Light coming up from the centre of the Sun goes through the outer layer where it encounters absorbtion by elements in the outer layer, and this gives rise to absorbtion lines in the spectrum.
It is the coolest layer of the Sun's atmosphere and when looking through it, you can see absorption spectrum lines.
absorption lines due to the thin outer layer above the photosphere
absorption lines! :)
Atoms in the atmosphere of the star is responsible for the dark lines in its spectrum.
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It is the coolest layer of the Sun's atmosphere and when looking through it, you can see absorption spectrum lines.
absorption lines due to the thin outer layer above the photosphere
Absorption lines
An emission spectrum depend on electrons transition in the atom of a chemical element; and elements are different.Absorption spectrum is based on the different absorption pics of different molecules, depending on the frequency of radiation.Spectral methods are largely used in analytical chemistry.
absorption lines! :)
Dark lines especially in solar spectrum have been named as Fraunhofer lines. These line are good examples for line absorption spectrum
Atoms in the atmosphere of the star is responsible for the dark lines in its spectrum.
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The dark lines are absorption spectrum, the energy absorbed by Atoms in the atmosphere of the star. ================================ Fraunhofer's spectral lines.
A band spectrum is an absorption or emission spectrum consisting of bands of closely-spaced lines, characteristic of polyatomic molecules.
A band spectrum is an absorption or emission spectrum consisting of bands of closely-spaced lines, characteristic of polyatomic molecules.
The absorption lines in the infrared portion of the spectrum of a star that are produced by hydrogen are from the Balmer series. The Balmer series were discovered by Johann Balmer in 1885.