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The science case for the EISCAT_3D radar

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The science case for the EISCAT_3D radar. / Mccrea, Ian; Aikio, Anita; Alfonsi, Lucilla et al.
In: Progress in Earth and Planetary Science, Vol. 2, No. 1, 21, 29.07.2015.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Mccrea, I, Aikio, A, Alfonsi, L, Belova, E, Buchert, S, Clilverd, M, Engler, N, Gustavsson, B, Heinselman, C, Kero, J, Kosch, M, Lamy, H, Leyser, T, Ogawa, Y, Oksavik, K, Pellinen-wannberg, A, Pitout, F, Rapp, M, Stanislawska, I & Vierinen, J 2015, 'The science case for the EISCAT_3D radar', Progress in Earth and Planetary Science, vol. 2, no. 1, 21. https://doi.org/10.1186/s40645-015-0051-8

APA

Mccrea, I., Aikio, A., Alfonsi, L., Belova, E., Buchert, S., Clilverd, M., Engler, N., Gustavsson, B., Heinselman, C., Kero, J., Kosch, M., Lamy, H., Leyser, T., Ogawa, Y., Oksavik, K., Pellinen-wannberg, A., Pitout, F., Rapp, M., Stanislawska, I., & Vierinen, J. (2015). The science case for the EISCAT_3D radar. Progress in Earth and Planetary Science, 2(1), Article 21. https://doi.org/10.1186/s40645-015-0051-8

Vancouver

Mccrea I, Aikio A, Alfonsi L, Belova E, Buchert S, Clilverd M et al. The science case for the EISCAT_3D radar. Progress in Earth and Planetary Science. 2015 Jul 29;2(1):21. doi: 10.1186/s40645-015-0051-8

Author

Mccrea, Ian ; Aikio, Anita ; Alfonsi, Lucilla et al. / The science case for the EISCAT_3D radar. In: Progress in Earth and Planetary Science. 2015 ; Vol. 2, No. 1.

Bibtex

@article{4d0730cea50040af907d843bb89e7935,
title = "The science case for the EISCAT_3D radar",
abstract = "The EISCAT (European Incoherent SCATer) Scientific Association has provided versatile incoherent scatter (IS) radar facilities on the mainland of northern Scandinavia (the EISCAT UHF and VHF radar systems) and on Svalbard (the electronically scanning radar ESR (EISCAT Svalbard Radar) for studies of the high-latitude ionised upper atmosphere (the ionosphere). The mainland radars were constructed about 30 years ago, based on technological solutions of that time. The science drivers of today, however, require a more flexible instrument, which allows measurements to be made from the troposphere to the topside ionosphere and gives the measured parameters in three dimensions, not just along a single radar beam. The possibility for continuous operation is also an essential feature. To facilitatefuture science work with a world-leading IS radar facility, planning of a new radar system started first with an EU-funded Design Study (2005–2009) and has continued with a follow-up EU FP7 EISCAT_3D Preparatory Phase project (2010–2014). The radar facility will be realised by using phased arrays, and a key aspect is the use of advanced software and data processing techniques. This type of software radar will act as a pathfinder for other facilities worldwide. The new radar facility will enable the EISCAT_3D science community to address new, significant science questions as well as to serve society, which is increasingly dependent on space-based technology and issues related to space weather. The location of the radar within the auroral oval and at the edge of the stratospheric polar vortex is also ideal for studies of the long-term variability in the atmosphere and global change. This paper is a summary of the EISCAT_3D science case, which was prepared as part of the EU-funded Preparatory Phase project for the new facility. Three science working groups, drawn from the EISCAT user community, participated in preparing this document. In addition to these working group members, who are listed as authors, thanks are due to many others in the EISCAT scientific community for useful contributions, discussions, and support.",
keywords = "EISCAT, EISCAT_3D , Radar, Incoherent scatter , Atmospheric science, Space physics , Plasma physics, Solar system research, Space weather, Radar techniques",
author = "Ian Mccrea and Anita Aikio and Lucilla Alfonsi and Evgenia Belova and Stephan Buchert and Mark Clilverd and Norbert Engler and Bj{\"o}rn Gustavsson and Craig Heinselman and Johan Kero and Michael Kosch and Herv{\'e} Lamy and Thomas Leyser and Yasunobu Ogawa and Kjellmar Oksavik and Asta Pellinen-wannberg and Frederic Pitout and Markus Rapp and Iwona Stanislawska and Juha Vierinen",
note = "{\textcopyright} 2015 McCrea et al. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.",
year = "2015",
month = jul,
day = "29",
doi = "10.1186/s40645-015-0051-8",
language = "English",
volume = "2",
journal = "Progress in Earth and Planetary Science",
issn = "2197-4284",
publisher = "Springer",
number = "1",

