Haldoupis, C. Schlegel, K. Hussey, G.
Published in
Annales Geophysicae
In the theory of E-region plasma instabilities, the ambient electric field and electron density gradient are both included in the same dispersion relation as the key parameters that provide the energy for the generation and growth of electrostatic plasma waves. While there exist numerous measurements of ionospheric electric fields, there are very f...
Kero, A. Bösinger, T. Pollari, P. Turunen, E. Rietveld, M.
Published in
Annales Geophysicae
The ionospheric electron gas can be heated artificially by a powerful radio wave. According to our modeling, the maximum effect of this heating occurs in the D-region where the electron temperature can increase by a factor of ten. Ionospheric plasma parameters such as Ne,Te and Ti are measured by EISCAT incoherent scatter radar on a routine basis. ...
Guio, P. Børve, S. Pécseli, H. L. Trulsen, J.
Published in
Annales Geophysicae
Low frequency electrostatic waves are studied in magnetized plasmas with an electron temperature which varies with position in a direction perpendicular to the magnetic field. For wave frequencies below the ion cyclotron frequency, the waves need not follow any definite dispersion relation. Instead a band of phase velocities is allowed, with a rang...
Lilensten, J. Amblard, P. O.
Published in
Annales Geophysicae
We examine the oscillations of the meridional neutral wind in the F region as seen by the EISCAT radar. We propose an interpretation in term of eddies (tourbillons) of typical size of a few tens to a few hundreds of kilometers. The observed rotation velocity is a few hundreds of meters per second. We suggest that the tourbillons are a common featur...
Moen, J. Carlson, H. C. Milan, S. E. Shumilov, N. Lybekk, B. Sandholt, P. E. Lester, M.
Published in
Annales Geophysicae
The 2D morphology of coherent HF radar and optical cusp aurora has been studied for conditions of predominantly southward IMF conditions, which favours low-latitude boundary layer reconnection. Despite the variability in shape of radar cusp Doppler spectra, the spectral width criterion of ≥220 m s−1 proves to be a robust cusp discriminator. For ext...
MacDougall, J. W. Andre, D. A. Sofko, G. J. Huang, C.-S. Koustov, A. V.
Published in
Annales Geophysicae
Based on modeling of the perturbations in power and elevation angle produced by travelling ionospheric disturbances (TIDs), and observed by the Super Dual Auroral Radar Network, procedures for determining the TID properties are suggested. These procedures are shown to produce reasonable agreement with those properties of the TIDs that can be measur...
McWilliams, K. A. Yeoman, T. K. Cowley, S. W. H.
Published in
Annales Geophysicae
Line-of-sight Doppler velocities from the SuperDARN CUTLASS HF radar pair have been combined to produce the first two-dimensional vector measurements of the convection pattern throughout the ionospheric footprint of a flux transfer event (a pulsed ionospheric flow, or PIF). Very stable and moderate interplanetary magnetic field conditions, along wi...
Gupta, J. K. Singh, Lakha
Published in
Annales Geophysicae
Ionospheric electron content (IEC) observed at Delhi (geographic co-ordinates: 28.63°N, 77.22°E; geomagnetic co-ordinates: 19.08°N, 148.91E; dip Latitude 24.8°N), India, for the period 1975/80 and 1986/89 belonging to an ascending phase of solar activity during first halves of solar cycles 21 and 22 respectively have been used to study the diurnal,...
Uspensky, M. Eglitis, P. Opgenoorth, H. Starkov, G. Pulkkinen, T. Pellinen, R.
Published in
Annales Geophysicae
Observations and modelling are presented which illustrate the ability of the Finland CUTLASS HF radar to monitor the afternoon-evening equatorward auroral boundary during weak geomagnetic activity. The subsequent substorm growth phase development was also observed in the late evening sector as a natural continuation of the preceding auroral oval dy...
Stening, R. J. Jacobi, C.
Published in
Annales Geophysicae
The lunar semidiurnal tide in winds measured at around 90 km altitude has been isolated with amplitudes observed up to 4 m s−1. There is a marked amplitude maximum in October and also a considerable phase variation with season. The average variation of phase with height indicated a vertical wavelength of more than 80 km but this, and other results,...