Physics
Scientific paper
Jul 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...93..289h&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 93, July 1984, p. 289-299.
Physics
14
Broadband, Circular Polarization, Polarimetry, Solar Magnetic Field, Solar Spectra, Sunspots, Near Infrared Radiation, Penumbras, Solar Flux Density, Spatial Resolution, Umbras
Scientific paper
Spatial scans with a resolution of 3.4 arc sec of the broad-band circular polarization of several sunspots have been made in five filter bands over the wavelength range 0.4- 1.7μ with a sensitivity of 1 x 10- 6 fractional polarization. The scans, across a spot through the penumbra and umbra center, revealed two important features: (1) The broad-band circularly polarized flux V reverses in sign, or diminishes to near zero, at the center of the umbral region relative to the outer penumbra. This effect was wavelength dependent and was most clearly detected as a definite reversal in a band at 1.2μ, although a reversal was also detected in a very broad band extending from 0.8 to l.6μ. (2) There is a marked asymmetry: in all cases the limbward penumbral region exhibited stronger V values than did the disk-center (inward) side of the spot, at all observed wavelengths. Such previously unreported structure in the magnetic circular polarization of sunspots provides new clues for understanding the 'anomalous' large broad-band polarization at short wavelengths and at the same time imposes new constraints on sunspot models. For example, the polarization reversal in the umbra relative to the penumbra can be naively explained by return-flux sunspot models; but this is not the only interpretation. Alternatively, it can relate to reversals in mass-flow velocities and/or vertical velocity gradients, as between the umbra and penumbra.
Henson Gary D.
Kemp James C.
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