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Cited article:

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

S. Javadi, J. Büchner, A. Otto, J. C. Santos

A&A, 529 (2011) A114

Published online: 2011-04-14

DOI: https://doi.org/10.1051/0004-6361/201015614

This article has been cited by the following article(s):

A 2D Model for Coronal Bright Points: Association with Spicules, UV Bursts, Surges, and EUV Coronal Jets

D. Nóbrega-Siverio and F. Moreno-Insertis
The Astrophysical Journal Letters 935 (2) L21 (2022)
https://doi.org/10.3847/2041-8213/ac85b6

Coronal bright points

Maria S. Madjarska
Living Reviews in Solar Physics 16 (1) (2019)
https://doi.org/10.1007/s41116-019-0018-8

The 3D MHD code GOEMHD3 for astrophysical plasmas with large Reynolds numbers

J. Skála, F. Baruffa, J. Büchner and M. Rampp
Astronomy & Astrophysics 580 A48 (2015)
https://doi.org/10.1051/0004-6361/201425274

On the role of current dissipation in the energization of coronal bright points

E. Adamson, J. Büchner and A. Otto
Astronomy & Astrophysics 557 A118 (2013)
https://doi.org/10.1051/0004-6361/201321281