Physics
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992esasp.356..353m&link_type=abstract
In ESA, Proceedings of an ESA Symposium on Photon Detectors for Space Instrumentation p 353-356 (SEE N94-15025 03-19)
Physics
Balloon-Borne Instruments, Gallium, Infrared Telescopes, Photoconductors, Silicon, Emission Spectra, Infrared Radiation, Spaceborne Experiments
Scientific paper
The measurement of IR emission features in extended sources originating from PAH's (Polycyclic Aromatic Molecules) material is addressed by the AROME instrument, a balloon borne telescope. For this purpose four Si:Ga photoconductors were developed. They operate at 1.6K inside an integrating cavity. A cold FET based TIA preamplifier provides low noise photocurrent measurement. The estimated noise equivalent power (blip) is 8 times 10 to the minus 14th power W/square root of Hz.
Giard Martin
Leotin Jean
Lucas Guillaume
Mény Claude
Ristorcelli Isabelle
No associations
LandOfFree
Silicon gallium doped photoconductor development for the AROME balloon borne instrument does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Silicon gallium doped photoconductor development for the AROME balloon borne instrument, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Silicon gallium doped photoconductor development for the AROME balloon borne instrument will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1114477