Investigation on the Spectral Intensity of Ultraviolet Sky Radiation Under Various Conditions at 1590 M A.s.l PDF Download
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Author: Paul Bener
Publisher:
ISBN:
Category :
Languages : en
Pages : 24
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Book Description
Author: Paul Bener
Publisher:
ISBN:
Category :
Languages : en
Pages : 24
Get Book Here
Book Description
Author: Paul Bener
Publisher:
ISBN:
Category :
Languages : en
Pages : 24
Get Book Here
Book Description
Author: Paul Bener
Publisher:
ISBN:
Category : Atmospheric radiation
Languages : en
Pages : 24
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Book Description
Author: PA. BENER
Publisher:
ISBN:
Category :
Languages : en
Pages : 1
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Book Description
Author: Paul Bener
Publisher:
ISBN:
Category :
Languages : en
Pages : 136
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Book Description
Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 1
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Book Description
The results are presented of extended records of the spectral distribution of ultraviolet solar and sky radiation in the spectral region between 295 millimicrons and 370 millimicrons. The records were obtained with a recording spectrometer consisting of a double monochromator combined with a photomultiplier and a recorder. A diffuser sphere was applied as receiver for the incoming radiation to obtain measurements following the cosine law. Diagrams showing the spectral intensity as a function of wavelength, solar altitude and amount of atmospheric ozone are presented. Up to 330 millimicrons the spectral intensity of ultraviolet sky and global radiation increases rapidly because of diminishing ozone absorption; this increase covers between wavelengths of 297.5 millimicrons and 330 millimicrons several orders of magnitude. No considerable change of spectral intensity is observed in the wavelength region between 330 millimicrons and 370 millimicrons. The effect of ozone increase from 0.200 cm to 0.300 cm on the spectral intensity of ultraviolet sky radiation corresponds for 300 millimicrons to a diminuation of intensity by factors varying between 3, 5 and 16, depending on solar altitude. The corresponding variation in the case of global radiation amounts to factors between 8 and 16. (Author).
Author: Paul Bener
Publisher:
ISBN:
Category : Solar radiation
Languages : en
Pages : 1
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Book Description
The results are presented of extended records of the spectral distribution of ultraviolet solar and sky radiation in the spectral region between 295 millimicrons and 370 millimicrons. The records were obtained with a recording spectrometer consisting of a double monochromator combined with a photomultiplier and a recorder. A diffuser sphere was applied as receiver for the incoming radiation to obtain measurements following the cosine law. Diagrams showing the spectral intensity as a function of wavelength, solar altitude and amount of atmospheric ozone are presented. Up to 330 millimicrons the spectral intensity of ultraviolet sky and global radiation increases rapidly because of diminishing ozone absorption; this increase covers between wavelengths of 297.5 millimicrons and 330 millimicrons several orders of magnitude. No considerable change of spectral intensity is observed in the wavelength region between 330 millimicrons and 370 millimicrons. The effect of ozone increase from 0.200 cm to 0.300 cm on the spectral intensity of ultraviolet sky radiation corresponds for 300 millimicrons to a diminuation of intensity by factors varying between 3, 5 and 16, depending on solar altitude. The corresponding variation in the case of global radiation amounts to factors between 8 and 16. (Author).
Author: Paul Bener
Publisher:
ISBN:
Category :
Languages : en
Pages :
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Author: Ann R Webb
Publisher: CRC Press
ISBN: 9789056991210
Category : Science
Languages : en
Pages : 116
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Book Description
An excellent summary of solar UV measurement for anyone involved in, or contemplating, measuring the UV part of the solar spectrum. The book is addressed predominantly to the newcomer to this expanding area of environmental measurement, but contains sufficient detail and practical information to be a valuable reference for the more experienced worker. The practical considerations of solar UV measurement are clearly described and the book explores the current state of the art of UV monitoring, explained by the historical demand for data. The many applications of solar UV data are discussed and the importance of making appropriate measurements and collecting sufficient supporting data for the analysis required of these applications is highlighted.
Author: Paul Bener
Publisher:
ISBN:
Category : Atmospheric ozone
Languages : en
Pages : 72
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Book Description
