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Generation and Propagation of Oscillatory Motions in the Solar Atmosphere

Published online by Cambridge University Press:  16 November 2021

F. Meyer  and
H. U. Schmidt
F. Meyer
Affiliation:
High Altitude Observatory, Boulder, Colorado, and Sacramento Peak Observatory, Sunspot, New Mexico; on leave from Max-Planck-Institut für Astrophysik, Munich
H. U. Schmidt
Affiliation:
High Altitude Observatory, Boulder, Colorado, and Sacramento Peak Observatory, Sunspot, New Mexico; on leave from Max-Planck-Institut für Astrophysik, Munich

Abstract

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Information

Type
Part 4 Joint Discussions
Information
Transactions of the International Astronomical Union , Volume 12 , Issue 2 , 1966 , pp. 559 - 561
Copyright
Copyright © Academic Press 1966 

References

1. Evans, J. W., Michard, R. Astrophys. J., 136, 493, 1962.Google Scholar
2. Schmidt, H. U., Zirker, J. B. Astrophys. J., 138, 1310, 1963.Google Scholar
3. Moore, D. W., Spiegel, E. A. Astrophys. J., 139, 48, 1964.Google Scholar
4. Whitney, C. Smithson. Contr. Astrophys., 2, 365, 1958.Google Scholar
5. Bahng, J. D., Schwarzschild, M. Astrophys. J., 137, 901, 1963.Google Scholar
6. Bahng, J. D., Schwarzschild, M. Astrophys. J., 134, 312, 1961.Google Scholar