Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/8733
DC Field | Value | Language |
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dc.contributor.authorall | Romano, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Pau, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Pezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Spogli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Zuccheretti, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.authorall | Aquino, M.; Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom | en |
dc.contributor.authorall | Hancock, C. M.; Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom | en |
dc.date.accessioned | 2013-08-01T08:47:53Z | en |
dc.date.available | 2013-08-01T08:47:53Z | en |
dc.date.issued | 2013 | en |
dc.identifier.uri | http://hdl.handle.net/2122/8733 | en |
dc.description.abstract | The electronic space weather upper atmosphere (eSWua) is a hardware– software system that is based on measurements collected by instruments installed by the Upper Atmosphere Physics Group of the Istituto Nazionale di Geofisica e Vulcanologia (INGV, Italy). More recently, it has also included the Global Navigation Satellite System (GNSS) ionospheric scintillation and total electron content (TEC) monitor (GISTM) stations that are managed and operated by the University of Nottingham (UK). By visiting the eSWua website, it is possible to access the database that has been implemented to organize and manage the large amount of information acquired. The section of the database designed for the TEC and scintillation data has been designed to address the needs of the space weather community as well as of scientific users. Through the web tools, it is possible to visualize, plot, extract and download the data from each station. This interactive website is supported by a structured database, and it provides a powerful tool for the scientific and technological community in the field of telecommunications and space weather. At present, the data transmission procedure, the database population algorithm, the linear plot and polar plot visualization tools, the statistics page, and the user management system are fully operational. Web access to the data and tools has been realized to handle the data from the sites at low, mid and high latitudes. In this report, we present the results of the system for the GNSS data in the Arctic, the Antarctica, and the three GISTM stations operated by the University of Nottingham: Nottingham, Trondheim and Dourbes. Case studies of the efficacy of this system for scientific and application purposes are also presented and discussed. | en |
dc.language.iso | English | en |
dc.publisher.name | INGV | en |
dc.relation.ispartof | Annals of Geophysics | en |
dc.relation.ispartofseries | 2 / 56 (2013) | en |
dc.subject | Database | en |
dc.subject | GNSS | en |
dc.subject | Global positioning system | en |
dc.subject | Ionosphere | en |
dc.subject | Total electron content | en |
dc.subject | Ionospheric scintillation | en |
dc.title | eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.description.pagenumber | R0223 | en |
dc.subject.INGV | 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques | en |
dc.subject.INGV | 01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations | en |
dc.subject.INGV | 05. General::05.01. Computational geophysics::05.01.01. Data processing | en |
dc.subject.INGV | 05. General::05.02. Data dissemination::05.02.05. Collections | en |
dc.identifier.doi | 10.4401/ag-6244 | en |
dc.relation.references | Alfonsi, L., L. Spogli, G. De Franceschi, V. Romano, M. Aquino, A. Dodson and C.N. Mitchell (2011). Bipolar climatology of GPS ionospheric scintillation at solar minimum, Radio Sci., 46, RS0D05; doi:10.102 9/2010RS004571. Feldstein, Y.I. (1963). On morphology and auroral and magnetic disturbances at high latitudes, Geomagn. Aeron., 3, 183-192. Holzworth, R.H., and C.-I. Meng (1975). Mathematical representation of the auroral oval, Geophys. Res. Lett., 2, 377-380. Romano, V., S. Pau, M. Pezzopane, E. Zuccheretti, B. Zolesi, G. De Franceschi and S. Locatelli (2008). The electronic space weather upper atmosphere (eSWua) project at INGV: advancements and state of the art,Annales Geophysicae, 26, 345-351. Spogli, L., L. Alfonsi, G. De Franceschi, V. Romano, M.H.O. Aquino and A. Dodson (2009). Climatology of GPS ionospheric scintillations over high and midlatitude European regions, Annales Geophysicae, 27, 3429-3437. Spogli, L., L. Alfonsi, G. De Franceschi, V. Romano, M.H.O. Aquino and A. Dodson (2010). Climatology of GNSS ionospheric scintillation at high and midlatitudes under different solar activity conditions, Nuovo Cimento della Società Italiana di Fisica BGeneral Physics Relativity Astronomy And Mathematical Physics And Methods, 125 B (5/6), ISSN 1826-9877; doi:10.1393/ncb/i2010-10857-7. Van Dierendonck, A.J., J. Klobuchar and Q. Hua (1993). Ionospheric scintillation monitoring using commercial single frequency C/A code receivers, In: ION GPS-93 Proceedings of the Sixth International Technical Meeting of the Satellite Division of theInstitute of Navigation (Salt Lake City, U.S.A., September 22-24), 1333-1342. | en |
dc.description.obiettivoSpecifico | 1.7. Osservazioni di alta e media atmosfera | en |
dc.description.obiettivoSpecifico | 5.4. Banche dati di geomagnetismo, aeronomia, clima e ambiente | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | open | en |
dc.contributor.author | Romano, V. | en |
dc.contributor.author | Pau, S. | en |
dc.contributor.author | Pezzopane, M. | en |
dc.contributor.author | Spogli, L. | en |
dc.contributor.author | Zuccheretti, E. | en |
dc.contributor.author | Aquino, M. | en |
dc.contributor.author | Hancock, C. M. | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.contributor.department | Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom | en |
dc.contributor.department | Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | open | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.dept | Institute of Engineering Surveying and Space Geodesy (IESSG), Nottingham, UK | - |
crisitem.author.orcid | 0000-0002-7532-4507 | - |
crisitem.author.orcid | 0000-0003-4321-4546 | - |
crisitem.author.orcid | 0000-0001-5800-2322 | - |
crisitem.author.orcid | 0000-0003-2310-0306 | - |
crisitem.author.orcid | 0000-0003-1732-4557 | - |
crisitem.author.orcid | 0000-0003-2733-4716 | - |
crisitem.author.orcid | 0000-0002-9692-0439 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.classification.parent | 05. General | - |
crisitem.classification.parent | 05. General | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
Appears in Collections: | Article published / in press |
Files in This Item:
File | Description | Size | Format | |
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2013_Romano_et_al_AG_eswua.pdf | 8.85 MB | Adobe PDF | View/Open |
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