Results 181 to 190 of about 471 (212)

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

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

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

Outstanding Questions and Future Research on Magnetic Reconnection. [PDF]

open access: yesSpace Sci Rev
Nakamura R   +24 more
europepmc   +1 more source

Overshoots in planetary bow shocks

open access: yesNature, 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.
C T Russell, M M Hoppe, Russell C T
exaly   +3 more sources

Planetary Bow Shocks

open access: yes, 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   +2 more
exaly   +3 more sources

Heliospheric shocks (excluding planetary bow shocks)

open access: yesReviews of Geophysics, 1987
Even 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 ...
J D Mihalov
exaly   +3 more sources

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