Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..321i&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.321
Computer Science
Scientific paper
We have developed a modified version of the Cooling model [3] to trace the motion of flux tubes generated by reconnection at Mercury, and in this paper we compare the model FTEs with observations of FTEs made by MESSENGER. We use these comparisons to determine the most likely location and orientation of the magnetic X-lines at Mercury's magnetopause during a variety of solar wind conditions.
Boardsen Scott A.
Imber S. M.
Korth Haje
Solomon Stanley C.
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