The solar spectrum is an example of

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(D) The solar spectrum consists of a continuous spectrum of light emitted by the hot interior of the Sun,which is crossed by numerous dark lines known

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line absorption spectrum

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(D) The solar spectrum consists of a continuous spectrum of light emitted by the hot interior of the Sun,which is crossed by numerous dark lines known as Fraunhofer lines. These dark lines are produced because the cooler gases in the Sun's outer atmosphere (the photosphere and chromosphere) absorb specific wavelengths of light from the continuous spectrum. Therefore,the solar spectrum is classified as a line absorption spectrum.

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