A spectroscopic method for calibration of solar extreme ultraviolet instrumentation

Details A spectroscopic method for calibration of solar extreme ultraviolet instrumentation A spectroscopic method for calibration of solar extreme ultraviolet instrumentation

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...128..181n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 128, no. 1, Nov. 1983, p. 181-189.

Astronomy and Astrophysics

Astronomy

32

Calibrating, Extreme Ultraviolet Radiation, Solar Corona, Solar Instruments, Solar Spectra, Ultraviolet Spectroscopy, Oso-5, Plasma Diagnostics, Satellite-Borne Instruments, Solar Spectrometers, Spaceborne Astronomy

Scientific paper

A method of calibrating solar extreme ultraviolet spectrographs in space using coronal emission lines of known relative intensity is presented and demonstrated. This approach is useful for recalibrating orbiting instruments that may be subject to degradation during extended periods of operation. The calibration results are insensitive to the physical distribution of emitting plasma in any likely solar coronal source. It is suggested that this technique may be useful for calibration of spectrographs used in the study of laboratory plasmas.

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