Abstract
Progressive Alfvén waves set the atoms in oscillatory motion. The radiation will be absorbed (emitted) at a Doppler-shifted wavelength; the Doppler shift is determined by the velocity given to the atoms by the wave. The effect of the waves on the line profile, integrated over one period, is given for a few simple cases. A brief discussion of the possible application to sunspots is presented.
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Alfvén, H. and Fälthammar, C. G.: 1963, Cosmical Electrodynamics, 2d. ed., Clarendon Press, Oxford, p. 80.
Billings, D. E.: 1959, Astrophys. J. 130, 215.
Braginsky, S. I.: 1965, Reviews of Plasma Physics (ed. by M. A. Leontovich), Consultants Bureau, New York, Vol. 1, p. 205.
Danielson, R. E.: 1965, I.A.U. Symposium No. 22, Stellar and Solar Magnetic Fields (ed. by R. Lüst), North-Holland Publishing Company, Amsterdam, p. 314.
Eriksen, G.: 1961a, Nature 189, 651.
Eriksen, G.: 1961b, Astrophys. Norvegica 8, 1.
Eriksen, G. and Maltby, P.: 1967, Astrophys. J. 148, 833.
Ferraro, V. C. A.: 1955, Proc. Roy. Soc. London A 233, 310.
Gussmann, E. A.: 1967, Z. Astrophys. 65, 456.
Holweger, H.: 1967, Z. Astrophys. 65, 365.
KjeldsethMoe, O.: 1968, Solar Phys. 4, 267.
Maltby, P.: 1968, Solar Phys. 4, 96.
Maltby, P. and Eriksen, G.: 1967, Solar Phys. 2, 249.
Musman, S.: 1967, Astrophys. J. 149, 201.
Montgomery, D.: 1959, Phys. Rev. Letters 2, 36.
Parker, E. N.: 1958, Phys. Rev. 109, 1328.
Savage, B. D.: 1967, Astron. J. 72, 1130.
Tanenbaum, B. S. and Mintzer, D.: 1962, Phys. Fluids 5, 1226.
Weichel, H., Avizonis, P. V., and Vonderhaar, D. F.: 1967, Phys. Rev. Letters 19, 10.
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Maltby, P. Effect of progressive Alfvén waves on the profiles of solar spectral lines. Sol Phys 5, 3–14 (1968). https://doi.org/10.1007/BF00147115
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DOI: https://doi.org/10.1007/BF00147115