Investigation of Non-steady Flow Solutions in the Coronal Heating Problem

Details Investigation of Non-steady Flow Solutions in the Coronal Heating Problem Investigation of Non-steady Flow Solutions in the Coronal Heating Problem

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh11a0691b&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH11A-0691

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7546 Transition Region

Scientific paper

Observations made by the TRACE satellite show intermittent intensity fluctuations in coronal loops that suggest non-steady mass flows. These flows are not explained by previous work on coronal loop models, which focus on static and steady flow solutions. To investigate these flows we have written a code that looks for thermally stable, non-steady solutions to the hydrodynamic equations that govern coronal loops. These solutions will be used to determine if an asymmetric heating function reproduces the observed intensities.

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