On the Origin of Metal Ions in Cometary Comae / Refractory Elements / Impacts / Dust Particles / Interplanetary Dust Clouds

Details On the Origin of Metal Ions in Cometary Comae / Refractory Elements / Impacts / Dust Particles / Interplanetary Dust Clouds On the Origin of Metal Ions in Cometary Comae / Refractory Elements / Impacts / Dust Particles / Interplanetary Dust Clouds

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1531...27i&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1531/SEPT, P.27 , 1988

Astronomy and Astrophysics

Astronomy

Scientific paper

Ions of refractory elements (Fe+, Si+ etc.)
detected in cometary comae by spacecraft may be generated due to
high-velocity impacts between cometary and zodiacal dust particles. Such
metallic ions in cometary comae may serve as indicators of
interplanetary dust clouds.

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