The stratospheric emission in the submillimeter spectral region has been measured from 38.2 km atltitude with a resolution of 0.0033 cm-1. In most cases this resolution makes possible the separation of contributions caused by the individual rotational transitions. An atlas of the observed features is given as a guide to both the measurements of minor stratospheric constituents concentration and the evaluation of stratospheric transparency for the measurement of nontelluric sources.