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Dusty space plasma diagnosis using temporal behavior of polar mesospheric summer echoes during active modification

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Dusty space plasma diagnosis using temporal behavior of polar mesospheric summer echoes during active modification. / Mahmoudian, Alireza; Scales, Wayne; Kosch, Michael et al.
In: Annales Geophysicae, Vol. 29, No. 11, 11.2011, p. 2169-2179.

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Mahmoudian A, Scales W, Kosch M, Senior A, Rietveld M. Dusty space plasma diagnosis using temporal behavior of polar mesospheric summer echoes during active modification. Annales Geophysicae. 2011 Nov;29(11):2169-2179. doi: 10.5194/angeo-29-2169-2011

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Mahmoudian, Alireza ; Scales, Wayne ; Kosch, Michael et al. / Dusty space plasma diagnosis using temporal behavior of polar mesospheric summer echoes during active modification. In: Annales Geophysicae. 2011 ; Vol. 29, No. 11. pp. 2169-2179.

Bibtex

@article{e38ef3881ca44f03956ede84334017a0,
title = "Dusty space plasma diagnosis using temporal behavior of polar mesospheric summer echoes during active modification",
abstract = "The objective of this paper is to study the effect of different plasma and dust parameters on Polar Mesospheric Summer Echoes (PMSE) temporal behavior after turn-on and turn-off of radio wave heating and to use these responses to diagnose the properties of the dust layer. The threshold radar frequency and dust parameters for the enhancement or suppression of radar echoes after radio wave heating turn-on are investigated for measured mesospheric plasma parameters. The effect of parameters such as the electron temperature enhancement during heating, dust density, dust charge polarity, ion-neutral collision frequency, electron density and dust radius on the temporal evolution of electron irregularities associated with PMSE are investigated. The possible diagnostic information for various charged dust and background plasma quantities using the temporal behavior of backscattered radar power in active experiments is discussed. The computational results are used to make predictions for PMSE active modification experiments at 7.9, 56, 139, 224 and 930MHz corresponding to existing radar facilities. Data from a 2009 VHF (224 MHz) experiment at EISCAT is compared with the computational model to obtain dust parameters in the PMSE. ",
author = "Alireza Mahmoudian and Wayne Scales and Michael Kosch and Andrew Senior and Mike Rietveld",
note = "{\textcopyright} Author(s) 2011. This work is distributed under the Creative Commons Attribution 3.0 License.",
year = "2011",
month = nov,
doi = "10.5194/angeo-29-2169-2011",
language = "English",
volume = "29",
pages = "2169--2179",
journal = "Annales Geophysicae",
issn = "0992-7689",
publisher = "European Geosciences Union",
number = "11",

}

RIS

TY - JOUR

T1 - Dusty space plasma diagnosis using temporal behavior of polar mesospheric summer echoes during active modification

AU - Mahmoudian, Alireza

AU - Scales, Wayne

AU - Kosch, Michael

AU - Senior, Andrew

AU - Rietveld, Mike

N1 - © Author(s) 2011. This work is distributed under the Creative Commons Attribution 3.0 License.

PY - 2011/11

Y1 - 2011/11

N2 - The objective of this paper is to study the effect of different plasma and dust parameters on Polar Mesospheric Summer Echoes (PMSE) temporal behavior after turn-on and turn-off of radio wave heating and to use these responses to diagnose the properties of the dust layer. The threshold radar frequency and dust parameters for the enhancement or suppression of radar echoes after radio wave heating turn-on are investigated for measured mesospheric plasma parameters. The effect of parameters such as the electron temperature enhancement during heating, dust density, dust charge polarity, ion-neutral collision frequency, electron density and dust radius on the temporal evolution of electron irregularities associated with PMSE are investigated. The possible diagnostic information for various charged dust and background plasma quantities using the temporal behavior of backscattered radar power in active experiments is discussed. The computational results are used to make predictions for PMSE active modification experiments at 7.9, 56, 139, 224 and 930MHz corresponding to existing radar facilities. Data from a 2009 VHF (224 MHz) experiment at EISCAT is compared with the computational model to obtain dust parameters in the PMSE.

AB - The objective of this paper is to study the effect of different plasma and dust parameters on Polar Mesospheric Summer Echoes (PMSE) temporal behavior after turn-on and turn-off of radio wave heating and to use these responses to diagnose the properties of the dust layer. The threshold radar frequency and dust parameters for the enhancement or suppression of radar echoes after radio wave heating turn-on are investigated for measured mesospheric plasma parameters. The effect of parameters such as the electron temperature enhancement during heating, dust density, dust charge polarity, ion-neutral collision frequency, electron density and dust radius on the temporal evolution of electron irregularities associated with PMSE are investigated. The possible diagnostic information for various charged dust and background plasma quantities using the temporal behavior of backscattered radar power in active experiments is discussed. The computational results are used to make predictions for PMSE active modification experiments at 7.9, 56, 139, 224 and 930MHz corresponding to existing radar facilities. Data from a 2009 VHF (224 MHz) experiment at EISCAT is compared with the computational model to obtain dust parameters in the PMSE.

U2 - 10.5194/angeo-29-2169-2011

DO - 10.5194/angeo-29-2169-2011

M3 - Journal article

VL - 29

SP - 2169

EP - 2179

JO - Annales Geophysicae

JF - Annales Geophysicae

SN - 0992-7689

IS - 11

ER -