Related Experiment Video
Updated: Jun 16, 2026

Measurement of Aerosols Optical Thickness of the Atmosphere using the GLOBE Handheld Sun Photometer
Published on: May 29, 2019
Summary of sky brightness measurements during eclipses of the sun
Abstract:
A selected group of measurements of the sky brightness during total solar eclipses is used to determine a standard light curve during the period from no obscuration to totality. It is found that the sky light may be considered as attenuated sunlight up to at least 99.8% obscuration. During totality, the sky light consists of multiply scattered light from outside the umbral region. The effects of solar elevation angle, cloud cover, and albedo and the variability of the light curve during totality are discussed.
Related Concept Videos
Flame Photometry: Overview
Flame Photometry: Lab
Radiation Pressure: Problem Solving
The average value of the rate of momentum transfer divided by the absorbing area represents the average force per...
Eccentricity of an Ellipse
Calculation of Electric Flux
UV–Vis Spectrometers

