KGRKJGETMRETU895U-589TY5MIGM5JGB5SDFESFREWTGR54TY
Server : Apache/2.4.62
System : FreeBSD fbsdweb2.web.rcn.net 14.1-RELEASE FreeBSD 14.1-RELEASE releng/14.1-n267679-10e31f0946d8 GENERIC amd64
User : www ( 80)
PHP Version : 8.3.8
Disable Function : NONE
Directory :  /domains/astrosfm/AAS_meetings/1997_astro/abstracts/

Upload File :
current_dir [ Writeable ] document_root [ Writeable ]

 

Current File : /domains/astrosfm/AAS_meetings/1997_astro/abstracts/97-665.html
<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 3.2//EN">
<HTML>
<HEAD>
<TITLE>Abstract AAS 97-665</TITLE>
</HEAD>
<BODY BGCOLOR="ffffff">
<h2>AAS 97-665</h2>
<h2>EVALUATION OF J2-PERTURBED APSIS HEIGHT COMPUTATION METHODS                                                                                      </h2>
<h4> D.R. Adamo - NASA/JSC                                                                                                                                                    </h4>
<h2> Abstract </h2>
Accurate computation of apsis heights is nearly always essential to spacecraft mission success.  It is often convenient and computationally efficient to perform this task using an analytic method which receives an osculating state vector as input.  When periapsis height is sufficiently low, the analytic method must account for perturbations from the J2 zonal gravity harmonic, or inaccuracies and time-dependent inconsistencies will result.                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                              
 <br><br>
Various analytic methods are applied to the problem of apsis height computation in which otherwise conic spacecraft trajectories are perturbed only by the gravitating body's J2 harmonic.  Computation results are presented which serve as the basis for evaluating each method's merit using multiple criteria.                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                                      

Anon7 - 2021