About the relative importance of compressional heating and current dissipation for the formation of coronal X-ray bright points

Author: Javadi S.   Büchner J.   Otto A.   Santos J. C.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|529|issue|A114-A114

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.529, Iss.issue, 2011-04, pp. : A114-A114

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Abstract