Skyspec instruments

Passive remote sensing of atmospheric particles and gases

SkySpec instruments measure ultraviolet and visible light from the sun and sky to remotely detect atmospheric pollutants like nitrogen dioxide (NO2), sulfur dioxide (SO2), formaldehyde (HCHO), ozone (O3), water vapor (H2O), and aerosols. 

The motorized telescope adjusts its angle to collect data from different parts of the sky. The high-precision spectrometer analyzes the light to identify specific gases. 

Our software turns the data into measurements of pollution levels, showing how much pollution is in the air and at what height. 

Category:

Measurement Accuracy

  • Individual in-house spectrometer fine-tuning for optimal spectral properties. 
  • Comprehensive spectrometer characterization including wavelength calibration, offset and dark current spectra, and detector non-linearity function. 
  • Active spectrometer temperature stabilization for consistent performance. 
  • High spectral sampling rate to prevent quantization errors. 
  • Low noise and high precision in narrow-band optical density measurements. 
  • Color filters and optimized optical bench design to minimize stray light. 
  • Cross-section converting fiber bundle for maximum light transmission and uniform spectrometer illumination. 
  • Real-time telescope elevation correction using an inclination sensor, ideal for measurements on moving platforms (ships, cars) or in changing environments. 
  • Prism deflector and optical fiber configuration to eliminate polarization-induced biases. 
  • Small vertical field of view optimized for vertical profiling applications. 

Setup, Lifetime & Maintenance

  • Quartz Glass Enclosure: Minimizes external moving parts for: 
  • Long lifespan even under harsh environmental conditions 
  • Easy cleaning 
  • Integrated Telescope Heating (activates at < 5°C) prevents: 
  • Freezing of mechanical components 
  • Water condensation, snow, and ice on the quartz cylinder and other optics 
  • Weatherproof and UV Resistant IP64 housings 
  • 12V/DC Power Supply with low consumption, ideal for mobile operation via battery or car cigarette lighter 
  • Easily Adaptable Measurement Routines 
  • Fast Instrument Power-Up 

Customization

  • Individual spectrometer configurations to best meet your spectral requirements. 
  • Various optical fiber configurations available. 
  • 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 into any spectroscopic measurement system. 
Model         
  MINI  COMPACT  1D  2D 
Measurement PC  External  Embedded  External  External 
Direct sun mode available  No  No  No  Yes 
Data communication  USB  LAN/WIFI  USB  USB 
Azimuth angle range and accuracy  Fixed  Fixed  Fixed  -5° to 185°, ± 2° 
Camera options  None or single  None, single or dual  None, single or dual 
Weight  ≈ 7 kg  ≈13 kg  ≈ 14 kg 
Size of telescope unit (WxDxH)  Box *8: 30 x 20 x 13.2 cm3  

Quartz tube length: 16 cm 

Box *8: 20 x 20 x 13.2 cm3  

Quartz tube: 16 cm 

Boxes *8: 20 x 20 x 29 cm3  

Quartz tube: 16 cm 

Telescope stand-alone possibility  No  Yes 
Size of spectrometer unit (WxDxH)  Embedded in telescope  Box *8: 40 x 30 x 13.2 cm3 
Operation temperature  -10°C to 40°C  -30°C to 50°C (telescope unit) 
GPS option  Yes  No 
Calibration lamp options  External handheld lamp  Integrated and/or external handheld lamp 
Spectrometers  Single  Single or dual (UV and Vis) 
Typical spectral range  300–460 nm  300-405 nm (UV) and 410–553 nm (Vis) 
Typical spectral resolution (FWHM)  < 0.7 nm  < 0.5 nm (UV) and < 0.6 nm (Vis) 
Spectral sampling  > 5 sampling points over spectrometer slit function FWHM 
Available detectors  back-thinned CCD or CMOS (back-thinned CCD highly recommended for UV) 
Elevation angle range and accuracy  -10° to 190°, automatic adjustment with inclination sensor to < 0.1° accuracy (1σ) 
Field of view FWHM, vertical x horizontal  Scattered skylight: < 0.3°x 1°, direct sunlight (SkySpec 2D with diffusor system): 10° x 10° 
Tripod & adapter  Adapter for telescope and outdoor tripod 
Power consumption  Average < 30 W (100 W max.), supply voltage 9-15 V, 110–220 V AC power supply incl., operation with battery possible 
Housing material  Polycarbonate (IP64), UV resistant 
Additional sensors  Ambient temperature, pressure, humidity in spectrometer housing, temperature on electronic board 

SKYSPEC MODEL OVERVIEW

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SKYSPEC ADVANTAGES

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SKYSPEC MODEL CONFIGURATION GUIDE

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SKYSPEC 1D

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SKYSPEC 1D STANDALONE TELESCOPE

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SKYSPEC 2D

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SKYSPEC 2D STANDALONE TELESCOPE

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SKYSPEC COMPACT

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SKYSPEC MINI

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SKYSPEC SPECBOX MINI

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EVAL SOFTWARE PACKAGE DATASHEET

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IMAGING SOFTWARE PACKAGE DATASHEET

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Passive Differential Optical Absorption Spectroscopy (DOAS) is a multifaceted technique. This section will outline its basic principles. For in-depth information, please refer to the comprehensive book by Platt and Stutz (2008). 

Spectra Acquisition 

SkySpec systems are designed to capture UV/Vis spectra of direct sunlight and scattered skylight from various directions. Common observation configurations include direct sun and zenith sky measurements, as well as elevation scans (multiple measurements at different viewing angles). 

