Kosch, M.J. and Mjølhus, E. and Ashrafi, M. and Rietveld, M.T. and Yeoman, T. and Nozawa, S. (2011) Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT. Journal of Geophysical Research - Space Physics, 116 (A03322). pp. 1-9. ISSN 0148-0227Full text not available from this repository.
We experimentally observe the location and angular size of the high-frequency (HF) radio window in the bottomside ionosphere, which permits radio wave propagation to the topside ionosphere, with high angular resolution at the European Incoherent Scatter (EISCAT) facility. HF pump-induced ion line enhancements were observed by the EISCAT UHF incoherent scatter radar on the ionospheric bottomside and topside. The radar zenith angle was scanned in small steps in the magnetic meridian. The HF pump duty cycle was deliberately kept low enough to minimize the growth of artificial field-aligned irregularities. The locations of the bottomside radio window and topside enhanced radar echoes are consistent with the expected position determined by ray tracing performed using the observed plasma densities.
|Journal or Publication Title:||Journal of Geophysical Research - Space Physics|
|Additional Information:||Copyright (2011) American Geophysical Union. Further reproduction or electronic distribution is not permitted.|
|Uncontrolled Keywords:||eiscat ; heating DCS-publications-id ; art-1031 ; DCS-publications-credits ; iono-fa ; DCS-publications-personnel-id ; 7 ; DCS-publications-personnel-id ; 66|
|Subjects:||Q Science > Q Science (General)|
|Departments:||Faculty of Science and Technology > School of Computing & Communications|
Faculty of Science and Technology > Physics
|Deposited By:||Dr Steve Marple|
|Deposited On:||31 May 2011 12:00|
|Last Modified:||06 Aug 2013 05:01|
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