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1 - 10 of 17 Search Results for auto-correlation

1. MIRAseed_DS	Best match in this PDF \| All matches in this PDF
`...` 's optional SPO-II prism pair accessory. MIRASeed Femtosecond Modelocked Ti:Sapphire Laser Solid-State UltrafastCoherent 17 fs FWHM Interferometric autocorrelation of 17 fs pulse from Mira-SEED with GVD dispersion compensation. 60 nm FWHM Frequency spectrum of Mira-SEED modelocked output. FEATURES · `...` Related Searches: tomography \| birefringent filter

2. Mantis_DS	Best match in this PDF \| All matches in this PDF
`...` Specifications 579.44 mm (22.81 in.) 330.2 mm (13.0 in.) 129.43 mm (5.1 in.) 120.78 mm (4.76 in.) 168.4 mm (6.63 in.) Front ViewSide View Top View Autocorrelation ~75 nm FWHM of Spectrum - Pulse Measured After Compression with CPC Delay (fs) Autocorrelation FWHM = 26.3 fs Deconvolved Pulse FWHM = 17 `...` Related Searches: mantis \| cpc compact pulse compressor

3. tech_bullfourier_transform	Best match in this PDF \| All matches in this PDF
`...` techniques that allow iterative reconstruction of the pulse shape [1-6], the most common techniques used to determine pulse shape information are autocorrelations (intensity or interferometric) or spectral measurements. Autocorrelations suffer from the fact that the autocorrelation function, not the `...` Related Searches: positive light \| pulse shaper

4. ChameleonUltraFamily_DS (PAGE 2 OF 2)
`...` .Coherent.com 1 Specified at peak of tuning range. 2 Average speed measured over entire tuning range. 3 Based on sech2 deconvolution of 0.65 times autocorrelation width. 4 Measured RMS in a 10 Hz to 20 MHz bandwidth. 5 Power drift in any two-hour period with less than ±1°C temperature change after a `...`

5. ChameleonVision_DS (PAGE 2 OF 2)
`...` .Coherent.com 1 Specified at peak of tuning range. 2 Average speed measured over entire tuning range. 3 Based on sech2 deconvolution of 0.65 times autocorrelation width. 4 Measured RMS in a 10 Hz to 20 MHz bandwidth. 5 Power drift in any two-hour period with less than ±1°C temperature change after a `...`

6. CPC_DSrevA	Best match in this PDF \| All matches in this PDF
`...` +49 (6071) 968 333 Italy +39 (02) 34 530 214 Japan +81 (3) 5635 8700 Korea +82 (2) 460 7900 UK +44 (1353) 658 833 www.Coherent.com 1 Assumes an autocorrelation deconvolution factor of 0.65. 2 Pulse length and bandwidth defined at FWHM. Typical Autocorrelation of ~75 nm Bandwidth Pulse from Mantis Compressed `...`

7. tech_bullfourier_transform (PAGE 1 OF 2)
`...` techniques that allow iterative reconstruction of the pulse shape [1-6], the most common techniques used to determine pulse shape information are autocorrelations (intensity or interferometric) or spectral measurements. Autocorrelations suffer from the fact that the autocorrelation function, not the `...`

8. CPC_DSrevA (PAGE 2 OF 2)
`...` +49 (6071) 968 333 Italy +39 (02) 34 530 214 Japan +81 (3) 5635 8700 Korea +82 (2) 460 7900 UK +44 (1353) 658 833 www.Coherent.com 1 Assumes an autocorrelation deconvolution factor of 0.65. 2 Pulse length and bandwidth defined at FWHM. Typical Autocorrelation of ~75 nm Bandwidth Pulse from Mantis Compressed `...`

9. Mantis_DS (PAGE 2 OF 2)
Autocorrelation ~75 nm FWHM of Spectrum - Pulse Measured After Compression with CPC Delay (fs) Autocorrelation FWHM = 26.3 fs Deconvolved Pulse FWHM = 17.1 fs 0 1 2 3 4 5 6 7 8 9 -70 -60 -50 -40 -30 -20 -10 0 10 20 30 40 50 60 70 Au tocorrelation of Compressed Pulse (a.u.) Typical Beam Profile Avg `...`

10. Vitesse800_DSrevC_3	Best match in this PDF \| All matches in this PDF
`...` Power Supply Laser Cavity Schematic 1 Nominal center wavelength ±1 nm. 2 Full width at half maximum. 3 Based on sech2 deconvolution of 0.65 times autocorrelation width. 4 Nominal repetition rate ±0.8 MHz. 5 Measured over 2 hours after 15-minute warm-up. 6 Measured from 10 Hz to 10 MHz. 7 1/e2 at exit `...`

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