Johnson (tuna@indra.com) for the program
XEarth. The map comes with NO WARRANTY. An ASCII version of the map, and a sample PDL function to read
it, may be found in the Demos subdirectory of the PDL source distribution.
FUNCTIONS
The module exports both transform constructors ('t_<foo>') and some auxiliary functions (no leading
't_').
graticule
$lonlatp = graticule(<grid-spacing>,<line-segment-size>);
$lonlatp = graticule(<grid-spacing>,<line-segment-size>,1);
(Cartography) PDL constructor - generate a lat/lon grid.
Returns a grid of meridians and parallels as a list of vectors suitable for sending to
PDL::Graphics::PGPLOT::Window::lines for plotting. The grid is in degrees in (theta, phi) coordinates --
this is (E lon, N lat) for terrestrial grids or (RA, dec) for celestial ones. You must then transform
the graticule in the same way that you transform the map.
You can attach the graticule to a vector map using the syntax:
$out = graticule(10,2)->glue(1,$map);
In array context you get back a 2-element list containing an ndarray of the (theta,phi) pairs and an
ndarray of the pen values (1 or 0) suitable for calling PDL::Graphics::PGPLOT::Window::lines. In scalar
context the two elements are combined into a single ndarray.
The pen values associated with the graticule are negative, which will cause
PDL::Graphics::PGPLOT::Window::lines to plot them as hairlines.
If a third argument is given, it is a hash of options, which can be:
nan - if true, use two columns instead of three, and separate lines with a 'nan' break
lonpos - if true, all reported longitudes are positive (0 to 360) instead of (-180 to 180).
dup - if true, the meridian at the far boundary is duplicated.
earth_coast
$x = earth_coast()
(Cartography) PDL constructor - coastline map of Earth
Returns a vector coastline map based on the 1987 CIA World Coastline database (see author information).
The vector coastline data are in plate carree format so they can be converted to other projections via
the apply method and cartographic transforms, and are suitable for plotting with the lines method in the
PGPLOT output library: the first dimension is (X,Y,pen) with breaks having a pen value of 0 and
hairlines having negative pen values. The second dimension broadcasts over all the points in the data
set.
The vector map includes lines that pass through the antipodean meridian, so if you want to plot it
without reprojecting, you should run it through "clean_lines" first:
$w = pgwin();
$w->lines(earth_coast->clean_lines); # plot plate carree map of world
$w->lines(earth_coast->apply(t_gnomonic))# plot gnomonic map of world
"earth_coast" is just a quick-and-dirty way of loading the file "earth_coast.vec.fits" that is part of
the normal installation tree.
earth_image
$rgb = earth_image()
(Cartography) PDL constructor - RGB pixel map of Earth
Returns an RGB image of Earth based on data from the MODIS instrument on the NASA EOS/Terra satellite.
(You can get a full-resolution image from <http://earthobservatory.nasa.gov/Newsroom/BlueMarble/>). The
image is a plate carree map, so you can convert it to other projections via the map method and
cartographic transforms.
This is just a quick-and-dirty way of loading the earth-image files that are distributed along with PDL.
earth_shape
$fits_shape = earth_shape()
(Cartography) PDL constructor - height map of Earth
Returns a height map of Earth based on data from the General Bathymetric Chart of the Oceans (GEBCO)
produced by the British Oceanographic Data Centre. (You can get a full-resolution image from
<http://visibleearth.nasa.gov/view.php?id=73934>). The image is a plate carree map, so you can convert
it to other projections via the map method and cartographic transforms. The data is from 8-bit grayscale
(so only 256 levels), but is returned in a similar format to "earth_image". The range represents a span
of 6400m, so Everest and the Marianas Trench are not accurately represented.
To turn this into a "float", ("lonlatradius,x,y") with "x" and "y" in radians, and the radius as a
"float" as a proportion of the Earth's mean radius, use "t_raster2float". The Earth is treated here as a
perfect sphere with sea level at radius 6,371km.
