How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?-Reference-Cited by-同舟云学术

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How Can Active Region Plasma Escape into the Solar Wind from Below a Closed Helmet Streamer?

Published:2014-08-21 Issue:11 Volume:289 Page:4151-4171
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Mandrini C. H.,Nuevo F. A.,Vásquez A. M.,Démoulin P.,van Driel-Gesztelyi L.,Baker D.,Culhane J. L.,Cristiani G. D.,Pick 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/s11207-014-0582-y.pdf

Reference93 articles.

1. Antiochos, S.K., DeVore, C.R., Karpen, J.T., Mikić, Z.: 2007, Astrophys. J. 671, 936. DOI . ADS .

2. Antiochos, S.K., Mikić, Z., Titov, V.S., Lionello, R., Linker, J.A.: 2011, Astrophys. J. 731, 112. DOI . ADS .

3. Antiochos, S.K., Linker, J.A., Lionello, R., Mikić, Z., Titov, V., Zurbuchen, T.H.: 2012, Space Sci. Rev. 172, 169. DOI . ADS .

4. Aulanier, G., DeLuca, E.E., Antiochos, S.K., McMullen, R.A., Golub, L.: 2000, Astrophys. J. 540, 1126. DOI . ADS .

5. Aulanier, G., Pariat, E., Démoulin, P., Devore, C.R.: 2006, Solar Phys. 238, 347. DOI .

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