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Distribution of magnetic shear angle in an emerging flux region

Published online by Cambridge University Press:  26 August 2011

Sanjay Gosain
Sanjay Gosain*
Affiliation:
Udaipur Solar Observatory, Physical Research Laboratory, P. Box No. 198, Udaipur 313001, Rajasthan, India email: [email protected]
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Abstract

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We study the distribution of magnetic shear in an emerging flux region using the high-resolution Hinode/SOT SP observations. The distribution of mean magnetic shear angle across the active region shows large values near region of flux emergence i.e., in the middle of existing bipolar region and decreases while approaching the periphery of the active region.

Keywords

Sun: active regionssunspot: flux emergence
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S273: The Physics of Sun and Star Spots , August 2010 , pp. 347 - 350
Copyright
Copyright © International Astronomical Union 2011

References

Hagyard, M. J., Teuber, D., West, E. A., & Smith, J. B. 1984, Solar Phys., 91, 115CrossRefGoogle Scholar
Ichimoto, K., et al. 2008, Solar Phys., 249, 233CrossRefGoogle Scholar
Kosugi, T., et al. 2007, Solar Phys., 243, 3CrossRefGoogle Scholar
Lites, B., Casini, R., Garcia, J., & Socas-Navarro, H. 2007, Solar Phys., 78, 148.Google Scholar
Schmieder, B., Demoulin, P., Aulanier, G., & Golub, L. 1996, Astrophys. J., 467, 881CrossRefGoogle Scholar
Tsuneta, S., et al. 2008, Solar Phys., 249, 167CrossRefGoogle Scholar