Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986spie..689..224n&link_type=abstract
IN: X-ray calibration: Techniques, sources, and detectors; Proceedings of the Meeting, San Diego, CA, Aug. 19, 20, 1986 (A88-126
Astronomy and Astrophysics
Astronomy
1
Calibrating, Extreme Ultraviolet Radiation, Solar Instruments, Ultraviolet Astronomy, Chromosphere, Equipment Specifications, Line Spectra, Microwave Emission, Solar Corona, Solar Radiation
Scientific paper
Accurate measurements of the Sun's extreme ultraviolet (EUV) emission are of major importance in aeronomical studies of the Earth's upper atmosphere and for studies of the Sun's outer atmosphere, where the radiation originates in the tenuous, high-temperature chromosphere and corona. Current levels of calibration accuracy of space instrumentation used to observe this radiation and accuracies desired in the future are discussed. Several suggestions are made for methods that can provide approximate recalibrations of instruments in orbit using the radiation from the Sun itself.
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