The deep layers of solar magnetic elements

Details The deep layers of solar magnetic elements The deep layers of solar magnetic elements

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...285..648g&link_type=abstract

Astronomy and Astrophysics 285, 648-654 (1994)

Astronomy and Astrophysics

Astrophysics

47

Sun: Magnetic Fields, Sun: Faculae, Sun: Activity, Mhd

Scientific paper

We compare self-consistent theoretical models of solar magnetic flux sheets with spectropolarimetric observations of a solar plage and a network region. Our observational diagnostics mainly provide information on temperature and magnetic field of the deep photospheric layers. They are used to constrain the two free parameters of the models, viz. width and initial evacuation of the flux sheets. We find that the width of flux sheets in the network is approximately 200 km, while it is 300-350 km in an active plage. The flux sheets turn out to be less evacuated than previously thought, so they have continuum intensities close to unity. Since these are average values, however, our results do not exclude the presence of either smaller and brighter or larger and darker magnetic structures.

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