Sheared flows and small-scale Alfven wave generation in the auroral acceleration region

被引:43
|
作者
Asamura, K. [1 ]
Chaston, C. C. [2 ]
Itoh, Y. [1 ,4 ]
Fujimoto, M. [1 ]
Sakanoi, T. [5 ]
Ebihara, Y. [3 ]
Yamazaki, A. [1 ]
Hirahara, M. [4 ]
Seki, K. [7 ]
Kasaba, Y. [5 ]
Okada, M. [6 ]
机构
[1] JAXA, Inst Space & Astronaut Sci, Sagamihara, Kanagawa 2298510, Japan
[2] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[3] Nagoya Univ, Inst Adv Res, Nagoya, Aichi 4648601, Japan
[4] Univ Tokyo, Grad Sch Sci, Tokyo 1130033, Japan
[5] Tohoku Univ, Grad Sch Sci, Sendai, Miyagi 9808578, Japan
[6] Natl Inst Polar Res, Tokyo 1738515, Japan
[7] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan
基金
日本学术振兴会;
关键词
ELECTRIC-FIELDS; INSTABILITY; IONOSPHERE; ONBOARD; DRIVEN; ARCS;
D O I
10.1029/2008GL036803
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Coincident particle and optical measurements from the Reimei spacecraft suggest that sheared flows through an inverted-V arc may be unstable to the emission of Alfven waves. The particle measurements reveal time dispersed field-aligned electron bursts typical of low energy electrons accelerated by inertial Alfven waves (IAWs). These Alfven wave accelerated electrons are embedded within multi-keV inverted-V electron structures. The optical measurements at the footprint of the inverted-V structures reveal counter propagating and folded/vortical discrete auroral forms moving with speeds of similar to 14-18 km/s. We show that the flow shear inferred from this motion exceeds that required for instability to the emission of Alfven waves on scales of the order of an electron inertial length. The emission of these waves provides a likely means for driving the low energy dispersed electron bursts we observe. Citation: Asamura, K., et al. (2009), Sheared flows and small-scale Alfven wave generation in the auroral acceleration region, Geophys. Res. Lett., 36, L05105, doi:10.1029/2008GL036803.
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页数:5
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