To illustrate: the gases and vapors forming the outer strata of

the Sun"s atmosphere would in themselves produce bright-line
spectra of the elements involved
To illustrate: the gases and vapors forming the outer strata of
the Sun"s atmosphere would in themselves produce bright-line
spectra of the elements involved. If these gases and vapors
could in effect be removed, without changing underlying
conditions, the remaining condensed body of the Sun should have
a continuous spectrum. The cooler overlying gases and vapors
absorb those radiations from the deeper and hotter sources
which the gases and vapors would themselves emit, and thus form
the dark-line spectrum of the Sun. The stretches of spectrum
between the dark lines are of course continuous-spectrum
radiations.


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