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Hudson, H.; Levan, P.; Lindsey, C.
California Univ., San Diego, La Jolla (USA). Dept. of Physics1979
California Univ., San Diego, La Jolla (USA). Dept. of Physics1979
AbstractAbstract
[en] The far-infrared wavelengths (10 microns to 1 mm) were used to study the spatial and temporal structure of the solar atmosphere. Observational results were obtained on flares, faculae, sunspots, and on the center-to-limb intensity distribution, as well as on time variability within these regions. A program of precise monitoring of slow variations in the integrated solar luminosity was shown to be feasible, and initial steps to implement observations were completed
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Mar 1979; 33 p; Available from NTIS., PC A03/MF A01
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