Solar Magnetic Loops Observed with TRACE and EIT

Details Solar Magnetic Loops Observed with TRACE and EIT Solar Magnetic Loops Observed with TRACE and EIT

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..219..503a&link_type=abstract

Stars as suns : activity, evolution and planets, Proceedings of the 219th symposium of the International Astronomical Union held

Astronomy and Astrophysics

Astronomy

Scientific paper

We review major discoveries and new physical results that have been obtained from the TRACE mission over the last 4 years such as: (1) the temperature and density inhomogeneity of the coronal plasma (2) hydrostatic and non-hydrostatic loops (3) plasma flows in loops (4) transverse oscillations in the MHD kink-mode (5) the spatial heating function of loops (6) intermittent heating and cooling time scales (7) iron abundance enhancements (8) magnetic nullpoints and separator regions (9) highly fragmented postflare loop arcades and (10) nanoflare loop phenomena. We transform the physical properties as measured by TRACE for the Sun to stellar coronae and show how information on heating and cooling processes can be obtained from stellar differential emission measure (DEM) distributions.

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