Comparative morphology of EIT/SOHO images and He II excitation

Details Comparative morphology of EIT/SOHO images and He II excitation Comparative morphology of EIT/SOHO images and He II excitation

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999soph..187...23v&link_type=abstract

Solar Physics, v. 187, Issue 1, p. 23-32 (1999).

Physics

2

Scientific paper

Morphological differences between coronal images on the one hand, and a Hei image on the other, are used to demonstrate the independence of Heii excitation from coronal radiation. The distribution of magnetic flux is found to be more important for Heii excitation. Collisional excitation by non-thermal electrons produced in nano-flare events is proposed as the mechanism for Heii excitation.

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