Results 201 to 210 of about 3,998,903 (250)
Efficient acceleration of energetic electrons upstream of Earth's bow shock. [PDF]
Liu YY +9 more
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Chang'E-6 reveals solar wind-dependent H<sup>-</sup> ions on the Moon. [PDF]
Zhong T +15 more
europepmc +1 more source
The abundances of carbon and nitrogen in the atmospheres of classical Be stars. [PDF]
Peters GJ +4 more
europepmc +1 more source
A hot white dwarf merger remnant revealed by an ultraviolet detection of carbon. [PDF]
Sahu S +9 more
europepmc +1 more source
Ionic Reactant Orientation Inhibits Ion-Neutral Reactions at Low Temperatures. [PDF]
Peng Y +9 more
europepmc +1 more source
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In Situ Observations of Interstellar Plasma with Voyager 1
Science, 2013Finally Out Last summer, it was not clear if the Voyager 1 spacecraft had finally crossed the heliopause—the boundary between the heliosphere and interstellar space. Gurnett et al. (p.
William Kurth
exaly +4 more sources
Radio Propagation Through the Turbulent Interstellar Plasma
Annual Review of Astronomy and Astrophysics, 1990Article de synthese traitant de la diffusion interstellaire et des plasmas turbulents dans le milieu ...
B J Rickett
exaly +3 more sources
Interstellar scintillation and the interstellar turbulent plasma
Astronomical and Astrophysical Transactions, 2002Data on interstellar diffractive and refractive scintillation of pulsars are analyzed. The comparison between the theory and the observational data shows that two types of spectra for electron density fluctuations are realized in the interstellar medium: simple power law and piecewise with a break. The distribution of turbulent plasma in the Galaxy has
V I Shishov
exaly +2 more sources
The outer turbulence scale in the interstellar plasma
Astronomy Reports, 2002The structure function for phase fluctuations on spatial scales from 106 to 1017 m is constructed using data on diffractive and refractive scintillation of pulsars, scattering angles, variations in pulse arrival times, and differences in dispersion measures observed for close pairs of pulsars in globular clusters.
V. Shishov, T. Smirnova
semanticscholar +2 more sources

