The radiation belts and ring current: The relationship between Dst and relativistic electron phase space density

M. Grande*, M. Carter, C. H. Perry

*Awdur cyfatebol y gwaith hwn

Allbwn ymchwil: Pennod mewn Llyfr/Adroddiad/Trafodion CynhadleddTrafodion Cynhadledd (Nid-Cyfnodolyn fathau)

1 Dyfyniad (Scopus)

Crynodeb

We briefly review the radiation belts, before moving on to a more detailed examination of the relationship between the Disturbance Storm Time Index (Dst) and relativistic electron flux. We show that there is a strong correlation between the growth phase of storms, as represented by Dst, and dropouts in electron flux. Recovery is accompanied by growth of the electron flux. We calculate Electron Phase Space Density (PSD) as a function of adiabatic invariants using electron particle measurements from the Imaging Electron Sensor (IES) and the High Sensitivity Telescope (HIST) on the CEPPAD experiment onboard POLAR. We present the time history of the phase space density through the year 1998 as L-sorted plots and look in detail at the May 98 storm. Comparison with the Tsyganenko 96 magnetic field model prediction for the last closed field line suggests that the loss of electrons may be directly caused by the opening of drift shells.

Iaith wreiddiolSaesneg
Teitl2nd Solar Cycle and Space Weather Conference, Vico Equense
CyhoeddwrElsevier
Tudalennau391-398
Nifer y tudalennau8
Argraffiad477
StatwsCyhoeddwyd - Maw 2002
Digwyddiad2nd Solar Cycle and Space Weather Conference - Vico Equense, Yr Eidal
Hyd: 24 Medi 200129 Medi 2001

Cyfres gyhoeddiadau

EnwEuropean Space Agency, (Special Publication) ESA SP
ISSN (Argraffiad)0379-6566

Cynhadledd

Cynhadledd2nd Solar Cycle and Space Weather Conference
Gwlad/TiriogaethYr Eidal
DinasVico Equense
Cyfnod24 Medi 200129 Medi 2001

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