Hostname: page-component-848d4c4894-pjpqr Total loading time: 0 Render date: 2024-06-21T05:45:18.060Z Has data issue: false hasContentIssue false

Change in the Zodiacal Light with Solar Activity

Published online by Cambridge University Press:  14 August 2015

R. Robley*
Affiliation:
Observatoire du Pic du Midi et Toulouse 1, Avenue C. Flammarion, 31500 Toulouse, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Gegenschein observed at the Pic du Midi Observatory during a solar cycle has a behaviour similar to that of the brightness of the eclipsed Moon. It is assumed that in both cases the solar wind ejected through the polar coronal holes is responsible for these variations.

Type
I: Zodiacal Light - Measurements and Models
Copyright
Copyright © Reidel 1980 

References

Asaad, A.S.: 1967, Nature 214, p. 259.Google Scholar
Danjon, A.: 1920, Compt. Rend. Acad. Sci. Paris 171, p. 1127.Google Scholar
Derham, C.J., Geake, J.E. and Walker, G.: 1964, Nature 203, p. 134.CrossRefGoogle Scholar
Dufay, J.: 1966, Compt. Rend. Acad. Sci. Paris 263, série B, p. 947.Google Scholar
Dumont, R. and Levasseur-Regourd, A.C.: 1978, Astron. Astrophys. 64, p. 9.Google Scholar
Gillett, F.C.: 1967, The zodiacal light and the interplanetary medium, Weinberg, J. L., NASA SP-150, p. 9.Google Scholar
Hanner, M.S., Weinberg, J.L., Deshields, L.M. II, Green, B.A. and Toller, G.N.: 1974, J. Geophys. Res. 79, p. 3671.Google Scholar
Hundhausen, A.J.: 1977, Coronal holes and high speed wind streams, J.B. Zirker, Boulder, p. 225.Google Scholar
Levasseur, A.C. and Blamont, J.E.: 1973, Nature 246, p. 26.CrossRefGoogle Scholar
Robley, R.: 1973, Ann. Géophys. 29, p. 321.Google Scholar
Robley, R. and Prêtre, P.: 1974, Compt. Rend. Acad. Sci. Paris 278, Série B, p. 671.Google Scholar
Sparrow, J.G. and Ney, E.P.: 1972, Astrophys. J. 174, p. 705.CrossRefGoogle Scholar
Tanabe, H.: 1965, Publ. Astron. Soc. of Japan 17, p. 339.Google Scholar
Weill, G.: 1966, Compt. Rend. Acad. Sci. Paris 263, Série B, p. 943.Google Scholar