Value Hex value Float From centre in km Float as radius
Base 00 0.0 6370.69873km 0.99995
Sea level 0C 0.04705 6371km 1.0
Highest FF 1.0 6377.09863km 1.00096
Code:
$shape = earth_shape();
$floats = t_raster2float()->apply($shape->mv(2,0));
$lonlatradius = $floats->slice('0:2'); # r g b all same
$lonlatradius->slice('(2)') *= float((6377.09863 - 6370.69873) / 6371);
$lonlatradius->slice('(2)') += float(6370.69873 / 6371);
clean_lines
$x = clean_lines(t_mercator->apply(scalar(earth_coast())));
$x = clean_lines($line_pen, [threshold]);
$x = $lines->clean_lines;
(Cartography) PDL method - remove projection irregularities
"clean_lines" massages vector data to remove jumps due to singularities in the transform.
In the first (scalar) form, $line_pen contains both (X,Y) points and pen values suitable to be fed to
lines: in the second (list) form, $lines contains the (X,Y) points and $pen contains the pen values.
"clean_lines" assumes that all the outline polylines are local -- that is to say, there are no large
jumps. Any jumps larger than a threshold size are broken by setting the appropriate pen values to 0.
The "threshold" parameter sets the relative size of the largest jump, relative to the map range (as
determined by a min/max operation). The default size is 0.1.
NOTES
This almost never catches stuff near the apex of cylindrical maps, because the anomalous vectors get
arbitrarily small. This could be improved somewhat by looking at individual runs of the pen and using a
relative length scale that is calibrated to the rest of each run. it is probably not worth the
computational overhead.
t_raster2float
$t = t_raster2float();
(Cartography) Convert a raster (3,x,y) to "float" (lonlatrgb,x,y)
Assumes "bytes" input, and radians and "float" output, with the first 2 coordinates suitable for use as
plate carree.
t_raster2fits
$t = t_raster2fits();
(Cartography) Convert a raster (3,x,y) to FITS plate carree (x,y,3)
Adds suitable "hdr". Assumes degrees. Used by "earth_image".
t_unit_sphere
$t = t_unit_sphere(<options>);
(Cartography) 3-D globe projection (conformal; authalic)
This is similar to the inverse of t_spherical, but the inverse transform projects 3-D coordinates onto
the unit sphere, yielding only a 2-D (lon/lat) output. Similarly, the forward transform deprojects 2-D
(lon/lat) coordinates onto the surface of a unit sphere.
The cartesian system has its Z axis pointing through the pole of the (lon,lat) system, and its X axis
pointing through the equator at the prime meridian.
Unit sphere mapping is unusual in that it is both conformal and authalic. That is possible because it
properly embeds the sphere in 3-space, as a notional globe.
This is handy as an intermediate step in lots of transforms, as Cartesian 3-space is cleaner to work with
than spherical 2-space.
Higher dimensional indices are preserved, so that "rider" indices (such as pen value) are propagated.
There is no oblique transform for t_unit_sphere, largely because it's so easy to rotate the output using
t_linear once it's out into Cartesian space. In fact, the other projections implement oblique transforms
by wrapping t_linear with "t_unit_sphere".
OPTIONS:
radius, Radius (default 1.0)
The radius of the sphere, for the inverse transform. (Radius is ignored in the forward transform).
Defaults to 1.0 so that the resulting Cartesian coordinates are in units of "body radii".
t_rot_sphere
$t = t_rot_sphere({origin=>[<theta>,<phi>],roll=>[<roll>]});
(Cartography) Generate oblique projections
You feed in the origin in (theta,phi) and a roll angle, and you get back out (theta', phi') coordinates.
This is useful for making oblique or transverse projections: just compose t_rot_sphere with your
favorite projection and you get an oblique one.
Most of the projections automagically compose themselves with t_rot_sphere if you feed in an origin or
roll angle.
t_rot_sphere converts the base plate carree projection (straight lon, straight lat) to a Cassini
projection.
OPTIONS
STANDARD POSITIONAL OPTIONS
t_orthographic
$t = t_orthographic(<options>);
(Cartography) Ortho. projection (azimuthal; perspective)
This is a perspective view as seen from infinite distance. You can specify the sub-viewer point in
(lon,lat) coordinates, and a rotation angle of the map CW from (north=up). This is equivalent to specify
viewer roll angle CCW from (north=up).
t_orthographic is a convenience interface to t_unit_sphere -- it is implemented as a composition of a
t_unit_sphere call, a rotation, and a slice.
