Techniques of observation and critical discussion of XUV emission

Details Techniques of observation and critical discussion of XUV emission Techniques of observation and critical discussion of XUV emission

Jun 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..239l&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, June 1977, p. 239-252. In Italian.

Astronomy and Astrophysics

Astronomy

Far Ultraviolet Radiation, Solar Flares, Solar Instruments, Solar X-Rays, Ultraviolet Astronomy, X Ray Astronomy, Astronomical Photometry, Energy Budgets, Solar Spectra, Spaceborne Astronomy, Temperature Distribution

Scientific paper

The paper reviews techniques for the observation of XUV emission from solar flares; emphasis is placed on spaceborne measurements (e.g., from Skylab, the OSO satellites, the Explorer satellites, the Helios spacecraft, etc.) using such instruments as photomultipliers, X-ray spectroheliographs, mapping heliometers, etc. Methods for extracting information on flare density and temperature from XUV data are considered. A flare-temperature model is constructed and its implications for the study of flare energy-balance are discussed.

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