Results 161 to 170 of about 260,255 (207)

Jovian Decameter radio bursts from the vicinity of Io's flux tube

EGS　Symposium　PS-5.01:　"Planetary　Magnetospheres　and ...
Ryabov, B. P., 0000-0002-9243-7597, Farges, T., 10325904, Abada-Simon, M., Prange, R., 5915, 5916, 5917, 5918, 5919, Zarka, P., V.B. , Ryabov, 64   +13 more
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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 of
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Recent advances in planetary ionospheres

Space Science Reviews, 1996
Recent results on the ionospheres of various planets are reviewed. In view of the large amount of data now available on Venus, much of the work relates to this planet. The outer planets received somewhat less attention partly due to lack of measurements in the post-Voyager era.
J Kar
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Current Systems in Planetary Magnetospheres and Ionospheres

Space Science Reviews, 2010
The interaction of planets with the solar wind produces a diversity of current systems, yet these can be classified into only a few different types, which include ionospheric currents, currents carried by magnetospheric boundaries like the magnetopause or ionopause, magnetotail currents, and currents flowing inside the magnetospheres, like ring ...
W Baumjohann, M Blanc, K -H Glasmeier
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Electric currents in E-like planetary ionospheres

Planetary and Space Science, 1990
In this paper an MHD approach is used to consider the conduction of electric current in a lightly ionized gas, taking into account the gradients of pressure in the ion and electron gases, in addition to the electric field. The coefficients of electrical conductivity are found for each driver of current.
K D Cole
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Thermal Structure of Planetary Ionospheres

1973
Electrons released in the photoionization process due to the absorption of solar XUV radiation in planetary atmospheres may have initially kinetic energies of one to 100 eV. The energy E of photoelectrons resulting from photons of energy h v interacting with an atmospheric constituent whose ionization potential is IP is given by $$E = hv - IP ...
S. Bauer
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Radio Occultation Experiment for Probing Planetary Ionospheres

2019 URSI Asia-Pacific Radio Science Conference (AP-RASC), 2019
Radio occultation (RO) is an important measurement technique for studying planetary atmospheres. It is based on the measurement of the frequency shift of the received radio signal from the spacecraft, caused by the bending of radio waves in the atmosphere.
Varun Sheel
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Planetary Ionospheres and Ionospheric Instabilities

International Astronomy and Astrophysics Research Journal
S. Gogoi
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The two-frequency bistatic radar-occultation method for the study of planetary ionospheres

Journal of Geophysical Research, 1965
G Fjeldbo, V R Eshleman
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Physics of Planetary Ionospheres

Physics of the Earth and Planetary Interiors, 1974
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