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

S. Y. Wu (1) , S. Y. Ye , G. Fischer , U. Taubenschuss , C. M. Jackman , E. O'Dwyer , W. S. Kurth , S. Yao , Z. H. Yao , J. D. Menietti , Y. Xu , M. Y. Long , B. Cecconi (1)

1 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics

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.

Domaines: Planète et Univers [physics]

S. Y. Wu, S. Y. Ye, G. Fischer, U. Taubenschuss, C. M. Jackman, et al.. Saturn Anomalous Myriametric Radiation, a New Type of Saturn Radio Emission Revealed by Cassini. Geophysical Research Letters, 2022, 49, ⟨10.1029/2022GL099237⟩. ⟨insu-03874902⟩