Multi-spacecraft observations of polar coronal plumes

Details Multi-spacecraft observations of polar coronal plumes Multi-spacecraft observations of polar coronal plumes

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008a%26a...481l..61c&link_type=abstract

Astronomy and Astrophysics, Volume 481, Issue 1, 2008, pp.L61-L64

Astronomy and Astrophysics

Astrophysics

15

Sun: Corona, Sun: Solar Wind, Techniques: Spectroscopic

Scientific paper

Aims:Coronal plumes, along with their structure and rôle in the acceleration of the fast solar wind, are of considerable importance in understanding the physics of the solar atmosphere, in particular, when contrasted with the adjacent plasma, the so-called interplume regions. Methods: Observations of coronal plumes in a coronal hole were obtained with the help of spectrographs and imagers on Hinode, SOHO, STEREO, TRACE, and with ground-based instrumentation. The measurements were performed by a large international team in April 2007. Results: First results of this study from Hinode, SOHO, and STEREO are presented here, at the level of observational facts, leaving the task of detailed analysis to the future.

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