[*] In the default case where the near hemisphere is mapped, the inverse exists. There is no single
inverse for the whole-sphere case, so the inverse transform superimposes everything on a single
hemisphere. If you want an invertible 3-D transform, you want "t_unit_sphere".
OPTIONS
STANDARD POSITIONAL OPTIONS
m, mask, Mask, h, hemisphere, Hemisphere [default 'near']
The hemisphere to keep in the projection (see PDL::Transform::Cartography).
NOTES
Alone of the various projections, this one does not use "t_rot_sphere" to handle the standard options,
because the cartesian coordinates of the rotated sphere are already correctly projected -- t_rot_sphere
would put them back into (theta', phi') coordinates.
t_carree
$t = t_carree(<options>);
(Cartography) Plate Carree projection (cylindrical; equidistant)
This is the simple Plate Carree projection -- also called a "lat/lon plot". The horizontal axis is
theta; the vertical axis is phi. This is a no-op if the angular unit is radians; it is a simple scale
otherwise.
OPTIONS
STANDARD POSITIONAL OPTIONS
s, std, standard, Standard (default 0)
The standard parallel where the transformation is conformal. Conformality is achieved by shrinking of
the horizontal scale to match the vertical scale (which is correct everywhere).
t_mercator
$t = t_mercator(<options>);
(Cartography) Mercator projection (cylindrical; conformal)
This is perhaps the most famous of all map projections: meridians are mapped to parallel vertical lines
and parallels are unevenly spaced horizontal lines. The poles are shifted to +/- infinity. The output
values are in units of globe-radii for easy conversion to kilometers; hence the horizontal extent is -pi
to pi.
You can get oblique Mercator projections by specifying the "origin" or "roll" options; this is
implemented via "t_rot_sphere".
OPTIONS
STANDARD POSITIONAL OPTIONS
c, clip, Clip (default 75 [degrees])
The north/south clipping boundary of the transformation. Because the poles are displaced to infinity,
many applications require a clipping boundary. The value is in whatever angular unit you set with the
standard 'units' option. The default roughly matches interesting landforms on Earth. For no clipping
at all, set b=>0. For asymmetric clipping, use a 2-element list ref or ndarray.
s, std, Standard (default 0)
This is the parallel at which the map has correct scale. The scale is also correct at the parallel of
opposite sign.
t_utm
$t = t_utm(<zone>,<options>);
(Cartography) Universal Transverse Mercator projection (cylindrical)
This is the internationally used UTM projection, with 2 subzones (North/South). The UTM zones are
parametrized individually, so if you want a Zone 30 map you should use t_utm(30). By default you get the
northern subzone, so that locations in the southern hemisphere get negative Y coordinates. If you select
the southern subzone (with the "subzone=>-1" option), you get offset southern UTM coordinates.
The 20-subzone military system is not yet supported. If/when it is implemented, you will be able to
enter "subzone=>[a-t]" to select a N/S subzone.
Note that UTM is really a family of transverse Mercator projections with different central meridia. Each
zone properly extends for six degrees of longitude on either side of its appropriate central meridian,
with Zone 1 being centered at -177 degrees longitude (177 west). Properly speaking, the zones only
extend from 80 degrees south to 84 degrees north; but this implementation lets you go all the way to 90
degrees. The default UTM coordinates are meters. The origin for each zone is on the equator, at an
easting of -500,000 meters.
The default output units are meters, assuming that you are wanting a map of the Earth. This will break
for bodies other than Earth (which have different radii and hence different conversions between lat/lon
angle and meters).
The standard UTM projection has a slight reduction in scale at the prime meridian of each zone: the
transverse Mercator projection's standard "parallels" are 180km e/w of the central meridian. However,
many Europeans prefer the "Gauss-Kruger" system, which is virtually identical to UTM but with a normal
tangent Mercator (standard parallel on the prime meridian). To get this behavior, set "gk=>1".
