Computer Science – Sound
Scientific paper
Jan 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kosis..23..113p&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 23, Jan.-Feb. 1985, p. 113-122. In Russian.
Computer Science
Sound
1
Ionospheric Sounding, Plasma Turbulence, Plasma-Electromagnetic Interaction, Radio Probing, Space Plasmas, Cavitons, Electron Acceleration, Ionospheric Disturbances, Plasma Resonance, Solitary Waves, Time Lag
Scientific paper
An intense-turbulence mechanism is proposed to explain long delays of excitation at characteristic plasma resonant frequencies during the external radio sounding of the ionosphere. Owing to ponderomotive forces the plasma density goes to zero in the near field of the emitting antenna; owing to modulational striction instability in the pump wave field, a turbulent region develops with the formation of a soliton structure, and cavitons arise and subsequently collapse. When the satellite intersects the turbulent region, long excitations at the characteristic frequencies are determined by the intersection by the receiving antennas of both stable and unstable solitons moving at velocities less than the satellite velocity. A surface-wave excitation mechanism is proposed to explain electron acceleration observed on the Intercosmos-19 satellite.
Pulinets S. A.
Selegei V. V.
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