Other
Scientific paper
Nov 1974
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974tsbb.nasa...26z&link_type=abstract
In NASA. Ames Res. Center Telescope Systems for Balloon-Borne Res. p 26-37 (SEE N75-12735 03-74)
Other
Balloon-Borne Instruments, High Altitude Balloons, Solar Instruments, Solar Spectra, Data Acquisition, Equipment Specifications, Infrared Imagery, Infrared Radiation
Scientific paper
The Liege-balloon program is intended to make high-spectral resolution observations of the sun in the near- and intermediate infrared regions not accessible from the ground. A description of the equipment, followed by a summary of the data obtained till now is presented. Except for ozone whose maximum of concentration lies near 25 Km altitude, the residual mass distribution of the other mentioned molecules decreases with altitude. This is a self-explanatory argument for carrying out spectroscopic observations from platforms transcending the densest layers of the earth's atmosphere. The Liege balloon equipment is primarily intended for very high-resolution solar observations from about 27-30 Km altitude, in all spectral regions between 1.5 and 15.0 microns, not accessible from the ground.
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