Isbn: 9783659937507 - solar wind interaction with ionosphere of mars: ionosphere of mars (7 resultados)

Taschenbuch. Condición: Neu. Solar wind interaction with Ionosphere of Mars | Ionosphere of Mars | Sharad Seth | Taschenbuch | 176 S. | Englisch | 2016 | LAP LAMBERT Academic Publishing | EAN 9783659937507 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu.…

Paperback. Condición: Brand New. 176 pages. 8.66x5.91x0.40 inches. In Stock.

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Taschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -The magnetosphere of Mercury,Earth,Jupiter,Saturn, Uranus and Neptune are described.Venus and Mars have no magnetosphere.The solar wind is able to penetrate directly into the atmospheres of these planets.Among them,Mars is the current interest of present book.In absence of Mars own magnetic field, its ionosphere is strongly influenced by solar wind/interplanetary magnetic field.In this book AYS approach, continuity and momentum equations and Steady state Kinetic model are solved. The results obtained from AYS approach and continuity and momentum equations are compared with experimental data measured by MGS/Viking spacecrafts and other calculations carried by MTGCM and Hybrid model.ER measurements carried on 2 April, 1998 by MGS at energy range 10-1000 eV are described in the dayside and nightside Martian atmosphere.The flux,ion production rates,ion and electron densities are calculated due to impact of solar EUV and electron-proton-hydrogen atom with the atmosphere of Mars.A steady state kinetic model is used to calculate parallel electron current density at different potential differences in the exosphere of Mars. 176 pp. Englisch.…

Condición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Seth SharadDr. Seth completed his Ph.D. degree in Planetary Sciences from Gujarat University in 2003. He visited Division of Astrophysics, INPE, Brazil on Post Doctoral Fellowship. He has published various research papers in national.…

Taschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -The magnetosphere of Mercury,Earth,Jupiter,Saturn, Uranus and Neptune are described.Venus and Mars have no magnetosphere.The solar wind is able to penetrate directly into the atmospheres of these planets.Among them,Mars is the current interest of present book.In absence of Mars own magnetic field, its ionosphere is strongly influenced by solar wind/interplanetary magnetic field.In this book AYS approach, continuity and momentum equations and Steady state Kinetic model are solved. The results obtained from AYS approach and continuity and momentum equations are compared with experimental data measured by MGS/Viking spacecrafts and other calculations carried by MTGCM and Hybrid model.ER measurements carried on 2 April, 1998 by MGS at energy range 10-1000 eV are described in the dayside and nightside Martian atmosphere.The flux,ion production rates,ion and electron densities are calculated due to impact of solar EUV and electron-proton-hydrogen atom with the atmosphere of Mars.A steady state kinetic model is used to calculate parallel electron current density at different potential differences in the exosphere of Mars.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 176 pp. Englisch.…

Taschenbuch. Condición: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The magnetosphere of Mercury,Earth,Jupiter,Saturn, Uranus and Neptune are described.Venus and Mars have no magnetosphere.The solar wind is able to penetrate directly into the atmospheres of these planets.Among them,Mars is the current interest of present book.In absence of Mars own magnetic field, its ionosphere is strongly influenced by solar wind/interplanetary magnetic field.In this book AYS approach, continuity and momentum equations and Steady state Kinetic model are solved. The results obtained from AYS approach and continuity and momentum equations are compared with experimental data measured by MGS/Viking spacecrafts and other calculations carried by MTGCM and Hybrid model.ER measurements carried on 2 April, 1998 by MGS at energy range 10-1000 eV are described in the dayside and nightside Martian atmosphere.The flux,ion production rates,ion and electron densities are calculated due to impact of solar EUV and electron-proton-hydrogen atom with the atmosphere of Mars.A steady state kinetic model is used to calculate parallel electron current density at different potential differences in the exosphere of Mars.…