Articles | Volume 28, issue 5
https://doi.org/10.5194/angeo-28-1053-2010
https://doi.org/10.5194/angeo-28-1053-2010
05 May 2010
 | 05 May 2010

Local influence of magnetosheath plasma beta fluctuations on magnetopause reconnection

T. V. Laitinen, Y. V. Khotyaintsev, M. André, A. Vaivads, and H. Rème

Abstract. We present observations from two subsolar Cluster magnetopause crossings under southward interplanetary magnetic field and strong mirror mode fluctuations in the magnetosheath. In both events the reconnection outflow jets show strong variations on the timescale of one minute. We show that at least some of the recorded variations are truly temporal, not spatial. On the same timescale, mirror mode fluctuations appear as strong magnetic fluctuations in the magnetosheath next to the magnetopause. This suggests that mirror modes can cause the variations either through modulation of continuous reconnection or through triggering of bursty reconnection. Using a theoretical scaling law for asymmetric reconnection we show that modulation of reconnection at a single x-line can explain the observations of the first event. The second event cannot be explained by a single modulated x-line: there the evidence points to patchy and bursty reconnection.