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Survey of Rural Wells in Missouri for Pesticides and Nitrate 总被引：2，自引：0，他引：2
Two hundred and one rural wells were sampled in eight agricultural areas of Missouri. Samples were analyzed for 25 pesticides and nitrate. Forty-three percent of the wells sampled had at least one pesticide detection. Thirteen percent of the wells had at least one detection ≧ 1 ppb and these concentrations were confirmed. Only one well exceeded U.S. EPA Health Advisory levels. Twenty-two percent of the wells exceeded the U.S. EPA Drinking Water Standard for nitrate. Pesticide detections were most strongly correlated to well depth. Nitrate levels were primarily related to well depth, well construction methods, and well siting. 相似文献
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A numerical scheme is described for the calculation of effective albedo values of long city street canyons. The method is based on a generalization of the radiation model for inclined surfaces recently presented by Brühl and Zdunkowski (1983). Calculated albedo values are compared with Aida's (1982) experimentally determined results. It is found that experiment and theory are in reasonable and in some cases in excellent agreement. Additional results obtained by varying the geometry of the street canyon as well as the surface reflectivities are shown to demonstrate the versatility of the calculation scheme. 相似文献
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Wink J. E. Altenhoff W. J. Bieging J. Butler B. Butner H. Haslam C.G.T. Kreysa E. Martin R. Mauersberger R. McMullin J. Muders D. Peters W. Schmidt J. Schraml J. B. Sievers A. Stumpff P. Von Kapp-Herr A. Thum C. Zylka R. 《Earth, Moon, and Planets》1997,77(3):165-165
Earth, Moon, and Planets - The concept of simultaneous multifrequency continuum observations, successfully tested on Comet Hyakutake, was applied to Comet Hale-Bopp, using the Heinrich Hertz... 相似文献
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J. E. Wink W. J. Altenhoff J. Bieging B. Butler H. Butner C.G.T. Haslam E. Kreysa R. Martin R. Mauersberger J. McMullin D. Muders W. Peters J. Schmidt J. B. Schraml A. Sievers P. Stumpff A. Von Kapp-Herr C. Thum R. Zylka 《Earth, Moon, and Planets》1997,77(3):165
The concept of simultaneous multifrequency continuum observations, successfully tested on Comet Hyakutake, was applied to
Comet Hale-Bopp, using the Heinrich Hertz Submillimeter Telescope (HHT) with the four color bolometer between 250 and 870
GHz, the IRAM 30m telescope at 240 Ghz, the MPIfR 100-m telescope at 32 GHz, and the IRAM interferometer near 90 and 240 GHz.
Near-simultaneous measurements were done between February 15 and April 26, 1997, mainly concentrated in mid March shortly
before perigee of the comet.
The measurements gave the following preliminary results:
Interferometer detection of the nuclear thermal emission. If the signal at the longest interferometer spacing of 170 mis due
to thermal emission from the nucleus only, its equivalent diameter is ∼49 km. If, however, this signal contains a contribution
from a strongly centrally peaked halo distribution(e.g., r−2 density variation) the diameter may be as low as 35 km. The emission found interferometrically was always 5″ north and 0.1
sec east from the position predicted by Yeoman's solution 55.The comparison of the interferometric continuum emission with
the simultanously obtained molecular line observations (reported on this conference) shows the origin of the strongest line
emission concentrated on the nucleus. The 30-m observations show a radio halo with a gaussian FWHP of ∼11, corresponding to
a diameter of 11000 km at geocentric distance of 1.2 a.u.
A spectral index of ∼3.0 for the total signal, which may indicate a smaller mean particle size than for Hyakutake. Assuming
an average cometary density of 0.5 gcm−3, the mass contained in the nucleus is ∼1$#x2013;3 1019 g and 1012 g in the particle halo.
This revised version was published online in July 2006 with corrections to the Cover Date. 相似文献
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Natalie E. Sievers Carrie A. Menold Marty Grove Matthew A. Coble 《International Geology Review》2017,59(5-6):621-638
ABSTRACTPrevious study of subducted continental crust within the Luliang Shan terrane in Northwest China has documented metasomatic formation of thick, hydrated phengite + garnet-rich selvages at the interface between mafic eclogite blocks and quartzofeldspathic host gneiss. Whole rock concentrations of Cs and Ba within the selvage are enriched by two orders of magnitude relative to the eclogite blocks and host gneiss. We performed in situ ion microprobe analyses of Li, Be, B, Rb, Sr, Cs and Ba and δ11B of phengite within the Luliang Shane terrane to better constrain the source(s) of the infiltrating fluid. The phengite within the selvage are enriched in Li, Cs and Ba and yield δ11B values between ?30‰ and ?9‰, values that are lower than mantle values. High Ba/Rb, Cs/Rb coupled with low B/Be, B/Li and highly negative δ11B values indicate that the high-pressure fluid that formed the selvage was derived from highly devolatilized rocks within the subduction channel. In contrast, muscovite, which crystallized in the adjacent host gneiss during a subsequent lower pressure phase of fluid infiltration at approximately 0.9 GPa depths, has much lower Li, Cs and Ba relative to the high-pressure phengite. These retrograde muscovite have very high concentrations of B (up to 5500 ppm) and Be (up to 50 ppm) and high (?2 to +8‰) δ11B values that are consistent with crystallization from a fluid derived from shallower and less devolatilized regions of the subduction zone. Additional host gneiss samples, regionally distributed and kilometres away from the studied area lack the B-rich signature and indicate that the late stage fluids were likely localized to the region near the studied traverse. 相似文献