id ftuppsalauniv:oai:DiVA.org:uu-274781
record_format openpolar
institution Open Polar
collection Uppsala University: Publications (DiVA)
op_collection_id ftuppsalauniv
language English
topic EISCAT
EISCAT_3D
Radar
Incoherent scatter
Atmospheric science
Space physics
Plasma physics
Solar system research
Space weather
Radar techniques
Fusion
Plasma and Space Physics
plasma och rymdfysik
Astronomy
Astrophysics and Cosmology
Astronomi
astrofysik och kosmologi
spellingShingle EISCAT
EISCAT_3D
Radar
Incoherent scatter
Atmospheric science
Space physics
Plasma physics
Solar system research
Space weather
Radar techniques
Fusion
Plasma and Space Physics
plasma och rymdfysik
Astronomy
Astrophysics and Cosmology
Astronomi
astrofysik och kosmologi
McCrea, Ian
Aikio, Anita
Alfonsi, Lucilla
Belova, Evgenia
Buchert, Stephan
Clilverd, Mark
Engler, Norbert
Gustavsson, Bjorn
Heinselman, Craig
Kero, Johan
Kosch, Mike
Lamy, Herve
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 EISCAT
EISCAT_3D
Radar
Incoherent scatter
Atmospheric science
Space physics
Plasma physics
Solar system research
Space weather
Radar techniques
Fusion
Plasma and Space Physics
plasma och rymdfysik
Astronomy
Astrophysics and Cosmology
Astronomi
astrofysik och kosmologi
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, Bjorn
Heinselman, Craig
Kero, Johan
Kosch, Mike
Lamy, Herve
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, Bjorn
Heinselman, Craig
Kero, Johan
Kosch, Mike
Lamy, Herve
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 Uppsala universitet, Institutet för rymdfysik, Uppsalaavdelningen
publishDate 2015
url http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-274781
https://doi.org/10.1186/s40645-015-0051-8
geographic Svalbard
geographic_facet Svalbard
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
op_relation Progress in Earth and Planetary Science, 2015, 2,
http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-274781
doi:10.1186/s40645-015-0051-8
ISI:000363945400001
op_rights info:eu-repo/semantics/openAccess
op_doi https://doi.org/10.1186/s40645-015-0051-8
container_title Progress in Earth and Planetary Science
container_volume 2
container_issue 1
_version_ 1766400030092034048
spelling ftuppsalauniv:oai:DiVA.org:uu-274781 2023-05-15T16:04:24+02:00 The science case for the EISCAT_3D radar McCrea, Ian Aikio, Anita Alfonsi, Lucilla Belova, Evgenia Buchert, Stephan Clilverd, Mark Engler, Norbert Gustavsson, Bjorn Heinselman, Craig Kero, Johan Kosch, Mike Lamy, Herve Leyser, Thomas Ogawa, Yasunobu Oksavik, Kjellmar Pellinen-Wannberg, Asta Pitout, Frederic Rapp, Markus Stanislawska, Iwona Vierinen, Juha 2015 application/pdf http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-274781 https://doi.org/10.1186/s40645-015-0051-8 eng eng Uppsala universitet, Institutet för rymdfysik, Uppsalaavdelningen STFC Rutherford Appleton Lab, RAL Space, Harwell, Oxon, England. Univ Oulu, Dept Phys, FIN-90570 Oulu, Finland. INGV, Rome, Italy. Swedish Inst Space Phys IRF, Kiruna, Sweden. British Antarctic Survey, Cambridge CB3 0ET, England. Leibniz Inst Atmospher Phys, Rostock, Germany. Univ Tromso, Dept Phys & Technol, Tromso, Norway. EISCAT Sci Assoc, Kiruna, Sweden. Univ Lancaster, Dept Phys, Lancaster, England.;South African Natl Space Agcy, Hermanus, South Africa. Belgian Inst Space Aeron, Brussels, Belgium. Natl Inst Polar Res, Tachikawa, Tokyo, Japan. Univ Bergen, Birkeland Ctr Space Sci, Bergen, Norway. Swedish Inst Space Phys IRF, Kiruna, Sweden.;Umea Univ, Dept Phys, Umea, Sweden. Univ Toulouse, UPS OMP, IRAP, Toulouse, France.;CNRS, IRAP, Toulouse, France. German Aerosp Ctr, Inst Atmospher Phys, Oberpfaffenhofen, Wessling, Germany. Polish Acad Sci, Space Res Ctr, PL-01237 Warsaw, Poland. Sodankyla Geophys Observ, Sodankyla, Finland. Progress in Earth and Planetary Science, 2015, 2, http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-274781 doi:10.1186/s40645-015-0051-8 ISI:000363945400001 info:eu-repo/semantics/openAccess EISCAT EISCAT_3D Radar Incoherent scatter Atmospheric science Space physics Plasma physics Solar system research Space weather Radar techniques Fusion Plasma and Space Physics plasma och rymdfysik Astronomy Astrophysics and Cosmology Astronomi astrofysik och kosmologi Article, review/survey info:eu-repo/semantics/article text 2015 ftuppsalauniv https://doi.org/10.1186/s40645-015-0051-8 2023-02-23T21:54:19Z 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 Uppsala University: Publications (DiVA) Svalbard Progress in Earth and Planetary Science 2 1