Article

A comparison between the Earth's and Mars' bow shocks detected by the Phobos Plasma-Wave System

Laboratoire de Physique et Chimie de l'Environnement, CNRS, F-45071 Orléans Cedex 02, France; R. Grard,; A. Pedersen; Space Science Department, ESA/ESTEC, Keplerlaan 1, NL-2200 AG Noordwijk, The Netherlands; S. Klimov,; S. Savin,; A. Skalsky; Space Research Institute, U.S.S.R. Academy of Sciences, Profsoyuznaya 84/32, Moscow 117810, U.S.S.R.; C. Kennel; Institute of Geophysics and Planetary Physics, University of California, CA 90024, U.S.A.
Planetary and Space Science DOI:10.1016/0032-0633(91)90132-T pp.99-112

ABSTRACT Among the scientific instruments on the Phobos spacecraft, one was expected to study the plasma and wave phenomena in the Martian environment: the Plasma-Wave System, PWS. Here we report on the PWS plasma and electric-field spectrum measurements during two Martian bow shock crossings by Phobos 2: one is located near the subsolar point and the other near the dusk terminator. A comparison is also made with the Earth's shock crossed by Phobos 1. As at Earth, three main regions were identified: the upstream region, the shock transition region and the downstream region. A shock foot boundary is often observed in front of the bow shock. This foot is known to be associated with gyrating ions reflected from the shock. Electric-field spectra are presented and tentatively interpreted. The dynamic spectrograms shown in this report differ from the ones published previously, for the fact that the filter channels are not sampled at the same time has been taken into account.

0 0
 · 
0 Bookmarks
 · 
13 Views

Keywords

bow shock
 
downstream region
 
dusk terminator
 
dynamic spectrograms
 
Earth's shock
 
electric-field spectrum measurements
 
main regions
 
Martian bow shock crossings
 
Phobos 1
 
Phobos 2
 
Phobos spacecraft
 
plasma
 
Plasma-Wave System
 
PWS
 
PWS plasma
 
shock foot boundary
 
shock transition region
 
upstream region
 
wave phenomena