************************************************************************** Background Information: The objective of this experiment was to measure the clear, cloudless sky solar irradiance at the surface with the best instrumentation available, and with the most appropriate procedures as followed by the solar measurement community. The irradiance measurements were carried out with extreme care, diligence and certainty with thorough documentation. The ultimate goals of this experiment were 1) to validate similar measurements being taken at the ARM/CART Central Facility site on a routine basis and 2) to provide a highly referenced and accurate measurement of clear sky irradiances at the ARM/CART CF Site. All measurements were taken at the ARM/CART Site from 17 April to 26 April. The data used in the resultant clear day analysis were taken on 18 and 19 April, 1996 (JD 109 and 110). The instrumentation used in the experiment is as follows: 1) 2 Eppley Hickey-Frieden Absolute Cavity Radiometers, model AHF sensitive to 280-2800 nm wavelengths. Measures direct solar radiation. (serial numbers 29222 and 30710) 2) 4 Eppley Precision Spectral Pyranometers, model PSP sensitive to 280-2800 nm wavelengths. 2 were shaded to collect diffuse radiation and 2 were unshaded to collect global radiation (diffuse + direct). (serial numbers 29613, 29614, 29616, and 29912) 3) 2 Eppley Precision Infrared Radiometers (Pyrgeometers) model PIR sensitive to 3500-50000 nm wavelengths. The PIRs were shaded. (serial numbers 29143 and 29144) 4) 2 Sci-Tec 2AP Suntrackers. They were used to point the cavities and to provide a platform for diffuse (shaded) measurements. 5) 1 Campbell CR10 datalogger and Campbell AM416 16 channel multiplexer was used for data collection. ************************************************************************** Please Note: This data is preliminary. In order to create the best data set possible, the instruments used in collecting this data, especially the Eppley PSPs (Global and Shaded) must be recalibrated to check for drift during the experiment. After recalibration, the PSP data will most likely not be changed by more than 2-3%. The AHF Cavity 30710 was compared directly to the World Radiation Reference Standards at Davos, Switzerland in October of 1995. The average comparison was within 0.2% of the WRR Standards. The Eppley PIRs were taken from a set of three reference ones used by the Solar Radiation Research Branch of The National Oceanic and Atmospheric Administration. ************************************************************************** This file contains information essential to the understanding of the data in cavity1.dat. The data file, cavity1.dat, contains the following data sets in comma delineated lines: Dec.Time,Avg_PIR,Avg_Cav,Avg_Shade,Avg_Global,Cos(sza) Dec.Time = Hour Decimal Time (Local Standard Time, add 6 for GMT) Avg_PIR = Average of the two shaded Eppley PIRs for times corresponding to cavity data taken. Avg_Cav = Average of the two Eppley AHF Cavites from days 109 and 110. Avg_Shade = Average of the two shaded Eppley PSPs for times corresponding to cavity data taken. Avg_Global = Average of the two Global Eppley PSPs for times corresponding to cavity data taken. Cos(sza) = Cosine of the solar zenith angle. The PSP and PIR data were taken using 1 second spot samples and logging 1-minute averages and standard deviations. The cavity data were taken as 1 second spot samples every 3 seconds and then averaged into 1 minute data during the data reduction procedures. Special Data Notes: ------------------- 1) -9999.0 in the data set implies missing data for that sample. 2) The constructed data set does not start at exactly sunrise nor end at exactly sunset due to limitations of the cavity radiometer at very high solar zenith angles. ************************************************************************** Note that this data set, representing 1 day, is actually comprised of two days: <9:30 am ---------- JD 109 ------------Sunset> The day was created this way due to clouds during the morning of JD 109 and the afternoon of JD 110. *************************************************************************** All inquries should be directed to: Mike Rubes NOAA/ARL/SRRB R/E/AR*1 325 Broadway Boulder, CO 80303 (303) 497-7316 rubes@srrb.noaa.gov Note also that a WWW page has been created for this data set. The raw data as well as processed data along with more information about the experiment is presented. http://www.srrb.noaa.gov/apr96iop/hagsie.html ****************************************************************************