Like the rest of the PDL::Transform::Cartography package, t_utm uses a spherical datum rather than the
"official" ellipsoidal datums for the UTM system.
This implementation was derived from the rather nice description by Denis J. Dean, located on the web at:
http://www.cnr.colostate.edu/class_info/nr502/lg3/datums_coordinates/utm.html
OPTIONS
STANDARD OPTIONS
(No positional options -- Origin and Roll are ignored)
ou, ounit, OutputUnit (default 'meters')
(This is likely to become a standard option in a future release) The unit of the output map. By
default, this is 'meters' for UTM, but you may specify 'deg' or 'km' or even (heaven help us) 'miles'
if you prefer.
sz, subzone, SubZone (default 1)
Set this to -1 for the southern hemisphere subzone. Ultimately you should be able to set it to a
letter to get the corresponding military subzone, but that's too much effort for now.
gk, gausskruger (default 0)
Set this to 1 to get the (European-style) tangent-plane Mercator with standard parallel on the prime
meridian. The default of 0 places the standard parallels 180km east/west of the prime meridian,
yielding better average scale across the zone. Setting gk=>1 makes the scale exactly 1.0 at the
central meridian, and >1.0 everywhere else on the projection. The difference in scale is about 0.3%.
t_sin_lat
$t = t_sin_lat(<options>);
(Cartography) Cyl. equal-area projection (cyl.; authalic)
This projection is commonly used in solar Carrington plots; but not much for terrestrial mapping.
OPTIONS
STANDARD POSITIONAL OPTIONS
s,std, Standard (default 0)
This is the parallel at which the map is conformal. It is also conformal at the parallel of opposite
sign. The conformality is achieved by matched vertical stretching and horizontal squishing (to
achieve constant area).
t_sinusoidal
$t = t_sinusoidal(<options>);
(Cartography) Sinusoidal projection (authalic)
Sinusoidal projection preserves the latitude scale but scales longitude according to sin(lat); in this
respect it is the companion to "t_sin_lat", which is also authalic but preserves the longitude scale
instead.
OPTIONS
STANDARD POSITIONAL OPTIONS
t_conic
$t = t_conic(<options>)
(Cartography) Simple conic projection (conic; equidistant)
This is the simplest conic projection, with parallels mapped to equidistant concentric circles. It is
neither authalic nor conformal. This transformation is also referred to as the "Modified Transverse
Mercator" projection in several maps of Alaska published by the USGS; and the American State of New
Mexico re-invented the projection in 1936 for an official map of that State.
OPTIONS
STANDARD POSITIONAL OPTIONS
s, std, Standard (default 29.5, 45.5)
The locations of the standard parallel(s) (where the cone intersects the surface of the sphere). If
you specify only one then the other is taken to be the nearest pole. If you specify both of them to
be one pole then you get an equidistant azimuthal map. If you specify both of them to be opposite and
equidistant from the equator you get a Plate Carree projection.
t_albers
$t = t_albers(<options>)
(Cartography) Albers conic projection (conic; authalic)
This is the standard projection used by the US Geological Survey for sectionals of the 50 contiguous
United States of America.
The projection reduces to the Lambert equal-area conic (infrequently used and not to be confused with the
Lambert conformal conic, "t_lambert"!) if the pole is used as one of the two standard parallels.
Notionally, this is a conic projection onto a cone that intersects the sphere at the two standard
parallels; it works best when the two parallels straddle the region of interest.
OPTIONS
STANDARD POSITIONAL OPTIONS
s, std, standard, Standard (default (29.5,45.5))
The locations of the standard parallel(s). If you specify only one then the other is taken to be the
nearest pole and a Lambert Equal-Area Conic map results. If you specify both standard parallels to be
the same pole, then the projection reduces to the Lambert Azimuthal Equal-Area map as aq special case.
(Note that "t_lambert" is Lambert's Conformal Conic, the most commonly used of Lambert's projections.)
