• Aucun résultat trouvé

Plasma boundaries at Mars: a 3-D simulation study

N/A
N/A
Info
Télécharger
Protected

Academic year: 2021

Partager "Plasma boundaries at Mars: a 3-D simulation study"

Copied!
18
0
0

Chargement.... (Voir le texte intégral maintenant)

Texte intégral

Figure

Fig. 1. Number density of the solar wind protons and heavy ions, proton temperature and magnetic field along a circular orbit from 16 March 1989 measured by ASPERA on board Phobos-2 (adapted from Sauer and Dubinin, 2000)
Fig. 2. Data obtained from different instruments on board Phobos-2 along an elliptical orbit from 8 February 1989 (adapted from Sauer and Dubinin, 2000)
Fig. 3. Cross sections of the simulation box at the plane x = 0, y = 0 and z =0 presented in Sect
Fig. 5. Neutral gas density (blue line), the ion production rate (red line in subsolar direction and green line at the terminator) of oxygen as a function of altitude at solar minimum (ν = 1 · 10 −7 s −1 )
+7

Références

Télécharger maintenant ( PDF - 18 Page - 3.09 MB )

Documents relatifs

Comparison of plasma data from ASPERA-3/Mars-Express with a 3-D hybrid simulation

Hybrid sim- ulations for unmagnetised planets (Shimazu, 2001; Ter- ada et al., 2002; Kallio and Janhunen, 2002; B¨oßwetter et al., 2004; Modolo et al., 2005), a statistical analysis

Electrostatic analyzer with a 3-D instantaneous field of view for fast measurements of plasma distribution functions in space

For three-axis stabilized (i.e., nonspinning) spacecraft, like STEREO which is continuously imaging the Sun, an alternative strategy is required to measure solar wind electrons: