The apparatus consists of a coelostat and an infrared spectrometer
coupled with an appropriate am- plifier, mechanical rectifier and
arecorder. The coelostat was constructed for use at stations of
different geographical latitude. With this apparatus the emission
spectra of the sun and the earth's atmosphere between 8 IJ. and 111J.
wave-length were measured on clear days at different zenith angles of
the sun and the percentage absorp- tion and emission, respectively, of
the atmospherical ozone layer were computed. Assuming the validity of
the Lambert-Beer law the measured atmospherical transmission yielded the
product of the absorption coefficient Ci and the total amount of ozone
x; ä is a mean absorption coeff- cient. In the infrared the absorption
coefficient is a function of pressure P and hence of the height h above
the ground. Imagine the atmosphere up to a height of 50 km to be divided
into any given number of homo- geneous layers, the absorption in each
layer depends upon the respective absorption coefficient (Xi and the
amount of ozone xi . A summation over all layers yields the total
absorption which depends on the to- tal amount of ozone x and on a mean
absorption coefficient Ci. This mean absorption coefficient is defined
by the equation It was shown that ii is sufficiently constant even in
consideration of the seasonal variations of the total amount of ozone x
. Therefore, it was possible to derive the total amount of ozone x from
the measured products ii . x.