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Sky brightness during eclipses: a review.

S M Silverman, E G Mullen

|February 16, 2010

Summary

This summary is machine-generated.

This paper summarizes sky brightness data during eclipses, drawing from a comprehensive literature review. It provides foundational information for understanding celestial light variations during these astronomical events.

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Area of Science:

Astronomy
Astrophysics
Optical Physics

Background:

Solar eclipses significantly alter the ambient light conditions on Earth's surface.
Previous research has documented variations in sky brightness during eclipses.
Understanding these variations is crucial for astronomical observations and atmospheric studies.

Purpose of the Study:

To compile and present existing literature on sky brightness measurements during solar eclipses.
To provide a consolidated reference for researchers studying eclipse phenomena.

Main Methods:

Literature review and data compilation from various sources.
Analysis of reported sky brightness measurements and observational data.

Main Results:

Sky brightness decreases significantly during the totality phase of a solar eclipse.
The rate of decrease and subsequent increase in brightness follows predictable patterns.
Variations in sky brightness are influenced by atmospheric conditions and eclipse path.

Conclusions:

The compendium provides a valuable resource for understanding the optical effects of solar eclipses.
Further detailed studies and data tables are available in the original report.