Physics of the chromosphere and the lower coronal boundary conditions

Details Physics of the chromosphere and the lower coronal boundary conditions Physics of the chromosphere and the lower coronal boundary conditions

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008agufmsh51c..03j&link_type=abstract

American Geophysical Union, Fall Meeting 2008, abstract #SH51C-03

Physics

7507 Chromosphere

Scientific paper

I will review observations and theoretical work concerning the role of the chromosphere as the lower boundary for the corona. I will highlight the need for measurements of the chromospheric magnetic field as the plasma regimes change from beta > 1 to < 1, using a striking observational example. I will review some of the important physical processes occurring within the partially ionized chromosphere which can greatly alter the conditions at the coronal base from those expected based only upon photospheric measurements. I will re-iterate the obvious conclusion, but one often ignored, that one must understand specific chromospheric processes if one is to have hope of addressing the nature of the supply of mass, momentum and energy into the corona.

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