Calculations of Photospheric Plasma Velocity Fields UsingPhotospheric Magnetic Field Measurements

Details Calculations of Photospheric Plasma Velocity Fields UsingPhotospheric Magnetic Field Measurements Calculations of Photospheric Plasma Velocity Fields UsingPhotospheric Magnetic Field Measurements

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..369..183s&link_type=abstract

New Solar Physics with Solar-B Mission ASP Conference Series, Vol. 369, proceedings of the conference held 8-11 November, 2005 a

Physics

Scientific paper

The amount of emergence and submergence of magnetized plasma through the photosphere might be crucial for modeling the solar coronal dynamics. It cannot be measured directly since it is too small to produce measurable doppler-shifts. We compare three methods to estimate the photospheric flow from magnetic field observations. The methods are tested using photospheric vector magnetic field data for active region NOAA 8210.

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