Acceleration and Extreme Distortion Within the Van Allen Radiation Belts During the Halloween Solar - PowerPoint PPT Presentation

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Acceleration and Extreme Distortion Within the Van Allen Radiation Belts During the Halloween Solar

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... Within the Van Allen Radiation Belts During the 'Halloween' Solar Storms of 2003 ... radiation belt 'slot' region at L = 2 ~ 3 was filled by relativistic electrons ... – PowerPoint PPT presentation

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Title: Acceleration and Extreme Distortion Within the Van Allen Radiation Belts During the Halloween Solar


1
Acceleration and Extreme Distortion Within the
Van Allen Radiation Belts During the Halloween
Solar Storms of 2003
  • D.N. Baker, S. P. Monk, S.G. Kanekal, X. Li
  • Laboratory for Atmospheric and Space Physics
  • University of Colorado-Boulder
  • J. Goldstein, J.L. Burch
  • Southwest Research Institute, San Antonio

2
October 2003 Events
3
October-November 2003 Storms
SOHO/LASCO CMEs and the storms they produced
10/28 ? - 310 nT 10/29 ? - 347 nT
11/02 ? - 40 nT 11/04 ? only SC
4
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6
High-Energy Electrons 17 Oct.-1 Dec.
7
Day-to-Day Variation of the Radiation Belts
8
Selected Days Outer Belt Properties
9
EUV Images of the Plasmasphere
Global EUV He Image
Plasmasphere
He 15
plasmasphere
10
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12
Sunward Flux in TEC/Plasmasphere PlumeMarch 31,
2001
Ground-Based GPS Maps TEC Plume
Foster et al., GRL 2002
Direct Observation of Velocity and Flux by
Millstone Hill ISR
13
Aurora Seen in Colorado
20 Nov. 2003
14
November 20, 2003 SED Plume
15
November 20, 2003 SED Plume
16
Regions of Wave-Particle Interactions
17
Conclusions
  • The October-November 2003 solar activity produced
    spectacular effects in Earths radiation
    environment
  • The radiation belt slot region at L 2 3 was
    filled by relativistic electrons to an
    unprecedented degree
  • SAMPEX, IMAGE and other data give a clear global
    picture of the plasmasphere and radiation belt
    enhancement and decay
  • Several important spacecraft operational
    anomalies were apparently associated with
    radiation environment changes

18
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19
High-Energy Electrons 17 Oct.-1 Dec.
20
GEO Solar Particle Measurements
Period of main DoD s/c anomalies
21
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