Bonn 2010 – wissenschaftliches Programm
EP 3.14: Poster
Montag, 15. März 2010, 17:45–19:00, AKM Foyer
Influence of radiative loss and heat conduction on the temperature variation in of a coronal bright point — •Setareh Javadi1, Jörg Büchner1, Jean-Carlo Santos1, and Antonius Otto2 — 1Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str.2, 37191, Katlenburg-Lindau, Germany — 2University of Alaska, Fairbanks
Using the 3D numerical simulation model LINMOD3d a realistic approach was taken to simulate the heating processes associated with the formation of solar coronal bright points (BPs). The thermal structure of a coronal BP region was investigated by taking into account the influence of heat losses through thermal conduction and radiation. Comparing the results for cases with and without taking into account radiative loss and heat conduction the influence of these two factors on the formation of the BP temparture is discussed.