High-resolution solar spectroscopy in the undergraduate physics laboratory

Details High-resolution solar spectroscopy in the undergraduate physics laboratory High-resolution solar spectroscopy in the undergraduate physics laboratory

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992amjph..60..645r&link_type=abstract

American Journal of Physics, Volume 60, Issue 7, pp. 645-649 (1992).

Physics

2

Visible, Solar Electromagnetic Emission

Scientific paper

The richness of the solar spectrum at visible wavelengths makes it ideally suited for many laboratory exercises in optical spectroscopy. A number of such experiments taking advantage of a high-resolution scanning spectrometer are described as they have been performed by seniors at Middlebury College. Physical principles emphasized include optical depth, the nature of molecular spectra, the Doppler effect, and the Zeeman effect. These experiments are suitable for advanced undergraduate physics and astronomy majors.

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