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Magnetic field overshoots in the Venus blow shock

Conference · · Adv. Space Res.; (United States)
OSTI ID:5604072
An examination of Pioneer Venus Orbiter fluxgate magnetometer data has shown that magnetic field overshoots occur not only behind quasi-perpendicular bow shocks but also behind quasi-parallel shocks. Overshoots are assocciated only with supercritical shocks. Their amplitudes increase with increasing fast Mach number. Solar wind beta has a lesser effect. The thickness of the overshoot increases with decreasing Theta-BN. The thickness of apparent overshoots detected behind 4 strong fast interplanetary shocks (M greater than M/crit) is about 3 orders of magnitude larger. Multiple crossings of the Venus bow shock were observed mainly at turbulent shocks. Their occurence is not influenced by Theta-BN. 15 references.
Research Organization:
Kozponti Fizikai Kutato Intezet, Budapest, Hungary
OSTI ID:
5604072
Report Number(s):
CONF-8406167-
Conference Information:
Journal Name: Adv. Space Res.; (United States) Journal Volume: 4
Country of Publication:
United States
Language:
English