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  • 1
    Electronic Resource
    Electronic Resource
    [s.l.] : Nature Publishing Group
    Nature 238 (1972), S. 447-448 
    ISSN: 1476-4687
    Source: Nature Archives 1869 - 2009
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Notes: [Auszug] These observations have been made with the Coude spectro-graph of the McDonald Observatory 268 cm (107 inch) reflector at a dispersion of 0.119 Å/mm (8.4 mm/Å). The rapid spectrum scanner (R. G. Tully, unpublished manuscript) was used in the pulse-counting, echelle mode with GaAs ...
    Type of Medium: Electronic Resource
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  • 2
    Publication Date: 1972-08-01
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Springer Nature
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  • 3
    Publication Date: 2011-08-16
    Description: Mars atmospheric water vapor detection during Southern Hemisphere spring and summer season
    Keywords: SPACE SCIENCES
    Type: ; YAL SOCIETY (
    Format: text
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  • 4
    Publication Date: 2011-08-16
    Description: Venus carbon dioxide band, deriving rotational temperatures at various phase angles
    Keywords: SPACE SCIENCES
    Type: ; ADEMIE DES SCIENCES
    Format: text
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  • 5
    Publication Date: 2011-08-16
    Description: Venus carbon dioxide spectrum, observing spatial and temporal variation in abundance
    Keywords: SPACE SCIENCES
    Type: ; 679-720. (
    Format: text
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  • 6
    Publication Date: 2011-08-16
    Description: Venus spectra 10488 A carbon dioxide band from high dispersion spectroscopy
    Keywords: SPACE SCIENCES
    Type: ; YAL SOCIETY (
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  • 7
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    In:  Other Sources
    Publication Date: 2011-08-16
    Description: Molecular oxygen has been detected spectroscopically in the atmosphere of Mars, using lines in the 7620 A A-band. Weak lines in the wings of the strong terrestrial atmospheric oxygen transitions show equivalent widths of 2 to 4 mA. Positive identification of the Martian atmosphere as the source of these lines is based on the facts that four separate lines are resolved, each line has been observed repeatedly, in each case falling at the appropriate predicted Doppler-shifted wavelength with an accuracy of plus or minus 0.01 A, all four lines are of similar strength as predicted by theory, and the observed lines are not solar Fraunhofer lines.
    Keywords: SPACE SCIENCES
    Type: Nature; 238; Aug. 25
    Format: text
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  • 8
    Publication Date: 2018-06-11
    Description: There have been extensive optical surveys for debris at geosynchronous orbit (GEO) conducted with meter-class telescopes, such as those conducted with MODEST (the Michigan Orbital DEbris Survey Telescope, a 0.6-m telescope located at Cerro Tololo in Chile), and the European Space Agency's 1.0-m space debris telescope (SDT) in the Canary Islands. These surveys have detection limits in the range of 18th or 19th magnitude, which corresponds to sizes larger than 10 cm assuming an albedo of 0.175. All of these surveys reveal a substantial population of objects fainter than R = 15th magnitude that are not in the public U.S. Satellite Catalog. To detect objects fainter than 20th magnitude (and presumably smaller than 10 cm) in the visible requires a larger telescope and excellent imaging conditions. This combination is available in Chile. NASA's Orbital Debris Program Office has begun collecting orbital debris observations with the 6.5-m (21.3-ft diameter) "Walter Baade" Magellan telescope at Las Campanas Observatory. The goal is to detect objects as faint as possible from a ground-based observatory and begin to understand the brightness distribution of GEO debris fainter than R = 20th magnitude.
    Keywords: Optics; Space Transportation and Safety
    Type: ARES Biennial Report 2012 Final; 77-80; JSC-CN-30442
    Format: application/pdf
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  • 9
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    In:  Other Sources
    Publication Date: 2019-06-27
    Description: Analysis of spectroscopic observations of Mars requires values of the effective Martian airmass to obtain true abundances. Semi-arbitrary assumptions for the airmass correction have been used in most of the past publications on the subject. We have computed detailed values corresponding to specified slits superimposed on the disk of the planet, giving useful output in the form of curves presenting the average airmass for different regions of the planet and various conditions of planet diameter, seeing and phase angle.
    Keywords: SPACE SCIENCES
    Type: Icarus; 19; May 1973
    Format: text
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  • 10
    Publication Date: 2019-07-27
    Description: Defining the risks present to both crewed and robotic spacecrafts is part of NASA s mission, and is critical to keep these resources out of harm s way. Characterizing orbital debris is an essential part of this mission. We present a proof-of-concept study that employs multiple techniques to demonstrate the efficacy of each approach. The targets of this study are IDCSPs (Initial Defense Communications Satellite Program). 35 of these satellites were launched by the US in the mid-1960s and were the first US military communications satellites in the GEO regime. They were emplaced in slightly sub-synchronous orbits. These targets were chosen for this proof-of-concept study for the simplicity of their observable exterior surfaces. The satellites are 26-sided polygons (86cm in diameter), initially spin-stabilized, and covered on all sides in solar panels. Data presented here include: (a) visible broadband photometry (Johnson/Kron-Cousins BVRI) taken with the 0.9m SMARTs telescope (Small and Medium Aperture Telescopes) at the Cerro Tololo Inter-American Observatory (CTIO) in Chile in April, 2012, (b) laboratory broadband photometry (Johnson/ Bessell BVRI) of solar cells, obtained using the Optical Measurements Center (OMC) at NASA/JSC [1], (c) visible-band spectra taken using the Magellan 6.5m Baade Telescope at Las Campanas Observatory in Chile in May, 2012 [2], and (d) visible-band laboratory spectra of solar cells using an ASD Field Spectrometer. Color-color plots using broadband photometry (e.g. B-R vs. B-V) demonstrate that different material types fall into distinct areas on the plots [1]. Spectra of the same material types as those plotted in the color-color plots each display their own signature as well. Here, we compare lab data with telescopic data, and photometric results with spectroscopic results. The spectral response of solar cells in the visible wavelength regime varies from relatively flat to somewhat older solar cells whose reflectivity can be gently or sharply peaked in the blue. With a target like IDCSPs, the material type is known a priori, aiding in understanding how material type affects one s observations.
    Keywords: Space Transportation and Safety
    Type: JSC-CN-27060 , 13 annual Advanced Maui Optical and Space Surveillance Technologies (AMOS) Conference; 11 - 14 Sept 2012; Kihei, HI; United States
    Format: application/pdf
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