LOFAR and Low-frequency Radio Emissions from Jupiter

Details LOFAR and Low-frequency Radio Emissions from Jupiter LOFAR and Low-frequency Radio Emissions from Jupiter

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....3135d&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #3135

Physics

Scientific paper

Jupiter emits synchrotron radiation at frequencies between ˜ 70 MHz up to over 20 GHz, and perhaps even outside this frequency range. At frequencies shortwards of 40 MHz the planet's radio emission is dominated by decametric bursts of emission, many orders of magnitude stronger than the synchrotron radiation. The low-frequency emission has been attributed to coherent cyclotron emission. I will discuss Jupiter's synchrotron radiation spectrum and spatial brightness distribution, whereby I will focus the discussion on future contributions with the LOFAR system. If time permits, I will also speculate on LOFAR contributions in the decametric frequency range.

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