Standard

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 изданияхстатьяРецензирование

Harvard

Sergeev, VA, Shukhtina, MA, Rasinkangas, R, Korth, A, Reeves, GD, Singer, HJ, Thomsen, MF & Vagina, LI 1998, 'Event study of deep energetic particle injections during substorm', JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, Том. 103, № A5, стр. 9217-9234. https://doi.org/10.1029/97JA03686

APA

Sergeev, VA., Shukhtina, MA., Rasinkangas, R., Korth, A., Reeves, GD., Singer, HJ., Thomsen, MF., & Vagina, LI. (1998). Event study of deep energetic particle injections during substorm. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 103(A5), 9217-9234. https://doi.org/10.1029/97JA03686

Vancouver

Sergeev VA, Shukhtina MA, Rasinkangas R, Korth A, Reeves GD, Singer HJ и пр. Event study of deep energetic particle injections during substorm. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. 1998 Май 1;103(A5):9217-9234. https://doi.org/10.1029/97JA03686

Author

Sergeev, VA ; Shukhtina, MA ; Rasinkangas, R ; Korth, A ; Reeves, GD ; Singer, HJ ; Thomsen, MF ; Vagina, LI. / Event study of deep energetic particle injections during substorm. в: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. 1998 ; Том 103, № A5. стр. 9217-9234.

BibTeX

@article{9633d278b59942d087c4cdf0c0609a13,
title = "Event study of deep energetic particle injections during substorm",
abstract = "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.",
keywords = "PROTON DRIFT ECHOES, GEOSYNCHRONOUS ORBIT, INNER MAGNETOSPHERE, SYNCHRONOUS ORBIT, MAGNETIC-FIELD, CURRENT WEDGE, GROWTH-PHASE, DYNAMICS, ONSET, CRRES",
author = "VA Sergeev and MA Shukhtina and R Rasinkangas and A Korth and GD Reeves and HJ Singer and MF Thomsen and LI Vagina",
year = "1998",
month = may,
day = "1",
doi = "10.1029/97JA03686",
language = "Английский",
volume = "103",
pages = "9217--9234",
journal = "Journal of Geophysical Research: Biogeosciences",
issn = "0148-0227",
publisher = "American Geophysical Union",
number = "A5",

}

RIS

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