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Broadband electrons observed by the DMSP satellites during storm‐time substorms
Author(s) -
Shiokawa K.,
Yumoto K.,
Meng C.I.,
Reeves G.
Publication year - 1996
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/96gl01955
Subject(s) - substorm , plasma sheet , electron precipitation , electron , geomagnetic storm , physics , storm , ionosphere , atmospheric sciences , geophysics , atomic physics , magnetosphere , plasma , solar wind , meteorology , nuclear physics
Electrons that have intense broadband spectra are found to precipitate in the equatorward part of the auroral oval. The electrons are observed by the DMSP satellites in association with particular substorms during the main phase of magnetic storms. Electron fluxes are drastically enhanced after the substorm onset at all the energies measured (32 eV to 30 keV) at magnetic latitudes lower than 60° (L < 4). The energy flux of the electrons exceeds 1.0 × 10 13 eV cm −2 s −1 sr −1 . The intense electron precipitation lasts less than 1 h. These characteristics are significantly different from those seen in the central plasma sheet region. We suggest that an unknown energization mechanism of these electrons exists at the inner part of the plasma sheet at L < 4 during these particular storm‐time substorms.