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Waves in the Magnetised Solar Atmosphere

Published online by Cambridge University Press:  13 May 2016

C. S. Rosenthal
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, Box 1029, N-0315, Blindern, Oslo, Norway
M. Carlsson
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, Box 1029, N-0315, Blindern, Oslo, Norway
V. Hansteen
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, Box 1029, N-0315, Blindern, Oslo, Norway
A. McMurry
Affiliation:
Institute of Theoretical Astrophysics, University of Oslo, Box 1029, N-0315, Blindern, Oslo, Norway
T. J. Bogdan
Affiliation:
HAO/NCAR, Box 3000, Boulder, Colorado, CO 80307-3000, USA
S. McIntosh
Affiliation:
HAO/NCAR, Box 3000, Boulder, Colorado, CO 80307-3000, USA
Å. Nordlund
Affiliation:
NBIfAFG, Københavns Universitet, Juliane Maries Vej 30, DK-2100 København Ø, Denmark
R. F. Stein
Affiliation:
Dept. of Physics and Astronomy, Michigan State University, East Lansing, MI 48824, USA
S. B. F. Dorch
Affiliation:
The Royal Swedish Academy of Sciences, Stockholm Observatory, SE-133 36 Saltsjöbaden, Sweden

Abstract

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We describe simulations of the propagation of waves in magnetised structures in the solar atmosphere.

Type
Session II: Convection Zone and Local Area Helioseismology
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Roberts, B. 2000, Sol. Phys., 193, 139.Google Scholar
Nordlund, Å. & Galsgaard, K. 1995, http://www.astro.ku.dk/∼aake/NumericalAstro/papers/kg/mhd.ps.gz Tsiropoula, G., Alissandrakis, C.E., & Mein, P. 2000, A&A, 355, 375.Google Scholar