Fundamental Jupiter millisecond radio burst characteristics

Details Fundamental Jupiter millisecond radio burst characteristics Fundamental Jupiter millisecond radio burst characteristics

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....3091r&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #3091

Physics

Scientific paper

The development of high spectral resolution instrumentation, i.e. the digital spectropolarimeter (DSP) and waveform receiver (WFR) and their installation at large decameter band radio telescopes (UTR-2 at Kharkov, Ukraine and Nancay, France) opened new possibilities in the investigation of fast Jupiter radio emissions in the decametric range. The internal structure of a drifting millisecond (S-)burst, being analyzed by means of the wavelet transform, reveals microsecond modulations which are visible as a train of signal bunches in the scalogram. Spectral characteristics of these superfine burst structures could be obtained from recent observations, and their implications are estimated with regard to radio source size and configuration. After decades of continuous Jupiter S-burst observations and investigations the physical fundamentals of this fast radio phenomenon seems to be unveiled.

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