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Detailed Reference Information |
Stüdemann, W., Wilken, B., Kremser, G., Korth, A., Fennel, J.F., Blake, B., Koga, R., Hall, D., Bryant, D., Søraas, F., Brønstad, K., Fritz, T.A., Lundin, R. and Gloecker, G. (1987). The May 2–3, 1986 magnetic storm: First energetic ion composition observations with the MICS instrument on Viking. Geophysical Research Letters 14: doi: 10.1029/GL014i004p00455. issn: 0094-8276. |
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Measurements with the Magnetospheric Ion Composition Spectrometer (MICS) onboard the polar orbiting Swedish satellite VIKING clearly show a strong asymmetry between the dusk- and dawnside ion distributions obtained after the onset of a magnetic storm on May 2--3, 1986. The eveningside of the inner ring current region is quickly filled by protons with energies of some tens of keV. The morningside continues for several hours to show the quiet-time inner ring current proton spectra in which protons below ~100 keV have been removed due to charge-exchange processes. The data obtained at high latitudes will be compared with measurements of the CHEM instrument on the AMPTE/CCE spacecraft near the equatorial plane. The observations are discussed in context of the convection of injected ions into the inner magnetosphere during magnetically active periods. ¿American Geophysical Union 1987 |
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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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