AIP Conference Proceedings 2009
DOI: 10.1063/1.3137703
|View full text |Cite
|
Sign up to set email alerts
|

UV Radiation from the Night-Time Atmosphere seen from the “Universitetsky-Tatiana” Satellite

Abstract: Articles you may be interested inA readout for large arrays of microwave kinetic inductance detectors Rev. Sci. Instrum. 83, 044702 (2012); 10.1063/1.3700812 HIRDES-The main instrument of the WSO/UV satellite AIP Conf.Characterization and real-time optical measurements of the ionizing radiation dose response for a new radiochromic medium Med.Abstract. Detectors on the "Universitetsky-Tatiana" satellite measured a smoothly varying intensity of UV radiation from the night-time atmosphere in the nadir direction a… Show more

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1

Citation Types

0
3
0

Year Published

2010
2010
2017
2017

Publication Types

Select...
3
2

Relationship

1
4

Authors

Journals

citations
Cited by 5 publications
(3 citation statements)
references
References 7 publications
0
3
0
Order By: Relevance
“…Tatiana data on the electron flux at the orbit allow comparison of the latitude profiles of electron flux and profiles of UV radiation. In auroral zone the position of UV intensity is correlated to electron intensity at the Tatiana orbit, if movement of electron to its track end in the atmosphere along the geomagnetic field is taken into account [ Dmitriev et al , 2009].…”
Section: Results Of the Universitetsky–tatiana Missionmentioning
confidence: 99%
“…Tatiana data on the electron flux at the orbit allow comparison of the latitude profiles of electron flux and profiles of UV radiation. In auroral zone the position of UV intensity is correlated to electron intensity at the Tatiana orbit, if movement of electron to its track end in the atmosphere along the geomagnetic field is taken into account [ Dmitriev et al , 2009].…”
Section: Results Of the Universitetsky–tatiana Missionmentioning
confidence: 99%
“…This perturbation was considerate as background noise in the tracking of the original particle. The high brightness of TLE may allow us to use the simplest pinhole optics for measuring the image in pixels of UV detector [5,6]. The optimal imaging quality in a pinhole camera is achieved if the hole size is equal to the detector pixel size.…”
Section: Pinhole Cameramentioning
confidence: 99%
“…The UV detector [1] consists of a very small scintillator plastic as first transducer, see figure 1. Scintillation detectors make use of special materials, when exposed to ionizing radiation, they emit a small flash of light.…”
Section: Ultraviolet Radiation Detector Setupmentioning
confidence: 99%