Physics
Scientific paper
Jan 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jgra..11001209b&link_type=abstract
Journal of Geophysical Research, Volume 110, Issue A1, CiteID A01209
Physics
21
Magnetospheric Physics: Solar Wind Interactions With Unmagnetized Bodies, Magnetospheric Physics: Planetary Magnetospheres (5443, 5737, 6033), Interplanetary Physics: Discontinuities (7811), Planetary Sciences: Solar System Objects: Mars, Planetary Sciences: Solar System Objects: Venus
Scientific paper
The magnetic pileup boundary (MPB) is a sharp, thin, and well-defined plasma boundary located between the bow shock and the inner ionospheric boundary at comets, Mars, and Venus. This boundary separates the magnetosheath, a region of low magnetic fields with a conspicuous wave activity, from the magnetic pileup region dominated by strong, highly organized magnetic fields as a result of the pileup and draping of the interplanetary magnetic field. In the present paper we study the magnetic structure of the magnetic pileup boundary at Mars and Venus by means of the technique of minimum variance of the magnetic field. For each one of the crossings analyzed, we obtain a very well defined minimum variance vector. At Mars the direction of this vector agrees with the normal to the MPB fit obtained from Mars Global Surveyor crossings. The results confirm that the MPB is a well-defined plasma boundary. According to empirical criteria based on minimum variance analysis results, the Martian and Venusian MPB crossings would resemble an MHD tangential discontinuity rather than a rotational discontinuity. However, spacecraft observations suggest that the nature of the MPB could be far more complex. We compare our results with similar studies at the MPB of comets and the magnetic tail boundary of Titan, and we discuss the nature of the boundary from a general perspective.
Acuña Mario Humberto
Bertucci Cesar
Mazelle Christian
Russell Christopher T.
Slavin James Arthur
No associations
LandOfFree
Structure of the magnetic pileup boundary at Mars and Venus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Structure of the magnetic pileup boundary at Mars and Venus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of the magnetic pileup boundary at Mars and Venus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-808578