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Central California Ozone Study (CCOS) - Desert Research Institute

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<strong>CCOS</strong> Field Operations Plan Version 2: 5/31/00<br />

2.3.4 Solar Radiation Measurements<br />

The US Department of Agriculture’s UVB Radiation Monitoring Program was initiated<br />

in 1992, through a grant to Colorado State University, to provide information on the<br />

geographical distribution and temporal trends of UVB radiation in the United States.The<br />

climatology network of the USDA-CSREES monitoring program is designed to provide an<br />

adequate density of measurement sites to establish the spatial and temporal characteristics of<br />

UVB irradiance. The United States is divided into 26 regions of about equal area. The<br />

measurement sites are located primarily in rural areas near agricultural and forested regions. The<br />

US Department of Agriculture operates a UVB radiation measurement network with the<br />

following two sites in <strong>California</strong>.<br />

Station Name Closest town Longitude Latitude Elevation<br />

UC Davis Climate (Davis) 121.8 38.5 18<br />

Station<br />

<strong>Desert</strong> <strong>Research</strong> and<br />

Extension Center<br />

(Holtville) 115.4 32.8 -18<br />

The US Department of Agriculture’s UVB Radiation Monitoring Program maintains one<br />

site, near Davis, <strong>California</strong> (Latitude: 38.529, Longitude: 121.761). The site is operated by the<br />

University of <strong>California</strong> at Davis. Co-location of one spectral radiometer for the measurement of<br />

actinic flux to this site will provide significant advantage to <strong>CCOS</strong>. There are two existing<br />

Multifilter Rotating Shadowband Radiometers (MFRSR) at the USDA, Davis site. A<br />

shadowband radiometer has a rotating metal band that periodically blocks the direct solar beam<br />

from entering the radiometer. This feature allows a measurement of the total horizontal, diffuse<br />

and direct normal components of the irradiance. One MFRS radiometer operates in the visible<br />

region and makes filter measurements at 415, 500, 610, 665, 862 and 940 nm and for the total<br />

visible radiation. The second MFRS operates in the UV and makes measurements at 300, 305.5,<br />

311.4, 317.6, 325.4, 332.4, 368 nm. The sampling time for the visible MFRSR is 15 seconds and<br />

the sampling time for the ultraviolet MFRSR is 20 seconds however data from both MFRSR’s<br />

are stored as 3-minute averages. There are several other measurements that support the UVB<br />

radiation measurements at this site including sensors for UVA, UVB-1 and surface reflection and<br />

measurements of relative humidity, temperature and barometric pressure. Sample data from this<br />

site may be obtained from:<br />

http://uvb.nrel.colostate.edu/UVB/cgi_scripts/uvb_site_info_page.cgi?CA01&C.<br />

Actinic flux in the troposphere depends most critically on the total ozone column, the<br />

aerosol loading, size and optical properties and the presence and characteristics of clouds. The<br />

UV and visible MFRSR will allow the total ozone column and the aerosol characteristics to be<br />

estimated. The total ozone column measured by an UV-MFRSR was compared with standard<br />

Brewer and Dobson spectrophotometers. The average ratio of ozone retrieved by the UV-<br />

MFRSR to that of the Brewer was found to be 1.02 and to the Dobson 1.03. The USDA’s visible<br />

and UV- MFRSRs data provides an estimate optical depths as a measure of the total aerosol<br />

loading. These data together with the actinic flux measurements will allow a direct evaluation of<br />

the photolysis rate parameters calculated for use in air quality models.<br />

Chapter 2: FIELD MEASUREMENTS 2-11

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