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Physics-tailored machine learning reveals unexpected physics in dusty plasmas. [PDF]
Yu W +3 more
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Uncovering the integral spectral characteristics of the planetary nebula IC 4642. [PDF]
Mohery M +4 more
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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
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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
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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
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Electromagnetic Instability of a Homogeneous Plasma in Interstellar Space
Technical Physics, 2005A study is made of an electromagnetic instability of a homogeneous plasma with an arbitrary velocity distribution in interstellar space on long time scales typical of gas-dust clouds without a significant magnetic field. It is shown that such instabilities develop on time scales of a few months or years and that it is only a narrow class of nearly ...
A S Baranov, Baranov A S
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Il Nuovo Cimento, 1959
Observational data and studies on material in the galactic system are reviewed. Mechanisms of radio emission are discussed relative to thermal radiation, synchrotron radiation, and the existence of non-thermal radiation. Observational data on the shell and the inner part of the Crab nebula are considered along with properties such as synchrotron ...
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Observational data and studies on material in the galactic system are reviewed. Mechanisms of radio emission are discussed relative to thermal radiation, synchrotron radiation, and the existence of non-thermal radiation. Observational data on the shell and the inner part of the Crab nebula are considered along with properties such as synchrotron ...
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Infrared Emission From Interstellar Plasma
Astrophysics and Space Science, 1988Small dust grains in hot interstellar plasmas are heated by electrons and emit near-infrared radiation. Its flux is estimated to be larger than that from small dust grains heated by stellar radiation and could explain the high infrared flux observed at wavelengths of about 5 µm.
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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. I. Shishov, T. V. Smirnova
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“Cold fusion”: Formation of molecules in interstellar plasmas
Plasma Physics and Controlled Fusion, 1992A brief overview is presented of the ionic reactions that occur in interstellar gas clouds which lead to the production of the complex molecules determined in those regions. It is shown that the interstellar clouds are weakly ionized plasmas and that the chemistry is largely plasma chemistry involving sequences of ion-molecule reactions producing ...
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