Characterization of intensity variations along Fe XIV coronal loops - A case 
study

Costa, A.; Stenborg, G.

doi:10.1023/B:SOLA.0000043570.97010.b7

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Characterization of intensity variations along Fe XIV coronal loops - A case study

Costa, A., & Stenborg, G. (2004). Characterization of intensity variations along Fe XIV coronal loops - A case study. Solar Physics, 222(2), 229-245. doi:10.1023/B:SOLA.0000043570.97010.b7.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-F119-E Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-F11A-C

Genre: Journal Article

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Costa, A., Author
Stenborg, G.¹, Author

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1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291

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MPIS_GROUPS: Sun and Heliosphere

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Dates: Date issued: 2004

Publication Status: Issued

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Rev. Type: Peer

Identifiers: DOI: 10.1023/B:SOLA.0000043570.97010.b7
BibTex Citekey: Costa:2004-188

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Title: Solar Physics

Source Genre: Journal

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Pages: - Volume / Issue: 222 (2) Sequence Number: - Start / End Page: 229 - 245 Identifier: -