The Bow Shock Current System

[1]  R. Kataoka,et al.  Generation of field‐aligned current (FAC) and convection through the formation of pressure regimes: Correction for the concept of Dungey's convection , 2016 .

[2]  W. Scales,et al.  Investigation of a rare event where the polar ionospheric reverse convection potential does not saturate during a period of extreme northward IMF solar wind driving , 2016 .

[3]  R. Lopez The integrated dayside merging rate is controlled primarily by the solar wind , 2016 .

[4]  R. Bruntz,et al.  Linear separation of orthogonal merging component and viscous interactions in solar wind‐geospace coupling , 2014 .

[5]  R. E. López,et al.  Reduction of viscous potential for northward interplanetary magnetic field as seen in the LFM simulation , 2013 .

[6]  S. Solomon,et al.  CMIT study of CR2060 and 2068 comparing L1 and MAS solar wind drivers , 2012 .

[7]  R. Bruntz,et al.  Simulation of the polar cap potential during periods with northward interplanetary magnetic field , 2012 .

[8]  J. Lyon,et al.  The role of the bow shock in solar wind-magnetosphere coupling , 2011 .

[9]  R. Bruntz,et al.  Role of magnetosheath force balance in regulating the dayside reconnection potential , 2010 .

[10]  R. Bruntz,et al.  Saturation of transpolar potential for large Y component interplanetary magnetic field , 2010 .

[11]  J. Kan,et al.  Bow shock and magnetopause contributions to the cross-tail current from global MHD simulations , 2009 .

[12]  Maria M. Kuznetsova,et al.  Polar cap potential saturation, dayside reconnection, and changes to the magnetosphere , 2009 .

[13]  P. Anderson,et al.  Field-aligned currents in the polar cap during saturation of the polar cap potential , 2008 .

[14]  John Lyon,et al.  The Lyon-Fedder-Mobarry (LFM) global MHD magnetospheric simulation code , 2004 .

[15]  A. Ridley,et al.  Transpolar potential saturation models compared , 2004 .

[16]  G. Siscoe,et al.  Transpolar potential saturation: Roles of region 1 current system and solar wind ram pressure , 2002 .

[17]  G. Siscoe,et al.  Dynamo circuits for magnetopause reconnection , 2002 .

[18]  V. Vasyliūnas Electric field and plasma flow: What drives what? , 2001 .

[19]  K. Powell,et al.  A model of solar wind–magnetosphere–ionosphere coupling for due northward IMF , 2000 .

[20]  P. Roe,et al.  A Solution-Adaptive Upwind Scheme for Ideal Magnetohydrodynamics , 1999 .

[21]  J. Lyon,et al.  MHD model merging with IMF By : Lobe cells, sunward polar cap convection, and overdraped lobes , 1998 .

[22]  C. Meng,et al.  Shape of the open–closed boundary of the polar cap as determined from observations of precipitating particles by up to four DMSP satellites , 1998 .

[23]  J. Lyon,et al.  A first comparison of POLAR magnetic field measurements and magnetohydrodynamic simulation results for field‐aligned currents , 1997 .

[24]  H. Washimi,et al.  3-D magnetic field and current system in the heliosphere , 1996 .

[25]  J. Lyon,et al.  The Earth's magnetosphere is 165 RE long: Self‐consistent currents, convection, magnetospheric structure, and processes for northward interplanetary magnetic field , 1995 .

[26]  R. Spiro,et al.  Generation of region 1 current by magnetospheric pressure gradients , 1994 .

[27]  C. Meng,et al.  DMSP F7 observations of a substorm field‐aligned current , 1991 .

[28]  M. Gussenhoven,et al.  Simultaneous relativistic electron and auroral particle access to the polar caps during interplanetary magnetic field Bz northward: A scenario for an open field line source of auroral particles , 1989 .

[29]  J. Lyon,et al.  The solar wind-magnetosphere-ionosphere current-voltage relationship , 1987 .

[30]  R. Heelis The effects of interplanetary magnetic field orientation on dayside high‐latitude ionospheric convection , 1984 .

[31]  C. Cesarsky,et al.  The maximum energy of cosmic rays accelerated by supernova shocks , 1983 .

[32]  L. Fisk,et al.  Shock acceleration of energetic particles in corotating interaction regions in the solar wind , 1980 .

[33]  T. Potemra,et al.  The amplitude distribution of field-aligned currents at northern high latitudes observed by TRIAD. Interim report , 1975 .

[34]  V. Formisano,et al.  Solar wind interaction with the earth's magnetic field. II - Magnetohydrodynamic bow shock. , 1973 .

[35]  C. O. Hines,et al.  A UNIFYING THEORY OF HIGH-LATITUDE GEOPHYSICAL PHENOMENA AND GEOMAGNETIC STORMS , 1961 .

[36]  J. Dungey Interplanetary Magnetic Field and the Auroral Zones , 1961 .