Infrared continuum observations of the solar atmosphere

Physics

Scientific paper

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Far Infrared Radiation, Solar Atmosphere, Luminosity, Solar Flares, Solar Physics, Sunspots

Scientific paper

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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