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| 1 | 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 |
| 2 | Long-term effect of aspirin on cancer risk in carriers of hereditary colorectal cancer: an analysis from the CAPP2 randomised controlled trial显示文摘 | John Burn Anne-Marie Gerdes Finlay Macrae Jukka-Pekka Mecklin Gabriela Moeslein Sylviane Olschwang Diane Eccles D Gareth Evans Eamonn R Maher Lucio Bertario Marie-Luise Bisgaard Malcolm G Dunlop Judy WC Ho Shirley V Hodgson Annika Lindblom Jan Lubinski Pa | 2011 | The Lancet2011，，9809： | 3 |
| 3 | 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 |
| 4 | 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 |
| 5 | Relative importance of enterochromaffin cell hyperplasia, anxiety, and depression in postinfectious IBS显示文摘 | Simon P Dunlop David Jenkins Keith R Neal Robin C Spiller | 2003 | Gastroenterology2003，，6： | 2 |
| 6 | Analytical development of loadability characteristics for EHV and UHV transmission line显示文摘 | Dunlop R D Gutman R Marchenko P P | 1979 | IEEE Trans on Power Apparatus and Systems1979，98，2： | 1 |
| 7 | Analytical development of loadability characteristics for EHV and UHV transmission line显示文摘 | DUNLOP R D GUTMAN R MARCHENKO P P | 1979 | IEEE Trans on Power Apparatus and System1979，98，2： | 1 |
| 8 | Novel use of hand fracture fixation plates in the surgical stabilisation of flail chest显示文摘 | DUNLOP R L TIONG W VEERASINGAM D | 2010 | J Plast Reeonstr Aesthet Surg2010，63，1： | 1 |
| 9 | Analytical de-velopment of loadability characteristics for EHV and UHV transmission lines显示文摘 | R Gutman P P Marchenko | 1979 | IEEE Transactions on Power Ap-paratus and System1979，98，2： | 1 |
| 10 | Precipitation and aging in high conductivity CuCr alloys with additions of zirconium and magnesium 显示文摘 | Tang N Y Taplin D M R Dunlop G L | 1985 | Mater Sci Tech1985，1，4： | 1 |
| 11 | Striking denervation of neuro- muscular junctions without lumbar motoneuron loss in geriatric mouse muscle 显示文摘 | Chai R J Vukovic J Dunlop S | 2011 | PLoS One2011，6，28： | 1 |
| 12 | Precipitation and aging in high-conductivity Cu-Cr alloys with additions of zirconium and magnesium 显示文摘 | TANG N Y TAPLIN D M R DUNLOP G L | 1985 | Mater Sci Tech1985，1，4： | 1 |
| 13 | Omnidirectional hexapod walking and efficient gaits using restrictedness显示文摘 | Fielding M R Dunlop G R | 2004 | The International Journal of Robotics Research2004，23，1011： | 1 |
| 14 | Analytical development of loadability characteristics for EHV and UHV transmission line显示文摘 | DUNLOP R D GUTMAN R MARCHENKO P P | 1979 | IEEE Transactions on Power Apparatus and System1979，98，2： | 1 |
| 15 | Turbine- generator shaft torques and fatigue, Part I : simulation methods and fatigue analysis 显示文摘 | JACKSON M C UMANS S D DUNLOP R D | 1979 | IEEE Trans on Power Apparatus and Systems1979，98，6： | 1 |
| 16 | Omnidirectional hexapod walking and efficient gaits using restrictedness显示文摘 | Fielding M R Dunlop G R | 2004 | The International Journal of Robotics Research2004，23，1011： | 1 |
| 17 | Dynamic equivalents for average system frequency behavior following major distur- bances显示文摘 | CHAN M L DUNLOP R D SCHWEPPE F | 1972 | 1EEE Transactions on Power Apparatus and Systems1972，91，4： | 1 |
| 18 | Analytical development of loadability characteristics for EGV and UHV transmission lines 显示文摘 | DUNLOP R D GUTMAN R MARCHENKO P P | 1979 | IEEE Transactions on Power Apparatus and System1979，98，2： | 1 |
| 19 | Analytic development of loadability characteristics for EHV and UHV transmission lines显示文摘 | DUNLOP R D GUTMAN R MARCHENKO P P | 1979 | IEEE Trans on Power Apparatus and Systems1979，98，2： | 1 |
| 20 | Mechanoreceptive and Nociceptive Responses in the Central Nervous System of Goldfish (Carassius auratus) and Trout (Oncorhynchus mykiss)显示文摘 | DUNLOP R LAMING P | | 0，，09： | 1 |
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