}

RIS

TY - JOUR

T1 - The science case for the EISCAT_3D radar

AU - Mccrea, Ian

AU - Aikio, Anita

AU - Alfonsi, Lucilla

AU - Belova, Evgenia

AU - Buchert, Stephan

AU - Clilverd, Mark

AU - Engler, Norbert

AU - Gustavsson, Björn

AU - Heinselman, Craig

AU - Kero, Johan

AU - Kosch, Michael

AU - Lamy, Hervé

AU - Leyser, Thomas

AU - Ogawa, Yasunobu

AU - Oksavik, Kjellmar

AU - Pellinen-wannberg, Asta

AU - Pitout, Frederic

AU - Rapp, Markus

AU - Stanislawska, Iwona

AU - Vierinen, Juha

N1 - © 2015 McCrea et al. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly credited.

PY - 2015/7/29

Y1 - 2015/7/29

N2 - The EISCAT (European Incoherent SCATer) Scientific Association has provided versatile incoherent scatter (IS) radar facilities on the mainland of northern Scandinavia (the EISCAT UHF and VHF radar systems) and on Svalbard (the electronically scanning radar ESR (EISCAT Svalbard Radar) for studies of the high-latitude ionised upper atmosphere (the ionosphere). The mainland radars were constructed about 30 years ago, based on technological solutions of that time. The science drivers of today, however, require a more flexible instrument, which allows measurements to be made from the troposphere to the topside ionosphere and gives the measured parameters in three dimensions, not just along a single radar beam. The possibility for continuous operation is also an essential feature. To facilitatefuture science work with a world-leading IS radar facility, planning of a new radar system started first with an EU-funded Design Study (2005–2009) and has continued with a follow-up EU FP7 EISCAT_3D Preparatory Phase project (2010–2014). The radar facility will be realised by using phased arrays, and a key aspect is the use of advanced software and data processing techniques. This type of software radar will act as a pathfinder for other facilities worldwide. The new radar facility will enable the EISCAT_3D science community to address new, significant science questions as well as to serve society, which is increasingly dependent on space-based technology and issues related to space weather. The location of the radar within the auroral oval and at the edge of the stratospheric polar vortex is also ideal for studies of the long-term variability in the atmosphere and global change. This paper is a summary of the EISCAT_3D science case, which was prepared as part of the EU-funded Preparatory Phase project for the new facility. Three science working groups, drawn from the EISCAT user community, participated in preparing this document. In addition to these working group members, who are listed as authors, thanks are due to many others in the EISCAT scientific community for useful contributions, discussions, and support.

AB - The EISCAT (European Incoherent SCATer) Scientific Association has provided versatile incoherent scatter (IS) radar facilities on the mainland of northern Scandinavia (the EISCAT UHF and VHF radar systems) and on Svalbard (the electronically scanning radar ESR (EISCAT Svalbard Radar) for studies of the high-latitude ionised upper atmosphere (the ionosphere). The mainland radars were constructed about 30 years ago, based on technological solutions of that time. The science drivers of today, however, require a more flexible instrument, which allows measurements to be made from the troposphere to the topside ionosphere and gives the measured parameters in three dimensions, not just along a single radar beam. The possibility for continuous operation is also an essential feature. To facilitatefuture science work with a world-leading IS radar facility, planning of a new radar system started first with an EU-funded Design Study (2005–2009) and has continued with a follow-up EU FP7 EISCAT_3D Preparatory Phase project (2010–2014). The radar facility will be realised by using phased arrays, and a key aspect is the use of advanced software and data processing techniques. This type of software radar will act as a pathfinder for other facilities worldwide. The new radar facility will enable the EISCAT_3D science community to address new, significant science questions as well as to serve society, which is increasingly dependent on space-based technology and issues related to space weather. The location of the radar within the auroral oval and at the edge of the stratospheric polar vortex is also ideal for studies of the long-term variability in the atmosphere and global change. This paper is a summary of the EISCAT_3D science case, which was prepared as part of the EU-funded Preparatory Phase project for the new facility. Three science working groups, drawn from the EISCAT user community, participated in preparing this document. In addition to these working group members, who are listed as authors, thanks are due to many others in the EISCAT scientific community for useful contributions, discussions, and support.

KW - EISCAT

KW - EISCAT_3D

KW - Radar

KW - Incoherent scatter

KW - Atmospheric science

KW - Space physics

KW - Plasma physics

KW - Solar system research

KW - Space weather

KW - Radar techniques

U2 - 10.1186/s40645-015-0051-8

DO - 10.1186/s40645-015-0051-8

M3 - Journal article

VL - 2

JO - Progress in Earth and Planetary Science

JF - Progress in Earth and Planetary Science

SN - 2197-4284

IS - 1

M1 - 21

ER -