Celestial infrared calibration sources in the 8-14 micrometer region : Venus and Jupiter / Thomas E. Cecil [and others]
Venus and Jupiter are often used as long wavelength infrared (LWIR) calibration sources. The authors have reviewed the literature on radiometric and spectrometric measurements of these two planets and adopted reasonable brightness temperatures and spectral dependencies for their thermal radiation. U...
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| Other title: | Celestial infrared calibration sources in the eight to fourteen micrometer region : Venus and Jupiter. |
| Format: | Government Document Book |
| Language: | English |
| Published: |
L.G. Hanscom Field, Mass. :
Air Force Cambridge Research Laboratories, Air Force Systems Command, United States Air Force,
1973.
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| Series: | AFCRL-TR (Series) ;
73-559. Physical sciences research papers (Air Force Cambridge Research Laboratories (U.S.)) ; no. 562. |
| Subjects: |
MARC
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| 245 | 0 | 0 | |a Celestial infrared calibration sources in the 8-14 micrometer region : |b Venus and Jupiter / |c Thomas E. Cecil [and others] |
| 246 | 3 | |a Celestial infrared calibration sources in the eight to fourteen micrometer region : |b Venus and Jupiter. | |
| 260 | |a L.G. Hanscom Field, Mass. : |b Air Force Cambridge Research Laboratories, Air Force Systems Command, United States Air Force, |c 1973. | ||
| 300 | |a 18 pages : |b illustrations ; |c 28 cm. | ||
| 336 | |a text |b txt |2 rdacontent. | ||
| 337 | |a unmediated |b n |2 rdamedia. | ||
| 338 | |a volume |b nc |2 rdacarrier. | ||
| 490 | 1 | |a AFCRL-TR ; |v 73-559. | |
| 490 | 1 | |a Physical Sciences Research Papers ; |v No. 562. | |
| 500 | |a "5 September 1973." | ||
| 500 | |a AD0772660 (From http://www.dtic.mil) | ||
| 500 | |a Terrestrial Sciences Laboratory Project 7670. | ||
| 500 | |a Research supported by the Air Force Cambridge Research Laboratories, Air Force Systems Command, United States Air Force, L.G. Hanscom Field, Bedford, Massachusetts. | ||
| 504 | |a Includes bibliographical references (pages 17-18) | ||
| 520 | |a Venus and Jupiter are often used as long wavelength infrared (LWIR) calibration sources. The authors have reviewed the literature on radiometric and spectrometric measurements of these two planets and adopted reasonable brightness temperatures and spectral dependencies for their thermal radiation. Using these data, irradiance coefficients that can be used to determine the irradiance reaching the earth from these planets at any time were calculated. A crucial factor in the utility of these planets as calibration sources is the constancy with which they radiate in the infrared. The authors conclude that Jupiter may be a variable source. Venus, on the other hand, appears to be generally quite constant, but brief temporal variations may take place. | ||
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| 650 | 0 | |a Infrared spectra. |0 http://id.loc.gov/authorities/subjects/sh85066328. | |
| 650 | 0 | |a Infrared radiation. |0 http://id.loc.gov/authorities/subjects/sh85066322. | |
| 650 | 0 | |a Infrared equipment |x Calibration. |0 http://id.loc.gov/authorities/subjects/sh2010006957. | |
| 651 | 0 | |a Venus (Planet) |0 http://id.loc.gov/authorities/subjects/sh85142768. | |
| 651 | 0 | |a Jupiter (Planet) |0 http://id.loc.gov/authorities/subjects/sh85071063. | |
| 650 | 7 | |a Venus atmosphere. |2 nasat. | |
| 650 | 7 | |a Jupiter atmosphere. |2 nasat. | |
| 700 | 1 | |a Cecil, T. E. |q (Thomas E.), |d 1945- |0 http://id.loc.gov/authorities/names/n84144039 |1 http://isni.org/isni/0000000109318152. | |
| 710 | 2 | |a Air Force Cambridge Research Laboratories (U.S.) |0 http://id.loc.gov/authorities/names/n81133515 |1 http://isni.org/isni/0000000121678046. | |
| 830 | 0 | |a AFCRL-TR (Series) ; |v 73-559. |0 http://id.loc.gov/authorities/names/no2011130362. | |
| 830 | 0 | |a Physical sciences research papers (Air Force Cambridge Research Laboratories (U.S.)) ; |v no. 562. |0 http://id.loc.gov/authorities/names/no2008179573. | |
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