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Retrievals of column PWV for the year 2000 data from the two MFRSRs at SGPs Central Facility (C1 and E13).

Retrievals of column PWV for the year 2000 data from the two MFRSRs at SGPs Central Facility (C1 and E13).

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The Multi-Filter Rotating Shadowband Radiometer (MFRSR) measures direct and diffuse irradiances in the visible and near IR spectral range. In addition to characteristics of atmospheric aerosols, MFRSR data also allow retrieval of precipitable water vapor (PWV) column amounts, which are determined from the direct normal irradiances in the 940 nm spe...

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... SGP's CF m at noon varies from 0.5 in winter to 0.97 % 1 in summer. As it is seen from Figure 4, the typical PWV column at this site also has a seasonal variation with a winter minimum of 0.5 cm and a summer maximum of around 4 cm. Using equation (19) we can estimate that for the instrument characteristics listed above and a calibration error with c = 0.03, the error induced in the PWV column will be 0.05 cm (10%) in winter and 0.18 cm (4.5%) in summer. ...
Context 2
... theory, some error in PWV retrievals by MFRSR may occur at large solar zenith angles because of the angular dependence of instrument's filters spectral responsivity coupled with imperfect performance of the diffusor, which allows change in the angle of incidence of light on the filter surface during the day. However, comparison with normal incidence Sun photometers (CIMEL, AATS-6) shown in Figures 4 and 9 do not show specific deviations in retrieved PWV column amount from MFRSRs at low Sun angles (at least for air masses smaller than 5 used for retrievals), thus, we consider this effect to be negligible. ...
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... in this study we focus on the Central Facility MFRSRs (C1, E13), for which the technical information was available, while using retriev- als from other SGP's EFs in a qualitative manner. Figure 4 shows the PWV retrievals (daily means) from C1 and E13 MFRSRs for the year 2000. A strong summer maximum in PWV column amount is clearly seen. ...
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... To illustrate the feasibility of using MFRSR net- work data for creation of 2D data sets comparable with the MODIS satellite water vapor product, we constructed a spatial distribution of columnar PWV from the MFRSR data obtained on 14 September 2000 at local noon (overpass time of Terra satellite) shown in Figure 14 (right). This distribution is in agreement with the corresponding map of the Terra MODIS PWV product (from NIR channels [Gao and Kaufman, 2003]) shown in Figure 14 (left). ...
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... To illustrate the feasibility of using MFRSR net- work data for creation of 2D data sets comparable with the MODIS satellite water vapor product, we constructed a spatial distribution of columnar PWV from the MFRSR data obtained on 14 September 2000 at local noon (overpass time of Terra satellite) shown in Figure 14 (right). This distribution is in agreement with the corresponding map of the Terra MODIS PWV product (from NIR channels [Gao and Kaufman, 2003]) shown in Figure 14 (left). While lacking small-scale details (some of which are due to cloud contamination, especially in the southern part of the MODIS image), the MFRSR network provides an accurate spatial trend of PWV: increasing column amount from north-west to south-east of the site. ...
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... lacking small-scale details (some of which are due to cloud contamination, especially in the southern part of the MODIS image), the MFRSR network provides an accurate spatial trend of PWV: increasing column amount from north-west to south-east of the site. This agreement is confirmed by the quantitative compar- ison shown in Figure 15 both for the exact MFRSR locations (left) and for all points in Figure 14 plots (right). The former expectedly demonstrates better agreement with MODIS, which values are smaller on average then the MFRSRs' by 0.2 cm with 0.2 cm standard deviation of the differences. ...
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... SGP site, in particular, provides a unique example of a dense regional MFRSR network capable of producing aerosol and PWV data sets character- izing both temporal and spatial variability of these atmo- spheric species. 2D slices of these data sets (for a specific moment of time) can be compared to satellite products (e.g., from MODIS, Figures 14 and 15) with help of a spatial interpolation technique, while evolution of these atmo- spheric fields can be tracked by MFRSR network beyond the time of satellite overpass. This ability is particularly significant for characterization of highly variable WV fields. ...
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... To make a practical estimate of the retrieval accuracy, the PWV column amounts derived from measurements by two SGP's CF MFRSRs (C1 and E13) were compared with each other and with a number of correlative measure- ments both by other solar radiometers (AERONET's CIMEL, AATS-6) and nonsolar instruments (microwave radiometers, GPS receiver). Data from the year 2000 ( Figure 4) were chosen for intercomparisons. Some of these instruments (C1 MWR, AERONET, NPN GPS) routinely provide data throughout the year, while the other (ETL CSR, JPL WVR, and AATS-6) were deployed at SGP's CF during the Water Vapor IOP (WVIOP2000) from 18 September to 8 October 2000. ...
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... It is well known that atmospheric WV is highly variable both temporary and spatially. High temporal vari- ability of PWV column amount is seen in Figure 4, while Figure 14 (right) shows up to 50% differences in value between neighboring MFRSR locations (the average spacing of SGP network is 80 km). Our structure function analysis [cf. ...
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... It is well known that atmospheric WV is highly variable both temporary and spatially. High temporal vari- ability of PWV column amount is seen in Figure 4, while Figure 14 (right) shows up to 50% differences in value between neighboring MFRSR locations (the average spacing of SGP network is 80 km). Our structure function analysis [cf. ...

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