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| 1 | 2004年2月11日Cluster卫星和CUTLASS雷达同时观测的磁通量传输事件显示文摘本文分析了2004年2月11日11:00-11:40UT期间Cluster卫星簇的磁通门磁力计(FGM)、等离子体电子及电流试验仪(PEACE)和CUTLASS芬兰雷达对多个磁通量传输事件(FTEs)的同时观测.在此期间,Cluster卫星簇位于北半球外极隙区附近,并于11:18UT左右穿出磁层顶进入磁鞘,四颗卫星同时观测到了多个FTEs,其出现具有准周期性,周期约为130s.利用Cluster四颗卫星的多点同时观测数据,采用最小方向微分法和时空微分方法,我们推断这些FTEs是尺度大小约为(0.87-1.81)RE的准二维结构,其运动方向为东北方向,与Cooling模型预测方向基本一致.CUTLASS芬兰雷达在相应的电离层区域观测到了明显的"极向运动雷达极光"结构,这些结构与Cluster卫星簇观测的FTEs有着很好的对应关系,它们是FTEs的雷达观测特征. | 张清和 刘瑞源 黄际英 M. W. Dunlop 胡红桥 胡泽骏 Y. V. Bogdanova M. Lester | 2008 | 地球物理学报2008，51，1： | 6 |
| 2 | Surveys on magnetospheric plasmas based on the Double Star Project (DSP) exploration显示文摘The equatorial and polar satellites of the Double Star Project (DSP) were launched successfully on December 29, 2003 and July 25, 2004, respectively, and both of them are operating smoothly. The DSP provides a good opportunity for investigat-ing the structure of the magnetosphere. Based on the DSP data collected during 2004, we have surveyed the distribution of the magnetic fields and plasmas in the magnetosphere. It is found that: (1) Near the Earth’s equatorial plane within geo-centric distances of less than 7 RE, the Earth’s magnetic field is dipolar. In the vi-cinity of the magnetopause, the magnetic field is enhanced by a factor of about 1.5, and on the nightside, the magnetic field can vary significantly from the Earth’s di-pole field, likely caused by the presence of the near-Earth tail current sheet. (2) In the day-side magnetosheath, the electron and ion densities are usually both in the range of 10―30 cm?3; the ion and electron temperatures are usually about 200 and 50 eV, respectively. The flow pattern is usually smooth, with a low velocity in the subsolar region and with significantly higher velocities in the dawn and dusk flanks. (3) In the region between the magnetopause and plasmasphere the density is low, approximately 0.5―5 cm?3, and the temperature is high, about 1―10 keV for ions and 0.1―5 keV for electrons. The ion temperature has an apparent anisotropy, with the ratio of the perpendicular and parallel temperatures being about 1.0―1.3 for the night- and dusk-side magnetosphere and about 1.3―2.0 for the day- and dawn-side magnetosphere. There is an evident sunward convection of about 50 km/s in the magnetosphere. On the dawn side, the flow becomes somewhat turbulent, and in the vicinity of the night-noon meridian plane, the convection is rather slow. (4) The high-energy electrons with energies higher than 2 MeV are mainly located in the regions with 3 < L < 4.5; the size of the high-energy electrons area varies with time, it may expand and shrink occasionally according to different solar wind conditions and magnetic activities. | C. P. ESCOUBET C. M. CARR H. RME A. FAZAKERLEY H. LAAKSO I. DANDOURAS M. DUNLOP | 2008 | Science China(Technological Sciences)2008，51，10： | 5 |
| 3 | Properties of Field Aligned Current in Plasma Sheet Boundary Layers in Magnetotail: Cluster Observation显示文摘地在在磁电机尾巴的血浆表边界层(PSBL ) 的排列水流(FAC ) 分发被从簇 4 点大小分析磁场数据统计上学习。结果证明黄昏方面上的 FAC 分发不在在磁电机尾巴的黎明方面上与那一样。在向地的每个方面和尾巴病房上, FAC 出现是不同的;出现和在北半球的 FAC 的平均当前的密度与在南部的半球的那些不同。这暗示 FAC 有黄昏黎明方面不对称现象,极性不对称现象并且内部在磁电机尾巴的半球差别。现在的结果在 FAC 机制上为学习给一条好观察证据。 | 史建魁 程征伟 T. L. Zhang M. Dunlop 刘振兴 | 2009 | Chinese Physics Letters2009，26，2： | 4 |
| 4 | Solar wind transport into magnetosphere caused by magnetic reconnection at high latitude magnetopause during northward IMF: Cluster-DSP conjunction observations显示文摘An event of Cluster-Double Star conjunction observations of magnetic reconnec-tion at high latitude magnetopause nightside of both cusps and solar wind trans-port into magnetosphere caused by such reconnection process has been investi-gated. During northward IMF, Cluster/SC1 observed accelerated flows and ion heating associated with magnetic reconnection at high latitude magnetopause nightside of southern cusp. And Double Star observed cold dense solar wind plasma transported