Review of the accomplishments of mid-latitude Super Dual Auroral Radar Network (SuperDARN) HF radars

The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both hemispheres that is operated under international cooperation. The network was originally designed for monitoring the dynamics of the ionosphere and upper...

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Published inProgress in earth and planetary science Vol. 6; no. 1; pp. 1 - 57
Main Authors Nishitani, Nozomu, Ruohoniemi, John Michael, Lester, Mark, Baker, Joseph Benjamin Harold, Koustov, Alexandre Vasilyevich, Shepherd, Simon G., Chisham, Gareth, Hori, Tomoaki, Thomas, Evan G., Makarevich, Roman A., Marchaudon, Aurélie, Ponomarenko, Pavlo, Wild, James A., Milan, Stephen E., Bristow, William A., Devlin, John, Miller, Ethan, Greenwald, Raymond A., Ogawa, Tadahiko, Kikuchi, Takashi
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 18.03.2019
Springer Nature B.V
Springer/Japan Geoscience Union
SpringerOpen
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Abstract The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both hemispheres that is operated under international cooperation. The network was originally designed for monitoring the dynamics of the ionosphere and upper atmosphere in the high-latitude regions. However, over the last approximately 15 years, SuperDARN has expanded into the mid-latitude regions. With radar coverage that now extends continuously from auroral to sub-auroral and mid-latitudes, a wide variety of new scientific findings have been obtained. In this paper, the background of mid-latitude SuperDARN is presented at first. Then, the accomplishments made with mid-latitude SuperDARN radars are reviewed in five specified scientific and technical areas: convection, ionospheric irregularities, HF propagation analysis, ion-neutral interactions, and magnetohydrodynamic (MHD) waves. Finally, the present status of mid-latitude SuperDARN is updated and directions for future research are discussed.
AbstractList Abstract The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both hemispheres that is operated under international cooperation. The network was originally designed for monitoring the dynamics of the ionosphere and upper atmosphere in the high-latitude regions. However, over the last approximately 15 years, SuperDARN has expanded into the mid-latitude regions. With radar coverage that now extends continuously from auroral to sub-auroral and mid-latitudes, a wide variety of new scientific findings have been obtained. In this paper, the background of mid-latitude SuperDARN is presented at first. Then, the accomplishments made with mid-latitude SuperDARN radars are reviewed in five specified scientific and technical areas: convection, ionospheric irregularities, HF propagation analysis, ion-neutral interactions, and magnetohydrodynamic (MHD) waves. Finally, the present status of mid-latitude SuperDARN is updated and directions for future research are discussed.
The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both hemispheres that is operated under international cooperation. The network was originally designed for monitoring the dynamics of the ionosphere and upper atmosphere in the high-latitude regions. However, over the last approximately 15 years, SuperDARN has expanded into the mid-latitude regions. With radar coverage that now extends continuously from auroral to sub-auroral and mid-latitudes, a wide variety of new scientific findings have been obtained. In this paper, the background of mid-latitude SuperDARN is presented at first. Then, the accomplishments made with mid-latitude SuperDARN radars are reviewed in five specified scientific and technical areas: convection, ionospheric irregularities, HF propagation analysis, ion-neutral interactions, and magnetohydrodynamic (MHD) waves. Finally, the present status of mid-latitude SuperDARN is updated and directions for future research are discussed.
ArticleNumber 27
Author Baker, Joseph Benjamin Harold
Makarevich, Roman A.
Greenwald, Raymond A.
Marchaudon, Aurélie
Ruohoniemi, John Michael
Wild, James A.
Ponomarenko, Pavlo
Bristow, William A.
Shepherd, Simon G.
Kikuchi, Takashi
Milan, Stephen E.
Lester, Mark
Hori, Tomoaki
Chisham, Gareth
Miller, Ethan
Nishitani, Nozomu
Koustov, Alexandre Vasilyevich
Thomas, Evan G.
