SEMI-ANNUAL STATUS REPORT Infrared Laboratory Studies of Synthetic Planetary Atmospheres Grant NCR 17-001-026

摘要

The high-resolution spectrograph has been used to measure the line strengths and self-broadening parameters in the v, fundamental of CO2 at laboratory temperature and at a reduced temperature approximating that of the Martian atmosphere. Similar studies have been made for the lines in the CO fundamental for self-broadening and for broadening by CO2 under conditions similar to those encountered on Mars.