Principal component analysis of background and sunspot magnetic field variations during solar cycles 21-23-Reference-Cited by-同舟云学术

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Principal component analysis of background and sunspot magnetic field variations during solar cycles 21-23

Published:2012-07-23 Issue:4 Volume:424 Page:2943-2953
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:Monthly Notices of the Royal Astronomical Society

Author:

Zharkova V. V.¹,Shepherd S. J.²,Zharkov S. I.³

Affiliation:

1. Department of Mathematics; School of Computing; Informatics and Media; University of Bradford; Bradford; BD7 1DP

2. Department of Mathematics; School of Engineering; Design and Technology; University of Bradford; Bradford; BD7 1DP

3. Mullard Space Science Laboratory; University College London; Holmbury St Mary; Dorking; RH5 6NT

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/424/4/2943/18712370/424-4-2943.pdf

Reference34 articles.

1. A Model of the Double Magnetic Cycle of the Sun

2. Active Region Detection and Verification With the Solar Feature Catalogue

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