Appropropriate Application of Source Surface Models

Details Appropropriate Application of Source Surface Models Appropropriate Application of Source Surface Models

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh23c..04h&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH23C-04

Physics

7509 Corona, 7524 Magnetic Fields

Scientific paper

Magnetostatic source surface models provide useful and reasonably reliable indications of the large-scale structure of coronal and interplanetary magnetic and velocity fields. Long term studies of the solar magnetic field can reveal much about the structure of the heliosphere. Improving data availability allows for more frequent calculations with higher spatial and temporal resolution, but still under highly idealized assumptions. The models provide at best a snapshot of a highly dynamic atmosphere. Appropriate application of the models provides a global context for many studies, but care must be exercised to address appropriate questions.

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