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Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT

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Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT. / Kosch, M.J.; Mjølhus, E.; Ashrafi, M. et al.
In: Journal of Geophysical Research, Vol. 116, No. A03322, 22.03.2011, p. 1-9.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

Kosch, MJ, Mjølhus, E, Ashrafi, M, Rietveld, MT, Yeoman, T & Nozawa, S 2011, 'Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT', Journal of Geophysical Research, vol. 116, no. A03322, pp. 1-9. https://doi.org/10.1029/2010JA016014

APA

Kosch, M. J., Mjølhus, E., Ashrafi, M., Rietveld, M. T., Yeoman, T., & Nozawa, S. (2011). Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT. Journal of Geophysical Research, 116(A03322), 1-9. https://doi.org/10.1029/2010JA016014

Vancouver

Kosch MJ, Mjølhus E, Ashrafi M, Rietveld MT, Yeoman T, Nozawa S. Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT. Journal of Geophysical Research. 2011 Mar 22;116(A03322):1-9. doi: 10.1029/2010JA016014

Author

Kosch, M.J. ; Mjølhus, E. ; Ashrafi, M. et al. / Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT. In: Journal of Geophysical Research. 2011 ; Vol. 116, No. A03322. pp. 1-9.

Bibtex

@article{5de0c552fb3e40cfa0f5ee48f2ba80ac,
title = "Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT",
abstract = "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.",
keywords = "eiscat, heating DCS-publications-id, art-1031, DCS-publications-credits, iono-fa, DCS-publications-personnel-id, 7, 66",
author = "M.J. Kosch and E. Mj{\o}lhus and M. Ashrafi and M.T. Rietveld and T. Yeoman and S. Nozawa",
note = "Copyright (2011) American Geophysical Union. Further reproduction or electronic distribution is not permitted.",
year = "2011",
month = mar,
day = "22",
doi = "10.1029/2010JA016014",
language = "English",
volume = "116",
pages = "1--9",
journal = "Journal of Geophysical Research",
issn = "0148-0227",
publisher = "American Geophysical Union",
number = "A03322",

}

RIS

TY - JOUR

T1 - Angular dependence of pump-induced bottomside and topside ionospheric plasma turbulence at EISCAT

AU - Kosch, M.J.

AU - Mjølhus, E.

AU - Ashrafi, M.

AU - Rietveld, M.T.

AU - Yeoman, T.

AU - Nozawa, S.

N1 - Copyright (2011) American Geophysical Union. Further reproduction or electronic distribution is not permitted.

PY - 2011/3/22

Y1 - 2011/3/22

N2 - 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.

AB - 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.

KW - eiscat

KW - heating DCS-publications-id

KW - art-1031

KW - DCS-publications-credits

KW - iono-fa

KW - DCS-publications-personnel-id

KW - 7

KW - 66

UR - http://www.scopus.com/inward/record.url?scp=79953022189&partnerID=8YFLogxK

U2 - 10.1029/2010JA016014

DO - 10.1029/2010JA016014

M3 - Journal article

VL - 116

SP - 1

EP - 9

JO - Journal of Geophysical Research

JF - Journal of Geophysical Research

SN - 0148-0227

IS - A03322

ER -