The refraction corrections of finite distance objects.
Abstract
New definition in astronomical refraction have been employed and a computation model of refraction for a finite distance object is considered in detail, that involves a change of angular argument in the mapping function from the conventionally used true zenith distance to the proper zenith distance.
- Publication:
-
Shanghai Observatory Annals
- Pub Date:
- 1997
- Bibcode:
- 1997AnShO..18..157Y
- Keywords:
-
- Earth Atmosphere: Refraction