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High-Latitude Magnetic Reconnection in
Sub-Alfvénic Flow: by Levon Avanov 12 October 2001 The Interball Tail spacecraft crossed the high-latitude magnetopause near the cusp region under northward IMF conditions on 29 May 1996, with magnetic local time and magnetic latitude of ~7.3 hours and ~65.4 degrees, respectively. Under these IMF conditions the Interball Tail spacecraft observed quasi-steady reconnection in progress and evidence for a relatively stable reconnection site at high latitudes. Sunward plasma flow observed by Interball Tail and a determination of the tangential stress balance indicated that reconnection was occurring poleward of the Earth's magnetic cusp, above the spacecraft location. At these high latitudes, the gas dynamic model of the solar wind/magnetosphere interaction indicates that the magnetosheath flow should be super-Alfvénic, and therefore that the reconnection site should have propagated tailward. However, the spacecraft observed sub-Alfvénic flow in the magnetosheath region adjacent to the magnetopause current layer near the reconnection site indicating that the reconnection site may have moved in the sunward direction. These observations suggest that the region of sub-Alfvénic flow and stable, quasi-steady reconnection extend to very high latitudes under northward IMF conditions. It is shown that the thickness of the magnetopause current layer for this event (estimated as ~1600 km) is consistent with that found for reconnection at the dayside magnetopause.
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