On the Reconstruction of the Convection Pattern Below an Active Region of Solar Corona

Publisher： IOP Publishing

ISSN： 1742-6596

Source： Journal of Physics: Conference Series , Vol.341, Iss.1, 2012-02, pp. : 36-48

Access to resources Favorite

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Related content

Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region⋆

By Bourdin Ph.-A.   Bingert S.   Peter H.  

Astronomy & Astrophysics, Vol. 555, Iss. issue, 2013-07 ,pp. : A123-A123

Edp Sciences

Access to resources Recommend Favorite

Fe XIX observations of active region brightenings in the corona

By  

Astronomy & Astrophysics, Vol. 455, Iss. 3, 2006-09 ,pp. : 1105-1113

Edp Sciences

Access to resources Recommend Favorite

Dynamics of the solar active region finestructure

By  

Astronomy & Astrophysics, Vol. 412, Iss. 1, 2003-12 ,pp. : 249-255

Edp Sciences

Access to resources Recommend Favorite

A model for the formation of the active region corona driven by magnetic flux emergence⋆

By Peter H.   Bingert S.   Cheung M. C. M.   Peter H.  

Astronomy & Astrophysics, Vol. 564, Iss. issue, 2014-03 ,pp. : A12-A12

Edp Sciences

Access to resources Recommend Favorite

Distribution of coronal heating in a solar active region

By  

Astronomy & Astrophysics, Vol. 489, Iss. 1, 2008-10 ,pp. : 441-447

Edp Sciences

Access to resources Recommend Favorite