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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 | The correlations of ions density with geomagnetic activity and solar dynamic pressure in cusp region显示文摘A statistical study of the properties of ions (O+, He+ and H+) measured by the Cluster-II in cusp region as a function of the solar wind dynamic pressure and geomagnetic index Kp respectively was made dur-ing the summer and fall of 2001-2003. The main results are that: (1) O+ ion density responds in a sig-nificant way to geomagnetic index Kp, and He+ ion density is not correlated with geomagnetic index Kp, both of them have a significant positive correlation with solar wind dynamic pressure; (2) H+ ion density is also observed to increase with solar wind dynamic pressure, and not correlated with geomagnetic index Kp. | GUO JianGuang SHI JianKui ZHANG TieLong LIU ZhenXing A. FAZAKERLEY H. REME I. DANDOURAS E. LUOEK | 2007 | Chinese Science Bulletin2007，52，7： | 3 |
| 3 | 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 |
| 4 | Novel attenuated chikungunya vaccine candidates elicit protective immunity in C57BL/6 mice 显示文摘 | Halleng/ird D Kakoulidou M Lulla A Kfimmerer BM Johansson DX Mutso M Lulla V Fazakerley JK Roques P Le Grand R Merits A Liljestr6m P | 2014 | J Viroh2014，88，5： | 1 |
| 5 | The Double Starplasma electron and current experiment显示文摘 | Fazakerley A N Carter P J Watson G | 2005 | Ann Geophys2005，23，8： | 1 |
| 6 | Mapping insulin/GLUT4 circuitry显示文摘 | Rowland AF Fazakerley DJ James DE | | 0，，： | 1 |
| 7 | The incorporation of acetate, stearate and D-β-hydroxybutyrate into milk fat by the isolated perfused mammary gland of the goat显示文摘 | Linzell J L Annison E F Fazakerley S | 1967 | Journal of Biochemistry1967，，104： | 1 |
| 8 | Virus demyelination显示文摘 | Fazakerley JK Walker R | 2003 | J Neurovirol2003，9，： | 1 |
| 9 | GLUT4 Exocytosis显示文摘 | St?ckli J Fazakerley DJ James DE | 2011 | J Cell Sci2011，124，24： | 1 |
| 10 | GLUT4 exocytosis显示文摘 | Stoeckli J Fazakerley D J James D E | 2011 | J Cell Sci2011，124，24： | 1 |
| 11 | Lymphoproliferative disease in mice infected with murine gammaherpesvirus 68显示文摘 | Sunil - Chandra N P Arno J Fazakerley J | 1994 | Am J Pathol1994，145，4： | 1 |
| 12 | Pathogenesis of virus-induced demyelination显示文摘 | Buchmcier MJ | 1993 | Adv Virus Res1993，42，： | 1 |
| 13 | GLUT4 exocytosis显示文摘 | Stuckli J Fazakerley D J James DE | 2011 | J Cell Sci2011，，： | 1 |
| 14 | Observation of energetic electrons within magnetic islands显示文摘 | Chen L-J Bhattacharjee A Puhl-Quinn P A Yang H Bessho N Imada S Mühlbachler S Daly P W Lefebvre B Khotyaintsev Y Vaivads A Fazakerley A Georgescu E | 2008 | Nature Physics2008，，1： | 1 |
| 15 | Mapping insulin/GLUT4 circuitry显示文摘 | Rowland AF Fazakerley DJ James DE | 2011 | Traffic2011，12，6： | 1 |
| 16 | GLUT4 exoeytosis显示文摘 | Stockli J Fazakerley D J James DE | 2011 | J Cell Sci2011，，： | 1 |
| 17 | Dynamic Adipocyte Phosphoproteome Reveals that Akt Directly Regulates mTORC2显示文摘 | Sean J. Humphrey Guang Yang Pengyi Yang Daniel J. Fazakerley Jacqueline St?ckli Jean Y. Yang David E. James | 2013 | Cell Metabolism2013，，6： | 1 |
| 18 | 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 |
| 19 | A common trafficking route for GLUT4 in cardiomyocytes in response to insulin,contraction and energy-status signalling 显示文摘 | Fazakerley DJ Lawrence SP Lizunov VA | 2009 | J cell sci2009，122，5： | 1 |
| 20 | The oxidation and utilization of palmitate,stearate,oleate and acetate by the mammary gland of the fed goat m relation to their overall metabolism,and the role of plasma phosphohpids and neutral lipids in milk-fat synthesis 显示文摘 | Annison E F Linzell J L Fazakerley S | 1967 | Biochem J1967，102，3： | 1 |
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