The paper contains the result description of the photometric observations of the Moon surface during the total lunar eclipse of June, 15, 2011 conducted in southern Russia and Ukraine in three narrow spectral bands with effective wavelengths equal to 503, 677, and 867 nm. The photometric maps of umbra are built, the radial dependencies of relative brightness are compared with the theoretical ones for gaseous atmosphere. Dark anomalies of umbra are shown and related with the aerosol air pollution of the definite regions above the surface of Earth
International audienceContext. An important goal within the quest for detecting an Earth-like extras...
This paper presents the preliminary results of nocturnal Aerosol Optical Depth (τa) and Angström Exp...
[1] The Moon’s changeable aspect during a lunar eclipse is largely attributable to variations in the...
Abstract. The work is devoted to the analysis of the surface photometric observations of two total l...
Abstract. The work contains the description of two narrow IR-bands observational data of total lunar...
Abstract. In this paper we present the high resolution spectral observations of the fragment of luna...
A technique is described for calculating the brightness of the atmosphere of the Earth that shines i...
We report a measurement of lunar spectral irradiance with an uncertainty below 1 % from 420 nm to 10...
During a solar eclipse the solar irradiance reaching the top of the atmosphere (TOA) is reduced in t...
Abstract. The variability of ultraviolet and photosyntheti-cally active radiation (PAR) during the t...
A three-color photometry of the eclipsed moon was carried out with a 12-inch reflector during the to...
During a solar eclipse the solar irradiance reaching the top-of-atmosphere (TOA) is reduced in the M...
Context. Observations of the Earthshine off the Moon allow for the unique opportunity to measure the...
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...
International audienceContext. An important goal within the quest for detecting an Earth-like extras...
This paper presents the preliminary results of nocturnal Aerosol Optical Depth (τa) and Angström Exp...
[1] The Moon’s changeable aspect during a lunar eclipse is largely attributable to variations in the...
Abstract. The work is devoted to the analysis of the surface photometric observations of two total l...
Abstract. The work contains the description of two narrow IR-bands observational data of total lunar...
Abstract. In this paper we present the high resolution spectral observations of the fragment of luna...
A technique is described for calculating the brightness of the atmosphere of the Earth that shines i...
We report a measurement of lunar spectral irradiance with an uncertainty below 1 % from 420 nm to 10...
During a solar eclipse the solar irradiance reaching the top of the atmosphere (TOA) is reduced in t...
Abstract. The variability of ultraviolet and photosyntheti-cally active radiation (PAR) during the t...
A three-color photometry of the eclipsed moon was carried out with a 12-inch reflector during the to...
During a solar eclipse the solar irradiance reaching the top-of-atmosphere (TOA) is reduced in the M...
Context. Observations of the Earthshine off the Moon allow for the unique opportunity to measure the...
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...
International audienceContext. An important goal within the quest for detecting an Earth-like extras...
This paper presents the preliminary results of nocturnal Aerosol Optical Depth (τa) and Angström Exp...
[1] The Moon’s changeable aspect during a lunar eclipse is largely attributable to variations in the...