Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9557
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dc.contributor.authorallMaterassi, M.; ISC-CNRen
dc.contributor.authorallArbesser-Rastburg, B.; ESAen
dc.contributor.authorallBanfi, E.; Thales Alenia Space Italiaen
dc.contributor.authorallCiraolo, L.; ISC-CNRen
dc.contributor.authorallDe Michelis, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallMuscinelli, R.; Thales Alenia Space Italiaen
dc.contributor.authorallPonzoni, C.; Thales Alenia Space Italiaen
dc.contributor.authorallScacchetti, C.; Thales Alenia Space Italiaen
dc.contributor.authorallSpalla, P.; ISC-CNRen
dc.contributor.authorallTozzi, R.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallZin, A.; Thales Alenia Space Italiaen
dc.date.accessioned2015-04-21T10:37:40Zen
dc.date.available2015-04-21T10:37:40Zen
dc.date.issued2013en
dc.identifier.urihttp://hdl.handle.net/2122/9557en
dc.description.abstractThe Earth’s plasmasphere variability is a consequence of the Sun’s forcing, determining our planet’s space weather. Plasmaspheric dynamics could be entirely caught only by studying together global and local proxies of the state of this extended system. The ISIS project (Inter-Satellite & In Situ plasmaspheric monitoring and modelling) aimed to design a system for the continuous monitoring of the Earth’s plasmasphere based on the future Galileo satellites. The efforts and expertise of ISC-CNR (Institute for Complex Systems of the National Research Council of Italy), INGV (Istituto Nazionale di Geofisica e Vulcanologia) and TAS-I (Thales Alenia Space - Italy) were put together in this work of assessment. ISIS Team proposed new experimental facilities of the Galileo satellites, designed to realize inter-satellite and in situ measurements to monitor global and local quantities; in particular, a scalable system of Langmuir probes was suggested, while the TEC along all possible inter-satellite ray paths throughout the plasmasphere could be monitored via phase- and group-delay analysis of inter-satellite radio signals.en
dc.language.isoEnglishen
dc.relation.ispartofProceedings of the 4th International Colloquium Scientific and Fundamental Aspects of the Galileo Programmeen
dc.relation.ispartofseries/ (2013)en
dc.subjectGalileo satellitesen
dc.subjectPlasmasphereen
dc.titleThe ISIS Project: Indications for Future Near-Earth Plasma Studies through Future Galileo Satellitesen
dc.typearticleen
dc.description.statusPublisheden
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.04. Plasma Physicsen
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.06. Instruments and techniquesen
dc.description.obiettivoSpecifico1A. Geomagnetismo e Paleomagnetismoen
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeN/A or not JCRen
dc.description.fulltextopenen
dc.contributor.authorMaterassi, M.en
dc.contributor.authorArbesser-Rastburg, B.en
dc.contributor.authorBanfi, E.en
dc.contributor.authorCiraolo, L.en
dc.contributor.authorDe Michelis, P.en
dc.contributor.authorMuscinelli, R.en
dc.contributor.authorPonzoni, C.en
dc.contributor.authorScacchetti, C.en
dc.contributor.authorSpalla, P.en
dc.contributor.authorTozzi, R.en
dc.contributor.authorZin, A.en
dc.contributor.departmentISC-CNRen
dc.contributor.departmentESAen
dc.contributor.departmentThales Alenia Space Italiaen
dc.contributor.departmentISC-CNRen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentThales Alenia Space Italiaen
dc.contributor.departmentThales Alenia Space Italiaen
dc.contributor.departmentThales Alenia Space Italiaen
dc.contributor.departmentISC-CNRen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentThales Alenia Space Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto dei Sistemi Complessi, Consiglio Nazionale delle Ricerche-
crisitem.author.deptESA-
crisitem.author.deptThales Alenia Space Italia-
crisitem.author.deptIstituto di Ricerche Sulle Onde Elettromagnetiche, Firenze, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptThales Alenia Space Italia-
crisitem.author.deptThales Alenia Space Italia-
crisitem.author.deptThales Alenia Space Italia-
crisitem.author.deptIstituto di Fisica Applicata «Nello Carrara» (IFAC), Firenze, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptThales Alenia Space Italia-
crisitem.author.orcid0000-0002-2708-0739-
crisitem.author.orcid0000-0002-1836-4078-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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