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Titlebook: Very High Energy Gamma Ray Astronomy; K. E. Turver Book 1987 D. Reidel Publishing Company, Dordrecht, Holland 1987 astronomy.astrophysics.

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楼主: BRISK
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A. M. Hillasounded theory, while engaging in a gross neglect of 90 % of its important ideas“ (Glaser 1992, S.2). Für die Einleitung eines wissenschaftlichen Buches ist das fürwahr starker Tobak, und auch was Glaser an anderer Stelle in diesem Buch (z. B. S.125f.) über Juliet Corbin schreibt, ist schwer nachvoll
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W. F. Fryd conditions (as opposed to controlled experimental settings) resulting from open system boundaries, contingencies and historicity. Ecology has long explored the transition zone between the natural and social sciences, and can significantly contribute to an interdisciplinary understanding of societa
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L. Resvanis,J. Learned,V. Stenger,D. Weeks,J. Gaidos,F. Loeffler,J. Olson,T. Palfrey,G. Sembroski,C.only on pore clogging, but also on degradation of groundwater quality, for example from solubilisation of iron, or formation of dissolved sulphides. Examples of approaches used to assess possible impact on groundwater quality are presented for an arid region in NW China where an assessment was made
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L. Resvanis,J. Learned,V. Stenger,D. Weeks,J. Gaidos,F. Loeffler,J. Olson,T. Palfrey,G. Sembroski,C.ama and spring as the Unica River. After flowing over Planinsko Polje, it continues its flow underground towards the springs of the Ljubljanica River in the north of the recharge area. To give a comprehensive overview of the study area, different aspects relevant for the research, ranging from a bro
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R. C. Lamb,M. F. Cawley,D. J. Fegan,K. G. Gibbs,A. G. Gregory,P. W. Gorham,D. A. Lewis,N. A. Porter, of overexploitation of its weathered hard rock aquifer, its cropping pattern, rural socio-economy, agricultural practices and semi-arid climate. The objective of this study is to develop and test well-suited modelling approaches to simulate the flow in the existing aquifer system that consist of tw
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High Energy Radiation from the Young PulsarsThe young pulsars, typified by the Crab and Vela Pulsars, are distinguished by their short periods and large rates of period increase. The category does not include the “millisecond” pulsars, which have very small rates of period increase: these are old pulsars, whose high spin rates are the result of a spin-up process in a binary system.
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