An Analysis of State Vector Propagation Using Differing Flight Dynamics Programs - PowerPoint PPT Presentation

1 / 30
About This Presentation
Title:

An Analysis of State Vector Propagation Using Differing Flight Dynamics Programs

Description:

Paper AAS-05-199, Presented at the AAS/AIAA Space Flight Mechanics Conference, ... Mean equator Mean equinox of J2000. Integrator. Gravitational Model / Constants ... – PowerPoint PPT presentation

Number of Views:96
Avg rating:3.0/5.0
Slides: 31
Provided by: AGI92
Category:

less

Transcript and Presenter's Notes

Title: An Analysis of State Vector Propagation Using Differing Flight Dynamics Programs


1
An Analysis of State Vector Propagation Using
Differing Flight Dynamics Programs
  • David A Vallado
  • Analytical Graphics Inc.
  • Center for Space Standards and Innovation

Paper AAS-05-199, Presented at the AAS/AIAA Space
Flight Mechanics Conference, Copper Mountain
Colorado, January 23-27, 2005
2
Overview
  • Introduction
  • Standards
  • Objective
  • Potential Error Sources
  • Initial State Vectors
  • Programs
  • Input Data Sources
  • Using the Input Data
  • Interpolation, timing, etc
  • State vector format
  • Study Process
  • Build up the force models

3
Overview (continued)
  • Results
  • Force Model Sensitivity Analysis
  • Individual Force Model Contributions
  • Gravity
  • Atmospheric Drag
  • Solar Radiation Pressure
  • Ephemeris Comparison Results
  • Gravity
  • Third Body
  • Solar Radiation Pressure
  • Atmospheric Drag
  • Combined Forces
  • POE Comparison Results
  • Community Standard Ephemeris Baseline
  • Conclusions

4
Introduction
  • Numerically derived state vectors
  • Not new to astrodynamics
  • Navy 1st full numerical catalog in 1997
  • Answer fundamental question
  • What observations and processing are needed to
    achieve a certain level of accuracy on a
    particular satellite, now, and at a future time?
  • Requires
  • Orbit Determination
  • Propagation
  • Standards
  • Other

5
Objectives
  • Demonstrate the inconsistencies of AFSPC
    Instructions
  • 33-105 and 60-102
  • Standards are useful when properly applied
  • Computer code is not a standard
  • Mathematical theory is a standard
  • Historically
  • SGP4 vs. PPT
  • Mathematical theory differences
  • Bad example of a need for standards ?
  • WGS-72 vs WGS-84
  • Good examples of a need for standards ?
  • 1950 Nutation theory and 1980 IAU nutation theory
  • Example of need for a recommended practice ?
  • 1980 IAU Nutation sum terms from 1-106 vs. 106 to
    1

6
Potential Error Sources
  • Inaccurate models
  • Measurement errors
  • Truncation error
  • Round-off
  • Mathematical simplifications
  • Human error
  • Tracking all input parameters
  • Treatment of input data
  • indicates important outcome from the paper

7
Tracking All Input Data
  • Critical to provide adequate information
  • Proposed format at end of paper and on web
  • Detail treatment of
  • Satellite positional information
  • Forces included
  • Sizes, coefficients, etc.
  • Satellite characteristics
  • BC, mass, area, attitude, etc.
  • Source and use of data
  • Solar weather data, EOP, other
  • Integrator information
  • Covariance information
  • Current formats simply not adequate

8
Programs
  • Legacy Programs
  • GEODYN
  • GTDS
  • Raytheon TRACE
  • Special-K
  • STK/HPOP

9
Input Data
  • Need correct constants and data
  • Coordinate system
  • Mean equator Mean equinox of J2000
  • Integrator
  • Gravitational Model / Constants
  • EGM-96 Rotational vel 0.0743668531687138 rad/min
  • EGM-96 Radius earth 6378.137 km
  • EGM-96 Gravitational param 398600.4418 km3/s2
  • EOP Timing coefficients from actual (EOPC04 or
    USNO)
  • Solar flux from actual (NGDC) measurements

10
Test Conditions
  • Best approach built up force models
    incrementally
  • Two-body
  • Numerical integrators, Coordinate and Time
    Systems
  • Gravity Field
  • Checks mu, re, gravitational coefficients
  • Two-body plus Atmospheric Drag
  • Atmospheric density model, solar weather data
    handling
  • Two-Body plus Third-body
  • JPL DE/LE file incorporation, constants
  • Two-body plus Solar Radiation Pressure
  • Earth shadow model, solar constants

11
Sensitivity Results
  • Force model contributions
  • Determine which forces contribute the largest
    effects
  • 12x12 gravity field is the baseline
  • Note
  • Gravity and Drag are largest contributors
  • 3rd body km effect for higher altitudes
  • Point to take away
  • Trying to get the last cm from solid earth tides
    no good unless all other forces are at least that
    precise

