Articles | Volume 18
https://doi.org/10.5194/ars-18-83-2020
https://doi.org/10.5194/ars-18-83-2020
10 Dec 2020
 | 10 Dec 2020

Observations of Solar Type III radio bursts by Cassini/RPWS experiment

Mohammed Y. Boudjada, Ahmed Abou el-Fadl, Patrick H. M. Galopeau, Eimad Al-Haddad, and Helmut Lammer

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Cited articles

Aubier, A., Boudjada, M. Y., Moreau, P., Galopeau, P. H. M., Lecacheux, A., and Rucker, H. O.: Statistical studies of jovian decameter emissions observed during the same period by Nançay Decameter Array (France) and WAVES experiment aboardWind spacecraft, Astron. Astrophys., 354, 1101–1109, 2000. a
Bonnin, X., Hoang, S., and Maksimovic, M.: The directivity of solar type III bursts at hectometer and kilometer wavelengths: Wind-Ulysses observations, Astron. Astrophys., 489, 419–427, 2008. a
Boudjada, M. Y., Lecacheux, A., Sawas, S., Stangl, A., and Voller, W. G.: Spectral study of solar Type III decametric bursts, in: Planetary Radio Emissions VI, edited by: Rucker, H. O., Kurth, W. S., and Mann, G., Austrian Academy of Sciences Press, Vienna, Austria, 401–408, 2006. a
Boudjada, M. Y., Galopeau, P. H. M., Maksimovic, M., and Rucker, H. O.: Visibility of Type III burst source location as inferred from stereoscopic space observations, Adv. Radio Sci., 12, 167–170, https://doi.org/10.5194/ars-12-167-2014, 2014. a, b
Dulk, G. A., Leblanc, Y., Bougeret, J.-L., and Hoang, S.: Type III bursts observed simultaneously by Wind and Ulysses, Geophys. Res. Lett., 23, 1203–1205, 1996. a
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Short summary
We investigate the solar Type III radio bursts recorded at about 10 AU by Cassini spacecraft. More than 300 bursts have been recorded by the RPWS experiment in the time interval from 01 Jan. 2008 to 31 Dec. 2014. We show that the solar Type III occurrence is mainly depending on the solar activity and also exhibits maxima and minima of detection. The source location of such solar bursts is the interplanetary medium because the dominant emission appears at frequency lower than 2.3 MHz.