A technique is described for calculating the brightness of the atmosphere of the Earth that shines into the Earth’s umbra during a total lunar eclipse making the Moon red. This ‘Rim of Fire’ is due to refracted un scattered light from all the sunrises and sunsets rimming the Earth. In this article, a photograph of the totally eclipsed Moon was compared with the Full Moon and the difference in brightness calculated taking into account the exposure time and ISO setting. The results show that the Full Moon is over 14 000 times brighter than the totally eclipsed Moon. The relative brightness of the eclipsed Moon can be used to estimate that the luminance of Rim of Fire is over 12 trillion watts. The experiment described in this paper would be s...
During a solar eclipse the solar irradiance reaching the top of the atmosphere (TOA) is reduced in t...
We have used the large database of photometric observations of the bright and dark portions of the f...
The paper contains the result description of the photometric observations of the Moon surface during...
A technique is described for calculating the brightness of the atmosphere of the Earth that shines i...
We present a simple method to estimate the size of Earth’s umbral shadow in a classroom setting. The...
A model based on celestial geometry and atmospheric physics predicts the dimming and the color of lu...
First place in the 2021 IAU OAE Astrophotography Contest, category Total lunar eclipse. A lunar ecl...
Aims. “Earthshine ” is the dim light seen on the otherwise dark side of the Moon, particularly when ...
Aims. “Earthshine” is the dim light seen on the otherwise dark side of the Moon, particularly when i...
In a total solar eclipse, the Moon completely covers the Sun, casting a shadow several hundred km wi...
A three-color photometry of the eclipsed moon was carried out with a 12-inch reflector during the to...
The writer measured the brightness of the Moon during the January 21, 2019 total lunar eclipse. He ...
The Moon appears to be much larger closer to the horizon than when higher in the sky. This is called...
During a solar eclipse the solar irradiance reaching the top-of-atmosphere (TOA) is reduced in the M...
The Moon's brightness during a lunar eclipse is indicative of the composition, cloudiness and aeroso...
During a solar eclipse the solar irradiance reaching the top of the atmosphere (TOA) is reduced in t...
We have used the large database of photometric observations of the bright and dark portions of the f...
The paper contains the result description of the photometric observations of the Moon surface during...
A technique is described for calculating the brightness of the atmosphere of the Earth that shines i...
We present a simple method to estimate the size of Earth’s umbral shadow in a classroom setting. The...
A model based on celestial geometry and atmospheric physics predicts the dimming and the color of lu...
First place in the 2021 IAU OAE Astrophotography Contest, category Total lunar eclipse. A lunar ecl...
Aims. “Earthshine ” is the dim light seen on the otherwise dark side of the Moon, particularly when ...
Aims. “Earthshine” is the dim light seen on the otherwise dark side of the Moon, particularly when i...
In a total solar eclipse, the Moon completely covers the Sun, casting a shadow several hundred km wi...
A three-color photometry of the eclipsed moon was carried out with a 12-inch reflector during the to...
The writer measured the brightness of the Moon during the January 21, 2019 total lunar eclipse. He ...
The Moon appears to be much larger closer to the horizon than when higher in the sky. This is called...
During a solar eclipse the solar irradiance reaching the top-of-atmosphere (TOA) is reduced in the M...
The Moon's brightness during a lunar eclipse is indicative of the composition, cloudiness and aeroso...
During a solar eclipse the solar irradiance reaching the top of the atmosphere (TOA) is reduced in t...
We have used the large database of photometric observations of the bright and dark portions of the f...
The paper contains the result description of the photometric observations of the Moon surface during...