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Rotation of Large Scale Patterns on the Solar Surface as Determined from Filament and Millimeter Data

Published online by Cambridge University Press:  12 April 2016

S. Pohjolainen ,
B. Vršnak ,
H. Teräsranta ,
S. Urpo ,
R. Brajša ,
V. Ruždjak ,
S. Jurač  and
A. Schroll
S. Pohjolainen
Affiliation:
Metsähovi Radio Research Station, 02540 Kylmälä, Finland
B. Vršnak
Affiliation:
Hvar Observatory, 58450 Hvar, Yugoslavia
H. Teräsranta
Affiliation:
Metsähovi Radio Research Station, 02540 Kylmälä, Finland
S. Urpo
Affiliation:
Metsähovi Radio Research Station, 02540 Kylmälä, Finland
R. Brajša
Affiliation:
Hvar Observatory, 58450 Hvar, Yugoslavia
V. Ruždjak
Affiliation:
Hvar Observatory, 58450 Hvar, Yugoslavia
S. Jurač
Affiliation:
Hvar Observatory, 58450 Hvar, Yugoslavia
A. Schroll
Affiliation:
Sonnenobservatorium Kanzelhöhe, 9520 Sattendorf, Austria

Abstract

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The rotation of large scale solar magnetic field patterns was studied using quiescent filaments and low temperature regions observed at 37 GHz as tracers.

Type
Part III Solar magnetism and large-scale flows
Information
International Astronomical Union Colloquium , Volume 130: The Sun and Cool Stars: activity, magnetism, dynamos , 1991 , pp. 279 - 281
Copyright
Copyright © Springer-Verlag 1991

References

Adams, W.M., Tang, F.: 1977, Solar Phys. 55, 499 CrossRefGoogle Scholar
Brajša, R., Vršnak, B., Ruždjak, V., Schroll, A.: 1989, Hvar Oba. Bull. 13, 449 Google Scholar
Vršnak, B., Pohjolainen, S., Teräsranta, H., Urpo, S., Brajša, R., Ruždjak, V., Schroll, A., Jurač, S.: 1991, these ProceedingsGoogle Scholar