Instrument Acronym:
SAFS
Instrument Measurements:
a) Trace Gas
b) Cloud Physics/Aerosol
c) Radiation/Optical/Electrical
Total actinic radiation 280-420 nm
d) Additional Capabilities
Calculation of photolysis frequencies for 12 molecular species. Longer wavelength scans possible.
Resource Person/Developer:
Name: Rick Shetter
Affiliation:NCAR/ACD
Phone:303-497-1480
Email:shetter@ucar.edu
Principle of Measurement:
True hemispherical collection of solar radiation with wavelength dependent output.
In situ/Remote/Flux Measurement:
In situ
Field projects in which the instrument has been used:
NASA PEM-Tropics A, NASA SONEX, NASA PEM-Tropics B.
Aircraft Platform:
NASA DC-8, NASA P3-B
Inlet Configuration/Location:
Optical collector and shadow ring at centerline Zenith and Nadir ports. Zenith location as far from the tail as possible. No other probes should be in the optical field of view.
Calibration/Cross Calibration:
Calibrations with NIST traceable irradiance sources. Cross calibrations with chemical actinometers.
Operator Requirements:
No operators required on board during flights. Scientist required for calibrations between flights.
Data Collection:
self
Post-flight Data Validation, Processing, Hours per Flight Hour etc.
Physical Characteristics:
Dimensions: 24" of 19" rack space
Weight: 140 lbs
Power: < 4 amps 115 volt 60 Hz
Other: access to zenith and nadir optical collectors for calibrations
Response Time:
5-10 sec/spectra
Detection Limits:
Actinic Flux ~0.5 uW/cm2/nm
Photolysis frequencies varies with molecule
Accuracy:
<10%
Precision:
3%
Limitations (such as altitude, airspeed, etc.)
none