Ring current behavior inferred from ground magnetic and space observations

被引:4
|
作者
Soraas, F. [1 ]
Sorbo, M. [1 ]
Aarsnes, K. [1 ]
Evans, D. S. [2 ]
机构
[1] Univ Bergen, Dept Phys & Technol, Bergen, Norway
[2] NOAA, Space Environm Ctr, Boulder, CO USA
来源
RECURRENT MAGNETIC STORMS: COROTATING SOLAR WIND STREAMS | 2006年 / 167卷
关键词
D O I
10.1029/167GM09
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The existence of an electric current encircling the Earth at a distance of several Earth radii was first predicted from ground based magnetic observations. These large variations in the Earth's magnetic field were called geomagnetic storms. The magnetic field at the Earth's surface exhibit an appreciable Magnetic Local Time (MLT) dependence in the initial and main phase of the storm. The field depression is very asymmetric, with the largest depression in the evening to midnight MLT sector. During such storms a well defined Storm Time Equatorial Belt (STEB) of Energetic Neutral Atoms (ENA) and ions is found to exist at low altitudes around the geomagnetic equator. Most of the particles measured at the equator by the vertical viewing detector on the NOAA satellites at an altitude of 800 km will be ENA. Ring Current (RC) asymmetry and symmetry inferred from the STEB are in accordance with results from ground based magnetic observations. The STEB first appears in the midnight/evening sector and then it appears in the morning sector largely consistent with the expected drift of RC ions. The local magnetic observations, on the other hand, show signatures both in the dusk and morning sectors simultaneously during the storm main phases. One possible explanation is that the large partial RC in the evening sector causes significant magnetic depression in the morning sector during deep injection (L similar to 2.0) events. STEB observations show that large convection fields can prevent the RC ions from passing local noon in their drift motion.
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页码:85 / +
页数:2
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