Observational Evidences for Heating of the Solar Corona by Nanoflares in the Network Derived from the Transition Region Spectral Lines

Details Observational Evidences for Heating of the Solar Corona by Nanoflares in the Network Derived from the Transition Region Spectral Lines Observational Evidences for Heating of the Solar Corona by Nanoflares in the Network Derived from the Transition Region Spectral Lines

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004esasp.575..529r&link_type=gif

Proceedings of the SOHO 15 Workshop - Coronal Heating. 6-9 September 2004, St. Andrews, Scotland, UK (ESA SP-575). Editors: R.W.

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