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设计论文参考文献

来源:学术堂 作者:韩老师致谢
发布于:2015-06-10 共1756字

  设计论文参考文献一:
  
  [1]舒远杰,李华荣,高晓敏,等.一类重要含能材料:5-取代四唾含能金属配合物.含能材料,2011,5: 588-596
  [2]侯向阳,焦宝娟,范广,等.含能配合物M(ATZ)--H20液相生成反应的热动力学研究.延安人学学报(自然科学版),2008,27: 41-47
  [3]肖鹤鸣,陈兆旭.四吨化学的现代理论.北京:科技出版社,2002
  [4]尚静,张建国,崔燕,等.含能配合[Zn(DAT)6](C104)2(DAT= 1,5-二氨基四[¢)的合成、晶体结构及性质.化学学报,2010,68: 233-238
  [5]冯金玲,张建国,李志敏等.高氮含能配合物[Co(AZT)2(H20)4](HTN R)2'4H20的合成、晶体结构及性质.化学学报,2010, 68: 2493-2499
  [6]李志敏,张建国,张同来,等.确基四哗及其高氮化合物.化学进展,2010,22:639-647
  [7]刘晓建,张慧娟,林秋汉,等.唑类含能离子化合物的合成研究进展.火炸药学报,2010,1:6-10
  [8]Huynh M H V. Preparation of terazole derivatives: US 2008/0200687 Al,2008
  [9]Huynh M H, Michael A H, Thomas J M,et al. Green primaries: environmentally friendly energetic complexes. Proceedings of the National Academy of Sciences,USA,2006,14:5409-5412
  [10]Huynh M H,Michael,D C,Thomas, J M,et al. Green primary explosives:5-Nitrotetrazolato-N -ferrate hierarchies. Proceedings of the National Academy of Sciences, USA, 2006,27: 10322-10327
  [11]Huynh M H. Simulant material for primary explosives: US 2009/019993 Al, 2009
  [12]Hiskey M A, Huynh M H. Primary explosives: US 007875725 B2,2011
  
  设计论文参考文献二:
  
  [1]汪晓莲,李澄,邵明,陈宏芳.2008.粒子探测技术,中国科学技术大学出版社.
  [2]刘佳.2013.LHAASO-KM2A探测器与原型阵列设计及性能研宄,博士论文,中国科学院高能物理研究所
  [3]郝新军,刘树彬,赵雷等.2012.羊八井大型水契伦科夫探测器中双增益大动态范围前放的研制,核电子学与探测技术,32 (3): 352-356.
  [4]Fukuda S, Fukuda Y, Hayakawa T et al. 2003. The Super-Kamiokande detector, NuclearInstruments and Methods in Physics Research A. 501:418-462.
  [5]Fukuda S, Fukuda Y, Ishitsuka M et all995. Determination of solar neutrino oscillationparameters using 1496 days of Super-Kamiokande-I data, Physics Letters B. 539:179-187.
  [6]AsakimoriK, Burnett T H,Cherry M L et al. 1990. Energy Spectra of Cosmic Rays Above 1TeV per Nucleon,The Astrophysics Journal. 349:25-28.
  [7]Heitler W. 1954. Quantum Theory of Radiation, Oxford University Press, London, Section38:386.
  [8]GaisserT. K 1990. Cambridge University Press,Cambridge.
  [9]KAMATAKoichi, et al. The Lateral and the Angular Structure Functions of Electron Showers,Progress of Theoretical Physics Supplement, 1958, 6: 93.
  [10]Atkins R, Benbow W, Berley D. 2003. Observation of TeV Gamma Rays from the Crab Nebula with Milagro Using a New Background Rejection Technique, The Astrophysical Journal. 595:803-811.
  
  设计论文参考文献三:
  
  [1]Wesson J 2004 TokamaJcs vol 149: Oxford University Press)
  [2]Dolan T J 1982 Fusion research: principles, experiments and technology:Pergamon Press)
  [3]Cousins S and Ware A1951 Pinch effect oscillations in a high current toroidal ring discharge Proceedings of the Physical Society. Section B 64 159
  [4]Bennett W H 1934 Magnetically self-focussing streams Physical Review 45-890
  [5]Dunway R and Phillips J 1958 Neutron Generation from Straight Pinches J Appl Phys 29 1137-43
  [6]Butt E Pand Carruthers R 1958 Proceedings of the Second United Nations International Conference on the Peaceful Uses of Atomic Energy, Geneva, 1958 32
  [7]Bodin H and Newton A 1980 Reversed-field-pinch research Nuclear fusion 20 1255
  [8]COLGATE S F 1958 JP and FURTH. HP. In: Proc. 2nd UN Int. Conf PUAE. Geneva, p 129
  [9]Bickerton R 1959 Brief review of the toroidal stabilised pinch Nuclear Instruments and Methods 4 273-8

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