The default values for the standard parallels are those chosen by Adams for maps of the lower 48 US
states: (29.5,45.5). The USGS recommends (55,65) for maps of Alaska and (8,18) for maps of Hawaii --
these latter are chosen to also include the Canal Zone and Philippine Islands farther south, which is
why both of those parallels are south of the Hawaiian islands.
The transformation reduces to the cylindrical equal-area (sin-lat) transformation in the case where
the standard parallels are opposite and equidistant from the equator, and in fact this is implemented
by a call to t_sin_lat.
t_lambert
$t = t_lambert(<options>);
(Cartography) Lambert conic projection (conic; conformal)
Lambert conformal conic projection is widely used in aeronautical charts and state base maps published by
the USA's FAA and USGS. It's especially useful for mid-latitude charts. In particular, straight lines
approximate (but are not exactly) great circle routes of up to ~2 radians.
The default standard parallels are 33 and 45 to match the USGS state 1:500,000 base maps of the United
States. At scales of 1:500,000 and larger, discrepancies between the spherical and ellipsoidal
projections become important; use care with this projection on spheres.
OPTIONS
STANDARD POSITIONAL OPTIONS
s, std, standard, Standard (default (33,45))
The locations of the standard parallel(s) for the conic projection. The transform reduces to the
Mercator projection in the case where the standard parallels are opposite and equidistant from the
equator, and in fact this is implemented by a call to t_mercator.
c, clip, Clip (default [-75,75])
Because the transform is conformal, the distant pole is displaced to infinity. Many applications
require a clipping boundary. The value is in whatever angular unit you set with the standard 'unit'
option. For consistency with "t_mercator", clipping works the same way even though in most cases only
one pole needs it. Set this to 0 for no clipping at all.
t_stereographic
$t = t_stereographic(<options>);
(Cartography) Stereographic projection (az.; conf.; persp.)
The stereographic projection is a true perspective (planar) projection from a point on the spherical
surface opposite the origin of the map.
OPTIONS
STANDARD POSITIONAL OPTIONS
c, clip, Clip (default 120)
This is the angular distance from the center to the edge of the projected map. The default 120
degrees gives you most of the opposite hemisphere but avoids the hugely distorted part near the
antipodes.
t_gnomonic
$t = t_gnomonic(<options>);
(Cartography) Gnomonic (focal-plane) projection (az.; persp.)
The gnomonic projection projects a hemisphere onto a tangent plane. It is useful in cartography for the
property that straight lines are great circles; and it is useful in scientific imaging because it is the
projection generated by a simple optical system with a flat focal plane.
OPTIONS
STANDARD POSITIONAL OPTIONS
c, clip, Clip (default 75)
This is the angular distance from the center to the edge of the projected map. The default 75 degrees
gives you most of the hemisphere but avoids the hugely distorted part near the horizon.
t_az_eqd
$t = t_az_eqd(<options>);
(Cartography) Azimuthal equidistant projection (az.; equi.)
Basic azimuthal projection preserving length along radial lines from the origin (meridians, in the
original polar aspect). Hence, both azimuth and distance are correct for journeys beginning at the
origin.
Applied to the celestial sphere, this is the projection made by fisheye lenses; it is also the projection
into which "t_vertical" puts perspective views.
The projected plane scale is normally taken to be planetary radii; this is useful for cartographers but
not so useful for scientific observers. Setting the 't=>1' option causes the output scale to shift to
camera angular coordinates (the angular unit is determined by the standard 'Units' option; default is
degrees).
OPTIONS
STANDARD POSITIONAL OPTIONS
c, clip, Clip (default 180 degrees)
The largest angle relative to the origin. Default is the whole sphere.
t_az_eqa
$t = t_az_eqa(<options>);
(Cartography) Azimuthal equal-area projection (az.; auth.)
OPTIONS
STANDARD POSITIONAL OPTIONS
c, clip, Clip (default 180 degrees)
The largest angle relative to the origin. Default is the whole sphere.
t_aitoff
"t_aitoff" in an alias for "t_hammer"
t_hammer
(Cartography) Hammer/Aitoff elliptical projection (az.; auth.)
