# mapproject¶

Forward and inverse map transformations, datum conversions and geodesy

## Synopsis¶

**gmt mapproject** [ *table* ] **-J***parameters*
**-R***region*
[ **-A****b**|**B**|**f**|**F**|**o**|**O**[*lon0*/*lat0*][**+v**] ]
[ **-C**[*dx*/*dy*][**+m**] ]
[ **-D****c**|**i**|**p** ]
[ **-E**[*datum*] ]
[ **-F**[**e**|**f**|**k**|**M**|**n**|**u**|**c**|**i**|**p**] ]
[ **-G**[*lon0*/*lat0*][**+a**][**+i**][**+u***unit*][**+v**] ]
[ **-I** ]
[ **-L***table*[**+p**][**+u***unit*] ]
[ **-N**[**a**|**c**|**g**|**m**] ]
[ **-Q**[**d**|**e**] ]
[ **-S** ]
[ **-T**[**h**]*from*[/*to*] ]
[ **-V**[*level*] ]
[ **-W**[**g**|**h**|**j**|**n**|**r**|**R**|**w**|**x**] ]
[ **-Z**[*speed*][**+a**][**+i**][**+f**][**+t***epoch*] ]
[ **-b**binary ]
[ **-d**nodata ]
[ **-e**regexp ]
[ **-f**flags ]
[ **-g**gaps ]
[ **-h**headers ]
[ **-i**flags ]
[ **-j**flags ]
[ **-o**flags ]
[ **-p**flags ]
[ **-q**flags ]
[ **-s**flags ]
[ **-:**[**i**|**o**] ]
[ **--PAR**=*value* ]

**Note:** No space is allowed between the option flag and the associated arguments.

## Description¶

**mapproject** reads (longitude, latitude) positions from *tables* [or
standard input] and computes (x,y) coordinates using the specified map
projection and scales. Optionally, it can read (x,y) positions and
compute (longitude, latitude) values doing the inverse transformation.
This can be used to transform linear (x,y) points obtained by digitizing
a map of known projection to geographical coordinates. May also
calculate distances along track, to a fixed point, or closest approach
to a line.
Alternatively, can be used to perform various datum conversions.
Additional data fields are permitted after the first 2 columns which
must have (longitude,latitude) or (x,y). See option **-:** on how to
read (latitude,longitude) files.
Finally, **mapproject** can compute a variety of auxiliary output
data from input coordinates that make up a track. Items like
azimuth, distances, distances to other lines, and travel-times
along lines can all be computed by using one or more of the options
**-A**, **-G**, **-L**, and **-Z**.

## Required Arguments¶

*table*One or more ASCII (or binary, see

**-bi**[*ncols*][*type*]) data table file(s) holding a number of data columns. If no tables are given then we read from standard input.

**-J***parameters*Specify the projection. (See full description) (See cookbook summary) (See projections table).

**-R***xmin*/*xmax*/*ymin*/*ymax*[**+r**][**+u***unit*]Specify the region of interest. Special case for the UTM projection: If

**-C**is used and**-R**is not given then the region is set to coincide with the given UTM zone so as to preserve the full ellipsoidal solution (See Restrictions for more information). (See full description) (See cookbook information).

## Optional Arguments¶

**-Ab**|**B**|**f**|**F**|**o**|**O**[*lon0*/*lat0*][**+v**]Calculate azimuth along track

*or*to the optional*fixed*point set with*lon0/lat0*.**-Af**calculates the (forward) azimuth to each data point. Use**-Ab**to get back-azimuth from data points to fixed point. Use**-Ao**to get orientations (-90/90) rather than azimuths (0/360). Upper case**F**,**B**or**O**will convert from geodetic to geocentric latitudes and estimate azimuth of geodesics (assuming the current ellipsoid is not a sphere). If no fixed point is given then we compute the azimuth (or back-azimuth) from the previous point. Alternatively, append**+v**to obtain a*variable*2nd point (*lon0*/*lat0*) via columns 3-4 in the input file. See Output Order for how**-A**affects the output record. If**-R**and**-J**are given the we project the coordinates first and then compute Cartesian angles instead.

