How do matter and light interact? This lecture is the first of a
two-part lecture on the physical basis of spectroscopy. Today we will
discuss the Kelvin Absolute Temperature scale, which provides a measure
of the internal energy content of matter, and Kirchoff's empirical Laws
of Spectroscopy, along with the Stefan-Boltzmann Law and the Wein Law to
describe the continuous emission from a blackbody. We will end by
briefly describing the suggestive properties of emission- and
absorption-line spectra, whose explanation in the details of atomic
structure will be the topic of the next lecture. Recorded 2006 Oct 25
in 100 Stillman Hall on the Columbus campus of The Ohio State
University.
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