Temperature Structure of Active Region Coronal Loops as seen by Hinode

Details Temperature Structure of Active Region Coronal Loops as seen by Hinode Temperature Structure of Active Region Coronal Loops as seen by Hinode

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.9437s&link_type=abstract

American Astronomical Society Meeting 210, #94.37; Bulletin of the American Astronomical Society, Vol. 39, p.327

Astronomy and Astrophysics

Astronomy

Scientific paper

We present preliminary results from Hinode of coronal loops. MSU's SEMAST code is used to perform differential emission measure analysis along active region coronal loops. The differential emission measures are then used to investigate the temperature and density structure of the loops. The results are then entered into the coronal loop database and compared to theoretical models for scaling laws and heating mechanisms.
This work is supported by NASA GSRP fellowship NNG05GK64H

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