The Hammer/Aitoff projection is often used to display the Celestial sphere. It is mathematically related
to the Lambert Azimuthal Equal-Area projection ("t_az_eqa"), and maps the sphere to an ellipse of unit
eccentricity, with vertical radius sqrt(2) and horizontal radius of 2 sqrt(2).
OPTIONS
STANDARD POSITIONAL OPTIONS
t_zenithal
Vertical projections are also called "zenithal", and "t_zenithal" is an alias for "t_vertical".
t_vertical
$t = t_vertical(<options>);
(Cartography) Vertical perspective projection (az.; persp.)
Vertical perspective projection is a generalization of gnomonic and stereographic projection, and a
special case of perspective projection. It is a projection from the sphere onto a tangent plane from a
point at the camera location.
OPTIONS
STANDARD POSITIONAL OPTIONS
m, mask, Mask, h, hemisphere, Hemisphere [default 'near']
The hemisphere to keep in the projection (see PDL::Transform::Cartography).
r0, R0, radius, d, dist, distance [default 2.0]
The altitude of the focal plane above the center of the sphere. The default places the point of view
one radius above the surface.
t, telescope, Telescope, cam, Camera (default '')
If this is set, then the central scale is in telescope or camera angular units rather than in
planetary radii. The angular units are parsed as with the normal 'u' option for the lon/lat
specification. If you specify a non-string value (such as 1) then you get telescope-frame radians,
suitable for working on with other transformations.
f, fish, fisheye (default '')
If this is set then the output is in azimuthal equidistant coordinates instead of in tangent-plane
coordinates. This is a convenience function for '(t_az_eqd) x !(t_gnomonic) x (t_vertical)'.
t_perspective
$t = t_perspective(<options>);
(Cartography) Arbitrary perspective projection
Perspective projection onto a focal plane from an arbitrary location within or without the sphere, with
an arbitrary central look direction, and with correction for magnification within the optical system.
In the forward direction, t_perspective generates perspective views of a sphere given (lon/lat) mapping
or vector information. In the reverse direction, t_perspective produces (lon/lat) maps from aerial or
distant photographs of spherical objects.
Viewpoints outside the sphere treat the sphere as opaque by default, though you can use the 'm' option to
specify either the near or far surface (relative to the origin). Viewpoints below the surface treat the
sphere as transparent and undergo a mirror reversal for consistency with projections that are special
cases of the perspective projection (e.g. t_gnomonic for r0=0 or t_stereographic for r0=-1).
Magnification correction handles the extra edge distortion due to higher angles between the focal plane
and focused rays within the optical system of your camera. If you do not happen to know the
magnification of your camera, a simple rule of thumb is that the magnification of a reflective telescope
is roughly its focal length (plate scale) divided by its physical length; and the magnification of a
compound refractive telescope is roughly twice its physical length divided by its focal length. Simple
optical systems with a single optic have magnification = 1. Fisheye lenses have magnification < 1.
This transformation was derived by direct geometrical calculation rather than being translated from
Voxland & Snyder.
OPTIONS
STANDARD POSITIONAL OPTIONS
As always, the 'origin' field specifies the sub-camera point on the sphere.
The 'roll' option is the roll angle about the sub-camera point, for consistency with the other
projectons.
p, ptg, pointing, Pointing (default (0,0,0))
The pointing direction, in (horiz. offset, vert. offset, roll) of the camera relative to the center of
the sphere. This is a spherical coordinate system with the origin pointing directly at the sphere and
the pole pointing north in the pre-rolled coordinate system set by the standard origin. It's most
useful for space-based images taken some distance from the body in question (e.g. images of other
planets or the Sun).
Be careful not to confuse 'p' (pointing) with 'P' (P angle, a standard synonym for roll).
c, cam, camera, Camera (default undef)
Alternate way of specifying the camera pointing, using a spherical coordinate system with poles at the
zenith (positive) and nadir (negative) -- this is useful for aerial photographs and such, where the
point of view is near the surface of the sphere. You specify (azimuth from N, altitude from
horizontal, roll from vertical=up). If you specify pointing by this method, it overrides the
'pointing' option, above. This coordinate system is most useful for aerial photography or low-orbit
work, where the nadir is not necessarily the most interesting part of the scene.
r0, R0, radius, d, dist, distance [default 2.0]
The altitude of the point of view above the center of the sphere. The default places the point of
view 1 radius aboove the surface. Do not confuse this with 'r', the standard origin roll angle!
