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    题名 作者 年代 出处 被引量
1Capillary continuity or discontinuity in cement pastes 显示文摘TC Powers LE Copeland HM Mann 1959Journal of the PCA Research and Development Laboratories1959,1,2:1
2The seasonal cycle in coupled ocean-atmosphere general circulation models显示文摘C. Covey A. Abe-Ouchi G. J. Boer B. A. Boville U. Cubasch L. Fairhead G. M. Flato H. Gordon E. Guilyardi X. Jiang T. C. Johns H. Le Treut G. Madec G. A. Meehl R. Miller A. Noda S. B. Power E. Roeckner G. Russell E. K. Schneider R. J. Stouffer L. Terray J. 2000Climate Dynamics (-)2000,,10:1
3An analysis of interplanetary sources of geomagnetic storm during November 7-8, 1998显示文摘We analyzed the properties of the solar wind appeared during November 7–8, 1998. Results show that the spaceship ACE spotted a shock (hereinafter referred to as the first shock) at 07:33 UT, November 7. The sheath appeared from the first shock to 22:00 UT November 7. A magnetic cloud-like (MCL) was observed during the period from 22:00 UT November 7 to 11:50 UT, November 8. Another shock was observed at 04:19 UT, November 8 (the second shock). It is apparent that the second shock has entered the rear part of the MCL (MCL_2), though the former part of the MCL (MCL_1) was not affected by the second shock. The main phase of the geomagnetic storm is split into three steps for the convenience of SYM-H index analysis. Step 1 covers the period from the sudden storm commence (SSC) at 08:15 UT, November 7 to the moment of 22:44 UT, November 7. Step 2 starts from 22:44 UT, November 7 and ends at 04:51 UT, November 8. The last step runs from 04:51 UT, November 8 to 06:21 UT, November 8. Step 2 has played a key role in the main development phase of the geomagnetic storm. Analysis of the solar wind properties associated with the main phase shows that the three steps in the main phase have sheath, MCL_1, and MCL_2 as their respective interplanetary source. Specifically, the sheath is covered by the solar wind data from 07:33 UT to 22:00 UT, November 7, MCL1 by the solar wind data from 22:00 UT, November 7 to 04:19 UT November 8, and MCL_2 by the solar wind data from 04:19 UT to 05:57 UT, November 8. MCL_1 had a strong and long lasting so UTh directed magnetic field, allowing it to play a key role in the development of the main phase. MCL_2 made a much smaller contribution to the main development phase, compared with MCL_1.LE GuiMing1,2,3, TANG YuHua1, ZHENG Liang5 & LIU LianGuang4 1 Department of Astronomy, Nanjing University, Nanjing 210093, China 2 National Center for Space Weather, China Meteorological Administration, Beijing 100081, China 3 Key Laboratory of Radiometric Calibration and Validation for Environmental Satellites, China Meteorological Administration (LRCVES/CMA), Beijing 100081, China 4 North China Electric Power University, Beijing 102206, China 5 Graduate University of Chinese Academy of Sciences, Beijing 100049, China 2010Chinese Science Bulletin2010,55,9:1
4The role of surgery in en- dometrial cancer 显示文摘Giede C Le T Power P 2013J Obstet Gynaecol Can2013,35,4:1
5ENSIP: the El Ni?o simulation intercomparison project显示文摘M. Latif K. Sperber J. Arblaster P. Braconnot D. Chen A. Colman U. Cubasch C. Cooper P. Delecluse D. Dewitt L. Fairhead G. Flato T. Hogan M. Ji M. Kimoto A. Kitoh T. Knutson H. Le Treut T. Li S. Manabe O. Marti C. Mechoso G. Meehl S. Power E. Roeckner J. 2001Climate Dynamics (-)2001,,3:1
6Platelet mitochondrial complex Ⅰand Ⅰ+Ⅲ activities do not correlate with cerebral mitochondrial oxidative metabolism显示文摘Powers WJ Haas RH Le T 2011J Cereb Blood Flow Metab2011,31,1:1
7Pyrethrin and pyrethroid exposures in the United States:a longitudinal analysis of incidents reported to poison centers 显示文摘Power LE Sudakin DL 2007J Med Toxicol2007,3,3:1
8Development of a practical large-scale synthesis of denagliptin tosylate显示文摘Patterson D E Powers J D Le Blanc M 2009Organic Process Research&Development2009,13,5:1
9ENSIP: the El Ni?o simulation intercomparison project显示文摘M. Latif K. Sperber J. Arblaster P. Braconnot D. Chen A. Colman U. Cubasch C. Cooper P. Delecluse D. Dewitt L. Fairhead G. Flato T. Hogan M. Ji M. Kimoto A. Kitoh T. Knutson H. Le Treut T. Li S. Manabe O. Marti C. Mechoso G. Meehl S. Power E. Roeckner J. 2001Climate Dynamics (-)2001,,3:1
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