The science case for the EISCAT_3D radar

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...

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Main Authors: McCrea, Ian, Aikio, Anita, Alfonsi, Lucilla, Belova, Evgenia, Buchert, Stephan, Clilverd, Mark, Engler, Norbert, Gustavsson, Björn, Heinselman, Craig, Kero, Johan, Kosch, Mike, Lamy, Hervé, Leyser, Thomas, Ogawa, Yasunobu, Oksavik, Kjellmar, Pellinen-Wannberg, Asta, Pitout, Frederic, Rapp, Markus, Stanislawska, Iwona, Vierinen, Juha
Format: Article in Journal/Newspaper
Language:English
Published: Berlin 2015
Subjects:
550
Online Access:https://oa.tib.eu/renate/handle/123456789/9828
https://doi.org/10.34657/8866
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spelling ftleibnizopen:oai:oai.leibnizopen.de:DiePVYsBBwLIz6xGmghi 2023-11-12T04:16:35+01:00 The science case for the EISCAT_3D radar McCrea, Ian Aikio, Anita Alfonsi, Lucilla Belova, Evgenia Buchert, Stephan Clilverd, Mark Engler, Norbert Gustavsson, Björn Heinselman, Craig Kero, Johan Kosch, Mike Lamy, Hervé Leyser, Thomas Ogawa, Yasunobu Oksavik, Kjellmar Pellinen-Wannberg, Asta Pitout, Frederic Rapp, Markus Stanislawska, Iwona Vierinen, Juha 2015 application/pdf https://oa.tib.eu/renate/handle/123456789/9828 https://doi.org/10.34657/8866 eng eng Berlin Heidelberg : SpringerOpen CC BY 4.0 Unported https://creativecommons.org/licenses/by/4.0/ Progress in Earth and Planetary Science 2 (2015), Nr. 1 Atmospheric science EISCAT EISCAT_3D Incoherent scatter Plasma physics Radar Radar techniques Solar system research Space physics Space weather 550 article Text 2015 ftleibnizopen https://doi.org/10.34657/8866 2023-10-22T23:35:56Z 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 ... Article in Journal/Newspaper EISCAT Svalbard Unknown Svalbard
institution Open Polar
collection Unknown
op_collection_id ftleibnizopen
language English
topic Atmospheric science
EISCAT
EISCAT_3D
Incoherent scatter
Plasma physics
Radar
Radar techniques
Solar system research
Space physics
Space weather
550
spellingShingle Atmospheric science
EISCAT
EISCAT_3D
Incoherent scatter
Plasma physics
Radar
Radar techniques
Solar system research
Space physics
Space weather
550
McCrea, Ian
Aikio, Anita
Alfonsi, Lucilla
Belova, Evgenia
Buchert, Stephan
Clilverd, Mark
Engler, Norbert
Gustavsson, Björn
Heinselman, Craig
Kero, Johan
Kosch, Mike
Lamy, Hervé
Leyser, Thomas
Ogawa, Yasunobu
Oksavik, Kjellmar
Pellinen-Wannberg, Asta
Pitout, Frederic
Rapp, Markus
Stanislawska, Iwona
Vierinen, Juha
The science case for the EISCAT_3D radar
topic_facet Atmospheric science
EISCAT
EISCAT_3D
Incoherent scatter
Plasma physics
Radar
Radar techniques
Solar system research
Space physics
Space weather
550
description 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 ...
format Article in Journal/Newspaper
author McCrea, Ian
Aikio, Anita
Alfonsi, Lucilla
Belova, Evgenia
Buchert, Stephan
Clilverd, Mark
Engler, Norbert
Gustavsson, Björn
Heinselman, Craig
Kero, Johan
Kosch, Mike
Lamy, Hervé
Leyser, Thomas
Ogawa, Yasunobu
Oksavik, Kjellmar
Pellinen-Wannberg, Asta
Pitout, Frederic
Rapp, Markus
Stanislawska, Iwona
Vierinen, Juha
author_facet McCrea, Ian
Aikio, Anita
Alfonsi, Lucilla
Belova, Evgenia
Buchert, Stephan
Clilverd, Mark
Engler, Norbert
Gustavsson, Björn
Heinselman, Craig
Kero, Johan
Kosch, Mike
Lamy, Hervé
Leyser, Thomas
Ogawa, Yasunobu
Oksavik, Kjellmar
Pellinen-Wannberg, Asta
Pitout, Frederic
Rapp, Markus
Stanislawska, Iwona
Vierinen, Juha
author_sort McCrea, Ian
title The science case for the EISCAT_3D radar
title_short The science case for the EISCAT_3D radar
title_full The science case for the EISCAT_3D radar
title_fullStr The science case for the EISCAT_3D radar
title_full_unstemmed The science case for the EISCAT_3D radar
title_sort science case for the eiscat_3d radar
publisher Berlin
publishDate 2015
url https://oa.tib.eu/renate/handle/123456789/9828
https://doi.org/10.34657/8866
geographic Svalbard
geographic_facet Svalbard
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
op_source Progress in Earth and Planetary Science 2 (2015), Nr. 1
op_rights CC BY 4.0 Unported
https://creativecommons.org/licenses/by/4.0/
op_doi https://doi.org/10.34657/8866
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