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Robert J. Munroe

Publications and source records attributed to Robert J. Munroe.

7 recordsLinked to original sources

Heat flow and near-surface radioactivity in the Australian continental crust

Heat-flow data have been obtained at 44 sites in various parts of Australia. These include seven sites from the old (~ 2500 m.y.) Precambrian shield of Western Australia, seventeen from the younger (~ 600- 2000 m.y.) Precambrian rocks of South Australia, the Northern Territory, and Queensland, and twenty within the eastern Paleozoic and younger rocks. Thirty of the sites are located where no previous heat-flow data existed, and the remainder provide significant extensions or refinements of areas previously studied. Where the holes studied penetrated the crystalline basement rocks, or where the latter rocks were exposed within a few kilometers of the holes, the upper crustal radiogenic heat production has been estimated based on gamma-ray spectrometric determinations of U, Th, and K abundances. Three heat-flow provinces are recognized in Australia based on the linear relation (q = q* + DA 0 ) between heat flow q and surface radioactivity A 0 . New data from the Western Australian shield support earlier studies showing that heat flow is low to normal with values ranging from 0.7 to 1.2 hfu and with the majority of values less than 1.0 hfu, and the parameters q* = 0.63 hfu and 0 = 4.5 km determined previously were confirmed. Heat flow in the Proterozoic shield of central Australia is quite variable, with values ranging between about l and 3 hfu. This variability is attributed mainly to variations in near-surface crustal radioactivity. The parameters of the heat-flow line are q* = 0.64 hfu and 0 = 11.1 km and moderately high temperatures are predicted for the lower crust and upper mantle. Previous suggestions of a band of l ow- to - normal heat flow near the coast in eastern Australia were confirmed in some areas, but the zone is interrupted in at least one region (the Sydney Basin), where heat flow is about 2.0 hfu over a large area. The reduced heat flow, q*, in the Paleozoic intrusive rocks of eastern Australia varies from about 0.8 to 2.0 hfu . This variability might be related to thermal transients associated with Late Tertiary and younger volcanic and tectonic activity, even though the relation between heat-flow values and the age of volcanism is not a simple one. Parts of the high heat-flow area in the southeast might be exploitable for geothermal energy.

Open-File Report

Abundances of uranium, thorium, and potassium for some Australian crystalline rocks

This report contains a tabulation of the basic radioelement and radiogenic heat data obtained during an Australian National University (ANU) - United States Geological Survey (USGS) heat-flow project, directed jointly by J. C. Jaeger (ANU) and J. H. Sass (USGS). Most samples were collected during the periods June through September, 1971 and 1972. The measurements were made subsequently by two of us (C. M. Bunker and C. A. Bush) using the gamma-ray spec trometric techniques described by Bunker and Bush (1966, 1967). Interpreting the spectra for quantitative analyses of the radioelements was accomplished with an iterative leastsquares computer program modified from one by Schonfeld (1966). Uranium content determined by gamma-ray spectrometry is based on a measurement of the daughter products of 226 Ra. Equilibrium in the uranium-decay series was assumed for these analyses . Throughout the report, when U content is stated, radium-equivalent uranium is implied. The coefficient of variation for the accuracy of the radioelement data, when compared to ana lyses by isotope dilution and flame photometry is about 3 percent for radium-equivalent uranium and thorium and about 1 percent for potassium. These percentages are in addition to minimum standard deviations of about 0.05 ppm for U and Th, and about 0.03 percent for K.

Open-File Report

Thermal data from heat-flow test wells near Long Valley, California

As part of the Geological Survey's study of the Long Valley area, an attempt was made to define the regional thermal setting of the caldera. The first phase of this study involved the drilling of four holes in granitic rocks outside of the caldera and two holes within it (Figure 1). LV was drilled as a hydrologic test well. In Figure 1, the light areas are areas of crystalline rocks and the stippled area, volcanic and sedimentary rocks. (For an explanation of the symbols, see Plate 1 of Bateman and others (1963).) Preliminary temperature measurements and thermal conductivity determinations have been completed and are presented in this report. Also presented herein are data obtained in November 1973 from the shallow holes drilled by Lewis (1974) and some thermal conductivity values from these short holes. These preliminary data are being released now because of intense public interest. The study is continuing, and an interpretive report will be written later this year. The temperature measurements are presented in both graphs and tables. Thermal conductivity data are tabulated as a function of depth for each hole. For locations of the shallow test wells, reference should be made to the quadrangle maps shown in Figures 3 through 13 of Lewis (1974).

California