Properties of the magnetic fields of coronal holes with active regions-Reference-Cited by-同舟云学术

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Properties of the magnetic fields of coronal holes with active regions

Published:2010-06 Issue:1 Volume:106 Page:1-7
ISSN:0190-2717
Container-title:Bulletin of the Crimean Astrophysical Observatory
language:en
Short-container-title:Bull.Crim. Astrophys. Observ.

Author:

Fainshtein V. G.,Stepanian N. N.,Rudenko G. V.,Malashchuk V. M.,Kashapova L. K.

Publisher

Allerton Press

Subject

General Medicine

Link

http://link.springer.com/content/pdf/10.3103/S0190271710010018.pdf

Reference7 articles.

1. O. I. Bugaenko, I. A. Zhitnik, et al., Izv. Krymsk. Astrofiz. Obs. 100, 123 (2004).

2. O. I. Bugaenko, I. A. Zhitnik, et al., Izv. Krymsk. Astrofiz. Obs. 100, 136 (2004a).

3. V. Bumba, M. Klvana, and A. Garcia, Izv. Krymsk. Astrofiz. Obs. 103, 153 (2007).

4. E. V. Malanushenko and N. N. Stepanian, Izv. Krymsk. Astrofiz. Obs. 97, 69 (2001).

5. G. V. Rudenko, Solar Phys. 198, 5 (2001).

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Coronal holes, large-scale magnetic field, and activity complexes in solar cycle 23;Geomagnetism and Aeronomy;2014-11-23

2. ROTATION RATES OF CORONAL HOLES AND THEIR PROBABLE ANCHORING DEPTHS;The Astrophysical Journal;2013-01-17

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