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10.4 Compton Normalization Method: The Compton normalization method is based on <br /> analysis of a single, certified standard and normalization for the Compton peak. The Compton peak <br /> is produced from incoherent backscattering of x-ray radiation from the excitation source and is <br /> present in the spectrum of every sample. The Compton peak intensity changes with differing <br /> matrices. Generally, matrices dominated by lighter elements produce a larger Compton peak, and <br /> those dominated by heavier elements produce a smaller Compton peak. Normalizing to the <br /> Compton peak can reduce problems with varying matrix effects among samples. Compton <br /> normalization is similar to the use of internal standards in organics analysis. The Compton <br /> normalization method may not be effective when analyte concentrations exceed a few percent. <br /> The certified standard used for this type of calibration could be an NIST SRM such as 2710 or <br /> 2711. The SRM must be a matrix similar to the samples and must contain the analytes of interests <br /> at concentrations near those expected in the samples. First, a response factor has to be determined <br /> for each analyte. This factor is calculated by dividing the net peak intensity by the analyte <br /> concentration. The net peak intensity is gross intensity corrected for baseline interference. <br /> Concentrations of analytes in samples are then determined by multiplying the baseline corrected <br /> analyte signal intensity by the normalization factor and by the response factor. The normalization <br /> factor is the quotient of the baseline corrected Compton K. peak intensity of the SRM divided by that <br /> of the samples. Depending on the FPXRF instrument used, these calculations may be done <br /> manually or by the instrument software. <br /> 11.0 PROCEDURE <br /> 11.1 Operation of the various FPXRF instruments will vary according to the manufacturers' <br /> protocols. Before operating any FPXRF instrument, one should consult the manufacturer's manual. <br /> Most manufacturers recommend that their instruments be allowed to warm up for 15 to 30 minutes <br /> before analysis of samples. This will help alleviate drift or energy calibration problems later on in <br /> analysis. <br /> 11.2 Each FPXRF instrument should be operated according to the manufacturer's <br /> recommendations. There are two modes in which FPXRF instruments can be operated: in situ and <br /> intrusive. The in situ mode involves analysis of an undisturbed soil sediment or sample. Intrusive <br /> analysis involves collection and preparation of a soil or sediment sample before analysis. Some <br /> FPXRF instruments can operate in both modes of analysis, while others are designed to operate in <br /> only one mode. The two modes of analysis are discussed below. <br /> 11.3 For in situ analysis, one requirement is that any large or nonrepresentative debris be <br /> removed from the soil surface before analysis. This debris includes rocks, pebbles, leaves, <br /> vegetation, roots, and concrete. Another requirement is that the soil surface be as smooth as <br /> possible so that the probe window will have good contact with the surface. This may require some <br /> leveling of the surface with a stainless-steel trowel. During the study conducted to provide data for <br /> this method, this modest amount of sample preparation was found to take less than 5 minutes per <br /> sample location. The last requirement is that the soil or sediment not be saturated with water. <br /> Manufacturers state that their FPXRF instruments will perform adequately for soils with moisture <br /> contents of 5 to 20 percent but will not perform well for saturated soils, especially if ponded water <br /> exists on the surface. Another recommended technique for in situ analysis is to tamp the soil to <br /> increase soil density and compactness for better repeatability and representativeness. This <br /> condition is especially important for heavy element analysis, such as barium. Source count times <br /> for in situ analysis usually range from 30 to 120 seconds, but source count times will vary among <br /> instruments and depending on required detection limits. <br /> CD-ROM 6200 - 16 Revision 0 <br /> January 1998 <br />