The Vertical Distribution of Ozone Between 35 and 55 Km as Determined from Satellite Ultraviolet Measurements PDF Download
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Author: Gail P. Anderson
Publisher:
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Category : Ozone layer
Languages : en
Pages : 114
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Book Description
Author: Gail P. Anderson
Publisher:
ISBN:
Category : Ozone layer
Languages : en
Pages : 114
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Book Description
Author:
Publisher:
ISBN:
Category : Aeronautics
Languages : en
Pages : 700
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Book Description
Lists citations with abstracts for aerospace related reports obtained from world wide sources and announces documents that have recently been entered into the NASA Scientific and Technical Information Database.
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Category : Artificial satellites
Languages : en
Pages : 96
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Author: William B. Grant
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Category : Science
Languages : en
Pages : 454
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Author:
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ISBN:
Category : Aeronautics
Languages : en
Pages : 460
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Author:
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ISBN:
Category :
Languages : en
Pages : 48
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Book Description
A satellite experiment to determine both the vertical distribution of ozone above 70 km and the radiance of the atmosphere at the center of the Hartley absorption band of ozone at 2550 Angstroms is described. Two flights of the experiment were made successfully, resulting in measurement of the vertical distribution between 60 and 85 km and of the radiance at the nadir for sun angles from 90 to about 49 degrees. The vertical distribution data agree with previous results below 70 km and with theory to 85 km. The radiance, which was not measured previously, is observed to have a maximum value of 2.0 times 10 to the 9th w/sq cm-sr-Angstroms for a solar zenith angle of 49 degrees.
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Category : Climatology
Languages : en
Pages : 340
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Author: University of Colorado. Dept. of Astro-Geophysics
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Category : Astrophysics
Languages : en
Pages : 620
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Author:
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Category :
Languages : en
Pages : 94
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Author: R. D. Rawcliffe
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ISBN:
Category :
Languages : en
Pages : 12
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Book Description
A satellite-borne radiometer has been used to determine the vertical distribution of ozone at high altitudes. The attenuation, due to the ozone, of solar ultraviolet radiation passing obliquely through the atmosphere was measured at times of sunrise and sunset(as seen by the orbit ing vehicle). The sensor employed a photomulti plier tube and filter combination plus a quartz light pipe that allowed a uniformly sensitive field of view of =10 deg in elevation and 350 deg in azimuth. A transition from full sunlight to signal extinction, or vice versa, occurred in a period of about 20 seconds, twice per orbit. The shape of this step has been analyzed with a 7090 computer program to deduce the vertical ozone distribution at altitudes above the maximum. The orbital parameters were such that sunset and sun rise occurred when the vehicle was near 33 de grees S and 13 degrees S latitudes, respectively. (Au.
