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Modeling of Infrasound from the Space Shuttle Columbia Reentry

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Title: Modeling of Infrasound from the Space Shuttle Columbia Reentry


1
Modeling of Infrasound from the Space Shuttle
Columbia Reentry
  • Robert Gibson and David Norris
  • BBN Technologies
  • Arlington, Virginia, USA
  • Infrasound Technology Workshop
  • La Jolla, California
  • 27-30 Oct 2003
  • Work sponsored by Air Force Research Laboratory,
    Contract DTRA01-01-C-0084

2
Introduction
  • Space Shuttle Columbia Reentry
  • STS-107
  • 01-Feb-2003
  • Loss of orbiter
  • 1400 UT
  • 0900 EST
  • 0600 PST
  • Nominal trajectory shown
  • Infrasound observed at multiple arrays in North
    America

3
Columbia Investigation
  • Purpose of this presentation
  • Explain the infrasound modeling conducted by BBN
  • Present example results
  • US Infrasound Working Group formed Feb 2003
  • Part of the US DoD Columbia Investigation Support
    Team
  • In support of NASA investigation
  • Participants
  • US Government Army Research Lab, Los Alamos
    National Lab, NOAA Environmental Technology Lab,
    Naval Research Lab
  • Industry BBN Technologies, Center for Monitoring
    Research (SAIC)
  • Academia Univ. of California-San Diego
    (L2A/Scripps), Univ. of Hawaii (ISLA), Univ. of
    Mississippi (NCPA)

Optical image, showing left wing damage From
AFRL, Kirtland AFB
4
Background
  • Infrasound from supersonic bodies has been
    observed
  • Bolides
  • Concorde
  • Rockets (Apollo, Titan, Ariane, etc.)
  • Space shuttle launches and reentries
  • BBN has used 3-d ray tracing to predict
    infrasound from Space Shuttle launches
  • Favorable model vs. data comparisons
  • Orbiter ascent
  • Solid rocket booster reentry
  • Ground truth events are of interest for
    validating or calibrating models
  • Propagation models
  • Atmospheric characterizations

5
Shuttle Modeling Approach
  • Source of infrasound is not impulsive, but
    continuous and moving
  • Approximate moving source by modeling a series of
    discrete events, each with appropriate time delay
  • Use 3-D ray tracing to find eigenrays from points
    on reentry trajectory to infrasound array
  • Determine arrival time and azimuth for each
    eigenray
  • Combine all predicted eigenray arrivals at each
    array

6
Sources of Information
  • Shuttle reentry trajectory
  • NASA, based on actual GPS
  • Propagation model
  • InfraMAP tool kit (BBN)
  • Implementation of HARPA 3-d ray tracing
  • Environmental characterization
  • Assimilation of climatology with synoptic model
    output
  • NRL-G2S (D. Drob, Naval Research Lab)
  • Observations, for comparison
  • US and Canadian station operators
  • Center for Monitoring Research (SAIC)

7
Columbia Trajectory and Arrays
Altitude (km)
Trajectory in white Arrays in red CPAs in
yellow
8
Examples of Model Results
  • Results are shown for representative arrays
  • Short range (in sonic boom carpet)
  • Medium range (100 1000 km)
  • Long range (gt 1000 km)
  • Atmospheric profiles along propagation path
  • Variability along path
  • Presence or absence of stratospheric duct
  • Typical ray paths
  • Azimuth vs. time
  • Color coded by source location
  • Apparent velocity vs. azimuth (polar plot)
  • Color coded by signal arrival time

9
Station List
10
Environmental Variability - SGAR
St. George, UT
(CPA range 23 km)
Atmospheric Characterizations from D. Drob, NRL
11
Environmental Variability - TXIAR
Lajitas, TX
(CPA range 522 km)
Atmospheric Characterizations from D. Drob, NRL
12
Environmental Variability IS10
Lac du Bonnet, Manitoba
(CPA range 1864 km)
Atmospheric Characterizations from D. Drob, NRL
13
Typical Ray Path SGAR
St. George, UT
14
Typical Ray Paths TXIAR
Lajitas, TX
15
Typical Ray Paths IS10
Lac du Bonnet, Manitoba
16
Azimuth vs. Time - SGAR
17
Azimuth vs. Time - TXIAR
18
Azimuth vs. Time - IS10
19
Polar Plot TXIAR(model)
20
Polar Plot TXIAR(data)
PMCC analysis of observed data from Garces and
Hetzer, U. Hawaii (ISLA), Summary of infrasonic
detections and propagation modeling estimates
associated with the Columbia reentry of
Februrary 1, 2003, March 2003
21
Model vs. Data for Pinon Flat (IS57)
Receiver azimuth (deg)
gmt (hrminsec)
Data analysis by BBN using InfraTool Passband
1-8 Hz
22
Conclusions
  • Model results largely consistent with reentry
    trajectory
  • Arrival time
  • Azimuth
  • Apparent velocity
  • Supersonic events with ground truth trajectories
    represent useful validation sources for
    infrasound modeling techniques
  • Modeling of the effects of atmospheric
    propagation was fairly successful but does not
    account for all of the signal complexity at the
    more distant stations
  • From Report to the Department of Defense on
    Infrasonic Re-Entry Signals from the Space
    Shuttle Columbia (STS-107), ed. by H. Bass,
    04-June-2003
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