Mars' L-Band Radio Emission

Details Mars' L-Band Radio Emission Mars' L-Band Radio Emission

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007dps....39.1704b&link_type=abstract

American Astronomical Society, DPS meeting #39, #17.04; Bulletin of the American Astronomical Society, Vol. 39, p.441

Astronomy and Astrophysics

Astronomy

Scientific paper

Several authors have suggested that martian dust storms should produce radio emission from electrostatic discharges between dust grains (e.g. Farrell et al. 1999, JGR 104, 3795-3801; Renno et al. 2003, GRL 30, 2140). We report results from ongoing VLA observations of Mars at L-band (20 cm). With the VLA in A-configuration (35 km maximum baseline), we resolve Mars and can compare the pattern of radio emission to the expected thermal flux and the positions of known dust storms.

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