During the anomalously low density solar wind interval of May 1999, GEOTAIL
was in the magnetosheath for similar to 37 hours after making an inbound c
rossing of the expanding bow shuck at similar to 8 R-E upstream of its nomi
nal position. Comparison among data sets obtained from GEOTAIL (magnetoshea
th), WIND (near upstream - bow shock), and ACE (far upstream) reveals sever
al unique features: Firstly, during the interval of 1430-1530 UT on 11 May,
we observed both in the solar wind and magnetosheath double-peaked protons
with a peak separation of 250-300 km/s, which was close to the local Alfve
n velocity during the event. Secondly, rye observed extremely strong strahl
electrons both in the solar wind and magnetosheath during the interval of
0600-2100 UT on 11 May 1999. We present an overview of the GEOTAIL observat
ions, and discuss their physical significance.