TRACE Active Region Loops: Observation and Modeling

Details TRACE Active Region Loops: Observation and Modeling TRACE Active Region Loops: Observation and Modeling

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...200.0210h&link_type=abstract

American Astronomical Society, 200th AAS Meeting, #02.10; Bulletin of the American Astronomical Society, Vol. 34, p.641

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent Transition Region and Coronal Explorer (TRACE) observations have detected active region coronal loops that can not be easily modeled using hydrostatic models. Analysis of these loops suggests that they are overdense relative to the predictions of hydrodynamic models with uniform heating. This modeling, however, assumes that the observed emission is near 1 MK. Since the TRACE filter ratios are actually multivalued and high-temperature, uniformly heated models are difficult to exclude based on the TRACE data alone. Using co-aligned CDS rasters of overdense TRACE loops we find that these loops contain material at 105.9 K to 106.2 K. From these rasters we perform a DEM analysis to constrain the input parameters to time-dependent hydrodynamic models of these loops. TRACE is supported by contract NAS5-38099 from NASA to LMATC.

Affiliated with

Also associated with

No associations

Rating

TRACE Active Region Loops: Observation and Modeling does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with TRACE Active Region Loops: Observation and Modeling, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and TRACE Active Region Loops: Observation and Modeling will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1716952