In 1802, William Wollaston noned that the spectrum of sunlight did not appear to be a continious band of colors, but quite a had a series of grisly lines superimposed on it. Wollaston attributed the lines to natural boundaries between colors. Joseph Fraunhofer made a more careful posit of observations of the solar spectrum in 1814 and found some 600 dark lines, and he specifically measured the wavelenght of 324 of them. umteen a(prenominal) of the Fraunhofer lines in the solar spectrum defend the n...If you want to get a full essay, order it on our website: Ordercustompaper.com
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