Astronomy and Astrophysics – Astrophysics
Scientific paper
Dec 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...316l..25g&link_type=abstract
Astronomy and Astrophysics, v.316, p.L25-L28
Astronomy and Astrophysics
Astrophysics
7
Solar Activity, Radio Emission, Magnetic Fields
Scientific paper
We present Very Large Array (VLA) observations of AR 7542 which demonstrate the existence of definite ring and horse-shoe structures of a sunspot in intensity (I) and polarization (V) at 8.46GHz (3.5cm wavelength) and compare them with model calculations of gyroresonance radiation. The VLA measurements have been made on three different days in July 1993 when AR 7542 was at three different longitudes which allows us to study the effect of viewing angle on sunspot-associated microwave emission. Model calculations of gyroresonance radiation have been carried out using a modified dipole model corresponding to the observed photospheric magnetic field strength and average temperature/electron density distributions consistent with soft X-ray and EUV observations (for the lower atmosphere) as well as theoretical assumptions (for the corona). The calculated I and V maps were found to be generally consistent with the radio observations. We obtain information on the magnetic scale length in vertical and horizontal directions above the sunspot and about the distribution of other plasma parameters (temperature, density) inside the radio source region.
Gopalswarmy N.
Hildebrandt Joachim
Hofmann Andrea
Krueger Andre
Kundu Mukul R.
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