Quantitative results on heating events in the quiet corona

Details Quantitative results on heating events in the quiet corona Quantitative results on heating events in the quiet corona

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aipc..471...67b&link_type=abstract

The solar wind nine conference. AIP Conference Proceedings, Volume 471, pp. 67-69 (1999).

Physics

2

Scientific paper

The emission measure of the quiet corona, defined by the plasma hotter than one million degrees, is fluctuating in nearly every 1900 km×1900 km pixel observed by EIT on SoHO. In the average, the larger the emission measure in a pixel, the more it fluctuates. Increases in emission measure constitute a major energy input into the corona, suggesting that the lower corona is not just heated, but continuously replenished by chromospheric material heated to coronal temperatures.

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