Detection of interstellar dust with STEREO/WAVES at 1AU

Details Detection of interstellar dust with STEREO/WAVES at 1AU Detection of interstellar dust with STEREO/WAVES at 1AU

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..925b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.925

Physics

Scientific paper

Here we will concentrate on the discussion of those impacts that were recorded with all three antennas and show characteristics similar as previous dust measurements with wave instruments. We interprate them as being produced by dust grains originating from the local interstellar cloud and by β-meteorites. From the study of these fluxes during 4 years of STEREO mission and their modelisation, we determined the direction of arrival of interstellar dust and its temporal variation at 1AU between 2007 and 2010. We also give an estimate of the mass distribution of interstellar dust and β-meteorites in the detected range.

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