Zajonc (1985) Emotion and facial efference. A theory reclaimed
نویسندگان
چکیده
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Kundu, in Radio Physics of the Sun (International Astronomical Union Symposium 86), M. R. Kundu and T. E. Gergely, Eds. (Reidel, Dordrecht, 1980), p. 457; G. D. Holman, Adv. Space Res. 2, 181 (1982); R. R. Sharma, L. Vlahos, K. Papadopoulos, Astron. Astrophys. 112, 337(1982); L. Vlahos, R. R. Sharma, K. Papadopoulos, Astrophys. J. 275, 374 (1983). 22. Adapted from (5), plate 2. 23. This review would have been impossible without the fine contributions to solar radio astronomy made by R. F. Willson at Tufts University and C. E. Alissandrakis, E. J. Schmahl, T. Velusamy, and L. Vlahos while working for the University of Maryland. Radio astronomical studies of the sun and other active stars at Tufts University are supported under Air Force Office of Scientific Research grant AFOSR-83-0019-B. Investigations of flare stars at Tufts University are also supported by NASA grant NAG 5477; whereas comparisons of VLA and Solar Maximum Mission satellite data are supported by NASA Guest Investigator grant NAG 5-501. Solar research in the Astronomy Program at the University of Maryland is supported under NSF grant ATM 84-15388, NASA grant NGR 21-002199, and NASA contract NSG 5320. The Very Large Array is operated by Associated Universities Inc., under contract with the National Science Foundation.
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