Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-19T12:17:36.702Z Has data issue: false hasContentIssue false
  • English
  • Français

Standard Magnetic Field Production at Huairou Solar Observing Station

Published online by Cambridge University Press:  27 November 2018

Suo Liu ,
Ganghua Lin ,
Xiao Yang ,
Xiaofan Wang ,
Jiangtao Su  and
Yuanyong Deng
Suo Liu
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences email: [email protected] School of Astronomy and Space Science, University of Chinese Academy of Sciences
Ganghua Lin
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences email: [email protected] School of Astronomy and Space Science, University of Chinese Academy of Sciences
Xiao Yang
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences email: [email protected] School of Astronomy and Space Science, University of Chinese Academy of Sciences
Xiaofan Wang
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences email: [email protected] School of Astronomy and Space Science, University of Chinese Academy of Sciences
Jiangtao Su
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences email: [email protected] School of Astronomy and Space Science, University of Chinese Academy of Sciences
Yuanyong Deng
Affiliation:
Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences email: [email protected] School of Astronomy and Space Science, University of Chinese Academy of Sciences
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The regular solar observations are operated at Huairou Solar Observing Station (HSOS) since 1987, which make the construction of long-term magnetic field datasets available to understand solar magnetic field and cycles. There exist some inconveniences for solar physicist to use these data, because the data storage medium and format at HSOS experienced some changes. Additionally, the processes of magnetic field calibration are not easy to deal with for who are not familiar with these data. Here shows that the magnetic field of HSOS are further processed toward international standards, in order to explore HSOS observations data for scientific research.

Keywords

Magnetic FieldData StandardizationSolar Magnetic Cycles
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S340: Long-term Datasets for the Understanding of Solar and Stellar Magnetic Cycles , February 2018 , pp. 49 - 50
Copyright
Copyright © International Astronomical Union 2018 

References

Ai, G. X. & Hu, Y. F., 1986, Acta Astronomica Sinica, 27, 173Google Scholar
Su, J. T. & Zhang, H. Q., 2004, Chin. J. Astron. Astrophys., 4, 365Google Scholar