A thermosphere/ionosphere general circulation model with coupled electrodynamics

A new simulation model of upper atmospheric dynamics is presented that includes self-consistent electrodynamic interactions between the thermosphere and ionosphere. This model, which we call the National Center for Atmospheric Research thermosphere-ionosphere-electrodynamic general circulation model (NCAR/TIE-GCM), calculates the dynamo effects of thermospheric winds, and uses the resultant electric fields and currents in calculating the neutral and plasma dynamics. A realistic geomagnetic field geometry is used. Sample simulations for solar maximum equinox conditions illustrate two previously predicted effects of the feedback. Near the magnetic equator, the afternoon uplift of the ionosphere by an eastward electric field reduces ion drag on the neutral wind, so that relatively strong eastward winds can occur in the evening. In addition, a vertical electric field is generated by the low-latitude wind, which produces east-west plasma drifts in the same direction as the wind, further reducing the ion drag and resulting in stronger zonal winds.

[1]  R. Roble,et al.  Electrodynamic effects of thermospheric winds from the NCAR Thermospheric General Circulation Model , 1987 .

[2]  R. Dickinson,et al.  Thermospheric general circulation with coupled dynamics and composition , 1984 .

[3]  R. Dickinson,et al.  Global circulation and temperature structure of thermosphere with high‐latitude plasma convection , 1982 .

[4]  H. G. Mayr,et al.  Tidal decomposition of zonal neutral and ion flows in the earth's upper equatorial thermosphere , 1986 .

[5]  R. W. Spiro,et al.  A model of the high‐latitude ionospheric convection pattern , 1982 .

[6]  H. Rishbeth Ion-drag effects in the thermosphere , 1979 .

[7]  N. Matuura Electric fields deduced from the thermospheric model , 1974 .

[8]  D. Anderson,et al.  The effect of vertical E × B ionospheric drifts on F region neutral winds in the low‐latitude thermosphere , 1974 .

[9]  V. A. Surotkin,et al.  A global numerical model of the thermosphere, ionosphere, and protonosphere of the Earth. , 1990 .

[10]  H. Volland,et al.  A hydromagnetic dynamo of the atmosphere , 1978 .

[11]  Raymond G. Roble,et al.  A coupled thermosphere/ionosphere general circulation model , 1988 .

[12]  H. Volland The atmospheric dynamo , 1976 .

[13]  P. C. Kendall,et al.  Electrical coupling of the E- and F-regions and its effect on F-region drifts and winds , 1974 .

[14]  R. Roble,et al.  Thermospheric tides at equinox: Simulations with coupled composition and auroral forcings: 2. Semidiurnal component , 1991 .

[15]  Raymond G. Roble,et al.  An auroral model for the NCAR thermospheric general circulation model (TGCM) , 1987 .

[16]  H. G. Mayr,et al.  The dynamo of the diurnal tide and its effect on the thermospheric circulation , 1990 .

[17]  R. Dickinson,et al.  Simulation of the thermospheric tides at equinox with the National Center for Atmospheric Research Thermospheric General Circulation Model , 1986 .

[18]  Raymond G. Roble,et al.  A three‐dimensional general circulation model of the thermosphere , 1981 .

[19]  H. Volland Coupling between the neutral tidal wind and the ionospheric dynamo current , 1976 .

[20]  N. Spencer,et al.  An equatorial temperature and wind anomaly (ETWA) , 1991 .

[21]  T. VanZandt,et al.  Magnetic apex coordinates: A magnetic coordinate system for the ionospheric F 2 layer , 1972 .

[22]  Henry Rishbeth,et al.  Polarization fields produced by winds in the equatorial F-region , 1971 .