Modeling the Coronal Loop of an X-ray Bright Point

Details Modeling the Coronal Loop of an X-ray Bright Point Modeling the Coronal Loop of an X-ray Bright Point

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh41a16m&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH41A-16

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona

Scientific paper

We use a time-dependent gasdynamic model to simulate the corona and transition region in an x-ray bright point loop. For this work we model a bright point observed by TRACE and SOHO on June 17, 1998. The magnetic field geometry is derived from an extrapolation of magnetograms. We study the effects of various hypothesized spatial and temporal distributions of heat deposition within the loop, including Joule heating at the footpoints or decay of standing Alfvén waves.

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