Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spd....37.0102l&link_type=abstract
American Astronomical Society, SPD meeting #37, #1.02; Bulletin of the American Astronomical Society, Vol. 38, p.215
Astronomy and Astrophysics
Astronomy
Scientific paper
The nature of coronal "moss" seen in Transition Region and Coronal Explorer (TRACE) images is investigated using a time series set of SOHO Coronal Diagnostic Spectrometer (CDS) and TRACE measurements of a moss region seen face-on. Spectral line fluxes obtained at different times are used to construct differential emission measure distribution snapshots in the moss line-of-sight, paying special attention to subtraction of background from unassociated structures. The results are used to investigate the variability of the moss itself and of the purported overlying hot loops whose footpoints Berger et al (1999) and Fletcher & De Pontieu (1999) have proposed as the origin of the moss emission. We conclude by discussing whether or not the loop footpoint nature of moss is compatible with our observations.
Cirtain Jonathan
DeLuca Edward E.
Drake Jeremy J.
Kashya V.
Lin Li Wei
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