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AERONET - Solar Flux
AEROSOL OPTICAL DEPTH AEROSOL INVERSIONS SOLAR FLUX OCEAN COLOR Maritime Aerosol Network
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Solar Flux
AEROSOL/FLUX NETWORKS
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AERONET DATA ACCESS
 
AERONET ALL Site Lists (V3)

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AERONET Active Site Lists (V3)

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MISSION
 
 

SolRad-Net (Solar Radiation Network) is an established network of ground-based sensors providing high-frequency solar flux measurements in quasi-realtime to the scientific community and various other end users.  This network was implemented as a companion to AERONET and its instrumentation are invariably collocated with AERONET sites.  The Brazilian core of the present network was developed within the scientific framework of the LBA-ECO component of the Large-Scale Biosphere-Atmosphere Experiment in Amazônia.  Historically, SolRad-Net has preferentially selected sites that routinely experience intervals of biomass-burning, such as Amazônia and Sub-Saharan Africa for its long-term monitoring.    

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CAUTION: Data presented in the real time data version are unscreened and may not have final calibration reprocessing.

NOTICE TO NON-SolRad-Net INVESTIGATORS: To maintain the integrity of the database and fairness to the individuals who have contributed, use of these data for publication requires an offer of authorship to the SolRad-Net PI(s)


 
NEWS
 
 

- Recently Added Sites

El Nido Airport (2012) Lulin (2009)
Penang_USM (2012) Barcelona (2009)
Palangkaraya (2012) Manaus (2008)
Yonsei University (2012) Pantnagar (2008)
Toravere BSRN (2012) Rio Gallegos, Argentina: CEILAP (2007)
Appalachian State (2012) Buenos Aires, Argentina: CEILAP (2007)
Bozeman (2011) Barrow BSRN (2007)
Silpakorn University (2010) Bermuda BSRN (2007)
Regina (2009) Boulder BSRN (2007)

- New and Updated Solrad-Net Documents

 
COLLABORATORS
 
 
Organizations
NASA Goddard Space Flight Center - USA
Instituto de Fisica
Universidade de Sao Paulo - Brazil
Departamento de Ciencias da Natureza (DCN)
Universidade Federal do Acre (UFAC) - Brazil
Universidade Federal de Rondonia - Brazil
Departamento de Fisica
Universidade Federal de Mato Grosso/ICE - Brazil
Atmospheric Research Group (ARG) Institute of Applied Physics
The Academy of Sciences of Moldova - Moldova
J. Blaustein Inst. for Desert Research
Ben Gurion University of the Negev - Israel
Department of Civil Engineering
Indian Institute of Technology
- India
Lulin Atmospheric background Station (LABS)
Environmental Protection Administration (Taiwan)
National Central University - Taiwan

Kenya Wildlife Service - Kenya

 
 
DATA
 
 
Data are available from several flux instruments including filtered and unfiltered pyranometers, photosynthetically active radiation (PAR) energy and quantum sensors, and UV-A and UV-B flux sensors.
 
Pyranometer PAR [Energy]
Distribution of Pyranometer Flux Sites for Level 1.5 Data
Distribution of PAR Flux Sites for Level 1.5 Data
Filtered Pyranometer PAR [Quantum]
Distribution of Filtered Pyranometer Flux Sites for Level 1.5 Data
Distribution of PAR Lite Flux Sites for Level 1.0 Data
UV-A UV-B
Distribution of UV-A Flux Sites for Level 1.0 Data
Distribution of UV-B Flux Sites for Level 1.0 Data
Diffuse Pyranometer  
Distribution of Diffuse Pyranometer Flux Sites for Level 1.0 Data
 
 
 
 
SYSTEM DESCRIPTION - Solar Radiation Network
 
 

SolRad-Net Calibration, Data Processing and Instrumentation

CALIBRATION PROCEDURE

    When possible, calibration of the PAR sensors was accomplished by using in-situ comparisons to a radiative transfer model calculations of flux on selected optimal days.  The 6S [Vermote et al, 1997] model we used for this purpose is based on the successive order of scattering method.  Field days used were of minimal aerosol-loading (AOT500nm < 0.1) under cloud-free conditions. Such aerosol levels are sufficiently low to render an exact knowledge of the absorption properties unimportant for computing clear-sky insolation to an accuracy of >1%.  The manufacturer (Skye Instruments) states an initial accuracy for its factory calibration of 5% (generally < 3%).   However, due to changes in the stability of the silicon detector (estimated by Skye as ~ 2% per year) and more notably, diminished transmittance of the bandpass interference filter upon prolonged exposure, we observed significant degradation of sensitivity in these sensors of approximately 6-8% per year.  This necessitated that we employ in-situ calibrations when possible to ensure the best possible determination of PAR calibration.  The utility of this technique varied greatly depending on local climatology (a cloudless sky with low AOT is required) and thus our estimation of PAR flux accuracy varies with site.   At some locations, such as Alta Floresta, Brazil, we benefited from an environment that presented numerous optimal calibrations dates and were able to characterize the trend in calibration drift with high confidence [In-situ calibration plot].  Locations with few, or no suitable calibration conditions (such as persistently cloudy locations) are necessarily calibrated with the manufacturer's calibration only, and thus are not considered suitable for promotion to the highest quality level (2.0).  More on data quality designations can be found in the Data Quality Assessment section below.

    Due to additional complicating factors, such as water vapor influence, thermal equilibrium issues, and also, because of the greater degree of accuracy (2%) provided by the manufacturer and generally much greater stability of this type of radiometer, the factory calibrations were used for the pyranometers.   These pyranometers have all been observed to retain consistent calibration coefficients (calibration drift less than 1% per year) between re-calibration sessions.

PROCESSING

Data from all AERONET sites are sent hourly from each fieldsite to the Wallops Receiving Center via transmissions to satellite (GOES, METEOSAT) using VITEL transmitters. These raw data are then transferred hourly from the Wallops receiving station to the Goddard Facility.

The instrument-specific calibrations are applied and the raw data are converted to flux data products that are made available on the website.   

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Last Updated: April 07, 2025