CMI growth rates for Saturnian kilometric radiation

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CMI growth rates for Saturnian kilometric radiation

[1] We calculate growth rates for extraordinary mode Saturnian kilometric radiation generated by the electron cyclotron maser instability using a ring‐type (DGH) electron phase distribution model fitted to measured electron energy dist r ibut ions in Saturn’s auroral acceleration region. The observed distributions are unstable in spatially isolated regions of transverse linear size of order 10 ...

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ژورنال

عنوان ژورنال: Geophysical Research Letters

سال: 2010

ISSN: 0094-8276

DOI: 10.1029/2010gl044940