N‐bursty emission from Uranus: A cyclotron maser source?

Ray tracing studies of RX‐mode emission from the north polar regions of Uranus indicate that the n‐bursty radio emission may have a source along field lines with footprints near the northern magnetic pole (perhaps in the cusp), but not necessarily associated with regions of strong UV emission. This is in contrast with similar studies for the Uranus nightside smooth radio emission, which are believed to be due to the cyclotron maser instability. Source regions can be found for both hollow and filled emission cones and for frequencies well above the local gyrofrequency implying that mechanisms other than the cyclotron maser mechanism may be operating.