Setting r0 < 1 gives a viewpoint inside the sphere. In that case, the images are mirror-reversed to
preserve the chiralty of the perspective. Setting r0=0 gives gnomonic projections; setting r0=-1
gives stereographic projections. Setting r0 < -1 gives strange results.
iu, im_unit, image_unit, Image_Unit (default 'degrees')
This is the angular units in which the viewing camera is calibrated at the center of the image.
mag, magnification, Magnification (default 1.0)
This is the magnification factor applied to the optics -- it affects the amount of tangent-plane
distortion within the telescope. 1.0 yields the view from a simple optical system; higher values are
telescopic, while lower values are wide-angle (fisheye). Higher magnification leads to higher angles
within the optical system, and more tangent-plane distortion at the edges of the image. The
magnification is applied to the incident angles themselves, rather than to their tangents (simple two-
element telescopes magnify tan(theta) rather than theta itself); this is appropriate because wide-
field optics more often conform to the equidistant azimuthal approximation than to the tangent plane
approximation. If you need more detailed control of the relationship between incident angle and
focal-plane position, use mag=1.0 and compose the transform with something else to tweak the angles.
m, mask, Mask, h, hemisphere, Hemisphere [default 'near']
'hemisphere' is by analogy to other cartography methods although the two regions to be selected are
not really hemispheres.
f, fov, field_of_view, Field_Of_View [default 60 degrees]
The field of view of the telescope -- sets the crop radius on the focal plane. If you pass in a
scalar, you get a circular crop. If you pass in a 2-element list ref, you get a rectilinear crop,
with the horizontal 'radius' and vertical 'radius' set separately.
EXAMPLES
Model a camera looking at the Sun through a 10x telescope from Earth (~230 solar radii from the Sun),
with an 0.5 degree field of view and a solar P (roll) angle of 30 degrees, in February (sub-Earth solar
latitude is 7 degrees south). Convert a solar FITS image taken with that camera to a FITS lon/lat map of
the Sun with 20 pixels/degree latitude:
# Define map output header (no need if you don't want a FITS output map)
$maphdr = {NAXIS1=>7200,NAXIS2=>3600, # Size of image
CTYPE1=>longitude,CTYPE2=>latitude, # Type of axes
CUNIT1=>deg,CUNIT2=>deg, # Unit of axes
CDELT1=>0.05,CDELT2=>0.05, # Scale of axes
CRPIX1=>3601,CRPIX2=>1801, # Center of map
CRVAL1=>0,CRVAL2=>0 # (lon,lat) of center
};
# Set up the perspective transformation, and apply it.
$t = t_perspective(r0=>229,fov=>0.5,mag=>10,P=>30,B=>-7);
$map = $im->map( $t , $maphdr );
Draw an aerial-view map of the Chesapeake Bay, as seen from a sounding rocket at an altitude of 100km,
looking NNE from ~200km south of Washington (the radius of Earth is 6378 km; Washington D.C. is at
roughly 77W,38N). Superimpose a linear coastline map on a photographic map.
$x = graticule(1,0.1)->glue(1,earth_coast());
$t = t_perspective(r0=>6478/6378.0,fov=>60,cam=>[22.5,-20],o=>[-77,36])
$w = pgwin(size=>[10,6],J=>1);
$w->fits_imag(earth_image()->map($t,[800,500],{m=>linear}));
$w->hold;
$w->lines($x->apply($t),{xt=>'Degrees',yt=>'Degrees'});
$w->release;
Model a 5x telescope looking at Betelgeuse with a 10 degree field of view (since the telescope is looking
at the Celestial sphere, r is 0 and this is just an expensive modified-gnomonic projection).
$t = t_perspective(r0=>0,fov=>10,mag=>5,o=>[88.79,7.41])
perl v5.38.2 2024-04-10 Cartography(3pm)