Results 161 to 170 of about 196,114 (210)

Solar Wind and planetary magnetospheres

open access: yes, 2015
Solar Wind interacts with solar system objects by exchanging momentum and energy. This transfer is particularly effective in the case of weakly magnetized bodies (Mars, Venus and comets) and small magnetosphere (Mercury).This interaction contributes to the erosion of the gaseous envelop and to the atmospheric dynamic and has therefore an important ...
Modolo, Ronan   +5 more
core   +11 more sources

Planetary magnetospheres

Reviews of Geophysics, 1975
The study of extraterrestrial planetary magnetospheres during the past 4 years has experienced a dramatic growth in the availability of observational data and a concomitant growth in the level of scientific interest comparable to the experience of the early 1960's in the study of earth's magnetosphere. Owing in large part to the success of space probes
T. W. Hill, F. C. Michel
exaly   +2 more sources

Planetary magnetospheres

Reviews of Geophysics, 1979
Although the Jupiter encounters of Pioneers 10 and 11 occurred in the previous quadrennium, the flood of new information that they released launched a wave of publications that crested in the present quadrennium. For completeness all of the magnetospheric literature relating to the two encounters is included in the bibliography. The present quadrennium
James Slavin
exaly   +2 more sources

Captured dust in planetary magnetospheres

AIP Conference Proceedings, 1998
Interplanetary and interstellar dust particles acquire a positive charge in the solar wind and can be strongly influenced by the Lorentz force as they pass through planetary magnetospheres. There, the charge on the particles changes rapidly when they pass through different plasma environments.
Joshua Colwell
exaly   +2 more sources

Plasma waves in planetary magnetospheres

Journal of Geophysical Research, 1991
With the completion of the Voyager 2 encounter with Neptune we have now surveyed the plasma wave spectra of five planetary magnetospheres: Earth, Jupiter, Saturn, Uranus, and Neptune. Here we provide a first general comparison of the various plasma wave modes at each of the planets with the use of a common format for displaying the spectra. The general
William Kurth
exaly   +2 more sources

Dust waves in rotating planetary magnetospheres

AIP Conference Proceedings, 2005
Low frequency electrostatic drift and acoustic waves are studied in rotating dusty plasmas. Linear dispersion relation is found. It is pointed out that rotation of the planet can introduce dust drift waves through Coriolis force in the planetary magnetospheres. This mode can couple with dust acoustic mode. Coriolis force effect may give rise to dipolar
Qamar Haque
exaly   +2 more sources

Planetary Magnetospheres

Annual Review of Astronomy and Astrophysics, 1982
D. P. Stern, N. F. Ness
exaly   +2 more sources

Planetary Magnetospheres

Thirty Years of Astronomical Discovery With UKIRT, 2010
Thomas Earle Moore
exaly   +2 more sources

Planetary magnetospheres

Reports on Progress in Physics, 1993
exaly   +2 more sources

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