Photospheric Magnetic Fields from Magneto-Convection Simulations
Abstract
We present the properties of photospheric magnetic fields from magneto-convection simulations and as they would be observed by Hinode, for both quiet Sun and plage regions. This will include statistical properties, morphology, Stokes spectra, energy fluxes and correlations with convection dynamics. The rate of flux emergence will be discussed as a constraint on model parameters.
- Publication:
-
SDO-4: Dynamics and Energetics of the Coupled Solar Atmosphere. The Synergy Between State-of-the-Art Observations and Numerical Simulations
- Pub Date:
- March 2012
- Bibcode:
- 2012decs.confE..95S
- Keywords:
-
- SDO;
- SDO-4;
- SDO 4;
- SDO Workshop;
- SDO-4/IRIS/Hinode Workshop;
- Solar Dynamic Observatory