radiation belt electron pitch angle measurements from the goes satellites t. g. onsager, j. c....
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Radiation Belt Electron Pitch Angle Measurements from the GOES Satellites
T. G. Onsager, J. C. Green, and H. J. Singer
NOAA Geostationary Operational Environmental Satellites (GOES):Normally 3-axis stabilized – Spinning while in on-orbit storage
• Demonstration of pitch angle measurements from GOES
• Statistical characterization of pitch angle distributions
• Variability of pitch angle distributions during radiation belt enhancement and loss
Multiple years of geosynchronous electron pitch angle distributions are becoming available to investigate radiation belt dynamics.
Ogo-5 Pitch Angle Measurements
West, 1979
Polar Pitch Angle MeasurementsSelesnick and Blake, 2002
8
4
0
-4
-8
-4-8 840Dipole L shell
Pitch Angle (degrees)
Pitch Angle (degrees)
Ele
ctro
n F
lux
Ele
ctro
n F
lux
B
p
Normal Distribution
Butterfly Distribution2.2 MeV
.
90
avespinj
j
Distinctive pitch angle distributions result from drift shell splitting in Earth’s asymmetric magnetic field combined with the radial gradient of electron flux
GOES 10 and 12 are 3-axis stabilized
GOES 11 is in storage and spinning
Spin period: ~ 8 min
Electron data: ~10.2 s resolutionMagnetic field: ~ 0.5 s resolution
Electron detector has a wide acceptance aperture - ~ 90º
Periodic measurements from late 1998 to the present
Pitch angle measurements from GOES 11 can be applied to data on GOES 10 and 12
GOES 11 Measures Pitch Angle Distributions
20 minutes of data
Pitch Angle Distributions are strongly peaked at 90ºnear local noon
B
p
20 minutes of data
Pitch Angle Distributions have minima at 90º near local midnight
Characterize Pitch Angle With sinm Function
Fit measurements over ~1 spin (8 min) to a sinm function
GOES 11 September 14, 20031800 – 1808 UT
0500 – 0508 UT
Day Sector:m ~ 0.9
Night Sector:m ~ -0.7
Pitch Angle Distribution versus Local Time
GOES 11 September, 2003
Pitch angle index is determined every 8 minutes (one spin) and binned in local time.
Pitch angle distributions are peaked at 90º near noon and have minima at 90º on the night side.
Local Time Dependence is Similar During High and Low Fluxes
GOES 11 September, 2003
Pitch Angle Distribution Versus Magnetic Field
Pitch angle index is strongly correlated with local magnetic field strength.
Local magnetic field can be used to estimate pitch angle distribution when pitch angle measurements are not available.
GOES 11 September, 2003Dusk local timesDawn local times
September 15-17, 2003
September 15
September 17
Flux dropout and recovery occurred over ~ 2 day interval
Pitch angle distributions remained peaked at 90º near dusk as fluxes decreased – indicating a highly distorted magnetic field
Fluxes recover abruptly as an isotropic distribution – perhaps indicating no preferred pitch angle for local acceleration
Summary
• GOES satellites which spin during on-orbit storage are acquiring a large data set of pitch angle distributions of radiation belt electrons
• Data are being used to study the statistic properties of the geosynchronous electron distributions and their variability during abrupt enhancements and loss
• Characterization of the pitch angle distributions as sinmα shows a strong correlation with the local magnetic field magnitude, yielding a relationship to estimate the pitch angle distribution at geosynchronous orbit
• Pitch angle distributions during flux enhancement and loss events will improve our future efforts to understand radiation belt source and loss processes