Physics
Scientific paper
May 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh13c..03m&link_type=abstract
American Geophysical Union, Spring Meeting 2005, abstract #SH13C-03
Physics
7507 Chromosphere, 7524 Magnetic Fields, 7529 Photosphere
Scientific paper
In this contribution we present an analysis of time sequences of MDI intensity and Doppler velocity together with simultaneous filtergrams taken by TRACE at 1700A in an active region. The high frequency halos found in MDI velocity and the deficiency of high frequency power sampled at the height of the TRACE UV filter around the active region can be explained by an interaction of the acoustic wave field with the magnetic field of the active region. From a magnetic field extrapolation we calculate the plasma β for the complete TRACE FOV up to the base of the corona. The contours giving the location of β approximately 1 where h=500 km agree very well with the decrease in 1700A high frequency power.
Hofmann Andrea
Muglach Karin
Staude Jakob
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