Abstract

This paper presents the principles of new methods and programs for calculating the transmittance of the atmosphere in the 0.2-2.5-µm region. These methods are based on direct line-by-line computations and their description, using the effective amounts of the absorbing gases (the spectral transmittance) and taking into account the effective parameters of the optoelectronic systems (the overall transmittance).

PDF Article

Cited By

You do not have subscription access to this journal. Cited by links are available to subscribers only. You may subscribe either as an OSA member, or as an authorized user of your institution.

Contact your librarian or system administrator
or
Login to access OSA Member Subscription