Line formation in turbulent magnetic atmospheres-Reference-Cited by-同舟云学术

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Line formation in turbulent magnetic atmospheres

Published:2005-04 Issue:3-4 Volume:326 Page:296-300
ISSN:0004-6337
Container-title:Astronomische Nachrichten
language:en
Short-container-title:Astron. Nachr.

Author:

Carroll T. A.,Staude J.

Publisher

Wiley

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference7 articles.

1. : 2005, A&A, in preparation

2. : 1985, Handbook of stochastic methods for physics, chemistry and the natural sciences, Springer-Verlag, Berlin

3. Line Asymmetries and the Microstructure of Photospheric Magnetic Fields

4. : 1994, Solar magnetic fields: Polarized radiation diagnostics, Astrophysics and Space Science Library 189, Kluwer Academic Publishers, Dordrecht

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3. Probability Density Functions to Represent Magnetic Fields at the Solar Surface;Magnetic Coupling between the Interior and Atmosphere of the Sun;2009-10-22

4. The Hanle effect in a random magnetic field;Astronomy & Astrophysics;2009-04-29

5. Comparison of Solar Magnetic Fields Measured at Different Observatories: Peculiar Strength Ratio Distributions Across the Disk;Solar Physics;2008-07-17

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