Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility
SPEAR is a new polar cap HF radar facility which is to be deployed on Svalbard. The principal capabilities of SPEAR will include the generation of artificial plasma irregularities, operation as an 'all-sky' HF radar, the excitation of ULF waves, and remote sounding of the magnetosphere...
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Copernicus Publications
2000-09-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/18/1248/2000/angeo-18-1248-2000.pdf |
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author | D. M. Wright J. A. Davies T. R. Robinson P. J. Chapman T. K. Yeoman E. C. Thomas M. Lester S. W. H. Cowley A. J. Stocker R. B. Horne F. Honary |
author_facet | D. M. Wright J. A. Davies T. R. Robinson P. J. Chapman T. K. Yeoman E. C. Thomas M. Lester S. W. H. Cowley A. J. Stocker R. B. Horne F. Honary |
author_sort | D. M. Wright |
collection | DOAJ |
description | SPEAR is a new polar cap HF radar facility
which is to be deployed on Svalbard. The principal capabilities of SPEAR will
include the generation of artificial plasma irregularities, operation as an
'all-sky' HF radar, the excitation of ULF waves, and remote sounding of the
magnetosphere. Operation of SPEAR in conjunction with the multitude of other
instruments on Svalbard, including the EISCAT Svalbard radar, and the overlap of
its extensive field-of-view with that of several of the HF radars in the
SuperDARN network, will enable in-depth diagnosis of many geophysical and plasma
phenomena associated with the cusp region and the substorm expansion phase.
Moreover, its ability to produce artificial radar aurora will provide a means
for the other instruments to undertake polar cap plasma physics experiments in a
controlled manner. Another potential use of the facility is in 'field-line
tagging' experiments, for coordinated ground-satellite experiments. Here the
scientific objectives of SPEAR are detailed, along with the proposed technical
specifications of the system.<br><br><b>Key words: </b>Ionosphere (active experiments) – Radio
science (instruments and techniques) – Space plasma physics (instruments and
techniques) |
first_indexed | 2024-12-11T21:56:25Z |
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id | doaj.art-39321788157a4364a0233dad982c6dc8 |
institution | Directory Open Access Journal |
issn | 0992-7689 1432-0576 |
language | English |
last_indexed | 2024-12-11T21:56:25Z |
publishDate | 2000-09-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Annales Geophysicae |
spelling | doaj.art-39321788157a4364a0233dad982c6dc82022-12-22T00:49:17ZengCopernicus PublicationsAnnales Geophysicae0992-76891432-05762000-09-01181248125510.1007/s00585-000-1248-7Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facilityD. M. Wright0J. A. Davies1T. R. Robinson2P. J. Chapman3T. K. Yeoman4E. C. Thomas5M. Lester6S. W. H. Cowley7A. J. Stocker8R. B. Horne9F. Honary10Department of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Physics & Astronomy, University of Leicester, University Road, Leicester, LE1 7RH, UKDepartment of Engineering, University of Leicester, University Road, Leicester, LE1 7RH, UKBritish Antarctic Survey, Madingley Road, Cambridge, CB3 0ET, UKDepartment of Communication Systems, University of Lancaster, Bailrigg, Lancaster, LA1 4YR, UKSPEAR is a new polar cap HF radar facility which is to be deployed on Svalbard. The principal capabilities of SPEAR will include the generation of artificial plasma irregularities, operation as an 'all-sky' HF radar, the excitation of ULF waves, and remote sounding of the magnetosphere. Operation of SPEAR in conjunction with the multitude of other instruments on Svalbard, including the EISCAT Svalbard radar, and the overlap of its extensive field-of-view with that of several of the HF radars in the SuperDARN network, will enable in-depth diagnosis of many geophysical and plasma phenomena associated with the cusp region and the substorm expansion phase. Moreover, its ability to produce artificial radar aurora will provide a means for the other instruments to undertake polar cap plasma physics experiments in a controlled manner. Another potential use of the facility is in 'field-line tagging' experiments, for coordinated ground-satellite experiments. Here the scientific objectives of SPEAR are detailed, along with the proposed technical specifications of the system.<br><br><b>Key words: </b>Ionosphere (active experiments) – Radio science (instruments and techniques) – Space plasma physics (instruments and techniques)https://www.ann-geophys.net/18/1248/2000/angeo-18-1248-2000.pdf |
spellingShingle | D. M. Wright J. A. Davies T. R. Robinson P. J. Chapman T. K. Yeoman E. C. Thomas M. Lester S. W. H. Cowley A. J. Stocker R. B. Horne F. Honary Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility Annales Geophysicae |
title | Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility |
title_full | Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility |
title_fullStr | Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility |
title_full_unstemmed | Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility |
title_short | Space Plasma Exploration by Active Radar (SPEAR): an overview of a future radar facility |
title_sort | space plasma exploration by active radar spear an overview of a future radar facility |
url | https://www.ann-geophys.net/18/1248/2000/angeo-18-1248-2000.pdf |
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