Diagnostics of the Solar Coronal Magnetic Field: 1878 - 2010

Details Diagnostics of the Solar Coronal Magnetic Field: 1878 - 2010 Diagnostics of the Solar Coronal Magnetic Field: 1878 - 2010

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsh42d..01h&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SH42D-01

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7509 Corona, 7524 Magnetic Fields, 7594 Instruments And Techniques

Scientific paper

The solar corona is today a subject of intense scientific scrutiny as the birthplace of space weather and the location of the largest explosions in the solar system. The dynamics and structure of the lower solar corona are controlled by its magnetic field. Diagnosing the magnetic field is a difficult task of astrophysics that has been pursued for 125 years. This brief review will examine optical and radio methods used to study the inner coronal magnetic field. The National Solar Observatory is operated by AURA, Inc. under a cooperative agreement with the National Science Foundation.

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