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Reconstruction of solar activity according to the data of centenary observations

Published online by Cambridge University Press:  27 November 2018

Kseniya A. Tlatova
Affiliation:
Kislovodsk mountain astronomical station of the Pulkovo observatory, 357700, Gagarina str. 100Russia email: [email protected]
Valeriya Vasil’eva
Affiliation:
Kislovodsk mountain astronomical station of the Pulkovo observatory, 357700, Gagarina str. 100Russia email: [email protected]
Andrey Tlatov
Affiliation:
Kislovodsk mountain astronomical station of the Pulkovo observatory, 357700, Gagarina str. 100Russia email: [email protected] Kalmyk State University, Elista, Russia
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Abstract

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Digitization of solar activity data over a period of more than 100 years has been performed. The database presents the characteristics of sunspots, sunspot umbras, filaments, plages in CaIIK line and prominences. The series of vector boundaries and photometric properties of the selected objects are created.

The characteristics of individual types of solar activity were determined. An interactive atlas of solar activity has been created, on which daily maps of solar activity, characteristics of individual elements and summary indices of solar activity are presented. The indices of solar activity were reconstructed and the analysis was carried out.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Tlatov, A. G., Pevtsov, A. A. & Singh, J. 2009 Solar Phys., 255, 239.Google Scholar
Tlatov, A. G., Kuzanyan, K. M., & Vasil’yeva, V. V., 2016, Solar Phys., 291, 1115Google Scholar
Tlatov, A. G., Vasilieva, V. V., Makarova, V. V., & Otkidychev, P. A. Solar Phys., 289, 1403Google Scholar
Tlatov, A. G., Tlatova, K. A.; Vasil’eva, V. V.; Pevtsov, A. A. & Mursula, K. Advances in Space Research., 55, 835Google Scholar