Fraunhofer lines are produced by the absorpti | vedclass

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(A) Fraunhofer lines are a set of dark absorption lines observed in the solar spectrum. These lines are produced when the continuous spectrum of light

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the chromosphere of the sun

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(A) Fraunhofer lines are a set of dark absorption lines observed in the solar spectrum. These lines are produced when the continuous spectrum of light emitted by the hot, dense core of the sun (the photosphere) passes through the cooler, thinner gases of the solar atmosphere (the chromosphere). The atoms in the chromosphere absorb specific wavelengths of light corresponding to their characteristic energy transitions, resulting in the dark lines observed in the spectrum.

Fraunhofer lines are produced by the absorption of light in

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