Strong Stokes V asymmetries of photospheric spectral lines: What can they tell 
us about the magnetic field structure?

Grossmann-Doerth, U.; Schüssler, M.; Sigwarth, M.; Steiner, O.

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Strong Stokes V asymmetries of photospheric spectral lines: What can they tell us about the magnetic field structure?

Grossmann-Doerth, U., Schüssler, M., Sigwarth, M., & Steiner, O. (2000). Strong Stokes V asymmetries of photospheric spectral lines: What can they tell us about the magnetic field structure? Astronomy and Astrophysics, 357, 351-358.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-DFF9-2 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-DFFA-F

Genre: Journal Article

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Grossmann-Doerth, U., Author
Schüssler, M.^{1, 2}, Author
Sigwarth, M., Author
Steiner, O., Author

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

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Dates: Date issued: 2000

Publication Status: Issued

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Rev. Type: Peer

Identifiers: BibTex Citekey: GrossmannDoerth:2000-029

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Title: Astronomy and Astrophysics

Source Genre: Journal

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Pages: - Volume / Issue: 357 Sequence Number: - Start / End Page: 351 - 358 Identifier: -