The Experts below are selected from a list of 291 Experts worldwide ranked by ideXlab platform
Richard T. White - One of the best experts on this subject based on the ideXlab platform.
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pulsed injection seeded optical parametric oscillator with low frequency chirp for High Resolution Spectroscopy
Optics Letters, 2003Co-Authors: Richard T. White, Yabai He, Mitsuhiko Kono, K G H BaldwinAbstract:An injection-seeded optical parametric oscillator (OPO), based on periodically poled KTiOPO4 and pumped by a frequency-doubled, nanosecond-pulsed Nd:YAG laser, generates continuously tunable, single-longitudinal-mode, pulsed output at ~842nm for High-Resolution Spectroscopy. Optical-heterodyne measurements show that the OPO frequency chirp increases linearly with detuning from the free-running (unseeded) OPO frequency and can be maintained as low as 10 MHz. Other factors affecting chirp are identified.
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Pulsed injection-seeded optical parametric oscillator with low frequency chirp for High-Resolution Spectroscopy
Optics letters, 2003Co-Authors: Richard T. White, Mitsuhiko Kono, Brian J. Orr, Kenneth BaldwinAbstract:An injection-seeded optical parametric oscillator (OPO), based on periodically poled KTiOPO4 and pumped by a frequency-doubled, nanosecond-pulsed Nd:YAG laser, generates continuously tunable, single-longitudinal-mode, pulsed output at approximately 842 nm for High-Resolution Spectroscopy. Optical-heterodyne measurements show that the OPO frequency chirp increases linearly with detuning from the free-running (unseeded) OPO frequency and can be maintained as low as 10 MHz. Other factors affecting chirp are identified.
Christian Veillet - One of the best experts on this subject based on the ideXlab platform.
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Spatial variations of the sodium/potassium ratio in Mercury's exosphere uncovered by High-Resolution Spectroscopy
Icarus, 2010Co-Authors: Alain Doressoundiram, François Leblanc, Cédric Foellmi, Adeline Gicquel, Gabriele Cremonese, Jean-françois Donati, Christian VeilletAbstract:High Resolution Spectroscopy of Mercury has been obtained with two different instruments in 2006: the EMMI instrument at the 3.6-m NTT telescope of ESO La Silla Chile and the Espadon spectrograph at the 3.6-m CFHT telescope on top of Mauna Kea (Hawaii). The disk of the planet has been scanned for spatial variation of the exospheric species. The large spectral range and High Resolution allow simultaneous measurements of the integrated column density of Na and K
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Spatial variations of the sodium/potassium ratio in Mercury’s exosphere uncovered by High-Resolution Spectroscopy ☆
Icarus, 2010Co-Authors: Alain Doressoundiram, François Leblanc, Cédric Foellmi, Adeline Gicquel, Gabriele Cremonese, Jean-françois Donati, Christian VeilletAbstract:High Resolution Spectroscopy of Mercury has been obtained with two different instruments in 2006: the EMMI instrument at the 3.6-m NTT telescope of ESO La Silla Chile and the Espadon spectrograph at the 3.6-m CFHT telescope on top of Mauna Kea (Hawaii). The disk of the planet has been scanned for spatial variation of the exospheric species. The large spectral range and High Resolution allow simultaneous measurements of the integrated column density of Na and K
K G H Baldwin - One of the best experts on this subject based on the ideXlab platform.
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pulsed injection seeded optical parametric oscillator with low frequency chirp for High Resolution Spectroscopy
Optics Letters, 2003Co-Authors: Richard T. White, Yabai He, Mitsuhiko Kono, K G H BaldwinAbstract:An injection-seeded optical parametric oscillator (OPO), based on periodically poled KTiOPO4 and pumped by a frequency-doubled, nanosecond-pulsed Nd:YAG laser, generates continuously tunable, single-longitudinal-mode, pulsed output at ~842nm for High-Resolution Spectroscopy. Optical-heterodyne measurements show that the OPO frequency chirp increases linearly with detuning from the free-running (unseeded) OPO frequency and can be maintained as low as 10 MHz. Other factors affecting chirp are identified.
Kenneth Baldwin - One of the best experts on this subject based on the ideXlab platform.
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Pulsed injection-seeded optical parametric oscillator with low frequency chirp for High-Resolution Spectroscopy
Optics letters, 2003Co-Authors: Richard T. White, Mitsuhiko Kono, Brian J. Orr, Kenneth BaldwinAbstract:An injection-seeded optical parametric oscillator (OPO), based on periodically poled KTiOPO4 and pumped by a frequency-doubled, nanosecond-pulsed Nd:YAG laser, generates continuously tunable, single-longitudinal-mode, pulsed output at approximately 842 nm for High-Resolution Spectroscopy. Optical-heterodyne measurements show that the OPO frequency chirp increases linearly with detuning from the free-running (unseeded) OPO frequency and can be maintained as low as 10 MHz. Other factors affecting chirp are identified.
Mitsuhiko Kono - One of the best experts on this subject based on the ideXlab platform.
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pulsed injection seeded optical parametric oscillator with low frequency chirp for High Resolution Spectroscopy
Optics Letters, 2003Co-Authors: Richard T. White, Yabai He, Mitsuhiko Kono, K G H BaldwinAbstract:An injection-seeded optical parametric oscillator (OPO), based on periodically poled KTiOPO4 and pumped by a frequency-doubled, nanosecond-pulsed Nd:YAG laser, generates continuously tunable, single-longitudinal-mode, pulsed output at ~842nm for High-Resolution Spectroscopy. Optical-heterodyne measurements show that the OPO frequency chirp increases linearly with detuning from the free-running (unseeded) OPO frequency and can be maintained as low as 10 MHz. Other factors affecting chirp are identified.
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Pulsed injection-seeded optical parametric oscillator with low frequency chirp for High-Resolution Spectroscopy
Optics letters, 2003Co-Authors: Richard T. White, Mitsuhiko Kono, Brian J. Orr, Kenneth BaldwinAbstract:An injection-seeded optical parametric oscillator (OPO), based on periodically poled KTiOPO4 and pumped by a frequency-doubled, nanosecond-pulsed Nd:YAG laser, generates continuously tunable, single-longitudinal-mode, pulsed output at approximately 842 nm for High-Resolution Spectroscopy. Optical-heterodyne measurements show that the OPO frequency chirp increases linearly with detuning from the free-running (unseeded) OPO frequency and can be maintained as low as 10 MHz. Other factors affecting chirp are identified.