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Solar corona-induced fluctuations on spacecraft signal amplitude observed during solar superior conjunctions of the Cassini spacecraft
DOI: 10.1029/2005RS003425 Bibcode: 2007RaSc...42.3002M

Morabito, David D.

During the superior solar conjunctions of interplanetary spacecraft, the emitted radio signals undergo increased amplitude scintillation, phase scintillation, and spectral broadening due to the intervening charged particles of the solar corona. The magnitude of these parameters generally increases as the angle between the spacecraft and the center…

2007 Radio Science
Cassini 11
A finite difference time domain model for the Titan ionosphere Schumann resonances
DOI: 10.1029/2006RS003490 Bibcode: 2007RaSc...42.2S04N

Navarro, E. A.; Soriano, A.; Morente, J. A. +1 more

This paper presents a numerical approach to model the electrical properties of Titan's atmosphere. The finite difference time domain technique is applied to model the atmosphere of Saturn's satellite in order to determine Schumann resonant frequencies and electromagnetic field distributions at the extremely low frequency range. Spherical coordinat…

2007 Radio Science
Huygens 7