RhumbSolve -- perform rhumb line calculations
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
]
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.
- 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.
- 3.
- 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.
- -i
- perform an inverse calculation (see 2 above).
-
-L lat1 lon1 azi12
- line mode (see 3 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.
(-l is an alternative, deprecated, spelling of this flag.)
-
-e a f
- specify the ellipsoid via the equatorial radius, a
and the flattening, 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 prec
- 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 commentdelim
- 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 infile
- read input from the file infile instead of from
standard input; a file name of "-" stands for standard
input.
-
--input-string instring
- 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 linesep
- set the line separator character to linesep. By
default this is a semicolon.
-
--output-file outfile
- write output to the file outfile instead of to
standard output; a file name of "-" stands for standard
output.
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).
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.
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.
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.
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 0
36:24:30.3N 051:28:26.4W 9817078307821
32:10:26.8N 030:20:57.3W 18224745682005
27:56:13.2N 010:10:54.2W 25358020327741
23:41:50.1N 009:12:45.5E 31321269267102
19:27:18.7N 027:59:22.1E 36195163180159
15:12:40.2N 046:17:01.1E 40041499143669
10:57:55.9N 064:12:52.8E 42906570007050
06:43:07.3N 081:53:28.8E 44823504180200
02:28:16.2N 099:24:54.5E 45813843358737
01:46:36.0S 116:52:59.7E 45888525219677
GeoConvert(1),
GeodSolve(1),
TransverseMercatorProj(1).
An online version of this utility is availbable at
<
https://geographiclib.sourceforge.io/cgi-bin/RhumbSolve>.
The Wikipedia page, Rhumb line,
<
https://en.wikipedia.org/wiki/Rhumb_line>.
RhumbSolve was written by Charles Karney.
RhumbSolve was added to GeographicLib,
<
https://geographiclib.sourceforge.io>, in version 1.37.