Probing the structure of the interplanetary dust cloud using the AMOR meteoroid orbit radar

Details Probing the structure of the interplanetary dust cloud using the AMOR meteoroid orbit radar Probing the structure of the interplanetary dust cloud using the AMOR meteoroid orbit radar

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495..569g&link_type=abstract

In: Proceedings of the Meteoroids 2001 Conference, 6 - 10 August 2001, Kiruna, Sweden. Ed.: Barbara Warmbein. ESA SP-495, Noordw

Physics

1

Radar Meteors, Zodiacal Light, Interplanetary Dust

Scientific paper

The Advanced Meteor Orbit Radar (AMOR) routinely determines the heliocentric orbits of Earth-impacting dust particles. Radar meteoroid orbital distributions have a number of inherent biases. This paper details a work in progress whose aim is to determine and correct these biases on the data set of ~5×105 meteoroid orbits provided by AMOR between 1995 - 1999. Interim orbital distributions corrected for some of the identified biases are presented. These illustrate the importance of careful correction of the data set.

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