Different types of temporal variations in the decameter emission of Jupiter
2010
In 2009 year with the UTR-2 radio telescope (Kharkov, Ukraine) several observational campaigns have been performed with the aim to investigate the fine temporal structures in the Jovian decameter radio emission (DAM). As recording equipment the broad band digital receiver with 8192 frequency channels (33 MHz frequency band in common) and 0.25 ms time resolution was put into operation. Experiments have been arranged in accordance to the known diagram occurrence of Io-dependent sources. Periods of the different sources have been chosen, which enable to obtain possible new results for the sporadic S-emission of Io-A, Io-B, Io-C and Io-D sources and their combinations. Continuous measurements for IoB source lasted approximately 3.5 hours. Long duration of observations provided the possibility to watch the continuous time evolution of the Jovian radiation with complete coverage of the planet’s culmination and consideration of the different stages of radiation variation in detail.
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