New aspects of thermospheric and ionospheric storms revealed by CHAMP

被引:54
|
作者
Balan, N. [1 ,2 ,3 ]
Yamamoto, M. [2 ]
Liu, J. Y. [3 ]
Otsuka, Y. [5 ]
Liu, H. [2 ]
Luehr, H. [4 ]
机构
[1] Univ Sheffield, Sheffield S10 3JD, S Yorkshire, England
[2] Kyoto Univ, RISH, Kyoto 6110011, Japan
[3] Natl Cent Univ, Inst Space Sci, Chungli 32001, Taiwan
[4] German Res Ctr Geosci, GFZ, D-14473 Potsdam, Germany
[5] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan
关键词
MAGNETIC STORM; GEOMAGNETIC STORMS; ELECTRIC-FIELDS; LOW-LATITUDE; LOCAL TIME; DISTURBANCE; DENSITY; REGION; MIDDLE; PENETRATION;
D O I
10.1029/2010JA016399
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The neutral mass density N and electron density Ne at 400 km height measured by CHAMP during nine intense geomagnetic storms bring out some new aspects of the thermospheric and ionospheric storms. The thermospheric storms (increase of N) develop with the onset of the main phases (MP) of the geomagnetic storms and reach their peak phases before or by the end of the MPs. The ionospheric storms (change of Ne) in general undergo an initial negative phase (with the equatorial ionization anomaly (EIA) crests shifting poleward) before turning positive, and the positive storms reach their peak strengths (or phases) centered at +/- 25 degrees-30 degrees magnetic latitudes; in some (4) cases the positive storms develop without an initial negative phase and with the EIA crests shifting equatorward; in all cases the positive storms reach their peak phases before the end of the MPs and turn to conventional negative storms by the end of the MPs. The observations agree with the different aspects of a physical mechanism of the positive storms. The observations also reveal that the Halloween storms of 30 October 2003 with a short MP without fluctuations produced the strongest positive ionospheric storms through impulsive response, and there is strong equinoctial asymmetry in the ionosphere and thermosphere during geomagnetic storms.
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页数:17
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