Conjugate observations of electromagnetic ion cyclotron waves associated with traveling convection vortex events

被引:7
作者
Kim, Hyomin [1 ]
Clauer, C. Robert [2 ,3 ]
Gerrard, Andrew J. [1 ]
Engebretson, Mark J. [4 ]
Hartinger, Michael D. [2 ,3 ]
Lessard, Marc R. [5 ]
Matzka, Juergen [6 ]
Sibeck, David G. [7 ]
Singer, Howard J. [8 ]
Stolle, Claudia [6 ]
Weimer, Daniel R. [2 ,3 ]
Xu, Zhonghua [2 ,3 ]
机构
[1] New Jersey Inst Technol, Ctr Solar Terr Res, Newark, NJ 07102 USA
[2] Virginia Polytech Inst & State Univ, Ctr Space Sci & Engn Res, Blacksburg, VA 24061 USA
[3] Virginia Polytech Inst & State Univ, Dept Elect & Comp Engn, Blacksburg, VA 24061 USA
[4] Augsburg Coll, Dept Phys, Minneapolis, MN USA
[5] Univ New Hampshire, Space Sci Ctr, Durham, NH 03824 USA
[6] GFZ German Res Ctr Geosci, Potsdam, Germany
[7] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA
[8] NOAA, Space Weather Predict Ctr, Boulder, CO USA
基金
美国国家科学基金会;
关键词
WIND DYNAMIC PRESSURE; DAWN-DUSK ASYMMETRY; SOLAR-WIND; EMIC WAVES; PROTON PRECIPITATION; GEOMAGNETIC CONDITIONS; IMPULSE EVENTS; MAGNETOSPHERE; VORTICES; MAGNETOPAUSE;
D O I
10.1002/2017JA024108
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report on simultaneous observations of electromagnetic ion cyclotron (EMIC) waves associated with traveling convection vortex (TCV) events caused by transient solar wind dynamic pressure (P-d) impulse events. The Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft located near the magnetopause observed radial fluctuations of the magnetopause, and the GOES spacecraft measured sudden compressions of the magnetosphere in response to sudden increases in Pd. During the transient events, EMIC waves were observed by interhemispheric conjugate ground-based magnetometer arrays as well as the GOES spacecraft. The spectral structures of the waves appear to be well correlated with the fluctuating motion of the magnetopause, showing compression-associated wave generation. In addition, the wave features are remarkably similar in conjugate hemispheres in terms of bandwidth, quasiperiodic wave power modulation, and polarization. Proton precipitation was also observed by the DMSP spacecraft during the wave events, from which the wave source region is estimated to be 72 degrees-74 degrees in magnetic latitude, consistent with the TCV center. The confluence of space-borne and ground instruments including the interhemispheric, high-latitude, fluxgate/induction coil magnetometer array allows us to constrain the EMIC source region while also confirming the relationship between EMIC waves and the TCV current system.
引用
收藏
页码:7336 / 7352
页数:17
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