Hostname: page-component-7c8c6479df-8mjnm Total loading time: 0 Render date: 2024-03-28T15:27:05.585Z Has data issue: false hasContentIssue false

The Effects of Lamp Spectral Distribution on Sky Glow over Observatories

Published online by Cambridge University Press:  05 March 2015

C. B. Luginbuhl
Affiliation:
U.S. Naval Observatory Flagstaff Station, Flagstaff, Arizona, U.S.A. email: cbl@nofs.navy.mil
P. A. Boley
Affiliation:
Max-Planck-Institut für Astronomie, Heidelberg, Germany
D. R. Davis
Affiliation:
Planetary Science Institute, Tucson, Arizona, U.S.A.
D. M. Duriscoe
Affiliation:
National Park Service, Bishop, California, U.S.A.
Rights & Permissions [Opens in a new window]

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.

Using a wavelength-generalized version of the Garstang (1991) model, we evaluate overhead sky glow as a function of distance up to 300 km, from a variety of lamp types, including common gas discharge lamps and several types of LED lamps. We conclude for both professional, and especially cultural (visual), astronomy, that low-pressure sodium and narrow-spectrum amber LED lamps cause much less sky glow than all broad-spectrum sources.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Garstang, R. H. 1991, PASP, 103, 1109Google Scholar