1 / 1

K. Sauer (1,2) , Ch. Mazelle (3) , K. Baumgärtel (4) and R. Sydora (2)

5th Alfven Conference on Plasma Interaction with Non-magnetized Planets/Moons and its Influence on Planetary Evolution, Sapporo, Japan , October 4-8, 2010. Multi-fluid and Hybrid Code Simulations of Solar-Wind Interaction with the Martian Hydrogen Exosphere: PCW Generation.

fordon
Download Presentation

K. Sauer (1,2) , Ch. Mazelle (3) , K. Baumgärtel (4) and R. Sydora (2)

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript

  1. 5th Alfven Conference on Plasma Interaction with Non-magnetized Planets/Moons and its Influence on Planetary Evolution, Sapporo, Japan , October 4-8, 2010 Multi-fluid and Hybrid Code Simulations of Solar-Wind Interaction with the Martian Hydrogen Exosphere: PCW Generation K. Sauer(1,2), Ch. Mazelle(3), K. Baumgärtel(4) and R. Sydora(2) Summary: The interaction of two different proton (ion) populations with relative drift leads to the generation of large-amplitude waves near Ωp. At the final state the differential velocity reaches about ∆v~2VA.

More Related