The solar wind interaction with Comets Machholz (C/2004 Q2) and NEAT (C/2001 Q4) as revealed by amateur images.

Details The solar wind interaction with Comets Machholz (C/2004 Q2) and NEAT (C/2001 Q4) as revealed by amateur images. The solar wind interaction with Comets Machholz (C/2004 Q2) and NEAT (C/2001 Q4) as revealed by amateur images.

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..982r&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.982

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Scientific paper

Using images acquired from a global community of amateur astronomers, we investigate the interaction between solar wind flow and the plasma tail of comets Machholz and NEAT. We attribute disconnection events, kinks and other cometary tail features to the following heliospheric phenomena: coronal mass ejections [3], movement between fast and slow solar wind regimes, and heliospheric current sheet crossings.

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