Ubuntu Manpage: RhumbSolve -- perform rhumb line calculations

Provided by: geographiclib-tools_1.45-2_amd64

NAME

       RhumbSolve -- perform rhumb line calculations

SYNOPSIS

       RhumbSolve [ -i | -l lat1 lon1 azi12 ] [ -e a f ] [ -d | -: ] [ -w ] [ -p prec ] [ -s ] [
       --comment-delimiter commentdelim ] [ --version | -h | --help ] [ --input-file infile | --input-string
       instring ] [ --line-separator linesep ] [ --output-file outfile ]

DESCRIPTION

The path with constant heading between two points on the ellipsoid at (lat1, lon1) and (lat2, lon2) is
called the rhumb line or loxodrome. Its length is s12 and the rhumb line has a forward azimuth azi12
along its length. Also computed is S12 is the area between the rhumb line from point 1 to point 2 and
the equator; i.e., it is the area, measured counter-clockwise, of the geodesic quadrilateral with corners
(lat1,lon1), (0,lon1), (0,lon2), and (lat2,lon2). A point at a pole is treated as a point a tiny
distance away from the pole on the given line of longitude. The longitude becomes indeterminate when a
rhumb line passes through a pole, and RhumbSolve reports NaNs for the longitude and the area in this
case.

NOTE: the rhumb line is not the shortest path between two points; that is the geodesic and it is
calculated by GeodSolve(1).

RhumbSolve operates in one of three modes:

1. By default, RhumbSolve accepts lines on the standard input containing lat1 lon1 azi12 s12 and prints
lat2 lon2 S12 on standard output. This is the direct calculation.

2. Command line arguments -l lat1 lon1 azi12 specify a rhumb line. RhumbSolve then accepts a sequence
of s12 values (one per line) on standard input and prints lat2 lon2 S12 for each. This generates a
sequence of points on a rhumb line.

3. With the -i command line argument, RhumbSolve performs the inverse calculation. It reads lines
containing lat1 lon1 lat2 lon2 and prints the values of azi12 s12 S12 for the corresponding shortest
rhumb lines. If the end points are on opposite meridians, there are two shortest rhumb lines and the
east-going one is chosen.

OPTIONS

-i perform an inverse calculation (see 3 above).

-l line mode (see 2 above); generate a sequence of points along the rhumb line specified by lat1 lon1
azi12. The -w flag can be used to swap the default order of the 2 geographic coordinates, provided
that it appears before -l.

-e specify the ellipsoid via a f; the equatorial radius is a and the flattening is f. Setting f = 0
results in a sphere. Specify f < 0 for a prolate ellipsoid. A simple fraction, e.g., 1/297, is
allowed for f. By default, the WGS84 ellipsoid is used, a = 6378137 m, f = 1/298.257223563.

-d output angles as degrees, minutes, seconds instead of decimal degrees.

-: like -d, except use : as a separator instead of the d, ', and " delimiters.

-w on input and output, longitude precedes latitude (except that on input this can be overridden by a
hemisphere designator, N, S, E, W).

-p set the output precision to prec (default 3); prec is the precision relative to 1 m. See
"PRECISION".

-s By default, the rhumb line calculations are carried out exactly in terms of elliptic integrals. This
includes the use of the addition theorem for elliptic integrals to compute the divided difference of
the isometric and rectifying latitudes. If -s is supplied this divided difference is computed using
Krueger series for the transverse Mercator projection which is only accurate for |f| < 0.01. See
"ACCURACY".

--comment-delimiter
set the comment delimiter to commentdelim (e.g., "#" or "//"). If set, the input lines will be
scanned for this delimiter and, if found, the delimiter and the rest of the line will be removed
prior to processing and subsequently appended to the output line (separated by a space).

--version
print version and exit.

-h print usage and exit.

--help
print full documentation and exit.

--input-file
read input from the file infile instead of from standard input; a file name of "-" stands for
standard input.