The path of light through the atmosphere varies based on the viewing direction, as does the amount of gas encountered (see figure on the left). It’s important to note that the light path is also influenced by current visibility conditions, including the presence and properties of atmospheric particles like fog and clouds. 

Each gas absorbs specific light wavelengths, leaving a unique signature in the spectrum. These absorption effects are generally small. For many gases, detecting changes less than 0.1% is required to achieve meaningful measurement limits. 

DOAS Spectral Analysis 

DOAS spectral analysis involves comparing two spectra: 

    1. Reference spectrum: Ideally recorded in a direction with minimal light-gas interaction (e.g., zenith).
    2. Measurement spectrum: Acquired in the desired direction, such as through an exhaust plume. 

The DOAS fit identifies and separates the characteristic absorption patterns of trace gases in the spectral intensity differences. The magnitude of these patterns directly corresponds to the differential slant column density (dSCD), which can be broken down as follows: 

    • Column density: The integrated concentration of a trace gas along the light path. 
    • Slant: The light path through the atmosphere is slanted, as opposed to vertical column densities. 
    • Differential: The dSCD represents the difference in slant column density between the measurement and reference light paths, not an absolute gas amount. 

DSCDs are calculated for each viewing direction and gas with significant absorption in the studied spectral range. 

Post-Processing 

DSCDs are valuable for determining the integrated emissions of local sources. However, many applications, such as regional air quality assessment, require vertical column densities or even concentrations. 

Vertical columns and ground-level concentrations can be estimated by approximating light paths geometrically. More accurate results are obtained using profile retrieval algorithms, which fit an atmospheric model (considering photon physics and measurement geometry) to observed DSCDs along different light paths to derive concentrations at multiple altitudes. This approach is often simplified as “atmospheric tomography.” The proxy gas O4 can even be used to estimate particle concentration (see e.g., Frieß, 2004). 

General monitoring  

SkySpec observations deliver trace gas and aerosol optical thickness data averaged across several kilometers, offering a significant advantage over in-situ measurements that can be heavily influenced by local conditions. As a result, SkySpec systems are perfectly suited for evaluating regional air quality, even in extremely remote and pristine areas due to their high sensitivity. Airyx provides software solutions to convert raw data into light path integrated gas abundances (slant and vertical columns), and even vertical concentration profiles. 

Gas Imaging 

Sequential scanning and real-time data processing enable the visualization and quantification of invisible gases in a user-friendly manner. The Airyx imaging package automatically generates overlays combining camera and slant column images. 

Point Source Monitoring 

Targeted vertical scanning enables the determination of the composition of point emission plumes (factories, power plants, volcanoes, etc.) from a safe distance of up to several kilometers from potentially restricted or hazardous sources. Combining SkySpec observations with wind data allows for highly accurate gas emission rate calculations. 

Mobile Applications 

SkySpec’s automated elevation angle correction and compact design make it ideal for mobile use on vehicles such as cars or ships. For example, driving through industrial parks or cities enables the determination of pollutant inflow and outflow, allowing for the calculation of emission rates within the enclosed area. 

Satellite Validation 

The spatial averaging interval of SkySpecs and the typical size of satellite ground pixels are comparable. As a result, SkySpecs can offer datasets with exceptional representativeness for validating satellite data. 

Further Applications 

Due to their high modularity and customization, SkySpec systems can be applied to a variety of spectroscopic applications, including: 

  • Remote measurements of surface reflection properties 
  • Biomedical spectroscopy 
  • Remote measurements of solar-induced plant fluorescence 
  • Material science 
SkySpec 1D SkySpec 2D SKYSPEC COMPACT
SkySpec1D SkySpec 2D SKYSPEC COMPACT
SkySpec1D_v210 SkySpec1D_v210 SkySpecCompact
SkySpec1D_v210 SkySpec 2D SkySpecCompact_v200
SkySpec1D_v210 SkySpec2D_v210 SkySpecCompact_v200
SkySpec1D
  • 2 CHANNEL SPECTROMETER
    UV (300-404nm) AND VIS (420-565nm), TEMPERATURE STABILIZED
  • INDUSTRIAL AND OPERATIONAL APPLICATIONS
    AIR QUALITY AND EMISSION MONITORING
  • FLEXIBLE MOUNTING OPTIONS
    TRIPOD, WALL MOUNT OR MAST
  • 2 CHANNEL SPECTROMETER
    UV (300-404nm) AND VIS (420-565nm), TEMPERATURE STBILIZED
  • INDUSTRIAL AND OPERATIONAL APPLICATIONS
    AIR QUALITY AND EMISSION MONITORING
  • AZIMUTHAL SCANNING
    HEMISPHERICAL MONITORING, DIRECT SUNLIGHT SPECTROSCOPY, TOTAL COLUMN MEASUREMENTS
  • FLEXIBLE MOUNTING OPTIONS
    TRIPOD, WALL MOUNT OR MAST

 

  • PORTABLE
    QUICK SET UP IN REMOTE AREAS
  • EMBEDDED PC
    FOR DATA ACQUISITION & STORAGE, WI-FI & LAN CONNECTIVITY
  • BATTERY OPERATION
    OPTIONAL BATTERIES AVAILABLE
  • MOBILE APPLICATIONS
    FIELD CAMPAIGNS, MOVING PLATFORMS (CAR, SHIPS, AIRCRAFTS)

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