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<br />I' <br /> <br />... <br />.. <br /> <br />A complete system calibration is performed on <br />each of the radars at the beginning and end of <br />each operational season. This calibration con- <br />tlsts of a measurement of the effective antenna <br />stem gain using the method described by <br />ith (1974), The indicated value of effective <br />antenna system gain is 43.7 dB (Smith, 1977). <br />This figure incorporates all waveguide, mis- <br />match. and similar losses beyond the directional <br />coupler as well as any radome loss (Smith. <br />1977). It also incorporates a Pre-. Mid-, and <br />Post-season antenna boresighting, elevation and <br />azimuth error determinations and corrections <br />using solar evaluations. These checks consist <br />of measuring with a gunner's quadrant the tilt <br />~rom the vertical of the azimuth rotation axis <br />of the antenna. The procedure used is an <br />adaptation of the Air Weather Service gunners' <br />quadrant procedure (Smith, 1977). Elevation <br />boresighting is accomplished by a solar method <br />of using the gunners' quadrant, a plumbline, and <br />solar azimuth and elevation data obtained from <br />a computer program called "Angles" that is <br />available on the Bureau of Reclamation Environ- <br />mental Data Network. Details of the solar <br />method for boresighting the antenna are given <br />in Section 4 of Whiton ~ al (1976). Boresight <br />errors as determined by this method are typi- <br />cally between 0.010 and 0.060 (Smith, 1977). <br /> <br />The azimuth orientation of the antenna is <br />checked by a solar method similar to that used <br />for elevation boresighting. The azimuth <br />orientation error is determined by noting the <br />differences between the antenna azimuth dial and <br />the true solar positions, The azimuth orienta- <br />tion error is determined as the average of a <br />series of 20 repeated measurements. The eleva- <br />~on orientation is accomplished by comparin~ <br />~e elevation indications with the true solar <br />elevation angles. The details of this procedure <br />are outlined in the paper by Whiton ~ al (1976). <br /> <br />The weekly DVIP calibration consists basically <br />of injecting RF test signals of specified power <br />levels through the directional coupler into the <br />receiver. The offset and gain variable <br />resistors of the DVIP are set so that the given <br />test signals just trigger the appropriate DVIP <br />level thresholds. The test signals are varied <br />to determine the triggering thresholds of all <br />the DVIP levels, and the results are recorded <br />both on tape in DVIP units and on the calibra- <br />tion sheet in dBm. The total procedure is <br />described in Smith (1977), which is included in <br />the Operations Plans of each of the sites. <br /> <br />The data tape with the recorded DVIP values is <br />processed and the DVIP unit values for each of <br />the levels are combined with the recorded dBm <br />values in a computer program known as CALSUB <br />which resides in the Environmental Data Network. <br />This program calculates third-order equation <br />coefficients for a polynomial regression <br />analysis of DVIP/dBm calibration data. The <br />third order equation is of the form: <br />Y = A + B(X) + C(X2) + D(X3), where X is the <br />DVIP value and Y is the corresponding estimated <br />dBm value. These coefficients are then used in <br />the computer processing to determine reflectivity <br />values. <br /> <br />e <br /> <br />The daily checks conducted by the electronic <br />technician consist of measuring those values <br />needed for calculation of Ze in the Operational <br />torm of the Probert-Jones radar equation: <br /> <br />Ze <br /> <br />1024 dn2 <br />, 'w! <br /> <br />PRF -1-- <br />(aver. power)(Freq)2 g2e~ <br /> <br />rz. Pr <br />/k12 <br /> <br />The technician measures daily: '(1) PRF, <br />(2) Average Power, (3) Transmitter Frequency, <br />(4) Minimum Discernible Signal, and (5) checks <br />three levels of t~.DVIP using the procedure <br />described above. If the DVIP varies by more <br />than 1 dBm from the weekly calibration, a com- <br />plete recalibration is performed. The stability <br />of the DVIP during the 1977 seasons was such <br />that they did not require recalibration, and <br />calibration data indicate that the DVIP varied <br />only by 2 DVIP units (2/3 dB) over the season. <br /> <br />The technicians rigorously apply these calibra- <br />tion procedures, and their dedication to pro- <br />viding the most quantitative data possible has <br />resulted in an extremely high percentage of <br />on-the-air time at all sites. <br /> <br />References <br /> <br />Smith, P.L., Jr., 1974: The measurement of <br />antenna gain in radar systems, <br />Microwave J., 17, 4 (April), 37-40. <br /> <br />. 1977: Evaluation of Miles City <br />SWR-75 weather radar. Report 77-1, <br />Institute of Atmospheric Sciences, South <br />Dakota School of Mines and Technology, <br />April. <br /> <br />Whiton, R.C., P,L. Smith, Jr., and A.C. Harbuck, <br />1976: Calibration of weather radar <br />systems using the sun as a radio source. <br />Preprints, 17th Radar Meteorology Conf., <br />Seattle, Washington, Amer. Meteor. Soc., <br />60-65. <br />