Observations of Jovian decimetric radiation at a frequency of 327MHz
Author:
Publisher
Elsevier BV
Subject
Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics
Reference14 articles.
1. Multi-Station System for Solar Wind Observations Using the Interplanetary Scintillation Method.
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4. Physics of the Jovian Magnetosphere;Carr,1983
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1. Short-term Variation in the Dawn–Dusk Asymmetry of the Jovian Radiation Belt Obtained from GMRT and Hisaki EXCEED Observations;The Astrophysical Journal;2019-02-19
2. Relation between the short‐term variation of the Jovian radiation belt and thermosphere derived from radio and infrared observations;Journal of Geophysical Research: Space Physics;2015-08
3. Effect of solar UV/EUV heating on the intensity and spatial distribution of Jupiter's synchrotron radiation;Journal of Geophysical Research: Space Physics;2013-10
4. Short-term changes in Jupiter's synchrotron radiation at 325 MHz: Enhanced radial diffusion in Jupiter's radiation belt driven by solar UV/EUV heating;Journal of Geophysical Research: Space Physics;2011-09
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