cenang: Central Angle

In astro: Astronomy Functions, Tools and Routines

Description

Calculates the angle between two points on a sphere

Usage

cenang(a1, d1, a2, d2, units = "deg", method = "vincenty")

Arguments

a1	right ascension of point 1
d1	declination of point 1
a2	right ascension of point 2
d2	declination of point 2
units	input/output units [deg/rad]
method	angle calculation method (see below)

Details

The central angle describes the angle, from the origin, between two points lying on the surface of a sphere (e.g., the celestial sphere). Three commonly used methods employed in its calculation are: the Spherical Law of Cosines (sloc); the Haversine Formula (haversine), and; the Vincenty Formula (vincenty). The Spherical Law of Cosines suffers from severe rounding errors for small angles (theta < 1E-5). The Haversine Formula generally works well at all angles, but suffers from rounding errors for antipodal points. The Vincenty Formula is accurate for all angles, and is recommended. The three methods may be chosen by specifying ‘sloc’, ‘haversine’ or ‘vincenty’, or by their respective first letters: s, h or v.

Value

The central angle: the angle between two points lying on the surface of a sphere, with reference at the origin/centroid.

Author(s)

Lee Kelvin <[e-mail]>

References

http://en.wikipedia.org/wiki/Great-circle_distance

See Also

The astronomy package: astro.

astro documentation built on May 2, 2019, 2:14 a.m.