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In situ and remote observations of the ultraviolet footprint of the moon Callisto by the Juno spacecraft. [PDF]
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Science, 1991
Degenerate bodies composed primarily of dense hydrogen and helium plasmas range from giant planets to the so far hypothetical brown dwarfs. More massive objects begin their lives as nondegenerate stars and may end as white dwarfs, composed primarily of carbon and oxygen, or as neutron stars, with solid crusts of iron or heavier elements and cores of ...
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Degenerate bodies composed primarily of dense hydrogen and helium plasmas range from giant planets to the so far hypothetical brown dwarfs. More massive objects begin their lives as nondegenerate stars and may end as white dwarfs, composed primarily of carbon and oxygen, or as neutron stars, with solid crusts of iron or heavier elements and cores of ...
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Astrophysical plasma laboratories
Physics World, 1994Almost all of the material in the Universe is in the form of ionized gas or plasma. The interstellar medium is a low-temperature, low-density plasma whilst the interiors of stars are made of extremely hot and dense plasmas. A variety of different plasma conditions can exist within the same star; the centre of the Sun, for example, is at a temperature ...
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Numerical methods for astrophysical plasmas
Computer Physics Communications, 1986This review covers some numerical methods used for astrophysical plasmas and centers mainly on methods developed for astrophysical problems. After general remarks on DELTA multiplied by (times) B in astrophysical MHD calculations, a first-order, one-sided finite-difference formulation is derived for spherical and cylindrical geometries, respectively ...
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Plasma physics and astrophysics
1971Wir veranschaulichen die Bedeutung des astrophysischen Plasmas mit einer Besprechung einiger astrophysischen Probleme.
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Plasma-maser effects in plasma astrophysics
Space Science Reviews, 1986The role of a new mode coupling effect (plasma-maser) in space plasma physics is reviewed. The new maser effect, the idea that the resonant electrons with the low-frequency mode can amplify the high-frequency mode, does not require population inversion of electrons. The generation mechanisms of ULF modulated ELF emissions, auroral kilometric radiation,
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Collisionless Plasmas in Astrophysics
2013International ...
Belmont, Gérard +4 more
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2019
Dusty plasmas have first been studied in astrophysical situations. Here, we now like to highlight a few aspects of dust in the ionosphere or in our solar system. We start with noctilucent clouds and polar mesospheric summer echoes. Then, we look into dust streams near Jupiter and Saturn and how our knowledge of dusty plasmas can be used as a ...
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Dusty plasmas have first been studied in astrophysical situations. Here, we now like to highlight a few aspects of dust in the ionosphere or in our solar system. We start with noctilucent clouds and polar mesospheric summer echoes. Then, we look into dust streams near Jupiter and Saturn and how our knowledge of dusty plasmas can be used as a ...
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Introduction to plasma astrophysics
Plasma Physics and Controlled Fusion, 1999We discuss the importance of plasma physics in various areas of cosmology and astrophysics: (1) the primordial plasma spectrum, (2) the cosmic microwave background, (3) the large-scale structure of the universe, (4) reionization and the metalicity of the primordial universe, (5) the first objects, (6) the primordial magnetic field, (7) clusters of ...
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