**-C**[*dx*/*dy*][**+m**]Set center of projected coordinates to be at map projection center [Default is lower left corner]. Optionally, add offsets in the projected units to be added (or subtracted when

**-I**is set) to (from) the projected coordinates, such as false eastings and northings for particular projection zones [0/0]. The unit used for the offsets is the plot distance unit in effect (see PROJ_LENGTH_UNIT) unless**-F**is used, in which case the offsets are in meters. Alternatively, for the Mercator projection only, append**+m**to set the origin of the projected*y*coordinates to coincide with the standard parallel [Equator].

**-Dc**|**i**|**p**Temporarily override PROJ_LENGTH_UNIT and use

**c**(cm),**i**(inch), or**p**(points) instead. Cannot be used with**-F**.

**-E**[*datum*]Convert from geodetic (lon, lat, height) to Earth Centered Earth Fixed (ECEF) (x,y,z) coordinates (add

**-I**for the inverse conversion). Append datum ID (see**-Qd**) or give*ellipsoid*:*dx*,*dy*,*dz*where*ellipsoid*may be an ellipsoid ID (see**-Qe**) or given as*a*[,*inv_f*], where*a*is the semi-major axis and*inv_f*is the inverse flattening (0 if omitted). If*datum*is - or not given we assume WGS-84.

**-F**[**e**|**f**|**k**|**M**|**n**|**u**|**c**|**i**|**p**]Force 1:1 scaling, i.e., output (or input, see

**-I**) data are in actual projected meters. To specify other units, append the desired unit (see Units). Without**-F**, the output (or input, see**-I**) are in the units specified by PROJ_LENGTH_UNIT (but see**-D**).

**-G**[*lon0*/*lat0*][**+a**][**+i**][**+u***unit*][**+v**]Calculate distances along track

*or*to the optional*fixed*point set with**-G***lon0*/*lat0*. Append the distance unit with**+u**(see Units for available units and how distances are computed [great circle using authalic radius]), including**c**(Cartesian distance using input coordinates) or**C**(Cartesian distance using projected coordinates). The**C**unit requires**-R**and**-J**to be set and all output coordinates will be reported as projected. If no fixed point is given we calculate*accumulated*distances whereas if a fixed point is given we calculate*incremental*distances. You can override these defaults by adding**+a**for accumulated or**+i**for incremental distances. If both**+a**and**+i**are given we will report both types of distances. Append**+v**to obtain a*variable*2nd point (*lon0*/*lat0*) via columns 3-4 in the input file; this updates the fixed point per record and thus the selection defaults to incremental distances. See Output Order for how**-G**affects the output record.

**-I**Do the Inverse transformation, i.e., get (longitude,latitude) from (x,y) data.

**-L***table*[**+p**][**+u***unit*|*c*|*C*]Determine the shortest distance from the input data points to the line(s) given in the ASCII multisegment file

*table*. The distance and the coordinates of the nearest point will be appended to the output as three new columns. Append the distance unit via**+u**(see Units for available units and how distances are computed [great circle using authalic radius]), including**c**(Cartesian distance using input coordinates) or**C**(Cartesian distance using projected coordinates). Note that these**c**and**C**are not listed in Units and would be used for example as**+uc**. The**C**unit requires**-R**and**-J**to be set. Finally, append**+p**to report the line segment id and the fractional point number instead of lon/lat of the nearest point. See Output Order for how**-L**affects the output record.**Note**: Calculation mode for geographic data is spherical, hence**-je**cannot be used in combination with**-L**.

**-N**[**a**|**c**|**g**|**m**]Convert from geodetic latitudes (using the current ellipsoid; see PROJ_ELLIPSOID) to one of four different auxiliary latitudes (longitudes are unaffected). Choose from

**a**uthalic,**c**onformal,**g**eocentric, and**m**eridional latitudes [geocentric]. Use**-I**to convert from auxiliary latitudes to geodetic latitudes.

