LC001	   Tracking the Dynamic Spectrum of Jupiter 
Clarke, T. (NRL),

We propose to use the high temporal and spectral resolution of the first LWA station to study the properties of
the decametric emission from Jupiter. The observations will be tied to predictions of emission storms (i.e. when
the Io torus is favorably aligned for maximum emission). We will study the fine temporal structure of the
S-bursts and also track details of the rapid time switching of the emission from right hand circular to left hand
circular. These observations will also set the ground work for future initiatives such as VLBI between LWA and
LOFAR for study of the locations of emitting sources. We separate our project into subcomponents which are
tied to the three phases of development of the first LWA station. Observations during the first two phases will
be used to develop software and analysis techniques which will be ready once the full station and BFU/DRX
capabilities are available.