Stellar winds and planetary bodies simulations: Magnetized obstacles in super-Alfvénic and sub-Alfvénic flows
Authors:
- Y. VernisseYVY. Vernisse
- J.A. RioussetJRJ.A. Riousset
- U. MotschmannUMU. Motschmann
- K.-H. GlassmeierKGK.-H. Glassmeier
- 1 March 2017
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 137, 40-51
Abstract
No abstract availableKeywords
Funding Information
- Deutsches Zentrum für Luft- und Raumfahrt (50QW1101, 50OC1102, 50OW1501, 50QP1401, 50 OC 1001)
This publication has 47 references indexed in Scilit:
- A 3D hybrid simulation study of the electromagnetic field distributions in the lunar wakeIcarus, 2011
- First lunar wake passage of ARTEMIS: Discrimination of wake effects and solar wind fluctuations by 3D hybrid simulationsPlanetary and Space Science, 2011
- Plasma boundaries at Mars: a 3-D simulation studyAnnales Geophysicae, 2004
- Surface conductivity of Mercury provides current closure and may affect magnetospheric symmetryAnnales Geophysicae, 2004
- Cusp observations of high‐ and low‐latitude reconnection for northward interplanetary magnetic fieldJournal of Geophysical Research, 2000
- Three‐dimensional plasma simulation of Io's interaction with the Io plasma torus: Asymmetric plasma flowJournal of Geophysical Research, 1999
- On the possibility of coherent cyclotron emission from extrasolar planetsJournal of Geophysical Research, 1999
- The sub‐Alfvénic interaction of the Galilean satellites with the Jovian magnetosphereJournal of Geophysical Research, 1998
- A new functional form to study the solar wind control of the magnetopause size and shapeJournal of Geophysical Research, 1997
- Magnetospheric electric fields and currentsReviews of Geophysics, 1987