**-Q**[**d**|**e**]List all projection parameters. To only list datums, use

**-Qd**. To only list ellipsoids, use**-Qe**.

**-S**Suppress points that fall outside the region.

**-T**[**h**]*from*[/*to*]Coordinate conversions between datums

*from*and*to*using the standard Molodensky transformation. Use**-Th**if 3rd input column has height above ellipsoid [Default assumes height = 0, i.e., on the ellipsoid]. Specify datums using the datum ID (see**-Qd**) or give*ellipsoid*:*dx*,*dy*,*dz*where*ellipsoid*may be an ellipsoid ID (see**-Qe**) or given as*a*[,*inv_f*], where*a*is the semi-major axis and*inv_f*is the inverse flattening (0 if omitted). If*datum*is - or not given we assume WGS-84.**-T**may be used in conjunction with**-R****-J**to change the datum before coordinate projection (add**-I**to apply the datum conversion after the inverse projection). Make sure that the PROJ_ELLIPSOID setting is correct for your case.

**-V**[*level*]Select verbosity level [

**w**]. (See full description) (See cookbook information).

**-W**[**g**|**h**|**j**|**n**|**r**|**R**|**w**|**x**]Prints map width and height on standard output. No input files are read. To only output the width or the height, append

**w**or**h**, respectively. To output the plot coordinates of a map point, give**g***lon*/*lat*. The units of reported plot dimensions may be changed via**-D**. To output the map coordinates of a reference point, select**j***code*(with standard two-character justification codes),**n***rx*/*ry*, where the reference point is given as normalized positions in the 0-1 range, or**x***px*/*py*, where a plot point is given directly. To output the rectangular domain that covers an oblique area as defined by**-R -J**, append**r**, or use**R**to get the result in -Rw/e/s/n string format [Default returns the width and height of the map].

**-Z**[*speed*][**+a**][**+i**][**+f**][**+t***epoch*]Calculate travel times along track as specified with

**-G**. Append a constant speed unit; if missing we expect to read a variable speed from column 3. The speed is expected to be in the distance units set via**-G**per time unit controlled by TIME_UNIT [m/s]. Append**+i**to output*incremental*travel times between successive points,**+a**to obtain*accumulated*travel times, or both to get both kinds of time information. Use**+f**to format the accumulated (elapsed) travel time according to the ISO 8601 convention. As for the number of decimals used to represent seconds we consult the FORMAT_CLOCK_OUT setting. Finally, append**+t***epoch*to report absolute times (ETA) for successive points. Finally, because of the need for incremental distances the**-G**option with the**+i**modifier is required. See Output Order for how**-Z**affects the output record.

**-bi***record*[**+b**|**l**] (more …)Select native binary format for primary table input. [Default is 2 input columns].

**-bo***record*[**+b**|**l**] (more …)Select native binary format for table output. [Default is same as input].

**-d**[**i**|**o**]*nodata*(more …)Replace input columns that equal

*nodata*with NaN and do the reverse on output.

**-e**[**~**]*“pattern”*|**-e**[**~**]/*regexp*/[**i**] (more …)Only accept data records that match the given pattern.

**-f**[**i**|**o**]*colinfo*(more …)Specify data types of input and/or output columns.

**-g****x**|**y**|**z**|**d**|**X**|**Y**|**D***gap*[**u**][**+a**][**+c***col*][**+n**|**p**] (more …)Determine data gaps and line breaks.

**-h**[**i**|**o**][*n*][**+c**][**+d**][**+m***segheader*][**+r***remark*][**+t***title*] (more …)Skip or produce header record(s).

**-i***cols*[**+l**][**+d***divisor*][**+s***scale*][**+o***offset*][,*…*][,**t**[*word*]] (more …)Select input columns and transformations (0 is first column,

**t**is trailing text, append*word*to read one word only).

**-je**|**f**|**g**(more …)Determine how spherical distances are calculated.

**-o***cols*[,…][,**t**[*word*]] (more …)Select output columns (0 is first column;

**t**is trailing text, append*word*to write one word only).

**-p**[**x**|**y**|**z**]*azim*[/*elev*[/*zlevel*]][**+w***lon0*/*lat0*[/*z0*]][**+v***x0*/*y0*] (more …)Select perspective view.

**-q**[**i**|**o**][~]*rows*|*limits*[**+c***col*][**+a**|**f**|**s**] (more …)Select input or output rows or data limit(s) [all].

**-s**[*cols*][**+a**][**+r**] (more …)Set handling of NaN records for output.

**-:**[**i**|**o**] (more …)Swap 1st and 2nd column on input and/or output.

**-^**or just**-**Print a short message about the syntax of the command, then exit (NOTE: on Windows just use

**-**).**-+**or just**+**Print an extensive usage (help) message, including the explanation of any module-specific option (but not the GMT common options), then exit.

**-?**or no argumentsPrint a complete usage (help) message, including the explanation of all options, then exit.

**--PAR**=*value*Temporarily override a GMT default setting; repeatable. See gmt.conf for parameters.

## Units¶

For map distance unit, append *unit* **d** for arc degree, **m** for arc
minute, and **s** for arc second, or **e** for meter [Default], **f**
for foot, **k** for km, **M** for statute mile, **n** for nautical mile,
and **u** for US survey foot. By default we compute such distances using
a spherical approximation with great circles (**-jg**) using the authalic radius
(see PROJ_MEAN_RADIUS). You can use **-jf** to perform
“Flat Earth” calculations (quicker but less accurate) or **-je** to perform
exact geodesic calculations (slower but more accurate; see
PROJ_GEODESIC for method used).

## ASCII Format Precision¶

The ASCII output formats of numerical data are controlled by parameters
in your gmt.conf file. Longitude and latitude are formatted
according to FORMAT_GEO_OUT, absolute time is
under the control of FORMAT_DATE_OUT and
FORMAT_CLOCK_OUT, whereas general floating point values are formatted
according to FORMAT_FLOAT_OUT. Be aware that the format in effect
can lead to loss of precision in ASCII output, which can lead to various
problems downstream. If you find the output is not written with enough
precision, consider switching to binary output (**-bo** if available) or
specify more decimals using the FORMAT_FLOAT_OUT setting.

## Examples¶

**Note**: Below are some examples of valid syntax for this module.
The examples that use remote files (file names starting with `@`

)
can be cut and pasted into your terminal for testing.
Other commands requiring input files are just dummy examples of the types
of uses that are common but cannot be run verbatim as written.

To transform a remote file with (latitude,longitude) into (x,y) positions in cm on a Mercator grid for a given scale of 0.5 cm per degree and selected region, run

gmt mapproject @waypoints.txt -R-180/180/-72/72 -Jm0.5c -: > xyfile

To convert UTM coordinates in meters to geographic locations, given a file utm.txt and knowing the UTM zone (and zone or hemisphere), try

gmt mapproject utm.txt -Ju+11/1:1 -C -I -F

To transform several 2-column, binary, double precision files with (latitude,longitude) into (x,y) positions in inch on a Transverse Mercator grid (central longitude 75W) for scale = 1:500000 and suppress those points that would fall outside the map area, run

gmt mapproject tracks.* -R-80/-70/20/40 -Jt-75/1:500000 -: -S -Di -bo -bi2 > tmfile.b

To convert the geodetic coordinates (lon, lat, height) in the file old.txt from the NAD27 CONUS datum (Datum ID 131 which uses the Clarke-1866 ellipsoid) to WGS 84, run

gmt mapproject old.txt -Th131 > new.txt

To compute the closest distance (in km) between each point in the input file quakes.txt and the line segments given in the multisegment ASCII file coastline.txt, run

gmt mapproject quakes.txt -Lcoastline.txt+uk > quake_dist.txt

Given a file with longitude and latitude, compute both incremental and accumulated distance along track, and estimate travel times assuming a fixed speed of 12 knots. We do this with

`gmt mapproject track.txt -G+un+a+i -Z12+a --TIME_UNIT=h > elapsed_time.txt`

where TIME_UNIT is set to hour so that the speed is
measured in nm (set by **-G**) per hour (set by TIME_UNIT).
Elapsed times will be reported in hours (unless **+f** is added to **-Z**
for ISO elapsed time).

