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Simulation Models for Exploring Magnetic Reconnection. [PDF]
Shay M +24 more
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The Interplay Between Collisionless Magnetic Reconnection and Turbulence. [PDF]
Stawarz JE +15 more
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Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]
Liu YH +14 more
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SMILE Modeling Working Group: Modeling and Analysis of X-ray and Ultraviolet Images of Solar Wind - Earth Interactions. [PDF]
Connor HK +15 more
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PLANETARY EMBRYO BOW SHOCKS AS A MECHANISM FOR CHONDRULE FORMATION [PDF]
ABSTRACT We use radiation hydrodynamics with direct particle integration to explore the feasibility of chondrule formation in planetary embryo bow shocks. The calculations presented here are used to explore the consequences of a Mars-size planetary embryo traveling on a moderately excited orbit through the dusty, early environment of the
Christopher Mann
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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.
Christopher T. Russell, M M Hoppe
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Planetary bow shocks: Gasdynamic analytic approach [PDF]
A new analytical model of the bow shock surface is suggested for reasonably accurate and fast prediction of this boundary's position near obstacles of different shape. For axially symmetric obstacles the model was verified by comparison with experiments and results of gasdynamic code application for a wide range of upstream polytropic indexes, 1.15 <
Tamás G. Gombosi +2 more
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CHONDRULE FORMATION IN BOW SHOCKS AROUND ECCENTRIC PLANETARY EMBRYOS [PDF]
Accepted for publication in The Astrophysical ...
Steven Desch
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Geophysical Monograph Series, 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.
Christopher T. Russell
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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.
Christopher T. Russell
exaly +2 more sources

