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From Fig. 3 and Eqn. (17) we see that:
|
(18) |
and thus
|
(19) |
with the sign being that of . We now substitute
, where is the
arc-length along the great circle on the auxiliary sphere, measured
from where it crosses the equator in a Northerly direction, obtaining:
|
(20) |
where
. By expanding in a power
series in and integrating term by term[3,5], we
obtain in the form:
The distance between two points
, on a geodesic arc is best obtained, after differencing
Eqn. (21), by using the identity
, where
. This avoids excessive loss of
significant digits when the two points are close together.
Vincenty[5] has rearranged a subset of the resulting equations
into
nested forms more suitable for computation:
In equations (22) the origins of and have
been shifted from the equator to the initial point (), where the reduced
latitude is and the azimuth of the geodesic is .
Next: Longitude difference
Up: Geodesics on a spheroid
Previous: Geodesics on a spheroid
Ed Williams
2002-03-21