After having crossed an absorbing cloud, the intensity of a source,
I,
is received by the observer as I(
) = I
, where
is the optical depth of the cloud.
Let's connect to the physical parameters.
N : column densitya(
: line absorption coefficient
: broadening function
a(
=
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l : lower level of the atomic transition
k : upper level of the atomic transition
: rest wavelength of the transition
g
: statistical weight of the lower level
g
: statistical weight of the upper level
a
: spontaneous transition probability
f= upward oscillator strength