Devlin, John
Ogawa, Tadahiko
Author_xml – sequence: 1
  givenname: Nozomu
  orcidid: 0000-0001-9842-5119
  surname: Nishitani
  fullname: Nishitani, Nozomu
  email: nisitani@isee.nagoya-u.ac.jp
  organization: Institute for Space-Earth Environmental Research, Nagoya University
– sequence: 2
  givenname: John Michael
  surname: Ruohoniemi
  fullname: Ruohoniemi, John Michael
  organization: Virginia Tech Department of Electrical and Computer Engineering
– sequence: 3
  givenname: Mark
  surname: Lester
  fullname: Lester, Mark
  organization: University of Leicester
– sequence: 4
  givenname: Joseph Benjamin Harold
  surname: Baker
  fullname: Baker, Joseph Benjamin Harold
  organization: Virginia Tech Department of Electrical and Computer Engineering
– sequence: 5
  givenname: Alexandre Vasilyevich
  surname: Koustov
  fullname: Koustov, Alexandre Vasilyevich
  organization: University of Saskatchewan
– sequence: 6
  givenname: Simon G.
  surname: Shepherd
  fullname: Shepherd, Simon G.
  organization: Thayer School of Engineering, Dartmouth College
– sequence: 7
  givenname: Gareth
  surname: Chisham
  fullname: Chisham, Gareth
  organization: British Antarctic Survey
– sequence: 8
  givenname: Tomoaki
  surname: Hori
  fullname: Hori, Tomoaki
  organization: Institute for Space-Earth Environmental Research, Nagoya University
– sequence: 9
  givenname: Evan G.
  surname: Thomas
  fullname: Thomas, Evan G.
  organization: Thayer School of Engineering, Dartmouth College
– sequence: 10
  givenname: Roman A.
  surname: Makarevich
  fullname: Makarevich, Roman A.
  organization: University of Alaska Fairbanks
– sequence: 11
  givenname: Aurélie
  surname: Marchaudon
  fullname: Marchaudon, Aurélie
  organization: Institut de Recherche en Astrophysique et Planétologie, University of Toulouse, CNRS, CNES
– sequence: 12
  givenname: Pavlo
  surname: Ponomarenko
  fullname: Ponomarenko, Pavlo
  organization: University of Saskatchewan
– sequence: 13
  givenname: James A.
  surname: Wild
  fullname: Wild, James A.
  organization: Lancaster University
– sequence: 14
  givenname: Stephen E.
  surname: Milan
  fullname: Milan, Stephen E.
  organization: University of Leicester
– sequence: 15
  givenname: William A.
  surname: Bristow
  fullname: Bristow, William A.
  organization: University of Alaska Fairbanks
– sequence: 16
  givenname: John
  surname: Devlin
  fullname: Devlin, John
  organization: La Trobe University
– sequence: 17
  givenname: Ethan
  surname: Miller
  fullname: Miller, Ethan
  organization: Applied Physics Laboratory, Johns Hopkins University
– sequence: 18
  givenname: Raymond A.
  surname: Greenwald
  fullname: Greenwald, Raymond A.
  organization: Virginia Tech Department of Electrical and Computer Engineering
– sequence: 19
  givenname: Tadahiko
  surname: Ogawa
  fullname: Ogawa, Tadahiko
  organization: National Institute of Information and Communications Technology
– sequence: 20
  givenname: Takashi
  surname: Kikuchi
  fullname: Kikuchi, Takashi
  organization: Institute for Space-Earth Environmental Research, Nagoya University
BackLink https://hal.science/hal-02322069$$DView record in HAL
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ContentType Journal Article
Copyright The Author(s). 2019. corrected publication [July/2019]
Progress in Earth and Planetary Science is a copyright of Springer, (2019). All Rights Reserved. © 2019. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
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Copyright_xml – notice: The Author(s). 2019. corrected publication [July/2019]
– notice: Progress in Earth and Planetary Science is a copyright of Springer, (2019). All Rights Reserved. © 2019. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.
– notice: Distributed under a Creative Commons Attribution 4.0 International License
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Keywords Ion-neutral interactions
MHD waves
Mid-latitude SuperDARN
HF propagation analysis
Magnetosphere
Ionosphere
Convection
Ionospheric irregularities
Language English
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Snippet The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both hemispheres...
The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high-and mid-latitude regions of both hemispheres...
Abstract The Super Dual Auroral Radar Network (SuperDARN) is a network of high-frequency (HF) radars located in the high- and mid-latitude regions of both...
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SubjectTerms 1. Space and planetary sciences
Astrophysics
Atmospheric Sciences
Biogeosciences
Convection
Earth and Environmental Science
Earth and Planetary Astrophysics
Earth Sciences
Geophysics/Geodesy
HF propagation analysis
Hydrogeology
International cooperation
Ionosphere
Ionospheric irregularities
Latitude
Magnetosphere
Mid-latitude SuperDARN
Planetology
Radar
Review
Sciences of the Universe
Upper atmosphere
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Title Review of the accomplishments of mid-latitude Super Dual Auroral Radar Network (SuperDARN) HF radars
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