Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini

Bibliographische Detailangaben
Veröffentlicht in:	Geophysical research letters. - 1984. - 49(2022), 16 vom: 28. Aug., Seite e2022GL099237
1. Verfasser:	Wu, S Y (VerfasserIn)
Weitere Verfasser:	Ye, S Y, Fischer, G, Taubenschuss, U, Jackman, C M, O'Dwyer, E, Kurth, W S, Yao, S, Yao, Z H, Menietti, J D, Xu, Y, Long, M Y, Cecconi, B
Format:	Online-Aufsatz
Sprache:	English
Veröffentlicht:	2022
Zugriff auf das übergeordnete Werk:	Geophysical research letters
Schlagworte:	Journal Article

Beschreibung
Zusammenfassung:	© 2022. The Authors. A new radio component namely Saturn Anomalous Myriametric Radiation (SAM) is reported. A total of 193 SAM events have been identified by using all the Cassini Saturn orbital data. SAM emissions are L-O mode radio emission and occasionally accompanied by a first harmonic in R-X mode. SAM's intensities decrease with increasing distance from Saturn, suggesting a source near Saturn. SAM has a typical central frequency near 13 kHz, a bandwidth greater than 8 kHz and usually drifts in frequency over time. SAM's duration can extend to near 11 hr and even longer. These features distinguish SAM from the regular narrowband emissions observed in the nearby frequency range, hence the name anomalous. The high occurrence rate of SAM after low frequency extensions of Saturn Kilometric Radiation and the SAM cases observed during compressions of Saturn's magnetosphere suggest a special connection to solar wind dynamics and magnetospheric conditions at Saturn
Beschreibung:	Date Revised 05.09.2024 published: Print-Electronic Citation Status PubMed-not-MEDLINE
ISSN:	0094-8276
DOI:	10.1029/2022GL099237