Home > Research > Publications & Outputs > Dusty Space Plasma Diagnosis Using the Behavior...

Electronic data

  • agutmpl1 - Alireza

    Rights statement: An edited version of this paper was published by AGU. Copyright 2018 American Geophysical Union. Mahmoudian, A., Senior, A., Scales, W. A., Kosch, M. J., & Rietveld, M. T. (2018). Dusty space plasma diagnosis using the behavior of polar mesospheric summer echoes during electron precipitation events. Journal of Geophysical Research: Space Physics, 123, 7697–7709. https://doi.org/10.1029/2018JA025395

    Accepted author manuscript, 1.54 MB, PDF document

    Available under license: CC BY-NC: Creative Commons Attribution-NonCommercial 4.0 International License

Links

Text available via DOI:

View graph of relations

Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Published

Standard

Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events. / Mahmoudian, A.; Senior, A.; Scales, W.A. et al.
In: Journal of Geophysical Research: Space Physics, Vol. 123, No. 9, 09.2018, p. 7697-7709.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Mahmoudian, A, Senior, A, Scales, WA, Kosch, MJ & Rietveld, MT 2018, 'Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events', Journal of Geophysical Research: Space Physics, vol. 123, no. 9, pp. 7697-7709. https://doi.org/10.1029/2018JA025395

APA

Mahmoudian, A., Senior, A., Scales, W. A., Kosch, M. J., & Rietveld, M. T. (2018). Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events. Journal of Geophysical Research: Space Physics, 123(9), 7697-7709. https://doi.org/10.1029/2018JA025395

Vancouver

Mahmoudian A, Senior A, Scales WA, Kosch MJ, Rietveld MT. Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events. Journal of Geophysical Research: Space Physics. 2018 Sept;123(9):7697-7709. Epub 2018 Aug 22. doi: 10.1029/2018JA025395

Author

Mahmoudian, A. ; Senior, A. ; Scales, W.A. et al. / Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events. In: Journal of Geophysical Research: Space Physics. 2018 ; Vol. 123, No. 9. pp. 7697-7709.

Bibtex

@article{66e060c0fffd40e0b70a4ce97a92dd7b,
title = "Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events",
abstract = "The behavior of polar mesospheric summer echoes (PMSEs) during an electron precipitation event is investigated by including dusty plasma effects for the first time. The observational data recorded with the very high frequency (224 MHz) and ultrahigh frequency (930 MHz) radars at the European Incoherent SCATter Scientific Association on 10 and 11 July 2012 are presented. The observed radar echoes show that the PMSEs are both correlated and anticorrelated with the increased electron density associated with electron precipitation events on the two consecutive days. The experimental observations are compared with numerical simulations of the temporal evolution of PMSE with different background dusty plasma parameters during the electron precipitation event. Specifically, the effect of dust radius, dust density, recombination/photoionization rates, photo-detachment current, and electron density enhancement ratio on the behavior of a PMSE layer and the associated dust charging process in the course of electron precipitation events is studied. It is observed that the ratio of electron density fluctuation amplitude δne to the plasma density (ne) plays a critical role in the appearance/disappearance of the layer. The simulation results revealed that the existence of PMSE is mainly determined by dust radius and dust density. The dusty plasma parameters associated with each event are estimated. The condensation nuclei of the ice particles such as proton hydrate clusters (H+(H2O)n) or meteoric smoke particles can be determined by employing the microphysical models along with the dusty plasma simulations. This can resolve any discrepancy in the description of the observed phenomena. {\textcopyright}2018. American Geophysical Union. All Rights Reserved.",
keywords = "electron precipitation events, mesospheric dusty plasma, PMSE, remote sensing",
author = "A. Mahmoudian and A. Senior and W.A. Scales and Kosch, {Michael J.} and M.T. Rietveld",
note = "An edited version of this paper was published by AGU. Copyright 2018 American Geophysical Union. Mahmoudian, A., Senior, A., Scales, W. A., Kosch, M. J., & Rietveld, M. T. (2018). Dusty space plasma diagnosis using the behavior of polar mesospheric summer echoes during electron precipitation events. Journal of Geophysical Research: Space Physics, 123, 7697–7709. https://doi.org/10.1029/2018JA025395",
year = "2018",
month = sep,
doi = "10.1029/2018JA025395",
language = "English",
volume = "123",
pages = "7697--7709",
journal = "Journal of Geophysical Research: Space Physics",
issn = "2169-9380",
publisher = "Blackwell Publishing Ltd",
number = "9",

}

RIS

TY - JOUR

T1 - Dusty Space Plasma Diagnosis Using the Behavior of Polar Mesospheric Summer Echoes During Electron Precipitation Events

AU - Mahmoudian, A.

