Spatial Distribution and North–South Asymmetry of Coronal Bright Points from Mid-1998 to Mid-1999-Reference-Cited by-同舟云学术

Spatial Distribution and North–South Asymmetry of Coronal Bright Points from Mid-1998 to Mid-1999

Published:2005-09 Issue:1-2 Volume:231 Page:29-44
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Brajša R.,Wöhl H.,Vršnak B.,Rušdjak V.,Clette F.,Hochedez J.-F.,Verbanac G.,Temmer M.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s11207-005-8784-y.pdf

Reference45 articles.

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2. Ballester, J. L., Oliver, R., and Carbonell, M.: 2005, Astron. Astrophys. 431, L5.

3. Balthasar, H., Vázquez, M., and Wöhl, H.: 1986, Astron. Astrophys. 155, 87.

4. Benevolenskaya, E. E., Kosovichev, A. G., and Scherrer, P. H.: 2001, Astrophys. J. 554, L107.

5. Brajša, R., Pohjolainen, S., Ruždjak, V., Teräsranta, H., Urpo, S., Vršnak, B., and Wöhl, H.: 1994, in M. Schüssler and W. Schmidt (eds.), Solar Magnetic Fields, Proceedings of International Conference held in Freiburg, Cambridge University Press, Cambridge, p. 62.

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