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
相关论文
共 52 条
[1]   On determining polarization characteristics of ion cyclotron wave magnetic field fluctuations [J].
Anderson, BJ ;
Denton, RE ;
Fuselier, SA .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A6) :13195-13213
[2]   Observational test of local proton cyclotron instability in the Earth's magnetosphere [J].
Anderson, BJ ;
Denton, RE ;
Ho, G ;
Hamilton, DC ;
Fuselier, SA ;
Strangeway, RJ .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A10) :21527-21543
[3]   Source region of 0.2 to 1.0 Hz geomagnetic pulsation bursts [J].
Anderson, BJ ;
Erlandson, RE ;
Engebretson, MJ ;
Alford, J ;
Arnoldy, RL .
GEOPHYSICAL RESEARCH LETTERS, 1996, 23 (07) :769-772
[4]   A STATISTICAL STUDY OF PC 1-2 MAGNETIC PULSATIONS IN THE EQUATORIAL MAGNETOSPHERE .1. EQUATORIAL OCCURRENCE DISTRIBUTIONS [J].
ANDERSON, BJ ;
ERLANDSON, RE ;
ZANETTI, LJ .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1992, 97 (A3) :3075-3088
[5]  
[Anonymous], 1996, ESA SPECIAL PUBLICAT
[6]   The Cluster Magnetic Field Investigation:: overview of in-flight performance and initial results [J].
Balogh, A ;
Carr, CM ;
Acuña, MH ;
Dunlop, MW ;
Beek, TJ ;
Brown, P ;
Fornacon, KH ;
Georgescu, E ;
Glassmeier, KH ;
Harris, J ;
Musmann, G ;
Oddy, T ;
Schwingenschuh, K .
ANNALES GEOPHYSICAE, 2001, 19 (10-12) :1207-1217
[7]   Ion observations from geosynchronous orbit as a proxy for ion cyclotron wave growth during storm times [J].
Blum, Lauren W. ;
MacDonald, Elizabeth A. ;
Gary, S. Peter ;
Thomsen, Michelle F. ;
Spence, Harlan E. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2009, 114
[8]   Global simulation of EMIC wave excitation during the 21 April 2001 storm from coupled RCM-RAM-HOTRAY modeling [J].
Chen, Lunjin ;
Thorne, Richard M. ;
Jordanova, Vania K. ;
Wang, Chih-Ping ;
Gkioulidou, Matina ;
Lyons, Larry ;
Horne, Richard B. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2010, 115
[9]   Simulation of EMIC wave excitation in a model magnetosphere including structured high-density plumes [J].
Chen, Lunjin ;
Thorne, Richard M. ;
Horne, Richard B. .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2009, 114
[10]   PRECIPITATION OF AURORAL AND RING CURRENT PARTICLES BY ARTIFICIAL PLASMA INJECTION [J].
CORNWALL, JM .
REVIEWS OF GEOPHYSICS AND SPACE PHYSICS, 1972, 10 (04) :993-&