EUV Observations of Active Region Dynamics

Details EUV Observations of Active Region Dynamics EUV Observations of Active Region Dynamics

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp33a..03d&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP33A-03

Physics

7507 Chromosphere, 7509 Corona

Scientific paper

Data collected during SoHO JOP 146, in collaboration with TRACE, is used to investigate the physical characteristics of coronal active region loops as a function of time and position along and across loop structures. These data include TRACE images in all three EUV passbands, and simultaneous CDS spectroscopic observations. Preliminary measurements of the loop temperature both along the loop half-length and loop cross-section are presented as a function of time. We will show the temperature and density profiles of several structures as a function of position, show changes in temperature and density with time and characterize the coronal background emission. Questions raised by these results will be greatly advanced with the high resolution spectra available from the EIS on Solar-B.

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