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  Effect of anisotropic velocity distribution on the linear polarization of coronal lines. Does the ion cyclotron exist in the inner corona?

Raouafi, N.-E., & Solanki, S. K. (2003). Effect of anisotropic velocity distribution on the linear polarization of coronal lines. Does the ion cyclotron exist in the inner corona? Astronomy and Astrophysics, 412, 271-280.

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 Creators:
Raouafi, N.-E.1, Author           
Solanki, S. K.2, 3, Author           
Affiliations:
1IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
3MPI 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: SOHO: SUMER
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 Dates: 2003
 Publication Status: Issued
 Pages: -
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 Rev. Type: Peer
 Identifiers: BibTex Citekey: Raouafi:2003-133
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 412 Sequence Number: - Start / End Page: 271 - 280 Identifier: -