Interplanetary dust model: from micron-sized dust to meteors

Details Interplanetary dust model: from micron-sized dust to meteors Interplanetary dust model: from micron-sized dust to meteors

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.495..609d&link_type=abstract

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

Physics

3

Interplanetary Dust, Models, Meteors

Scientific paper

New populations of interplanetary dust are proposed for the ESA meteoroid model. Formulation of the new model extends earlier meteoroid models and is now tied to orbital evolution of the interplanetary dust. To validate the new model, infrared emission observations with COBE DIRBE instrument, impact counts with the dust detectors aboard Galileo and Ulysses spacecraft, and the radar meteors monitored with AMOR are used. Incorporation of meteor data in the model is discussed.

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