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Fundamental plasma phenomena studies - explosive transformation of magnetic energy into plasma thermal and kinetic energies
An artificial influence on the operation of
magnetospheric maser.
Artificial excitation and/or stimulation of wave modes;
- Modification of the flux of precipitating particles;
- Modification of reflection index at the ionospheric
footprint of the selected magnetic flux tube.
Galperin Yu.I., L.M.Zelenyi, M.V.Veselov, S.P.Savin, M.M.Mogilevsky, M.I.Yanovsky, V.I.Prokhorenko, N.A.Eismont, V.E.Kunitsyn, I.V.Silin, E.N.Sosnovets, J.Buchner, T.Wiegelmann, Closely-spaced multi-satellite project ROY to study small-scale structures during magnetic field annihilation and strong turbulence in critical magnetospheric regions: results of the phase a, Interball in the [bold]ISTP program[/bold], ed. D.G. Sibeek and K. Kudela, Kluwer Academic Publishers, 55-73, 1999.
An up-to-date progress report on the current status of solar-terrestrial relation studies with an emphasis on observations by the Russian Interball spacecraft and the Czech Magion subsatellites. Papers in the volume describe the various spacecraft in the International Solar-Terrestrial Program and the research questions that they are being used to address. The emphasis is on correlative studies employing multiple instruments and multiple spacecraft. The book begins with a description of each spacecraft active in 1998 and describes the roles they can play in correlative studies. This is followed by an up-to-date status report concerning ongoing studies of the solar wind, foreshock, bow shock, magnetopause, magnetotail, and ionosphere, with an emphasis on the observations made by the four Interball spacecraft. Readership: Researchers and graduate students of space physics and astrophysics.
The ROY Project is aimed to study previously unexplored small-scale phenomena within the so called 'diffusion region' where strong plasma turbulence and magnetic 'reconnection' occur in the critical magnetospheric domains.
An artificial influence on the operation of
magnetospheric maser.
Artificial excitation and/or stimulation of wave modes;
- Modification of the flux of precipitating particles;
- Modification of reflection index at the ionospheric
footprint of the selected magnetic flux tube.