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

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

doi:10.1051/0004-6361/201015614

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

Javadi, S., Büchner, J., Otto, A., & Santos, J. C. (2011). About the relative importance of compressional heating and current dissipation for the formation of coronal X-ray bright points. Astronomy and Astrophysics, 529: A114. doi:10.1051/0004-6361/201015614.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-063E-8 Version Permalink: https://hdl.handle.net/21.11116/0000-0007-2B09-0

Genre: Journal Article

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Javadi, S., Author
Büchner, J.^{1, 2}, Author
Otto, A., Author
Santos, J. C., Author

Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291

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MPIS_GROUPS: Sun and Heliosphere

MPIS_PROJECTS: Theory: Sim Sol Sys Plasma

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Dates: Date issued: 2011

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1051/0004-6361/201015614
BibTex Citekey: Javadi:2011-052

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Title: Astronomy and Astrophysics

Source Genre: Journal

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Pages: - Volume / Issue: 529 Sequence Number: A114 Start / End Page: - Identifier: -