Multipoint Validation of a Global 3D MHD Model for the Solar Corona and Inner Heliosphere

Details Multipoint Validation of a Global 3D MHD Model for the Solar Corona and Inner Heliosphere Multipoint Validation of a Global 3D MHD Model for the Solar Corona and Inner Heliosphere

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufmsh51b..06c&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #SH51B-06

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7524 Magnetic Fields, 7959 Models

Scientific paper

We present a long-term validation of a global, 3D MHD model for the solar corona and the solar wind. The model is driven by high resolution MDI magnetograms and is constrained by the empirical Wang-Sheeley-Arge (WSA) model. The model provides a three-dimensional steady-state structure of the heliosphere between the Sun and the Earth for a particular Carrington Rotation. We use the model to obtain the large-scale context for the information we collect from multipoint spacecraft observations and large-scale remote sensing imagine of the solar corona and the heliosphere. For the long-term validation of the model, we compare the result with ACE data and the available STEREO data.

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