Interplanetary magnetic field B(y) control of dayside auroras

Viking UV images for large positive and negative interplanetary magnetic field (IMF) are studied to ascertain IMF B(y) component effects on the dayside auroral oval in March-November 1986. It is found that the intensity of dayside auroras tends to increase for negative IMF B(y) and to increase for p...

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Published in:Journal of atmospheric and solar-terrestrial physics 1999-07, Vol.61 (11), p.829-840
Main Authors: Trondsen, T S, Cogger, L L, Murphree, J S, Lyatsky, W
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Language:English
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container_title Journal of atmospheric and solar-terrestrial physics
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creator Trondsen, T S
Cogger, L L
Murphree, J S
Lyatsky, W
description Viking UV images for large positive and negative interplanetary magnetic field (IMF) are studied to ascertain IMF B(y) component effects on the dayside auroral oval in March-November 1986. It is found that the intensity of dayside auroras tends to increase for negative IMF B(y) and to increase for positive B(y), so that the negative conditions appear preferable for observations of the dayside auroras. (AIAA)
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title Interplanetary magnetic field B(y) control of dayside auroras
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