The Shortwave Array Spectroradiometer – Zenith (SASZE) measures the zenith sky shortwave radiance over the spectral range from the near infrared to the ultraviolet. The SASZE incorporates two Avantes fiber-coupled spectroradiometers (Avaspec ULS 2048 CCD and Avaspec NIR256-1.7) for visible and near-infrared detection in the wavelength range 350–1700 nm. The sampling frequency is 1 Hz. The spectral resolution is 2.4 nm for the ULS 2048 CCD and 6 nm for the NIR256-1.7. The light collector has a narrow field of view (1° full-angle) collimator at the front end of a high-grade fiber optic. The SASZE measures sky radiance throughout the day including throughout twilight before the sun has risen and after it has set. The SASZE rack with spectroradiometers and data acquisition system is located within a temperature-controlled building isolated from the elements.
The SAS measurements can be used to retrieve cloud optical depth, particle size and cloud water path, test the cloud optical depth retrieval for overcast and broken cloud fields, validation/comparison with SGP surface remote sensors and future cloud IOP campaigns, multivariate analysis to derive information content in hyper spectral data sets and to improve cloud retrieval algorithm development, and compare with radiative transfer models for testing and validating retrieval procedures.
These two plots compare the visible zenith radiance (black) against the NFOV (green). This data comes from the filter bands data stream.
These plots are recorded at 673nm and 870nm.
There is no NFOV at SGP, so these plots do not exist there.
sas_spectra
These are plots of wavelength spectra for the visible (top) and near infrared (bottom) during the day.
Vertical banding (as seen here) correlates with cloud cover.
On clear days the plots should be ovular with the peak wavelengths at solar noon.
zenir_hour_spectra
This is a plot of the near-IR wavelength range vs spectral zenith irradiance measured each hour.
zevis_hour_spectra
This is a plot of the visible wavelength range vs spectral zenith irradiance measured each hour.
diagnostic_temp
Plots of the collection, chiller, and avantes diagnositc temperatures.
The avantes diagnostic temperature is comprised of a bench temperature (blue), ad temperature (green), saszevis bench temperature (brown), and saszevis ad temperature (purple).
mio_temperatures
Plot of the multi-IO temperature trh (green) and mems (blue).
diagnostic_rh
Plot of the spectrometer chiller internal RH (green) and the mulit-IO RH (blue).
diagnostic_dewpoint
Plots of the chiller dewpoint and collector internal dewpoint.
collector_tilt
Plot of the collector Y tilt (green) and X tilt (blue).
Plots of the collector X and Y tilts standard deviation.
List of past problems for this instrument that DO need to be mentioned in your DQA's:
Poor comparison with NFOV
At times the SASZE records far less zenith radiance and struggles to compare with the NFOV. This only occurs at AMF1 as there is not NFOV at SGP.
Missing filter bands data
At times the visible filter bands data goes missing showing a blank comparison against the NFOV. It also will show only the NIR plots in the sas_spectra and hour_spectra.