SDO in Pulkovo Observatory

  • E. Benevolenskaya
  • S. Efremov
  • V. Ivanov
  • N. Makarenko
  • E. Miletsky
  • O. Okunev
  • Yu. Nagovitsyn
  • L. Parfinenko
  • A. Solov’ev
  • A. Stepanov
  • A. Tlatov
Conference paper
Part of the Astrophysics and Space Science Proceedings book series (ASSSP, volume 30)

Abstract

We discuss effective applications of data obtained by both instruments of the Solar Dynamics Observatory: The Helioseismic & Magnetic Imager (HMI) and The Atmospheric Imaging Assembly (AIA). The purpose of this presentation is to show the most important problems of solar activity which are the main subjects in Pulkovo Observatory of the Russian Academy of Science. For these investigations uniform data sets of magnetic fields and coronal emissions in extreme ultra-violet bands are needed. Thus, we are planning to create SDO center in Pulkovo Observatory, which will help us in collaboration with existing SDO centers and provide more effective way of access to data for studies of the Sun.

Keywords

Magnetic Element Atmospheric Image Assembly Sunspot Data Polar Facula Pulkovo Observatory 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgements

Authors thank the AIA/SDO and HMI/SDO teams. This work was supported in part by grants of the Russian Foundation for Basic Research, the Program No. 20 of the Presidium of the Russian Academy of Sciences and the Program No. 15 of the Division of Physical Sciences of RAS.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2012

Authors and Affiliations

  • E. Benevolenskaya
    • 1
  • S. Efremov
    • 1
  • V. Ivanov
    • 1
  • N. Makarenko
    • 1
  • E. Miletsky
    • 1
  • O. Okunev
    • 1
  • Yu. Nagovitsyn
    • 1
  • L. Parfinenko
    • 1
  • A. Solov’ev
    • 1
  • A. Stepanov
    • 1
  • A. Tlatov
    • 1
  1. 1.Pulkovo Astronomical ObservatorySaint PetersburgRussia

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