Integrating Tomography and Global Simulation

Details Integrating Tomography and Global Simulation Integrating Tomography and Global Simulation

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh41b..03f&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH41B-03

Astronomy and Astrophysics

Astrophysics

[7509] Solar Physics, Astrophysics, And Astronomy / Corona

Scientific paper

Rotational tomography of the Sun's corona based on EUV and white-light images gives us unprecedented access to the quasi-steady component of its 3D temperature and density structure. We show how this 3D information can be used to drive and validate global MHD models as well shed new light on spatial relationship between the corona's temperature and magnetic field. The AIA impact of AIA's superior coverage temperature on these programs is discussed.

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