http://www.cnr.it/ontology/cnr/individuo/prodotto/ID263831
Absolute frequency spectroscopy of CO2 lines at around 2.09 mu m by combined use of an Er:fiber comb and a Ho:YLF amplifier (Articolo in rivista)
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- Label
- Absolute frequency spectroscopy of CO2 lines at around 2.09 mu m by combined use of an Er:fiber comb and a Ho:YLF amplifier (Articolo in rivista) (literal)
- Anno
- 2011-01-01T00:00:00+01:00 (literal)
- Alternative label
Gatti, D. and Coluccelli, N. and Gambetta, A. and Di Lieto, A. and Tonelli, M. and Galzerano, G. and Laporta, P. and Marangoni, M. (2011)
Absolute frequency spectroscopy of CO2 lines at around 2.09 mu m by combined use of an Er:fiber comb and a Ho:YLF amplifier
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- Gatti, D. and Coluccelli, N. and Gambetta, A. and Di Lieto, A. and Tonelli, M. and Galzerano, G. and Laporta, P. and Marangoni, M. (literal)
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- Coluccelli, N (Reprint Author), Politecn Milan, Dipartimento Fis, Piazza Leonardo da Vinci 32, I-20133 Milan, Italy. Gatti, D.; Coluccelli, N.; Gambetta, A.; Galzerano, G.; Laporta, P.; Marangoni, M., Politecn Milan, Dipartimento Fis, I-20133 Milan, Italy. Gatti, D.; Coluccelli, N.; Gambetta, A.; Galzerano, G.; Laporta, P.; Marangoni, M., CNR, Ist Foton & Nanotecnol, I-20133 Milan, Italy. Di Lieto, A.; Tonelli, M., Univ Pisa, Dipartimento Fis, I-56127 Pisa, Italy. Di Lieto, A.; Tonelli, M., CNR, NEST Ist Nanosci, I-56127 Pisa, Italy. (literal)
- Titolo
- Absolute frequency spectroscopy of CO2 lines at around 2.09 mu m by combined use of an Er:fiber comb and a Ho:YLF amplifier (literal)
- Abstract
- The low-frequency tail of an octave-spanning supercontinuum (SC) generated by an Er: fiber comb is enhanced by a multipass Ho:YLF amplifier and used in a sum-frequency-generation scheme to obtain absolute referencing of a single-mode Tm-Ho:YAG laser tunable around 2.09 mu m. By tuning the comb repetition frequency, the probing laser is scanned across the absorption lines of a CO2 gas sample and highly accurate absorption profiles are measured. This approach can be readily scaled to any wavelength above similar to 2 mu m. (C) 2011 Optical Society of America (literal)
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