Line width of the solar EUV He I resonance emissions at 584 and 537 A

Details Line width of the solar EUV He I resonance emissions at 584 and 537 A Line width of the solar EUV He I resonance emissions at 584 and 537 A

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.7537o&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, Sept. 1, 1984, p. 7537-7540.

Physics

12

Extreme Ultraviolet Radiation, Helium, Resonance Lines, Solar Spectra, Emission Spectra, Rocket-Borne Instruments, Solar Activity Effects, Spectral Line Width, Stellar Spectrophotometry

Scientific paper

Instrumentation was carried aloft on a Black Brant rocket in August 1982 to gather spectrometry on the solar He I resonance lines. The payload consisted of a He spectrometer which furnished 11 readings at FWHM of close to 97 and 132 mA for the 584 and 537 a lines, respectively. The results indicated a variation of the solar line width that was inversely correlated with solar activity and with the solar EUV flux. Further studies of the 522 A line are recommended to detect any unidentified first order solar emissions close to or within the absorption profile of the 537 A line that contributed to the observed line width.

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