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The Magnetic Fields and the Polarization of Radio Emission in the Active Center of October 1968

Published online by Cambridge University Press:  14 August 2015

N. Erushev
Affiliation:
Crimean Astrophysical Observatory, Nauchny, Crimea, U.S.S.R.
A. B. Severny
Affiliation:
Crimean Astrophysical Observatory, Nauchny, Crimea, U.S.S.R.
T. Tsap
Affiliation:
Crimean Astrophysical Observatory, Nauchny, Crimea, U.S.S.R.

Extract

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During the period of strong flare activity of the active center McMath No. 9740, from October 25 to November 2, 1968, 32 magnetograph records of longitudinal H and 20 of transverse fields, H, were obtained for this center with the Crimean magnetograph. Sometimes 5–7 daily records were made. Hα and K spectroheliograms, Hα cine film and routine determinations of sunspot magnetic fields were also obtained frequently. However the most important point is that all these optical observations were accompanied by simultaneous and continuous measurements of intensity and polarization of radio emission from this active center at a wavelength of 3 cm, recorded with the aid of the big 22-m radiotelescope of the Crimean Observatory (the resolution is 8′ for this wavelength), (Erushev and Zvetkov, 1970).

Type
Part IV: Observations of Magnetic Fields Associated with Flares and Other Transitory Phenomena
Copyright
Copyright © Reidel 1971 

References

Erushev, N. and Zvetkov, L.: 1970, Izv. Krymsk. Astrofiz. Obs. , in press.Google Scholar
Martres, M., Michard, R., Soru-Iscovoco, I., and Tsap, T.: Solar Phys. 5, 187.Google Scholar
Severny, A. and Zvereva, A.: 1970, Izv. Krvmsk. Astrofiz. Obs. 4142, in press.Google Scholar