Results 261 to 270 of about 116,603 (307)
First Detection of Deuterium in Venus's Extended Exosphere
Weichbold F +27 more
europepmc +1 more source
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Ion Acceleration at the Earth’s Bow Shock
Space Science Reviews, 2012The Earth’s bow shock is the most studied example of a collisionless shock in the solar system. It is also widely used to model or predict the behaviour at other astrophysical shock systems. Spacecraft observations, theoretical modelling and numerical simulations have led to a detailed understanding of the bow shock structure, the spatial organization ...
Burgess, D., Möbius, E., Scholer, M.
openaire +4 more sources
Cluster at the Bow Shock: Introduction
Space Science Reviews, 2005International ...
Balogh, A. +13 more
openaire +4 more sources
Journal of Geophysical Research: Space Physics, 1995
Voyager 2 crossed the inbound or upstream Neptunian bow shock at 1430 spacecraft event time on August 24 in 1989 (Belcher et al., 1989). The plasma and magnetic field measurements allow us to study the solar wind interaction with the outermost gas giant.
Adam Szabo, Ronald P. Lepping
openaire +1 more source
Voyager 2 crossed the inbound or upstream Neptunian bow shock at 1430 spacecraft event time on August 24 in 1989 (Belcher et al., 1989). The plasma and magnetic field measurements allow us to study the solar wind interaction with the outermost gas giant.
Adam Szabo, Ronald P. Lepping
openaire +1 more source
AIP Conference Proceedings, 2005
The study of pulsar bow‐shocks is one of the most promising ways towards the understanding of the interactions between neutron stars relativistic winds and their environment. These objects are best resolved as Hα nebulae but velocity‐driven features are seen also in the radio and X‐ray bands and represent interesting targets for future gamma‐rays ...
openaire +1 more source
The study of pulsar bow‐shocks is one of the most promising ways towards the understanding of the interactions between neutron stars relativistic winds and their environment. These objects are best resolved as Hα nebulae but velocity‐driven features are seen also in the radio and X‐ray bands and represent interesting targets for future gamma‐rays ...
openaire +1 more source
2013
Our present knowledge of the properties of the various planetary bow shocks is briefly reviewed. We do not follow the astronomical ordering of the planets. We rather distinguish between magnetised and unmagnetised planets which groups Mercury and Earth with the outer giant planets of the solar system, Mars and Moon in a separate group lacking magnetic ...
André Balogh, Rudolf A. Treumann
openaire +1 more source
Our present knowledge of the properties of the various planetary bow shocks is briefly reviewed. We do not follow the astronomical ordering of the planets. We rather distinguish between magnetised and unmagnetised planets which groups Mercury and Earth with the outer giant planets of the solar system, Mars and Moon in a separate group lacking magnetic ...
André Balogh, Rudolf A. Treumann
openaire +1 more source
Heliospheric shocks (excluding planetary bow shocks)
Reviews of Geophysics, 1987Even though it took place less than halfway through the last four year period, the AGU Chapman Conference in Napa Valley, California, during February, 1984, highlighted in many ways current U. S. contributions to the study of heliospheric shocks. Considerable recent progress in the theoretical understanding of these discontinuities has been summarized ...
openaire +1 more source
Structure of the Earth's bow shock
Journal of Geophysical Research, 1972Numerical simulations have provided detailed information of the microscopic processes that occur in a high Mach number oblique shock wave such as the bow shock. The gross feature of the ion dissipation is a strong interaction of the reflected ions with the whistler precursor, which can be explained by a nonlinear ion-ion counterstreaming instability ...
Biskamp, D., Welter, H.
openaire +2 more sources
Overshoots in planetary bow shocks
Nature, 1982The parametric variation with solar wind conditions in the overshoot in magnetic field strength observed in planetary bow shocks and believed to be associated with the ion reflection process is examined based on both terrestrial and planetary bow shock data.
C. T. Russell +2 more
openaire +1 more source
1985
Planetary bow shocks provide insight into both the behavior of collisionless shocks and the nature of the planetary obstacle responsible for creating those bow shocks. This review paper first presents a survey of the microstructure of planetary bow shocks using data obtained at Mercury, Venus, the earth, Mars, Jupiter, and Saturn.
openaire +1 more source
Planetary bow shocks provide insight into both the behavior of collisionless shocks and the nature of the planetary obstacle responsible for creating those bow shocks. This review paper first presents a survey of the microstructure of planetary bow shocks using data obtained at Mercury, Venus, the earth, Mars, Jupiter, and Saturn.
openaire +1 more source