Space physics coordinate transformations: the role of precession

Raw data on spacecraft orbits and attitude are usually supplied in "inertial" coordinates. The normal geocentric inertial coordinate system changes slowly in time owing to the effects of astronomical precession and the nutation of the Earth's rotation axis. However...

Full description

Bibliographic Details
Main Author: M. A. Hapgood
Format: Article
Language:English
Published: Copernicus Publications
Series:Annales Geophysicae
Online Access:http://www.ann-geophys.net/13/713/1995/angeo-13-713-1995.html
id doaj-add30a84117a434897dfe3f8056680fc
record_format Article
spelling doaj-add30a84117a434897dfe3f8056680fc2020-11-25T01:28:30ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-0576137713716Space physics coordinate transformations: the role of precessionM. A. HapgoodRaw data on spacecraft orbits and attitude are usually supplied in "inertial" coordinates. The normal geocentric inertial coordinate system changes slowly in time owing to the effects of astronomical precession and the nutation of the Earth's rotation axis. However, only precession produces a change that is significant compared with the errors in determining spacecraft position. We show that the transformations specified by Russell (1971) and Hapgood (1992) are strictly correct only if the epoch-of-date inertial system is used. We provide a simple formula for estimating the error in the calculated position if the inertial system for some other epoch is used. We also provide a formula for correcting inertial coordinates to the epoch-of-date from the standard fixed epoch of J2000.0. http://www.ann-geophys.net/13/713/1995/angeo-13-713-1995.html
collection DOAJ
language English
format Article
sources DOAJ
author M. A. Hapgood
spellingShingle M. A. Hapgood
Space physics coordinate transformations: the role of precession
Annales Geophysicae
author_facet M. A. Hapgood
author_sort M. A. Hapgood
title Space physics coordinate transformations: the role of precession
title_short Space physics coordinate transformations: the role of precession
title_full Space physics coordinate transformations: the role of precession
title_fullStr Space physics coordinate transformations: the role of precession
title_full_unstemmed Space physics coordinate transformations: the role of precession
title_sort space physics coordinate transformations: the role of precession
publisher Copernicus Publications
series Annales Geophysicae
issn 0992-7689
1432-0576
description Raw data on spacecraft orbits and attitude are usually supplied in "inertial" coordinates. The normal geocentric inertial coordinate system changes slowly in time owing to the effects of astronomical precession and the nutation of the Earth's rotation axis. However, only precession produces a change that is significant compared with the errors in determining spacecraft position. We show that the transformations specified by Russell (1971) and Hapgood (1992) are strictly correct only if the epoch-of-date inertial system is used. We provide a simple formula for estimating the error in the calculated position if the inertial system for some other epoch is used. We also provide a formula for correcting inertial coordinates to the epoch-of-date from the standard fixed epoch of J2000.0.
url http://www.ann-geophys.net/13/713/1995/angeo-13-713-1995.html
work_keys_str_mv AT mahapgood spacephysicscoordinatetransformationstheroleofprecession
_version_ 1725101285678514176