Results 181 to 190 of about 462,332 (215)

Simulation Models for Exploring Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Shay M   +24 more
europepmc   +1 more source

The Interplay Between Collisionless Magnetic Reconnection and Turbulence. [PDF]

open access: yesSpace Sci Rev
Stawarz JE   +15 more
europepmc   +1 more source

Ohm's Law, the Reconnection Rate, and Energy Conversion in Collisionless Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Liu YH   +14 more
europepmc   +1 more source

SMILE Modeling Working Group: Modeling and Analysis of X-ray and Ultraviolet Images of Solar Wind - Earth Interactions. [PDF]

open access: yesSpace Sci Rev
Connor HK   +15 more
europepmc   +1 more source

Hyperfine-resolved rovibrational and rotational spectroscopy of OH<sup>+</sup> (<i>X</i><sup>3</sup>Σ<sup>-</sup>).

open access: yesPhys Chem Chem Phys
Silva WGDP   +8 more
europepmc   +1 more source

PLANETARY EMBRYO BOW SHOCKS AS A MECHANISM FOR CHONDRULE FORMATION [PDF]

open access: yesAstrophysical Journal, 2016
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
exaly   +3 more sources

Overshoots in planetary bow shocks

Nature, 1982
The 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
exaly   +2 more sources

Planetary bow shocks: Gasdynamic analytic approach [PDF]

open access: yesJournal of Geophysical Research: Space Physics, 2003
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
exaly   +3 more sources

CHONDRULE FORMATION IN BOW SHOCKS AROUND ECCENTRIC PLANETARY EMBRYOS [PDF]

open access: yesAstrophysical Journal, 2012
Accepted for publication in The Astrophysical ...
Steven Desch
exaly   +3 more sources

Planetary Bow Shocks

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
exaly   +2 more sources

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