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

Authors: S. Javadi, J. Büchner, A. Otto and J. C. Santos.<br />Astronomy & Astrophysics Vol. 529 , page A114<br />Published online: 14/04/2011<br />
Keywords:
Sun: atmosphere ; Sun: magnetic topology ; magnetohydrodynamics (MHD) ; methods: numerical ; Sun: corona.

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