DocumentCode
1930060
Title
Propagation “over the horizon” of Saturn´s radio lightning studied by three-dimensional ray tracing
Author
Gautier, A.-L. ; Cecconi, B. ; Zarka, P. ; Fischer, G.
Author_Institution
LESIA, Obs. de Paris, Meudon, France
fYear
2011
fDate
13-20 Aug. 2011
Firstpage
1
Lastpage
1
Abstract
Saturn Electrostatic Discharges (SED) are radio signature of lightning flashes originating from Saturns cloud systems. Observations of SED show that the radio horizon is larger than the visible one, especially when Cassini is in Saturns morning side (“over the horizon” effect). Moreover, both apparition and disappearance of bursts appear to be frequency-dependent. We built a 3D ray tracing code, which computes the path propagation of radio waves through a realistic model of Saturns ionosphere, where electron density varies with local time, and were able to reproduce the typical dynamic spectrum of observed “over the horizon” events.
Keywords
Saturn; planetary atmospheres; radiowave propagation; 3D ray tracing code; Cassini; Saturn cloud system; Saturn electrostatic discharges; Saturn ionosphere; Saturn radio lightning; burst apparition; electron density; frequency-dependent burst disappearance; lightning flash; radio horizon; radio signature; radio wave path propagation; Computational modeling; Electrostatic discharge; Ionosphere; Lightning; Ray tracing; Saturn; Three dimensional displays;
fLanguage
English
Publisher
ieee
Conference_Titel
General Assembly and Scientific Symposium, 2011 XXXth URSI
Conference_Location
Istanbul
Print_ISBN
978-1-4244-5117-3
Type
conf
DOI
10.1109/URSIGASS.2011.6051302
Filename
6051302
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