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Rosetta uses 11 scientific instruments to study the nucleus, coma, and solar wind interaction.
The solar wind interaction with Venus is used to illustrate the induced magnetosphere that results from the solar wind interaction with an ionosphere.
Time dependent numerical simulation of relativistic wind interaction with interstellar medium was performed.
Therefore, these features seem to be common for the solar wind interaction of non-magnetized planets.
The solar wind interaction with the weakly magnetized Mars and Venus differs from the solar wind interaction with the Earth and other strongly magnetized planets in our solar system.
The results suggest that the Martian ionosphere is controlled both by solar wind interaction and by the crustal magnetic field.
We investigate the contribution of the radial component of the magnetic field in the solar wind interaction with Mars.
The solar wind interaction with the asteroid 433 Eros is investigated using magnetometer data from the NEAR-Shoemaker spacecraft.
The main power source for auroral emissions is planetary rotation at Jupiter, and the solar wind interaction at Earth.
The influence of cometary jets on the solar wind interaction is studied with a 3D hybrid simulation.
We have developed a real-time global MHD (magnetohydrodynamics) simulation of the solar wind interaction with the earth's magnetosphere.
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