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Detailed Reference Information |
Kataoka, R., Fukunishi, H., Lanzerotti, L.J., Rosenberg, T.J., Weatherwax, A.T., Engebretson, M.J. and Watermann, J. (2002). Traveling convection vortices induced by solar wind tangential discontinuities. Journal of Geophysical Research 107: doi: 10.1029/2002JA009459. issn: 0148-0227. |
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Two typical magnetic impulse events (MIEs) accompanied by traveling convection vortices (TCVs) are investigated. The analysis of their conjugate equivalent convection patterns is performed using magnetic field data obtained from high-latitude ground magnetometer networks in the Northern and Southern Hemispheres. A three-dimensional analysis of solar wind structures is also performed using solar wind data obtained from multiple International Solar-Terrestrial Physics satellites. In the first event observed at ~1310 UT on 22 May 1996, a westward moving TCV appeared simultaneously in the noon-to-dawn sector in the Northern and Southern Hemispheres. The solar wind source of this TCV is found to be a tangential discontinuity (TD), which causes a rapid northward turning of the interplanetary magnetic field (IMF) and abrupt dynamic pressure changes. In the second event observed at ~1610 UT on 27 May 1998, an eastward moving TCV appeared in the noon sector in the Northern and Southern Hemispheres, with a timing delay of 2 to 3 min in the Southern Hemisphere. The solar wind source of this TCV is found again to be a TD, which causes a rapid IMF By negative turning and an abrupt enhancement of dynamic pressure. Analyses show that the TDs driving these events have their motional electric fields pointing toward the TDs and their normal vectors with large cone angles from the sunward direction. These TDs satisfy the conditions for the formation of a hot flow anomaly (HFA) at the bow shock. The sweeping motion across the magnetosphere of the intersection of the TD and the bow shock is found to be consistent with the observed TCV motion in each event. Magnetopause deformations due to HFAs can explain all the observed morphological features and the triggering process of these two MIEs. It is suggested, however, that bursty merging and/or pressure pulses would reinforce the processes produced by the HFAs, since the TDs are usually accompanied by both abrupt IMF changes and pressure enhancements. Consequently, it seems reasonable to conclude that the integrated processes of HFA, bursty magnetic field merging, and pressure pulses produce the evolution of these MIEs and TCVs. |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Magnetospheric Physics, Solar wind/magnetosphere interactions, Magnetospheric Physics, Magnetopause, cusp, and boundary layers, Magnetospheric Physics, Current systems, Ionosphere, Plasma convection |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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