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Viscous Forces in Velocity Boundary Layers around Planetary Ionospheres
The Astrophysical Journal, 1999A discussion is presented to examine the role of viscous forces in the transport of solar wind momentum to the ionospheric plasma of weakly magnetized planets (Venus and Mars). Observational data are used to make a comparison of the Reynolds and Maxwell stresses that are operative in the interaction of the solar wind with local plasma (planetary ...
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Planetary Ionospheric Disturbance Inspired Optimization Algorithm
The planetary ionosphere is a region of the planetary atmosphere ionized by solar radiation and high-energy particles, and its electron density exhibits dynamic fluctuations. Ionospheric disturbances are characterized by rapid local response, wave propagation, random external perturbations, and recovery mechanisms. Drawing on the physical mechanisms ofopenaire +1 more source
Transplanet: A web service dedicated to modeling of planetary ionospheres
Planetary and Space Science, 2019Olivier Witasse
exaly
Physics of Planetary Ionospheres
Physics Today, 1975S. J. Bauer, A. Dalgarno
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