into dayside magnetosphere. The analysis on such conjunction observations shows that: (1) during northward IMF, magnetic reconnection occurs at high latitude nightside of southern cusp, accompanied by accelerated flows that are observed by Cluster/SC1; (2) the direction of the accelerated flows, with its sunward component Vx, dawnward component Vy, northward component Vz, is quite consistent with the theoretical anticipation under the condition of northward IMF with dawnward component By; (3) reconnection can heat plasma more in par-allel direction than in perpendicular direction, to a level of about 4 keV; (4) with reconnection taking place at high latitude magnetopause nightside of the southern cusp, TC-1 observed cold and dense plasma transported into magnetosphere; (5) by reconnection at high latitude magnetopause nightside of both cusps, solar wind flux tube can be captured by magnetosphere and pulled into dayside magneto-sphere. This event presents further observational evidence for magnetic reconnec-tion at high latitude magnetopause nightside of both cusps as an important mech-anism of sol-ar w-ind transport into magnetosphere. | M. DUNLOP E. LUCEK H. RME C. M. CARR | 2008 | Science China(Technological Sciences)2008，51，10： | 3 |
| 5 | Solar wind entry via flux tube into magnetosphere observed by Cluster measurements at dayside magnetopause during southward IMF显示文摘By analyzing hot ion and electron parameters together with magnetic field measurements from Cluster, an event of magnetopause crossing of the spacecraft has been investigated. At the latitude of about 40° and magnetic local time (MLT) of 13:20 during the southward interplanetary magnetic field (IMF), a transition layer was observed, with the magnetospheric field configuration and cold dense plasma features of the magnetosheath. The particle energy-time spectrograms inside the layer were similar to but still a little different from those in the magnetosheath, obviously indicating the solar wind entry into the magnetosphere. The direction and magnitude of the accelerated ion flow implied that reconnection might possibly cause such a solar wind entry phenomenon. The bipolar signature of the normal magnetic component BN in magnetopause coordinates further supported happening of reconnection there. The solar wind plasma flowed toward the magnetopause and entered the magnetosphere along the reconnected flux tube. The magnetospheric branch of the reconnected flux tube was still inside the magnetosphere after reconnection and supplied the path for the solar wind entry into the dayside magnetosphere. The case analysis gives observational evidence and more details of how the reconnection process at the dayside low latitude magnetopause caused the solar wind entry into the magnetosphere. | M. Dunlop A. Balogh H. Rème Y. V. Bogdanova A. Fazakerley | 2009 | Science China(Technological Sciences)2009，52，7： | 2 |
| 6 | The Cluster Magnetic Field Investigation: overview of in-flight performance and initial results显示文摘 | Balogh A. Carr C. M. Acu?a M. H. Dunlop M. W. Beek T. J. Brown P. Fornacon K.-H. Georgescu E. Glassmeier K.-H. Harris J. Musmann G. Oddy T. Schwingenschuh K | 1999 | Annales Geophysicae1999，，123： | 1 |
| 7 | The effect of silicon content on the microstructure and creep behavior in die-cast magnesium AS alloys显示文摘 | M. S. Dargusch G. L. Dunlop A. L. Bowles K. Pettersen P. Bakke | 2004 | Metallurgical and Materials Transactions A2004，，6： | 1 |
| 8 | Spatial distribution of rolled up Kelvin-Helmholtz vortices at Earth’s dayside and flank magnetopause显示文摘 | Taylor M. G. G. T. Hasegawa H. Lavraud B. Phan T. Escoubet C. P. Dunlop M. W. Bogdanova Y. V. Borg A. L. Volwerk M. Berchem J. Constantinescu O. D. Eastwood J. P. Masson A. Laakso H. Soucek J. Fazakerley A. N. Frey H. U. Panov E. V. Shen C. Shi J. K. Sibe | 2012 | 2012 (263)2012，，263： | 1 |
