Characterizing the Quiet Sun Scale Magnetic Field

Details Characterizing the Quiet Sun Scale Magnetic Field Characterizing the Quiet Sun Scale Magnetic Field

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..271...86t&link_type=abstract

Astrophysical Dynamics: From Stars to Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 271,

Astronomy and Astrophysics

Astrophysics

Sun: Magnetic Fields

Scientific paper

Observations with the Solar Optical Telescope on Hinode indicate that the Quiet Sun magnetic field occurs on every scale of convection including granulation. Data reported here show that, regardless of the position on the disk, the polarity in the inner network regions are balanced to 1 part in 72. This is consistent with both local dynamo processes or the creation of surface features by the granulation downflows.

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