| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |
| | | |
| | | 200-1100 nm Range, I Sample Spectrum 0.75 nm Resolution | | |
| | | |
| | | An irrad-iance =r HZ:: WHRh40h00CG. | | |
| | | The HR4000CG Spectrometer utilizes a proprietary grating and " order-sorting filter to provide a 200-1100 nm wavelength range and 0.75 optical resolution (FWHM). The revolutionary HR4000CG is a | | 18001600 ' 1400 12001000 1 800 600400 200 0 | | |
| | | |
| | | 300 400 500 600 700 800 900 1000 | | |
| | | preconfigured HR4000 Spectrometer — where all of the already selected for you. | | |
| | | |
| | | WAVELENGTH (nm) | | |
| | | |
| | | |
| | | |
| | | Sample Spectrum | | |
| | | Composite-grating & Order-sorting Filter The HR4000CG uses the HC-1 grating, which is a revolutionary and proprietary variable blazed grating designed to provide a 200-1100 nm wavelength range. (Though the spectrometer is configured for 200-1100 nm, its best efficiency is from 200-1 050 nm. See the grating efficiency curve for the HC-1 on page 23.) In addition to this new composite grating, the HR4000CG has an OFLV-200-1100 variable longpass order-sorting filter to eliminate second- and third-order effects. Both are installed | | |
| | | |
| | | CD TJ CD 0 ct 1 0 3 CD c CD 1 | | |
| | | 700 | | |
| | | |
| | | 600- | | |
| | | |
| | | 500 | | |
| | | |
| | | m CM < m u 2. | | |
| | | 400300 200100 | | |
| | | |
| | | |
| | | |
| | | |
| | | 200 300 ^00 500 600 700 800 900 1000 WAVELENGTH (nm) | | |
| | | CD < CD c CD 3 CD | | |
| | | at | | the time of manufacture and are fixed in place. | | |
| | | | | |
| | | |
| | | |
| | | A solar irradiance spectrum taken with the HR4000CG. | | |
| | | |
| | | | | | | | | | | | | | PHYSICAL | | | | Dimensions: | 148.6 mm x 104.8 mm x 45.1 mm | | | | Weight: | 570 g | | | | DETECTOR | | | | Detector: | Toshiba TCD1304AP linear CCD array (page 24) | | | | Pixels: | 3648 pixels, pixel size of 8 urn x 200 urn | | | | Pixel well depth: | ~100,000 electrons | | | | Sensitivity: | 130 photons/count at 400 nm; 60 photons/count at 600 nm | | | | OPTICAL BENCH | | | | Design: | f/4, Symmetrical crossed Czerny-Turner | | | | Focal length: | 101.6 mm input, 101.6 mm output | | | | Entrance aperture: | 5 urn wide slit (page 22) | | | | Grating: | HC-1, 300 lines per mm grating (page 23) | | | | Order-sorting filters: | Installed OFLV-200-1100 (page 24) | | | | | | | | SPECTROSCOPIC | | | | Wavelength range: | 200-1100 nm, best efficiency 200-1050 nm | | | | Optical resolution: | 0.75 nm FWHM | | | | Signal-to-noise ratio: 300:1 (at full signal) | | | | Dark noise: | 12 RMS counts | | | | Dynamic range: | 2 x 108 (system); 1300:1 for a single acquisition | | | | Integration time: | 3.8 ms to 10 seconds | | | | ELECTRONICS | | | | Power consumption: 450 mA @ 5 VDC | | | | Data transfer speed: Full spectrum to memory every 4 ms with USB 2.0 port, 18 ms with USB 1.1 port | | | | Inputs/Outputs: | 10 onboard digital user-programmable GPIOs* | | | | Analog channels: | One 13-bit analog input, One 9-bit analog output | | | | | | | | | |
| | | |
| | | CD CD c c TJ CD | | |
| | | |
| | | Optical Bench The HR4000CG Spectrometer uses the "HR" Optical Bench, comes with a 5 /vm entrance slit, and has a UV4 Detector Upgrade to enhance the performance of the spectrometer in the UV. The HR4000CG is an upgrade from the HR2000CG. The HR4000CG comes with a 3648-element linear-array Ccd detector that provides better optical resolution throughout the UV-NIR range. USB 2.0 Compatibility and New Digital I/Os The HR4000CG interfaces to a PC via a USB port. Software reads programmed data unique to each spectrometer for easy setup. The HR4000CG also offers 10 user-programmable digital inputs/outputs, 1 analog input and 1 analog output. HR4000CG-UV-NIR: $4,999 | | |
| | | |
| | | _USB port; any 32-bit Windows OS using serial port * Programming the GPIOs requires SpectraSuite or OmniDriver. See pages 80-82 for details. | | |
| | | |
| | | |
| | | Tei: 72"7'.733.244'7 • Email: Info@OceanOptics.com | | |
| | | 35 | | |
| | | |
| | | |
| | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | | |