Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993apjs...86..313h&link_type=abstract
Astrophysical Journal Supplement Series (ISSN 0067-0049), vol. 86, no. 1, p. 313-332.
Astronomy and Astrophysics
Astrophysics
22
Astronomical Polarimetry, Emission Spectra, Line Spectra, Metallicity, Solar Magnetic Field, Sunspots, Linear Polarization, Magnesium, Solar X-Rays
Scientific paper
Polarimetric observations at 12 microns of two sunpots are reported. The horizontal distribution of parameters such as magnetic field strength, inclination, azimuth, and magnetic field filling factors are presented along with information about the height dependence of the magnetic field strength. Comparisons with contemporary magnetostatic sunspot models are made. The magnetic data are used to estimate the height of 12 micron line formation. From the data, it is concluded that within a stable sunspot there are no regions that are magnetically filamentary, in the sense of containing both strong-field and field-free regions.
Deming Drake
Garcia Howard
Hewagama Tilak
Jennings Donald E.
Mickey Donald L.
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