Don Cross 4f842627da Fixed mistake in GeoVector(SUN): we do need to correct for light-travel time. ...

To be consistent, when calculating the geocentric position of the Sun,
we do need to correct for light travel time just like we would for any
other object. This reduces the maximum time error for predicting transits
from 25 minutes to 11 minutes.

Also had to disable aberration when calculating moon phases
(longitude from Sun) in order to keep a good fit with test data.

2020-06-13 13:45:59 -04:00

..

.gitignore

Added Python demo for calculating lunar eclipses.

2020-05-16 22:14:55 -04:00

culminate_correct.txt

Fixed mistake in GeoVector(SUN): we do need to correct for light-travel time.

2020-06-13 13:45:59 -04:00

horizon_correct.txt

Python: Use Espenak/Meeus formula for calculating Delta T.

2020-05-15 19:28:54 -04:00

lunar_eclipse_correct.txt

Added Python demo for calculating lunar eclipses.

2020-05-16 22:14:55 -04:00

moonphase_correct.txt

Python: Use Espenak/Meeus formula for calculating Delta T.

2020-05-15 19:28:54 -04:00

positions_correct.txt

Fixed mistake in GeoVector(SUN): we do need to correct for light-travel time.

2020-06-13 13:45:59 -04:00

riseset_correct.txt

Fixed mistake in GeoVector(SUN): we do need to correct for light-travel time.

2020-06-13 13:45:59 -04:00

seasons_correct.txt

Python: Use Espenak/Meeus formula for calculating Delta T.

2020-05-15 19:28:54 -04:00

test

Added Python demo for calculating lunar eclipses.

2020-05-16 22:14:55 -04:00