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Monitoring Program for Assessing the Impact of Rosemont Copper Mine Sky Brightness as Seen from the F.L. Whipple Observatory on Mt. Hopkins

Document ID: 
sao-2013
Year Published: 
2013
Summary: 

The purpose of this Rosemont Copper Mine sky brightness monitoring plan is to outline a selected approach to long term monitoring the sky brightness at telescopic sites at or near the summit of Mt. Hopkins. The plan outlines the monitoring that will take place on Mt. Hopkins to establish a baseline observatory sky brightness and how sky brightness changes over time as the result of the new Rosemont Mine site, and other related and unrelated activities. We will refer to this plan as the Rosemont Monitoring Plan (RMP).

Reference Information: 

Smithsonian Astrophysical Observatory. 2013. Monitoring Program for Assessing the Impact of Rosemont Copper Mine Sky Brightness as Seen from the F.L. Whipple Observatory on Mt. Hopkins. Tucson, AZ: Smithsonian Astrophysical Observatory. September 25.

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Content Disclaimer

The information appearing on this Web site is for general informational purposes only. Every effort is made to provide accurate and useful information.
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