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The theory of line shapes relevant to the spectra of cool stars

✍ Scribed by G. Peach; I.B. Whittingham


Publisher
Elsevier Science
Year
2009
Tongue
English
Weight
166 KB
Volume
53
Category
Article
ISSN
1387-6473

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A comparison of these with observational data lot the 1973 December 17 solar flare, obtained by the Naval Research Laboratory's $082A and S082B spectrographs on board AYolab, reveals reasonably good agreement between theory and observation tot/r [= I(242.07 J'\)/I(1354.08 ,.' ~.)q\_.. which provides