Inner Source Diffuse Helium Observations

Details Inner Source Diffuse Helium Observations Inner Source Diffuse Helium Observations

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008espm...12.2.88m&link_type=abstract

"12th European Solar Physics Meeting, Freiburg, Germany, held September, 8-12, 2008. Online at http://espm.kis.uni-freiburg.de/,

Physics

Scientific paper

Sensitive SOLARC imagining spectropolarimetric observations from Haleakala reveal a diffuse coronal surface brightness in the He I 1083nm line. A series of observations obtained during the last two years suggests that this signal originates from an "inner source" of neutral helium atoms in the solar corona. We argue here that this cold coronal component is likely to originate from the near-sun dust, and that there is a deficit of coronal dust close to the Sun.

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