| 9 | Multiple Flux Rope Events at the High-Latitude Magnetopause: Cluster/Rapid Observation on 26 January, 2001显示文摘 | Z. Y. Pu Q. -G. Zong T. A. Fritz C. J. Xiao Z. Y. Huang S. Y. Fu Q. Q. Shi M. W. Dunlop K. -H. Glassmeier A. Balogh P. Daly H. Reme J. Dandouras J. B. Cao Z. X. Liu C. Shen J. K. Shi | 2005 | Surveys in Geophysics (-)2005，，1： | 1 |
| 10 | The effect of silicon content on the microstructure and creep behavior in die-cast magnesium AS alloys显示文摘 | M. S. Dargusch G. L. Dunlop A. L. Bowles K. Pettersen P. Bakke | 2004 | Metallurgical and Materials Transactions A2004，，6： | 1 |
| 11 | THE CLUSTER MAGNETIC FIELD INVESTIGATION显示文摘 | A. Balogh M. W. Dunlop S. W. H. Cowley D. J. Southwood J. G. Thomlinson K. H. Glassmeier G. Musmann H. LüHR S. Buchert M. H. Acu?A D. H. Fairfield J. A. Slavin W. Riedler K. Schwingenschuh M. G. Kivelson | 1997 | Space Science Reviews (-)1997，，1： | 1 |
| 12 | Toll-like receptors in inflammation, infection and cancer显示文摘 | Keqiang Chen Jian Huang Wanghua Gong Pablo Iribarren Nancy M. Dunlop Ji Ming Wang | 2007 | International Immunopharmacology2007，，10： | 1 |
| 13 | The effect of silicon content on the microstructure and creep behavior in die-cast magnesium AS alloys显示文摘 | M. S. Dargusch G. L. Dunlop A. L. Bowles K. Pettersen P. Bakke | 2004 | Metallurgical and Materials Transactions A2004，，6： | 1 |
| 14 | The link between hyperglycaemia and diabetic nephropathy显示文摘 | R. G. Larkins M. E. Dunlop | 1992 | Diabetologia1992，，6： | 1 |
| 15 | The relative roles of advanced glycation, oxidation and aldose reductase inhibition in the development of experimental diabetic nephropathy in the Sprague-Dawley rat显示文摘 | T. Soulis-Liparota M. E. Cooper M. Dunlop G. Jerums | 1995 | Diabetologia1995，，4： | 1 |
| 16 | Inheritance of phosphorus response in white clover (Trifolium repens L.)显示文摘 | J. R. Caradus A. D. Mackay S. Wewala J. Dunlop A. Hart J. Bosch M. G. Lambert M. J. M. Hay | 1992 | Plant and Soil (-)1992，，1： | 1 |
| 17 | The influence of potassium content on the kinetics of potassium influx into excised ryegrass and barley roots显示文摘 | Anthony D. M. Glass James Dunlop | 1978 | Planta1978，，1： | 1 |
| 18 | The effect of silicon content on the microstructure and creep behavior in die-cast magnesium AS alloys显示文摘 | M. S. Dargusch G. L. Dunlop A. L. Bowles K. Pettersen P. Bakke | 2004 | Metallurgical and Materials Transactions A2004，，6： | 1 |
| 19 | Amiloride is neuroprotective in an MPTP model of Parkinson’s disease显示文摘 | Robert L. Arias Mei-Li A. Sung Dmytro Vasylyev Mei-Yi Zhang Kristin Albinson Katie Kubek Natasha Kagan Chad Beyer Qian Lin Jason M. Dwyer Margaret M. Zaleska Mark R. Bowlby John Dunlop Michael Monaghan | 2008 | Neurobiology of Disease2008，，3： | 1 |
| 20 | Near-Earth bursty bulk flows and AE index显示文摘With the 4-s resolution data of the magnetometer and the ion plasma analyzer on TC-1 from June to November of each year during the period of 2004―2006, we statistically analyzed the occurrence rate of both convective and field-aligned bursty flows (FABFs). A near-Earth bursty bulk flow (NEBBF) occurred during both the quiet time and substorm process. In general, the magnetic field and the plasma density began oscillating with the appearance of the NEBBF associated with a distinct increase of the AE index. The increase of AE index during the NEBBF was more than 100 nT in both quiet time and substorm process. The statistical analysis indicated that the occurrence rates of the FABFs were nearly the same in the dif-ferent stages of the AE index, but the occurrence rate of the NEBBFs was much higher in the growth stage of the AE index, indicating that the NEBBFs were di-rectly related to the growth and expansion phases of the substorm. The observa-tions suggested that the quite large number of BBFs from the mid magnetotail could enter into the near-Earth tail and play important role in triggering the sub-storm onset. | W BAUMJOHANN M. W. DUNLOP C. CARR H. RME | 2008 | Science China(Technological Sciences)2008，51，10： | 1 |
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