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
Link To Document :
بازگشت