The Temperature - Magnetic Field Relation in Observed and Simulated Sunspots

0485628 - ASÚ 2018 RIV NL eng J - Článek v odborném periodiku
Sobotka, Michal - Rezaei, R.
The Temperature - Magnetic Field Relation in Observed and Simulated Sunspots.
Solar Physics. Roč. 292, č. 12 (2017), 188/1-188/12. ISSN 0038-0938. E-ISSN 1573-093X
Grant CEP: GA ČR(CZ) GA14-04338S; GA MŠMT(CZ) 7E13003
GRANT EU: European Commission(XE) 312495 - SOLARNET
Institucionální podpora: RVO:67985815
Klíčová slova: sunspots * magnetic fields * comparison
Obor OECD: Astronomy (including astrophysics,space science)
Impakt faktor: 2.580, rok: 2017

This work presents full-Stokes measurements of the full-split (g = 3) line Fe I 1564.85 nm with a spatial resolution of 0.5 '' obtained with the GREGOR Infrared Spectrograph in three large sunspots. The continuum intensity is corrected for instrumental scattered light, and the brightness temperature is calculated. Magnetic field strength and inclination are derived directly from the line split and the ratio of Stokes components. The continuum intensity (temperature) relations to the field strength are studied separately in the umbra, light bridges, and penumbra. The results are consistent with previous studies, and it was found that the scatter of values in the relations increases with increasing spatial resolution thanks to resolved fine structures. The observed relations show trends common for the umbra, light bridges, and the inner penumbra, while the outer penumbra has a weaker magnetic field than the inner penumbra at equal continuum intensities. This fact can be interpreted in terms of the interlocking comb magnetic structure of the penumbra. A comparison with data obtained from numerical simulations was made. The simulated data generally have a stronger magnetic field and a weaker continuum intensity than the observations, which may be explained by stray light and limited spatial resolution of the observations, and also by photometric inaccuracies of the simulations.
Trvalý link: http://hdl.handle.net/11104/0280580