Physics – Plasma Physics
Scientific paper
Jul 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008georl..3513103s&link_type=abstract
Geophysical Research Letters, Volume 35, Issue 13, CiteID L13103
Physics
Plasma Physics
6
Magnetospheric Physics: Cusp, Space Plasma Physics: Neutral Particles (2151), Ionosphere: Auroral Ionosphere (2704), Interplanetary Physics: Solar Wind Plasma
Scientific paper
On 28 April 2001, significant enhancements of neutral atom signals were detected in the direction of a high-altitude cusp by the Low-Energy Neutral Atom (LENA) imager onboard the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE). Simultaneously, proton auroral emission was observed in the low-altitude cusp by the Far-Ultraviolet Instrument (FUV) on the IMAGE spacecraft. The temporal variations of their intensities showed a good correlation, suggesting they had a common source. During a brief period, the proton auroral spot moved antisunward and dawnward in conjunction with the motion of the ionospheric footprint of the LENA cusp signal. The Tsyganenko-96 model shows that the possible source location of the LENA cusp signals maps to the FUV spot. Considering the solar wind variations, we have attributed this ``moving proton auroral spot'' to a moving flux tube that was created by transient reconnection on the dayside magnetopause and contained relatively high proton densities.
Collier Michael R.
Frey Harald U.
Hosokawa Kazuo
Mende Stephen B.
Moore Thomas Earle
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