Preliminary Results
	The position of the various S/C at the time when they encountered the outward moving bow shock. Their distance from the Sun-Erath line is depicted as negative if they were on the dawn side and positive on the dusk side. The red curve is a model bow shock surface for the expected maximum extent of the bow shock. The nominal position of the bow shock and the lunar orbit is also depicted. (generated by Adam Szabo)
	Magnetosphere on May 11, 1999, the Day the Solar Wind Almost Disappeared: I. Current Systems
			GRL paper submitted by Guan Le.
	Magnetosphere on May 11, 1999, the Day the Solar Wind Almost Disappeared: II. Magnetic Pulsations break in Space and on the Ground
			GRL paper submitted by Guan Le.
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