12
Force Model Contributions
13
Sensitivity Results
  • Gravitational modeling
  • Typically square gravity field truncations
  • Appears the zonals contribute more
  • Point to take away
  • Use complete field
  • Any truncations should include additional, if not
    all, zonals

14
Gravitational Modeling
  • Satellite JERS (21867)
  • Note the dynamic variability over time

15
Sensitivity Results
  • Atmospheric Drag
  • Large variations
  • Several sources
  • Using predicted values of F10.7, kp, ap for
    real-time operations
  • Not using the actual measurement time for the
    values (particularly F10.7 at 2000 UTC)
  • Using step functions for the atmospheric
    parameters vs interpolation
  • Using the last 81-day average F10.7 vs. the
    central 81-day average
  • Using undocumented differences from the original
    atmospheric model definition
  • Not accounting for possibly known dynamic
    effects changing attitude, molecular
    interaction with the satellite materials, etc.
  • Inherent limitations of the atmospheric models
  • Use of differing interpolation techniques for the
    atmospheric parameters
  • Using approximations for the satellite altitude,
    solar position, etc.
  • Using ap or kp and converting between these
    values
  • Use of F10.7 vs E10.7 in the atmospheric models
    (not well characterized yet)

16
Sensitivity Results
  • Plot
  • Note Dap almost as large as ap values
  • Note Last - Ctrd 81 day, 30-50 SFU
  • Factors examined
  • Daily
  • 3-Hourly
  • 3-Hourly interp
  • Last 81 day
  • Last 81 day, 2000
  • F10.7 Day Con
  • F10.7 Avg Con
  • F10.7 All Con
  • All Con

17
Atmospheric Drag
  • Differing models (left)
  • Note grouping of similar models
  • transient effects only for first day or so
  • Options for processing data (right)
  • Note 10-100km effect

18
Sensitivity Results
  • Solar Radiation Pressure
  • Several variations shown
  • Notice maximum is only about 100m
  • Point to take away
  • Relatively small effect
  • Some variations

19
Ephemeris Comparisons
  • Gravitational
  • GTDS (left) and Ray TRACE (right) examples
  • Generally cm and mm-level comparisons
  • Regularized time not explored

20
Ephemeris Comparisons
  • Third-Body
  • GTDS (left) and Ray TRACE (right) examples
  • Generally a few cm

21
Ephemeris Comparisons
  • Solar Radiation Pressure
  • GTDS (left) and Ray TRACE (right) examples
  • Generally a few m

22
Ephemeris Comparisons
  • Atmospheric Drag
  • GTDS (left) and Ray TRACE (right) examples
  • A few km to many km
  • Recall sensitivity results which were even higher

23
Ephemeris Comparisons
  • Combined forces
  • Several runs made without detailed build-up of
    forces
  • Included drag

24
Ephemeris Comparisons
  • GEODYN tests
  • Starlette (7646)
  • Note plot on right
  • Difference of 2 GEODYN runs with different models
  • Nearly identical to sensitivity tests run for 7646

25
Ephemeris Comparisons
  • GEODYN (cont)
  • TDRS comparison (4 days and 1 month)

26
Ephemeris Comparisons
  • Special-K Comparisons

27
POE Ephemeris Comparisons
  • POE Comparisons
  • Initial state taken and propagated
  • No coordination, estimate of drag and solar
    radiation pressure
  • Perturbed initial state results

28
Community Ephemeris Baseline
  • Need to provide standard ephemeris comparison
    data
  • Provide community baseline on the web
  • Interactive forum for cooperative comparisons
  • Initial release designed to stimulate community
    involvement
  • NOT intended to force compliance
  • CSSI clearinghouse for this innovation
  • Data hosted under CenterForSpace website
  • www.centerforspace.com/EphemerisBaseline
  • Scenarios available for use in STK
  • CSSI available for consultation, analysis,
    inputs, questions

29
Conclusions
  • Numerous conclusions in topical areas
  • Standards, Code, Instructions
  • Recommended Practice needed
  • Data Formats
  • Proposed format of additional information
  • Force model contributions
  • Summary for a particular satellite
  • Identify which are important
  • Results for comparisons
  • Conservative, cm-level
  • Non Conservative, km-level
  • Tremendous variability just with input data
  • Sensitivity studies
  • Tremendous variation
  • POE analyses
  • No propagation perfectly matches truth

30
Conclusions
  • Bottom line
  • With variability on treatment of input data,
  • What does exact agreement mean?
  • Nothing
  • Right and wrong are indistinguishable!
  • Identical code is not needed to align programs
  • Attention to detail is
  • Adequate data formats is
  • Standardized approach for treating input data is
  • Cooperation is
  • Organizations involved in this study were
    tremendously helpful and cordial
Write a Comment
User Comments (0)
About PowerShow.com