Titlebook: International Handbook of Inter-religious Education; Kath Engebretson,Marian Souza,Liam Gearon Book 2010 Springer Science+Business Media B

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書目名稱International Handbook of Inter-religious Education影響因子(影響力)




書目名稱International Handbook of Inter-religious Education影響因子(影響力)學(xué)科排名




書目名稱International Handbook of Inter-religious Education網(wǎng)絡(luò)公開度




書目名稱International Handbook of Inter-religious Education網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱International Handbook of Inter-religious Education被引頻次




書目名稱International Handbook of Inter-religious Education被引頻次學(xué)科排名




書目名稱International Handbook of Inter-religious Education年度引用




書目名稱International Handbook of Inter-religious Education年度引用學(xué)科排名




書目名稱International Handbook of Inter-religious Education讀者反饋




書目名稱International Handbook of Inter-religious Education讀者反饋學(xué)科排名

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WATER

L. Philip Barnesw are investigated, using fluid-structure interaction (FSI). The FSI solution procedure developed for the study combines the modified characteristic-based split finite element method, dual-time stepping method, segment spring analogy technique, Galerkin finite element method, generalized-. method an

積云

Brendan Carmodyfluences with the Landquart River and the Ill River. The results show the relative importance of sorting effects at the beginning and the end of the study reach. In the middle part of the study reach, where sorting effects seem to be neglibile, the weight reduction coefficient . . reaches values def

披肩

John L. Eliased surface textures, research was carried out to develop a physical model that allows the stability and instability of river beds to be determined more precisely than previous ones (see .). The model is based on the exact knowledge of the turbulence characteristics of the liquid phase in combination

字形刻痕

Amjad Hussainental cosmological parameters. From the shapes of halo rotation curves (Quinn, Salmon and Zurek, 1986, QSZ) and the form of the two-point spatial correlation function (Davis et. al., 1985), it would appear that small and intermediate scale structures imply initial density perturbations with power sp

Painstaking

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Evelina Orteza y Mirandaental cosmological parameters. From the shapes of halo rotation curves (Quinn, Salmon and Zurek, 1986, QSZ) and the form of the two-point spatial correlation function (Davis et. al., 1985), it would appear that small and intermediate scale structures imply initial density perturbations with power sp

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