The spatial structure of the dayside ionospheric trough

Tomographic imaging provides a powerful technique for obtaining images of the spatial distribution of ionospheric electron density at polar latitudes. The method, which involves monitoring radio transmissions from the Navy Navigation Satellite System at a meridional chain of ground receivers, has particular potential for complementing temporal measurements by other observing techniques such as the EISCAT incoherent-scatter radar facility. Tomographic reconstructions are presented here from a two-week campaign in November 1995 that show large-scale structuring of the polar ionosphere. Measurements by the EISCAT radar confirm the authenticity of the technique and provide additional information of the plasma electron and ion temperatures. The dayside trough, persistently observed at high latitudes during a geomagnetically quiet period but migrating to lower latitudes with increasing activity, is discussed in relationship to the pattern of the polarcap convection.

[1]  M. Mallis,et al.  Diurnal and seasonal variability of the southern-hemisphere main ionospheric trough from differential-phase measurements , 1993 .

[2]  I. K. Walker,et al.  The correction for the satellite-receiver longitude difference in ionospheric tomography , 1997 .

[3]  Y. Feldstein,et al.  Electric potential patterns in the northern and southern polar regions parameterized by the interplanetary magnetic field , 1994 .

[4]  N. Maynard,et al.  Empirical high‐latitude electric field models , 1987 .

[5]  I. Häggström,et al.  Plasma convection and auroral precipitation processes associated with the main ionospheric trough at high latitudes , 1988 .

[6]  R. Schunk,et al.  Diurnal Variation of the Dayside, Ionospheric, mid-Latitude Trough in the Southern Hemisphere at 800 km: Model and Measurement Comparison , 1985 .

[7]  I. K. Walker,et al.  EISCAT verification in the development of ionospheric tomography , 1996 .

[8]  J. V. Evans,et al.  On the formation of daytime troughs in the F-region within the plasmasphere , 1983 .

[9]  E. J. Fremouw,et al.  A status report on applying discrete inverse theory to ionospheric tomography , 1994, Int. J. Imaging Syst. Technol..

[10]  I. K. Walker,et al.  Imaging of field-aligned structures in the auroral ionosphere , 1995 .

[11]  S. Quegan,et al.  The role of ion drift in the formation of ionisation troughs in the mid- and high-latitude ionosphere—a review , 1992 .

[12]  J. A. Whalen,et al.  Daytime F layer trough observed on a macroscopic scale , 1987 .

[13]  T. Raymund Comparisons of several ionospheric tomography algorithms , 1995 .

[14]  Cathryn N. Mitchell,et al.  Determination of the vertical electron-density profile in ionospheric tomography: experimental results , 1997 .

[15]  S. E. Pryse,et al.  Improved background representation, ionosonde input and independent verification in experimental ionospheric tomography , 1995 .

[16]  Mike Lockwood,et al.  Dependence of convective flows and particle precipitation in the high‐latitude dayside ionosphere on the X and Y components of the interplanetary magnetic field , 1991 .

[17]  Y. Tulunay,et al.  The noon and midnight mid-latitude trough as seen by Ariel 4 , 1978 .

[18]  S. Quegan,et al.  The mid-latitude trough in the electron concentration of the ionospheric F-layer: a review of observations and modelling , 1983 .

[19]  S. Franke,et al.  Application of computerized tomography techniques to ionospheric research , 1986 .

[20]  S. E. Pryse,et al.  Development of experimental ionospheric tomography , 1994, Int. J. Imaging Syst. Technol..

[21]  Cathryn N. Mitchell,et al.  The effects of receiver location in two-station experimental ionospheric tomography , 1997 .

[22]  J. A. Whalen,et al.  The daytime F layer trough and its relation to ionospheric-magnetospheric convection , 1989 .

[23]  J. Evans,et al.  Millstone Hill measurements on 26 February 1979 during the solar eclipse and formation of a midday F-region trough☆ , 1984 .