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UV Emitting Spicules

Published online by Cambridge University Press:  14 August 2015

Giannina Poletto
Giannina Poletto*
Affiliation:
Osservatorio Astrofisico di Arcetri, Firenze, Italia

Abstract

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Extreme ultraviolet observations of the chromospheric network in a coronal hole obtained in 1973 by the Harvard College Observatory experiment aboard Skylab are analyzed. Upper and lower limits to the actual emission measure in UV spicules have been obtained, and the consistency of the derived values with the hypothesis that UV spicules are Hα spicules falling back after being heated is discussed.

Type
Part III. Solar Transient Phenomena Affecting the Corona and Interplanetary Medium: Dynamics Deduced from Observations
Information
Symposium - International Astronomical Union , Volume 91: Solar and Interplanetary Dynamics , 1980 , pp. 199 - 201
Copyright
Copyright © Reidel 1980 

References

Beckers, J.M.: 1968, Solar Phys. 3, 367.Google Scholar
Bonnet, R.M.: 1978, Space Sci. Rev. 21, 379.Google Scholar
Feldman, U., Doschek, G.A., and Patterson, N.P.: 1976, Astrophys. J. 209 270.Google Scholar
Kanno, M.: 1978, Publ. Astron. Soc. Japan 30, 581.Google Scholar
Reeves, E.M., Vernazza, J.E., and Withbroe, G.L.: 1976 Phil. Trans. Roy. Soc. London A281, 319.Google Scholar
Withbroe, G.L.: 1977, Proc. 199 Nov. 7-10, OSO-8 Workshop, pp. 1–27.Google Scholar
Withbroe, G.L. and Mariska, J.T.: 1976, Solar Phys. 48, 21.CrossRefGoogle Scholar