--input-string
read input from the string instring instead of from standard input. All occurrences of the line
separator character (default is a semicolon) in instring are converted to newlines before the reading
begins.

--line-separator
set the line separator character to linesep. By default this is a semicolon.

--output-file
write output to the file outfile instead of to standard output; a file name of "-" stands for
standard output.

INPUT

       RhumbSolve measures all angles in degrees, all lengths (s12) in meters, and all areas (S12) in  meters^2.
       On input angles (latitude, longitude, azimuth, arc length) can be as decimal degrees or degrees, minutes,
       seconds.   For  example,  "40d30",  "40d30'", "40:30", "40.5d", and 40.5 are all equivalent.  By default,
       latitude precedes longitude for each point (the -w flag  switches  this  convention);  however  on  input
       either  may  be  given  first  by  appending  (or  prepending)  N  or S to the latitude and E or W to the
       longitude.  Azimuths are measured clockwise from north; however this may be overridden with E or W.

       For details on the allowed formats for angles, see the "GEOGRAPHIC COORDINATES" section of GeoConvert(1).

PRECISION

       prec gives precision of the output with prec = 0 giving 1 m precision, prec = 3 giving  1  mm  precision,
       etc.   prec is the number of digits after the decimal point for lengths.  For decimal degrees, the number
       of digits after the decimal point is prec + 5.  For DMS (degree, minute, seconds) output, the  number  of
       digits  after the decimal point in the seconds component is prec + 1.  The minimum value of prec is 0 and
       the maximum is 10.

ERRORS

       An illegal line of input will print an error message to  standard  output  beginning  with  "ERROR:"  and
       causes RhumbSolve to return an exit code of 1.  However, an error does not cause RhumbSolve to terminate;
       following lines will be converted.

ACCURACY

       The  algorithm  used  by  RhumbSolve  uses exact formulas for converting between the latitude, rectifying
       latitude (mu), and isometric  latitude  (psi).   These  formulas  are  accurate  for  any  value  of  the
       flattening.   The  computation  of rhumb lines involves the ratio (psi1 - psi2) / (mu1 - mu2) and this is
       subject to large round-off errors if lat1 is close to lat2.  So this  ratio  is  computed  using  divided
       differences  using  one of two methods: by default, this uses the addition theorem for elliptic integrals
       (accurate for all values of f); however, with the -s options, it is computed using the series  expansions
       used  by  TransverseMercatorProj(1)  for  the  conversions  between  rectifying  and  conformal latitudes
       (accurate for |f| < 0.01).  For the WGS84 ellipsoid, the  error  is  about  10  nanometers  using  either
       method.

EXAMPLES

       Route from JFK Airport to Singapore Changi Airport:

          echo 40:38:23N 073:46:44W 01:21:33N 103:59:22E |
          RhumbSolve -i -: -p 0

          103:34:58.2 18523563

       N.B. This is not the route typically taken by aircraft because it's considerably longer than the geodesic
       given by GeodSolve(1).

       Waypoints on the route at intervals of 2000km:

          for ((i = 0; i <= 20; i += 2)); do echo ${i}000000;done |
          RhumbSolve -l 40:38:23N 073:46:44W 103:34:58.2 -: -p 0

          40:38:23.0N 073:46:44.0W
          36:24:30.3N 051:28:26.4W
          32:10:26.8N 030:20:57.3W
          27:56:13.2N 010:10:54.2W
          23:41:50.1N 009:12:45.5E
          19:27:18.7N 027:59:22.1E
          15:12:40.2N 046:17:01.1E
          10:57:55.9N 064:12:52.8E
          06:43:07.3N 081:53:28.8E
          02:28:16.2N 099:24:54.5E
          01:46:36.0S 116:52:59.7E

AUTHOR

       RhumbSolve was written by Charles Karney.

HISTORY

       RhumbSolve was added to GeographicLib, <http://geographiclib.sf.net>, in version 1.37.

GeographicLib 1.45                                 2015-09-30                                      RHUMBSOLVE(1)