參考文獻是對學術(shù)論文引文進行統(tǒng)計和分析的重要信息源之一，下面是小編搜集整理的設計論文參考文獻，供大家閱讀借鑒。

　　參考文獻一：

　　[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

　　參考文獻二：

　　[1]舒遠杰，李華榮，高曉敏，等.一類重要含能材料：5-取代四唾含能金屬配合物.含能材料，2011,5: 588-596

　　[2]侯向陽，焦寶娟，范廣，等.含能配合物M(ATZ)--H20液相生成反應的熱動力學研究.延安人學學報(自然科學版)，2008,27: 41-47

　　[3]肖鶴鳴，陳兆旭.四噸化學的現(xiàn)代理論.北京：科技出版社，2002

　　[4]尚靜，張建國，崔燕，等.含能配合[Zn(DAT)6](C104)2(DAT= 1,5-二氨基四[￠)的合成、晶體結(jié)構(gòu)及性質(zhì).化學學報，2010,68: 233-238

　　[5]馮金玲，張建國，李志敏等.高氮含能配合物[Co(AZT)2(H20)4](HTN R)2'4H20的合成、晶體結(jié)構(gòu)及性質(zhì).化學學報，2010, 68: 2493-2499

　　[6]李志敏，張建國，張同來，等.確基四嘩及其高氮化合物.化學進展，2010,22:639-647

　　[7]劉曉建，張慧娟，林秋漢，等.唑類含能離子化合物的合成研究進展.火炸藥學報，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

　　參考文獻三：

　　[1]汪曉蓮，李澄，邵明，陳宏芳.2008.粒子探測技術(shù)，中國科學技術(shù)大學出版社.

　　[2]劉佳.2013.LHAASO-KM2A探測器與原型陣列設計及性能研宄，博士論文，中國科學院高能物理研究所

　　[3]郝新軍，劉樹彬，趙雷等.2012.羊八井大型水契倫科夫探測器中雙增益大動態(tài)范圍前放的研制，核電子學與探測技術(shù)，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.