Multiple bidirectional EMIC waves observed by Cluster at middle magnetic latitudes in the dayside magnetosphere

被引:33
作者
Allen, R. C. [1 ]
Zhang, J. -C. [1 ]
Kistler, L. M. [1 ]
Spence, H. E. [1 ]
Lin, R. -L. [1 ]
Dunlop, M. W. [2 ]
Andre, M. [3 ]
机构
[1] Univ New Hampshire, Ctr Space Sci, Durham, NH 03824 USA
[2] Rutherford Appleton Lab, Div Space Sci, Didcot OX11 0QX, Oxon, England
[3] Swedish Inst Space Phys, Uppsala, Sweden
关键词
magnetosphere; EMIC waves; solar wind; geomagnetic activity; Cluster; ION-CYCLOTRON WAVES; EARTHS MAGNETOSPHERE; SOURCE REGION; PLASMA; FIELD; DENSITY; PROPAGATION; INSTABILITY; FREQUENCY; FLUXES;
D O I
10.1002/jgra.50600
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It is well accepted that the propagation of electromagnetic ion cyclotron (EMIC) waves are bidirectional near their source regions and unidirectional when away from these regions. The generally believed source region for EMIC waves is around the magnetic equatorial plane. Here we describe a series of EMIC waves in the Pc1 (0.2-5 Hz) frequency band above the local He+ cyclotron frequency observed in situ by all four Cluster spacecraft on 9 April 2005 at midmagnetic latitudes (MLAT = similar to 33 degrees-49 degrees) with L = 10.7-11.5 on the dayside (MLT = 10.3-10.4). A Poynting vector spectrum shows that the wave packets consist of multiple groups of packets propagating bidirectionally, rather than unidirectionally, away from the equator, while the local plasma conditions indicate that the spacecraft are entering into a region sufficient for local wave excitation. One possible interpretation is that, while part of the observed waves are inside their source region, the others are either close enough to the source region, or mixed with the wave packets from multiple source regions at different latitudes.
引用
收藏
页码:6266 / 6278
页数:13
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