Features & Benefits:
Telescope-spectrometer systems for direct-sun and scattered skylight spectrum acquisition.
Optimized for UV/Vis aerosol and trace gas remote sensing with the DOAS method.
Other applications are possible.
Detectable gases: NO2, O3, SO2, HCHO, H2O, HONO, IO, BrO, Glyoxal, O4.
Modular and customizable to meet your specific requirements.
Software packages for spectral analysis, post-processing and data visualization .
Technical Specifications:
Measurement accuracy:
Individual in-house spectrometer fine adjustment to optimize spectral properties.
Spectrometer characterization included: wavelength calibration, offset and dark current spectra, detector non-linearity function.
Active spectrometer temperature stabilization ensures stable properties.
High spectral sampling prevents quantization errors.
Low noise and high precision in narrow-band optical density.
Color filters and optical bench design minimize spectrometer stray-light.
Cross-section converting fiber bundle for maximum light throughput and homogeneous spectrometer illumination.
Real-time correction of telescope elevation via inclination sensor, ideal for measurements on moving platforms. (ships, cars) or in changing environments.
Prism deflector and optical fiber setup prevent polarization induced biases.
Small vertical field of view optimized for vertical profiling applications .
Customization :
Individual spectrometer configurations to best meet your spectral requirements.
Various optical fiber configurations.
Different fiber and cable lengths available.
Integrable opto-mechanical components for direct-sun observations and calibration monitoring purposes.
Stand-alone operation of separate spectrometer and telescope units for.
integration in arbitrary spectroscopic measurement system
