In 1802, William Wollaston noted that the spectrum of sunlight did not appear to be a continious band of colors, but rather had a serial publication of p uritanic lines superimposed on it. Wollaston attributed the lines to natural boundaries between colors. Joseph Fraunhofer make a more careful set of observations of the solar spectrum in 1814 and found some 600 dark lines, and he specifically measurable the wavelenght of 324 of them. umteen of the Fraunhofer lines in the solar spectrum retain the not...If you want to expire a full essay, order it on our website: OrderEssay.net
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