Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-12T21:38:27.706Z Has data issue: false hasContentIssue false
  • English
  • Français

Zodiacal Light - Scattered Fraunhofer Line Profiles

Published online by Cambridge University Press:  27 February 2018

David Clarke
David Clarke*
Affiliation:
University Observatory, Acre Rd., GLASGOW G20 0TL, Scotland, U.K.

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 scattering function of Hong's successful model for the brightness variation with elongation, B(ε), of the Zodiacal Light has been used to calculate profiles of Doppler shifted Fraunhofer lines. Substantial line shape changes with ε are predicted with an indication of a bifurcation at ε < 30°, so offering an explanation for reported F corona observations.

Type
IX. Zodiacal Light and Thermal Emission
Information
International Astronomical Union Colloquium , Volume 150: Physics, Chemistry and Dynamics of Interplanetary Dust , 1996 , pp. 337 - 340
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Beavers, W.L., Eitter, J.J., Carr, P.H., & Cook, B.C. 1980, ApJ, 238, 349 CrossRefGoogle Scholar
Blackwell, D.E., & Ingham, M.F. 1961, MNRAS, 122, 129 CrossRefGoogle Scholar
Clarke, D., Matthews, S.S., Mundell, C.G., & Weir, A.S. 1995, A&A, AcceptedGoogle Scholar
East, I.R., & Reay, N.K. 1984, A&A, 139, 512 Google Scholar
Fried, J W. 1978, A&A, 68, 259 Google Scholar
Hong, S.S. 1985, A&A, 146, 67 Google Scholar
James, J.F. 1969, MNRAS, 142, 45 CrossRefGoogle Scholar
Leinert, C., Richter, I., Pitz, E., & Planck, B. 1981, A&A, 103, 177 Google Scholar
Mukai, T., & Mann, I. 1993, A&A, 271, 530 Google Scholar
Ring, J., Clarke, D., James, J.F., Daehler, M., & Mack, J.E. 1964, Nature, 202, 167 CrossRefGoogle Scholar