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Detailed Reference Information |
Sato, N., Murata, Y., Yamagishi, H., Yukimatu, A.S., Kikuchi, M., Watanabe, M., Makita, K., Yang, H., Liu, R. and Rich, F.J. (2001). Enhancement of optical aurora triggered by the solar wind negative pressure impulse (SI-). Geophysical Research Letters 28: doi: 10.1029/2000GL003742. issn: 0094-8276. |
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A geomagnetic negative sudden impulse (SI-) occurred on 3 August 1997 in association with a sudden decrease of solar wind dynamic pressure. The discrete auroras observed by an all-sky TV imager at Zhongshan in Antarctica (magnetic latitude is ~74.5 ¿S) suddenly enhanced their luminosity and moved poleward at the time of the SI-. Following the primary enhancement, three cycles of quasi-periodic luminosity pulsations were observed with periods of about 10--14 min and their average position drifted equatorward. The luminosity pulsations showed one-to-one correspondence with the magnetic pulsations, with the characteristic features of a field-line resonance. The low-altitude DMSP-F13 satellite was almost directly over Zhongshan and observed accelerated electron precipitation with an inverted 'V' structure and an upward field-aligned current. These signatures suggest that the solar wind negative pressure impulse triggered a field-line resonance of the geomagnetic field. The resonance caused the upward and downward field-aligned current sheets, and the field-aligned electron acceleration. ¿ 2001 American Geophysical Union |
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Abstract |
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Keywords
Magnetospheric Physics, Magnetopause, cusp, and boundary layers, Magnetospheric Physics, MHD waves and instabilities |
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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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