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Sökning: WFRF:(Thide B.)

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  • Morosan, D. E., et al. (författare)
  • LOFAR tied-array imaging of Type III solar radio bursts
  • 2014
  • Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 568, s. articl no. A67-
  • Tidskriftsartikel (refereegranskat)abstract
    • Context. The Sun is an active source of radio emission which is often associated with energetic phenomena such as solar flares and coronal mass ejections (CMEs). At low radio frequencies (
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  • Blagoveshchenskaya, N.F., Kornienko, V.A., Borisova, T.D., Thidé, B., Kosch, M.J., Rietveld, M.T., Mishin, E.V., Luk'yanova, R.Y. and Troshichev, O.A. (författare)
  • Ionospheric HF pump wave triggering of local auroral activation.
  • 2001
  • Ingår i: Journal of Geophysical Research. ; 106, s. 29071-29089
  • Tidskriftsartikel (refereegranskat)abstract
    • Experimental results from ionospheric HF pumping experiments in the nightside auroral E region above Tromso are reported. We found intriguing evidence that a modification of the ionosphere-magnetosphere coupling, due to the effects of powerful HF waves be
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  • Carozzi, TD, et al. (författare)
  • Full polarimetry measurements of stimulated electromagnetic emissions: First results
  • 2001
  • Ingår i: JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS. - : AMER GEOPHYSICAL UNION. - 0148-0227. ; 106:A10, s. 21395-21407
  • Tidskriftsartikel (refereegranskat)abstract
    • A theory and technique for the measurement of the full state of polarization (SOP) for wideband electromagnetic HF emissions from the ionosphere are introduced. The technique was employed in a recent experiment at the Sura ionospheric HF pumping facility
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  • Eliasson, B., et al. (författare)
  • Simulation study of the interaction between large-amplitude HF radio waves and the ionosphere
  • 2007
  • Ingår i: Geophysical Research Letters. - 0094-8276 .- 1944-8007. ; 34:L0610
  • Tidskriftsartikel (refereegranskat)abstract
    • The time evolution of a large-amplitude electromagnetic (EM) wave injected vertically into the overhead ionosphere is studied numerically. The EM wave has a carrier frequency of 5 MHz and is modulated as a Gaussian pulse with a width of approximately 0.1 milliseconds and a vacuum amplitude of 1.5 V/m at 50 km. This is a fair representation of a modulated radio wave transmitted from a typical high-power HF broadcast station on the ground. The pulse is propagated through the neutral atmosphere to the critical points of the ionosphere, where the L-O and R-X modes are reflected, and back to the neutral atmosphere. We observe mode conversion of the L-O mode to electrostatic waves, as well as harmonic generation at the turning points of both the R-X and L-O modes, where their amplitudes rise to several times the original ones. The study has relevance for ionospheric interaction experiments in combination with ground-based and satellite or rocket observations.
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