Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
Event study of deep energetic particle injections during substorm. / Sergeev, VA; Shukhtina, MA; Rasinkangas, R; Korth, A; Reeves, GD; Singer, HJ; Thomsen, MF; Vagina, LI.
в: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Том 103, № A5, 01.05.1998, стр. 9217-9234.Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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TY - JOUR
T1 - Event study of deep energetic particle injections during substorm
AU - Sergeev, VA
AU - Shukhtina, MA
AU - Rasinkangas, R
AU - Korth, A
AU - Reeves, GD
AU - Singer, HJ
AU - Thomsen, MF
AU - Vagina, LI
PY - 1998/5/1
Y1 - 1998/5/1
N2 - The origin of multiple energetic particle injections into the inner magnetosphere is addressed using a rare opportunity of measuring the energetic particle fluxes at different radial distances under known electric and magnetic fields. During a strong substorm on February 10, 1991, the CRRES spacecraft measured E and B fields and high-energy particle fluxes near the magnetic equator at r similar to 5 R-e, whereas particle injections, their azimuthal locations, and some other parameters were simultaneously monitored by three geostationary spacecraft and ground networks. We show a multitude of impulsive short-duration injection events which correlate with 1-2 min long pulses of dawn-dusk electric field. The observations suggest that some E field pulses recorded deep in the inner magnetosphere were fast magnetosonic waves radiated by the current disruption region. This supports the concept of impulsive dissipation event as an elementary building block of substorm expansion. Furthermore, our modeling results indicate that most of the flux variations of energetic particles can be explained by the global convective transport and corresponding particle acceleration. However, we emphasize that, depending on particle spectra and radial flux gradient, one can observe either flux increase, or decrease, or no variation (often seen in different energy ranges simultaneously and at the same point) as a response to the electric field pulse. Both the cloud of injected particles and magnetic field dipolarization region had a sharp inner boundary (injection front) which propagated inward at the convection speed. We document the complicated structure of this front, consisting of a diamagnetic hot proton layer followed by the dipolarixation front which contains enhanced energetic electron fluxes. Further study is required to understand hom common this structure is and, if common, how it may be formed.
AB - The origin of multiple energetic particle injections into the inner magnetosphere is addressed using a rare opportunity of measuring the energetic particle fluxes at different radial distances under known electric and magnetic fields. During a strong substorm on February 10, 1991, the CRRES spacecraft measured E and B fields and high-energy particle fluxes near the magnetic equator at r similar to 5 R-e, whereas particle injections, their azimuthal locations, and some other parameters were simultaneously monitored by three geostationary spacecraft and ground networks. We show a multitude of impulsive short-duration injection events which correlate with 1-2 min long pulses of dawn-dusk electric field. The observations suggest that some E field pulses recorded deep in the inner magnetosphere were fast magnetosonic waves radiated by the current disruption region. This supports the concept of impulsive dissipation event as an elementary building block of substorm expansion. Furthermore, our modeling results indicate that most of the flux variations of energetic particles can be explained by the global convective transport and corresponding particle acceleration. However, we emphasize that, depending on particle spectra and radial flux gradient, one can observe either flux increase, or decrease, or no variation (often seen in different energy ranges simultaneously and at the same point) as a response to the electric field pulse. Both the cloud of injected particles and magnetic field dipolarization region had a sharp inner boundary (injection front) which propagated inward at the convection speed. We document the complicated structure of this front, consisting of a diamagnetic hot proton layer followed by the dipolarixation front which contains enhanced energetic electron fluxes. Further study is required to understand hom common this structure is and, if common, how it may be formed.
KW - PROTON DRIFT ECHOES
KW - GEOSYNCHRONOUS ORBIT
KW - INNER MAGNETOSPHERE
KW - SYNCHRONOUS ORBIT
KW - MAGNETIC-FIELD
KW - CURRENT WEDGE
KW - GROWTH-PHASE
KW - DYNAMICS
KW - ONSET
KW - CRRES
U2 - 10.1029/97JA03686
DO - 10.1029/97JA03686
M3 - статья
VL - 103
SP - 9217
EP - 9234
JO - Journal of Geophysical Research: Biogeosciences
JF - Journal of Geophysical Research: Biogeosciences
SN - 0148-0227
IS - A5
ER -
ID: 36633725