Scanners & Imagery Systems for Earth Observation: Seminar , August 19-20, 1974, San Diego, CaliforniaSociety of Photo-optical Instrumentation Engineers, 1975 - Astronautics in earth sciences - 148 pages |
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Page 33
... Table 2 from Reference 1 to illustrate typical variations in spatial resolution and time of coverage for some potential remote sensing applications . ( Ref . 1 ) . Some of the information in the original table was deleted so that the table ...
... Table 2 from Reference 1 to illustrate typical variations in spatial resolution and time of coverage for some potential remote sensing applications . ( Ref . 1 ) . Some of the information in the original table was deleted so that the table ...
Page 82
... Table VI also shows results obtained using the cosine transformation C ( 43 ° ) = ( cos 43 ° / cos 34 ° ) C ( 340 ) . This transformation contains a large part of the variation due to a change in solar angle since it accounts for the ...
... Table VI also shows results obtained using the cosine transformation C ( 43 ° ) = ( cos 43 ° / cos 34 ° ) C ( 340 ) . This transformation contains a large part of the variation due to a change in solar angle since it accounts for the ...
Page 134
... Table 2 presents this data assuming diffraction limited per- formance at lum , a 20 urad IFOV , and the 85 % criterion ( 90 % requires larger apertures ) . TABLE 2 Linear Obscuration ( % ) Diameter ( cm ) f / # than 100 nm , but greater ...
... Table 2 presents this data assuming diffraction limited per- formance at lum , a 20 urad IFOV , and the 85 % criterion ( 90 % requires larger apertures ) . TABLE 2 Linear Obscuration ( % ) Diameter ( cm ) f / # than 100 nm , but greater ...
Contents
ww | 14 |
Feasibility of an Instrument for 15 Micrometer Mesoscale Geosynchronous Inversion | 21 |
SCANNING SYSTEMS FOR THE EARTH OBSERVATION SATELLITE | 31 |
Copyright | |
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Common terms and phrases
absorption aircraft albedo altitude applications atmos atmospheric effects calculated calibration Center changes channel clouds computed correction coverage curves detector array earth observation Earth Resources error ERTS ESMR-F factor flight haze level IFOV image surface infrared instrument lunar lunar mare Mare Serenitatis measured ment method microradians mirror multispectral multistage sampling nadir radiance NASA Nimbus noise obtained operational optical depth optical thickness orbit parameters particulates path radiance payload percent performance phase angle photodiode radi radiation radiometer radiosonde RAOB ratio remote sensing resolution response roof wheel sample satellite scan angle scanner scattering sensor development SESMR shown in Figure Shuttle Skylab solar irradiance solar zenith angle solid-state spacecraft Spacelab spectral bands SPECTRAL RADIANCE spherical sun angle surface reflectivity Table target reflectivity techniques temperature profile thermal tion total radiance transformation values variations vertical visual range VTPR wavelength weighting functions