The Complexity of Equatorial Coronal Holes

Details The Complexity of Equatorial Coronal Holes The Complexity of Equatorial Coronal Holes

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsp51b..05m&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SP51B-05

Astronomy and Astrophysics

Astrophysics

7500 Solar Physics, Astrophysics, And Astronomy, 7511 Coronal Holes, 7524 Magnetic Fields, 7546 Transition Region

Scientific paper

We will investigate the multi-thermal intensities, flow structures and extrapolated magnetic structures in an massive equatorial coronal holes that crossed the solar disk in early November of 1999. We will use a large suite of observations from the MDI and SUMER instruments on SOHO. We will use the insight developed from our understanding of the multi-thermal coronal hole topography to propose a consistent picture of solar wind structure at the base of the Sun-Earth Connection.

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