To determine the geographic coordinates of the mid-point of this transverse Mercator map, try

gmt mapproject -R-80/-70/20/40 -Jt-75/1:500000 -WjCM > mid_point.txt

To determine the rectangular region that encompasses the oblique region defined by an oblique Mercator projection, try

gmt mapproject -R270/20/305/25+r -JOc280/25.5/22/69/2c -WR

## Restrictions¶

The rectangular input region set with **-R** will in general be mapped
into a non-rectangular grid. Unless **-C** is set, the leftmost point on
this grid has xvalue = 0.0, and the lowermost point will have yvalue =
0.0. Thus, before you digitize a map, run the extreme map coordinates
through **mapproject** using the appropriate scale and see what (x,y)
values they are mapped onto. Use these values when setting up for
digitizing in order to have the inverse transformation work correctly,
or alternatively, use **awk** to scale and shift the (x,y) values before
transforming.

For some projection, a spherical solution may be used despite the user
having selected an ellipsoid. This occurs when the users **-R** setting
implies a region that exceeds the domain in which the ellipsoidal series
expansions are valid. These are the conditions: (1) Lambert Conformal
Conic (**-JL**)and Albers Equal-Area (**-JB**) will use the spherical
solution when the map scale exceeds 1.0E7. (2) Transverse Mercator
(**-JT**) and UTM (**-JU**) will will use the spherical solution when
either the west or east boundary given in **-R** is more than 10 degrees
from the central meridian, and (3) same for Cassini
(**-JC**) but with a limit of only 4 degrees.

## Ellipsoids And Spheroids¶

GMT will use ellipsoidal formulae if they are implemented and the user have selected an ellipsoid as the reference shape (see PROJ_ELLIPSOID). The user needs to be aware of a few potential pitfalls: (1) For some projections, such as Transverse Mercator, Albers, and Lambert’s conformal conic we use the ellipsoidal expressions when the areas mapped are small, and switch to the spherical expressions (and substituting the appropriate auxiliary latitudes) for larger maps. The ellipsoidal formulae are used as follows: (a) Transverse Mercator: When all points are within 10 degrees of central meridian, (b) Conic projections when longitudinal range is less than 90 degrees, (c) Cassini projection when all points are within 4 degrees of central meridian. (2) When you are trying to match some historical data (e.g., coordinates obtained with a certain projection and a certain reference ellipsoid) you may find that GMT gives results that are slightly different. One likely source of this mismatch is that older calculations often used less significant digits. For instance, Snyder’s examples often use the Clarke 1866 ellipsoid (defined by him as having a flattening f = 1/294.98). From f we get the eccentricity squared to be 0.00676862818 (this is what GMT uses), while Snyder rounds off and uses 0.00676866. This difference can give discrepancies of several tens of cm. If you need to reproduce coordinates projected with this slightly different eccentricity, you should specify your own ellipsoid with the same parameters as Clarke 1866, but with f = 1/294.97861076. Also, be aware that older data may be referenced to different datums, and unless you know which datum was used and convert all data to a common datum you may experience mismatches of tens to hundreds of meters. (3) Finally, be aware that PROJ_SCALE_FACTOR have certain default values for some projections so you may have to override the setting in order to match results produced with other settings.

## Output Order¶

The production order for the geodetic and temporal columns produced by the
options **-A**, **-G**, **-L**, and **-Z** is fixed and follows the
alphabetical order of the options. Hence, the order these options
appear on the command line is irrelevant. The actual output order
can of course be modulated via **-o**.

## References¶

Bomford, G., 1952, Geodesy, Oxford U. Press.

Snyder, J. P., 1987, Map Projections - A Working Manual, U.S. Geological Survey Prof. Paper 1395.

Vanicek, P. and Krakiwsky, E, 1982, Geodesy - The Concepts, North-Holland Publ., ISBN: 0 444 86149 1.