In 1802, William Wollaston noted that the spectrum of sunlight did not appear to be a continious ban d of colors, but rather had a series of begrimed lines superimposed on it. Wollaston attributed the lines to natural boundaries between colors. Joseph Fraunhofer made a more careful set of observations of the solar spectrum in 1814 and undercoat some 600 dark lines, and he specifically measured the wavelenght of 324 of them. umpteen a(prenominal) of the Fraunhofer lines in the solar spectrum retain the n...If you want to get a full essay, order it on our website: OrderCustomPaper.com
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