The Variation of Solar Chromospheric H-alpha Plage 2002-2009

Details The Variation of Solar Chromospheric H-alpha Plage 2002-2009 The Variation of Solar Chromospheric H-alpha Plage 2002-2009

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsh11a1492b&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SH11A-1492

Astronomy and Astrophysics

Astrophysics

[7500] Solar Physics, Astrophysics, And Astronomy, [7507] Solar Physics, Astrophysics, And Astronomy / Chromosphere, [7524] Solar Physics, Astrophysics, And Astronomy / Magnetic Fields, [7594] Solar Physics, Astrophysics, And Astronomy / Instruments And Techniques

Scientific paper

Solar Chromospheric Plages in H-alpha represent a thermal dissipative response to the underlying magnetic field. In this study we track the daily variation of active region and quiet-sun plages areas and the underlying magnetic fields, during 2002-2009. In this poster, we present the methodology used to understand this variation as a function of the magnetic field. We present variations of plage intensities and ares over the solar cycle and examine their cyclical and non-cyclical patterns.

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