Average Variations Of Photospheric FeI and FeII Line Parameters As Function Of The Magnetic Filling Factor-Reference-Cited by-同舟云学术

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Average Variations Of Photospheric FeI and FeII Line Parameters As Function Of The Magnetic Filling Factor

Published:1990 Issue: Volume: Page:41-46
ISSN:
Container-title:Solar Photosphere: Structure, Convection, and Magnetic Fields
language:
Short-container-title:

Author:

Brandt P. N.,Steinegger M.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-009-1061-4_5.pdf

Reference33 articles.

1. Adam, M.G., Ibbetson, P.A., Petford, A.D.: 1976, Mon. Not. Roy. Asiron. Soc. 177, 687.

2. Brandt, P.N., Schröter, E.-H.: 1982, Solar Phys. 79, 3.

3. Brandt, P.N., Schröter, E.-H.: 1984, Small-Scale Dynamical Processes in Quiet Stellar Atmospheres, ed. S. Keil, NSO Conf., 371.

4. Brandt, P.N., Solanki, S.K.: 1987, The Role of Fine-Scale Magnetic Fields on the Structure of the Solar Atmosphere, eds. E.-H. Schroter, M. Vazquez, A.A. Wyller, Cambridge Univ. Press, 82.

5. Brandt, P.N., Solanki, S.K.: 1989, in preparation.

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1. Velocity Fields in Stellar Photospheres;The Observation and Analysis of Stellar Photospheres;2021-12-16

2. Line profile steepness as an additional tool for studies of magnetic field total energy;Astronomical & Astrophysical Transactions;1996-11

3. Small-scale solar magnetic fields: An overview;Space Science Reviews;1993

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