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Structure and polarization of active region microwave emissionActive region radio emission observations made at 6.16 cm wavelength during May 20-27, 1980, are the bases of maps of total intensity and circular polarization presented for the three regions whose Hale numbers are 16850, 16863, and 16864. A detailed comparison is made between these maps and on- and off-band H-alpha pictures and magnetograms. The neutral lines with which the strongest sources were associated have their two opposite polarities close to each other, implying a high magnetic field gradient, and are also associated with arch filament systems. A detailed analysis is undertaken of observations of the circular polarization sense inversion in region 16863. The large scale structure of the magnetic field can be approximated by a dipole with its axis inclined by 11 deg with respect to the photosphere, and with a dipole moment of about 2 x 10 to the 31 power cgs units.
Document ID
19850044479
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kundu, M. R.
(Maryland, University College Park, MD, United States)
Alissandrakis, C. E.
(Athens, University Athens, Greece)
Date Acquired
August 12, 2013
Publication Date
September 1, 1984
Publication Information
Publication: Solar Physics
Volume: 94
ISSN: 0038-0938
Subject Category
Solar Physics
Accession Number
85A26630
Funding Number(s)
CONTRACT_GRANT: NSG-5320
CONTRACT_GRANT: NSF ATM-81-03089
CONTRACT_GRANT: NGR-21-002-199
Distribution Limits
Public
Copyright
Other

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