eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes
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 Glo...
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Format: | Article in Journal/Newspaper |
Language: | English |
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INGV
2013
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Online Access: | http://hdl.handle.net/2122/8733 https://doi.org/10.4401/ag-6244 |
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ftingv:oai:www.earth-prints.org:2122/8733 |
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Open Polar |
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Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) |
op_collection_id |
ftingv |
language |
English |
topic |
Database GNSS Global positioning system Ionosphere Total electron content Ionospheric scintillation 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques 01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations 05. General::05.01. Computational geophysics::05.01.01. Data processing 05. General::05.02. Data dissemination::05.02.05. Collections |
spellingShingle |
Database GNSS Global positioning system Ionosphere Total electron content Ionospheric scintillation 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques 01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations 05. General::05.01. Computational geophysics::05.01.01. Data processing 05. General::05.02. Data dissemination::05.02.05. Collections Romano, V. Pau, S. Pezzopane, M. Spogli, L. Zuccheretti, E. Aquino, M. Hancock, C. M. eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes |
topic_facet |
Database GNSS Global positioning system Ionosphere Total electron content Ionospheric scintillation 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques 01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations 05. General::05.01. Computational geophysics::05.01.01. Data processing 05. General::05.02. Data dissemination::05.02.05. Collections |
description |
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. Published R0223 1.7. Osservazioni di alta e media atmosfera 5.4. Banche dati di geomagnetismo, aeronomia, clima e ambiente JCR Journal open |
author2 |
Romano, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Pau, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Pezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Spogli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Zuccheretti, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Aquino, M.; Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom Hancock, C. M.; Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom |
format |
Article in Journal/Newspaper |
author |
Romano, V. Pau, S. Pezzopane, M. Spogli, L. Zuccheretti, E. Aquino, M. Hancock, C. M. |
author_facet |
Romano, V. Pau, S. Pezzopane, M. Spogli, L. Zuccheretti, E. Aquino, M. Hancock, C. M. |
author_sort |
Romano, V. |
title |
eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes |
title_short |
eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes |
title_full |
eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes |
title_fullStr |
eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes |
title_full_unstemmed |
eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes |
title_sort |
eswua: a tool to manage and access gnss ionospheric data from mid-to-high latitudes |
publisher |
INGV |
publishDate |
2013 |
url |
http://hdl.handle.net/2122/8733 https://doi.org/10.4401/ag-6244 |
long_lat |
ENVELOPE(161.983,161.983,-78.000,-78.000) |
geographic |
Alta Arctic Handle The |
geographic_facet |
Alta Arctic Handle The |
genre |
Antarc* Antarctica Arctic |
genre_facet |
Antarc* Antarctica Arctic |
op_relation |
Annals of Geophysics 2 / 56 (2013) 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. http://hdl.handle.net/2122/8733 doi:10.4401/ag-6244 |
op_rights |
open |
op_doi |
https://doi.org/10.4401/ag-6244 https://doi.org/10.1393/ncb/i2010-10857-7 |
_version_ |
1766271559227408384 |
spelling |
ftingv:oai:www.earth-prints.org:2122/8733 2023-05-15T14:01:37+02:00 eSWua: a tool to manage and access GNSS ionospheric data from mid-to-high latitudes Romano, V. Pau, S. Pezzopane, M. Spogli, L. Zuccheretti, E. Aquino, M. Hancock, C. M. Romano, V.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Pau, S.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Pezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Spogli, L.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Zuccheretti, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Aquino, M.; Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom Hancock, C. M.; Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia Nottingham Geospatial Institute, University of Nottingham, Nottingham, United Kingdom 2013 http://hdl.handle.net/2122/8733 https://doi.org/10.4401/ag-6244 en eng INGV Annals of Geophysics 2 / 56 (2013) 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. http://hdl.handle.net/2122/8733 doi:10.4401/ag-6244 open Database GNSS Global positioning system Ionosphere Total electron content Ionospheric scintillation 01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniques 01. Atmosphere::01.02. Ionosphere::01.02.07. Scintillations 05. General::05.01. Computational geophysics::05.01.01. Data processing 05. General::05.02. Data dissemination::05.02.05. Collections article 2013 ftingv https://doi.org/10.4401/ag-6244 https://doi.org/10.1393/ncb/i2010-10857-7 2022-07-29T06:06:30Z 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. Published R0223 1.7. Osservazioni di alta e media atmosfera 5.4. Banche dati di geomagnetismo, aeronomia, clima e ambiente JCR Journal open Article in Journal/Newspaper Antarc* Antarctica Arctic Earth-Prints (Istituto Nazionale di Geofisica e Vulcanologia) Alta Arctic Handle The ENVELOPE(161.983,161.983,-78.000,-78.000) |