Titlebook: Mars’ Magnetism and Its Interaction with the Solar Wind; Daniel Winterhalter,Mario Acuña,Alexander Zakharov Book 2004 Springer Science+Bus

Exploit

M. I. Verigin,J. Slavin,A. Szabo,G. A. Kotova,A. P. Remizov,H. Rosenbauer,S. Livi,K. Szegö,M. Tátral

ARBOR

Bow Shock and Upstream Phenomena at Marsmagnetic field data (Acuña ., 1998). As detailed by a series of review papers in this monograph, the Mars Global Surveyor (MGS) mission has now shown that the Mars environment is very complex with strong, highly structured crustal magnetic remnants in the southern hemisphere, while the northern hemi

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meditation

absorbed

Magnetic Flux Ropes in the Martian Atmosphere: Global Characteristicsentation is more horizontal near the terminator for altitudes greater than 200 km. We have identified fewer flux ropes for SZA between 40 to 60 deg and for SZA lower than 20 deg, like in the case of Venus (Elphic and Russell, 1983b). Statistically, Mars’ ionosphere with SZA range between 40. to 60.

hangdog

Mars Express and MARSISwhich have been predicted in the dayside/terminator ionosphere. Measurements on the nightside can be used to search for proposed fine structures (‘holes’) in the electron density. Hydrodynamic waves are predicted to be excited by the solar wind/ionosphere interaction and their influence on the elect

Arrhythmia

1385-7525 he solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions. .978-90-481-6582-7978-0-306-48604-3Series ISSN 1385-7525

Gourmet

Mars’ Magnetism and Its Interaction with the Solar Wind

Gourmet

Book 2004teraction between Mars and the solar wind comes, for the first time, into sharp focus. This work, detailing the integration and new interpretation of the MGS and Phobos results, is a primary reference for the researcher studying solar wind/planet interactions. .

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