Intensity Fluctuations in the Solar Chromosphere

Details Intensity Fluctuations in the Solar Chromosphere Intensity Fluctuations in the Solar Chromosphere

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sp41c05k&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SP41C-05

Physics

7507 Chromosphere, 7549 Ultraviolet Emissions

Scientific paper

We examine two very different empirical models of the solar chromosphere. The first model implies steady heating, is hot at the top of the chromosphere and has temperature fluctuations of relatively low amplitude; the second model is heated intermittently, is cold most of the time and undergoes large temperature variations. Estimates of intensity fluctuations of chromospheric radiation are very different for the two models. We compare the model predictions with observations made by Skylab and by SUMER.

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