Abstract
A new method for the determination of ray paths as well as
resulting path segments and partial gas columns within a layered
atmosphere is presented. Any singularity at the tangent point is
avoided. No use is made of the gross spherical symmetry of the
Earth’s atmosphere. Using this approach we examine the impact of
the Earth’s oblate shape and horizontal atmospheric inhomogeneities on
infrared limb spectra.
© 1999 Optical Society of America
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