Double source interference. Laser light through two closely spaced slits.
Multiple source interference. Laser light through a diffraction grating.
Single source interference. Laser light through a narrow opening.
continuous vs. discrete
Continuous: temperature from Wien's Displacement Law
Discrete: "bar codes" of the elements
The continuous spectrum of daylight. Note the absence of any significant gaps.
The discrete spectrum of excited mercury vapor.
The discrete spectrum of excited helium gas.
The discrete spectrum of a fluorescent light. These spectral lines are wider since they came from a wider source.
Quotes that need to be paraphrased.
Two German scientists, Robert Bunsen (a chemist) and Gustav Kirchhoff (a physicist), showed that the dark lines in the spectrum of sunlight corresponded to the bright lines of excited elements seen in laboratories on the earth.
Helium was discovered in 1868 by J. Norman Lockyear in the spectrum of a solar eclipse.
The French astronomer Pierre Janssen (1824-1907) discovered helium in the spectrum of the corona of the sun during an eclipse in 1868. Shortly afterward it was identified as an element and named by the British chemist Edward Frankland and the British astronomer Joseph Norman Lockyer. The gas was first isolated from terrestrial sources in 1895 by the British chemist William Ramsay, who discovered it in cleveite, a uranium-bearing mineral. In 1907 the British physicist Ernest Rutherford showed that alpha particles are the nuclei of helium atoms, which later investigation confirmed.