Prompt thermospheric response to the 6 November 2001 magnetic storm

被引:7
|
作者
Mishin, E. V.
Marcos, F. A.
Burke, W. J.
Cooke, D. L.
Roth, C.
Petrov, V. P.
机构
[1] Boston Coll, Inst Sci Res, Chestnut Hill, MA 02467 USA
[2] USAF, Res Lab, Space Vehicles Directorate, Hanscom Field, Hanscom AFB, MA 01731 USA
[3] RAS, IZMIR, Troitsk 142092, Moscow Reg, Russia
[4] AER Radex Inc, Lexington, MA USA
关键词
D O I
10.1029/2006JA011783
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[1] Thermospheric densities observed by the STAR accelerometer on CHAMP, near 400 km altitude, are used to examine the response to the major geomagnetic storm on 6 November 2001. This is the first large storm studied with CHAMP data at these near dawn-dusk local times. New features of the neutral density response at both global and local temporal/spatial scales have been revealed. Prompt response of the neutral atmosphere observed at the beginning of the storm was enriched by short- and meso-scale perturbations. Simultaneous observations of electromagnetic and ionospheric plasma perturbations and particle precipitations from the DMSP satellites, electron energy fluxes from NOAA-14 and Polar/UVI specified the energy source and the time delay. The suggested mechanism for this prompt thermospheric response appears to be due mainly to enhanced perpendicular electric fields. Large-scale, global changes caused by the geomagnetic storm show generally greater enhancements in the winter ( northern) hemisphere at both 0700 and 1900 local time and greater at 0700 LT than 1900 LT.
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页数:11
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