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Titel Entropy production at the multi-fluid MHD solar wind termination shock
VerfasserIn Hans-Jörg Fahr Link zu Wikipedia, Mark Siewert
Konferenz EGU General Assembly 2014
Medientyp Artikel
Sprache Englisch
Digitales Dokument PDF
Erschienen In: GRA - Volume 16 (2014)
Datensatznummer 250087568
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2014-1623.pdf
 
Zusammenfassung
In recent years it has become evident that the solar wind termination shock needs to be explained by a multi-fluid MHD phenomenon. To describe the entangled complexity of thermodynamic and dynamic interactions of several different fluids one has to start from a consistent multi-species MHD shock description. We treat the passage of three separate fluids over the shock, namely solar wind protons, pick-up protons and electrons. Associated with the different downstream fluid pressures we then calculate different fluid entropies that are produced at the shock passage. We do show that the most relevant contribution to the total particle entropy is connected with the electron pressure which actually by far dominates the downstream plasma dynamics.