AU - Senior, A.

AU - Scales, W.A.

AU - Kosch, Michael J.

AU - Rietveld, M.T.

N1 - An edited version of this paper was published by AGU. Copyright 2018 American Geophysical Union. Mahmoudian, A., Senior, A., Scales, W. A., Kosch, M. J., & Rietveld, M. T. (2018). Dusty space plasma diagnosis using the behavior of polar mesospheric summer echoes during electron precipitation events. Journal of Geophysical Research: Space Physics, 123, 7697–7709. https://doi.org/10.1029/2018JA025395

PY - 2018/9

Y1 - 2018/9

N2 - The behavior of polar mesospheric summer echoes (PMSEs) during an electron precipitation event is investigated by including dusty plasma effects for the first time. The observational data recorded with the very high frequency (224 MHz) and ultrahigh frequency (930 MHz) radars at the European Incoherent SCATter Scientific Association on 10 and 11 July 2012 are presented. The observed radar echoes show that the PMSEs are both correlated and anticorrelated with the increased electron density associated with electron precipitation events on the two consecutive days. The experimental observations are compared with numerical simulations of the temporal evolution of PMSE with different background dusty plasma parameters during the electron precipitation event. Specifically, the effect of dust radius, dust density, recombination/photoionization rates, photo-detachment current, and electron density enhancement ratio on the behavior of a PMSE layer and the associated dust charging process in the course of electron precipitation events is studied. It is observed that the ratio of electron density fluctuation amplitude δne to the plasma density (ne) plays a critical role in the appearance/disappearance of the layer. The simulation results revealed that the existence of PMSE is mainly determined by dust radius and dust density. The dusty plasma parameters associated with each event are estimated. The condensation nuclei of the ice particles such as proton hydrate clusters (H+(H2O)n) or meteoric smoke particles can be determined by employing the microphysical models along with the dusty plasma simulations. This can resolve any discrepancy in the description of the observed phenomena. ©2018. American Geophysical Union. All Rights Reserved.

AB - The behavior of polar mesospheric summer echoes (PMSEs) during an electron precipitation event is investigated by including dusty plasma effects for the first time. The observational data recorded with the very high frequency (224 MHz) and ultrahigh frequency (930 MHz) radars at the European Incoherent SCATter Scientific Association on 10 and 11 July 2012 are presented. The observed radar echoes show that the PMSEs are both correlated and anticorrelated with the increased electron density associated with electron precipitation events on the two consecutive days. The experimental observations are compared with numerical simulations of the temporal evolution of PMSE with different background dusty plasma parameters during the electron precipitation event. Specifically, the effect of dust radius, dust density, recombination/photoionization rates, photo-detachment current, and electron density enhancement ratio on the behavior of a PMSE layer and the associated dust charging process in the course of electron precipitation events is studied. It is observed that the ratio of electron density fluctuation amplitude δne to the plasma density (ne) plays a critical role in the appearance/disappearance of the layer. The simulation results revealed that the existence of PMSE is mainly determined by dust radius and dust density. The dusty plasma parameters associated with each event are estimated. The condensation nuclei of the ice particles such as proton hydrate clusters (H+(H2O)n) or meteoric smoke particles can be determined by employing the microphysical models along with the dusty plasma simulations. This can resolve any discrepancy in the description of the observed phenomena. ©2018. American Geophysical Union. All Rights Reserved.

KW - electron precipitation events

KW - mesospheric dusty plasma

KW - PMSE

KW - remote sensing

U2 - 10.1029/2018JA025395

DO - 10.1029/2018JA025395

M3 - Journal article

VL - 123

SP - 7697

EP - 7709

JO - Journal of Geophysical Research: Space Physics

JF - Journal of Geophysical Research: Space Physics

SN - 2169-9380

IS - 9

ER -