Abstract
We present here simultaneous H+ and O+ ion dispersion signatures observed by three Cluster spacecraft above the northern auroral zone. These observations occur during strong geomagnetic activity (Kp = 9) and are consistent with a time-of-flight (TOF) dispersion of the ions. Using the TOF dispersion of H+ and O+ and bouncing properties of H +, we show that the ions originate from a distant source located near 80 Re down tail. Our results show that the magnetotail is topographically stable to support multiple bouncing of H+ ions during a storm period. Furthermore these results could suggest that the plasmasheet H+ and O+ ions have been accelerated to the same velocity in the vicinity of a reconnection region. Copyright 2004 by the American Geophysical Union.
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Korth, A., Fränz, M., Zong, Q. G., Fritz, T. A., Sauvaud, J. A., Rème, H., … Daly, P. W. (2004). Ion injections at auroral latitude during the March 31, 2001 magnetic storm observed by Cluster. Geophysical Research Letters, 31(20). https://doi.org/10.1029/2004GL020356
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