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  • Inorganic Chemistry  (7,628)
  • SPACE RADIATION  (2,685)
  • 2025-2025
  • 2020-2023
  • 1975-1979  (4,476)
  • 1970-1974  (5,837)
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  • 1
    Publication Date: 2019-08-28
    Keywords: SPACE RADIATION
    Type: NASA-TT-F-14312
    Format: text
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  • 2
    Publication Date: 2019-08-28
    Description: Secondary heating and ionization of the intergalactic gas at redshifts z approximately 10-30 could lead to the large optical depth of the Universe for Thomson scattering and could smooth the primordial fluctuations formed at z approximately 1500. It is shown that the gas motions connected with the large scale density perturbations at z approximately 10-15 must lead to the generation of secondary fluctuations of microwave background. The contribution of the rich clusters of galaxies and young galaxies to the fluctuations of microwave background is also estimated.
    Keywords: SPACE RADIATION
    Type: NASA-TM-75619
    Format: application/pdf
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  • 3
    Publication Date: 2019-08-28
    Description: The progress made and techniques used by the Soviet-French group in the study of gamma and X ray pulses are described in abstracts of 16 reports. Experiments included calibration and operation of various recording instruments designed for measurements involving these pulses, specifically the location of sources of such pulses in outer space. Space vehicles are utilized in conjunction with ground equipment to accomplish these tests.
    Keywords: SPACE RADIATION
    Type: NASA-TM-75050
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  • 4
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    In:  Other Sources
    Publication Date: 2019-08-28
    Description: Approved NASA cosmic ray programs for the next five years are reviewed. In deep space, four new missions are planned. The first two, Helios A and B, will go inwards to approximately 0.3 AU, and the second two, Mariner Jupiter-Saturn, will go outwards to Saturn at 9.5 AU. Two missions in the earth orbital program promise to provide major new information on cosmic ray isotopes and on very heavy cosmic rays. These are the C mission of the International Sun-Earth Explorer, and the C mission of the High Energy Astronomy Observatory. The balloon research program is also mentioned.
    Keywords: SPACE RADIATION
    Type: ESA Res. Goals for Cosmic-Ray Astrophys. in the 1980's; p 47-49
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  • 5
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    In:  CASI
    Publication Date: 2019-08-28
    Description: Articles pertaining to the solar studies and the Skylab program are presented, with emphasis on the usefulness of the Apollo Telescope Mount (ATM) program. A description of Skylab objectives and key mission events is included along with articles about the sun. Skylab solar studies which are reported include these topics: ATM solar observatory, scientific instruments, crew operations and crew training, and the joint observing program. The Skylab associated solar programs are also reported.
    Keywords: SPACE RADIATION
    Type: NASA-EP-119
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  • 6
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    In:  CASI
    Publication Date: 2019-08-28
    Description: An up-to-date textbook of solar physics is presented. The solar structure and processes, and the interior are described along with the photosphere, the chromosphere, and the corona. The strongest Fraunhofer lines, visible coronal lines, and coronal UV, XUV, and X-ray lines are listed.
    Keywords: SPACE RADIATION
    Type: NASA-SP-303 , LC-72-600092
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  • 7
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    In:  Other Sources
    Publication Date: 2019-08-28
    Description: Particle and cosmic ray physics, X ray and gamma ray astronomy, and satellite, rocket, and balloon sounding
    Keywords: SPACE RADIATION
    Type: REPT. TO COSPAR, FRENCH SPACE PROGRAM FEB. 1970; P 47-63
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  • 8
    Publication Date: 2019-08-28
    Description: The simulated cosmic radiation effect on a spacecraft structure is evaluated by gamma ray testing in relation to structural thickness. A drawing of the test set-up is provided and measurement errors are discussed.
    Keywords: SPACE RADIATION
    Type: NASA-TM-75053
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  • 9
    Publication Date: 2019-08-28
    Description: Besides the identified sources of cosmic pulse X-ray radiation with globular clusters NGC 6624, NGC 1851 and MXB 1730-335 several new identifications were made. The source in Norma was probably identified with globular cluster NGC 5927, the source in Aquila with globular cluster NGC 6838 (M71), and the source in Puppis with globular cluster NGC 2298. Gamma pulses discovered by the Vela satellites and X-ray pulses thoroughly measured by the SAS-3, Ariel-5, and ANS satellites are thought to be the same phenomenon. The sources of such a radiation must be some kind of peculiarity at the central part of globular clusters; it is most probably a massive black hole. The sources of hard pulse radiation which cannot be identified with globular clusters are considered to be a new kind of galactic object, invisible globular clusters, which are naked nuclei of globular clusters.
    Keywords: SPACE RADIATION
    Type: NASA-TM-75561 , PR-280
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  • 10
    Publication Date: 2019-08-28
    Description: Values for solar constant and solar spectral irradiance based on air and spaceborne observations for use in design of spacecraft, space vehicles, subsystems, and experiments
    Keywords: SPACE RADIATION
    Type: NASA-SP-8005-REV
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