The differential emission measure of nested hot and cool magnetic loops

Details The differential emission measure of nested hot and cool magnetic loops The differential emission measure of nested hot and cool magnetic loops

Sep 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..147..199v&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 147, no. 1, p. 199-202.

Physics

2

Magnetic Field Configurations, Solar Magnetic Field, Solar Temperature, Solar Transition Region, Thermophysical Properties, Magnetohydrodynamics, Solar Corona, Thermal Stability

Scientific paper

The detailed thermal structure of the magnetized solar transition region, as measured by its differential emission measure (DEM(T)), is poorly known. Building on the fact that the solar surface is strongly magnetized and thereby structured, proposals have been made that envision a significant lower-temperature contribution to the energy balance from (ion) heat flux across an arcade of different temperature loops. In this paper, we describe a self-consistent 2D MHD simulation, which includes the full thermal effects of parallel stability and anisotropic conduction, of a nested-loop model of the thermal and magnetic structure of the transition region. We then demonstrate that the predicted DEM agrees with observations in the conceptually elusive T less than 10 exp 5 K regime.

Affiliated with

Also associated with

No associations

Rating

The differential emission measure of nested hot and cool magnetic loops 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 The differential emission measure of nested hot and cool magnetic loops, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The differential emission measure of nested hot and cool magnetic loops will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1543111