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PERMFILE128636
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PERMFILE128636
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Last modified
8/24/2016 10:25:46 PM
Creation date
11/25/2007 6:26:28 PM
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Template:
DRMS Permit Index
Permit No
M1999002
IBM Index Class Name
Permit File
Doc Date
6/18/1999
Doc Name
OBJECTORS EXHIBITS
Media Type
D
Archive
No
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4 • • <br />ih• Gamma iay Log /10 <br />THE GAMMA RAY LOG <br />The Gamma Ray Log is a measurement of the natural <br />radioactivity of the formations. The log is therefore useful <br />in detecting and evaluating deposits of radioactive minerals <br />such as potash or uranium ore. <br />In sedimentary formations the Gamma Ray Log nor- <br />mally reflects the shale content of the formations. This is <br />because [he radioactive elements tend to concentrate in clays <br />and shales. Clean formations usually have a very low level of <br />radioactivity, unless radioactive contaminants such as vo]- <br />canicash or granite sash are present, or when the formation <br />waters con[ain dissolved potassium salts. <br />The Gamma Ray Log can be recorded in cased wells, <br />which makes it very useful in completion and workover op- <br />erations. It is frequently used as a substitute for the SP in <br />cased holes where the SP is unavailable or in open holes <br />where the SP is unsatisfactory. In both cases it is useful for <br />the location of the non-shaly beds and for correlation. <br />PROPERTIES OF GAMMA RAYS <br />Gamma rays are bursts of high-energy electromagnetic <br />waves which are emitted spontaneously by some radioactive <br />elements. Nearly all of the gamma radiation encountered in <br />the earth is emiaed by the ndioaaive potassium isorope of <br />atomic weight 40 and [he radioactive elements of the ura- <br />nium and thorium series. <br />Each of these elements emits gamma rays, the number <br />and energies of which are distinctive of each element. Fig. <br />10-1 shows the energies of the gamma rays emitted: Pons- <br />sium (KA0) emits gamma rays of a single energy at 1.46 <br />DfeV, whereas the ruo radioactive series emit many gamma <br />ra}'s of various energies. <br />in passing through matter, gamma rays experience suc- <br />cessive Compmn-scutering collisions (Chaprer 1-S) with the <br />atoms of the Formation, losing energy with each collision. <br />Finally, af[er [he gamma ray has los[ enough energy, it is ab- <br />sorbed via the phoroelectric effect. (In the phoroelectxic e6 <br />feet, low energy gamma rays are completely absorbed b}' <br />atoms of the formation material, resulting in the ejection of <br />electrons (ram the absorbing aroms.) <br />EFFECT OF FORMATION DENSITY <br />Gamma rays are gradually absorbed and their energies <br />degraded as they pass through formations. The amount of <br />absorption varies with formation density. Tw-o formations <br />having the same amount of radioactive material per unit vol- <br />ume but having different densities will show, on the Gamma <br />z <br />0 <br />a P07A SSIUM <br />rt <br />u <br />w <br />_z <br />N <br />O <br />w <br />a <br />THORIUM SERIES <br />z <br />o_ <br />N <br />VI <br />w <br />0 <br />r <br />URANIUM-RADIUM SERIES <br />m <br />a <br />m <br />0 <br />a G N t ~..t .... .t . <br />0 .5 I I.5 2 2.5 - <br />G4MM4-RAY ENERGY IMEV) <br />Fig. 10-1 -Gan:n:a ray emisrion r¢ectra of radio- <br />actir•e rrrineralt (Ref. 4). <br />sy <br /> <br />
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