Recent Advances in Understanding Magnetic Fields in the Quiet Sun

Details Recent Advances in Understanding Magnetic Fields in the Quiet Sun Recent Advances in Understanding Magnetic Fields in the Quiet Sun

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009spd....40.0501t&link_type=abstract

American Astronomical Society, SPD meeting #40, #5.01; Bulletin of the American Astronomical Society, Vol. 41, p.811

Astronomy and Astrophysics

Astronomy

Scientific paper

I will describe recent advances in our understanding of magnetic fields in the quiet sun. These have been developed both from high resolution observations made by the Hinode Solar Optical Telescope and ground-based observatories and from increasingly realistic three-dimensional MHD models of the upper convection zone and atmosphere. Examples of flux emergence, evolution, transport and disappearance are included. Some observational and theoretical problems in relating the photospheric fields to the upper atmosphere are discussed.
This work is supported by the NASA Hinode contract with the Lockheed Martin Advanced Technology Center.

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