Abstract
We use search-coil magnetometer data from a low-latitude station in Parkfield, California (L = 1.77) to study the occurrence of Pc1 pulsations associated with geomagnetic storms. The Pc1 pulsations and storms are identified using automatic algorithms, and the statistical distributions are examined using a superposed epoch analysis technique, as a function of local time, time relative to storm main phase, and storm intensity. Results show that Pc1 pulsations are 2-3 times more likely (than normal) to be observed in the 2-4 d following moderate storms and 4-5 times more likely in the 2-7 d following intense storms. The Pc1 frequencies are higher in moderate storms than they are in nonstorm times and become even higher and occupy a greater range of local times as the strength of the storms increase. These results are consistent with the idea that the source of EMIC waves extends to lower L values as storm intensity increases. Copyright 2008 by the American Geophysical Union.
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CITATION STYLE
Bortnik, J., Cutler, J. W., Dunson, C., Bleier, T. E., & McPherron, R. L. (2008). Characteristics of low-latitude Pc1 pulsations during geomagnetic storms. Journal of Geophysical Research: Space Physics, 113(4). https://doi.org/10.1029/2007JA012867
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