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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/5994
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dc.contributor.authorallPezzopane, M.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallScotto, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallTomasik, L.en
dc.contributor.authorallKrasheninnikov, I.en
dc.date.accessioned2010-05-10T12:49:09Zen
dc.date.available2010-05-10T12:49:09Zen
dc.date.issued2010-06en
dc.identifier.urihttp://hdl.handle.net/2122/5994en
dc.description.abstractAutoscala is a software to automatically scale ionospheric characteristics from an ionogram. Initially it was only applied to the ionograms recorded by the AIS-INGV ionosondes installed at Rome (41.8N, 12.5E), Gibilmanna (37.9N, 14.0E), Italy, and Tucumán (26.9S, 294.6E), Argentina, that are not able to record the polarization of the received echo. Recently Autoscala was also applied to the ionograms recorded by the AIS-Parus ionosonde installed at Moscow (55.5N, 37.3E), Russia, that is not able to tag the received echo in terms of polarization, and by the VISRC2 ionosonde installed at Warsaw (52.2N, 21.1E), Poland, that is instead able to perform the polarization tagging of the ordinary and extraordinary echoes. This work shows different examples of processing performed on ionograms recorded by all these three different types of ionosondes.en
dc.language.isoEnglishen
dc.publisher.nameVersita - Springer Verlagen
dc.relation.ispartofActa Geophysicaen
dc.relation.ispartofseries3/58(2010)en
dc.subjectionogramen
dc.subjectionosondeen
dc.subjectAutoscala programen
dc.subjectautomatic scalingen
dc.subjectionospheric monitoringen
dc.titleAutoscala: an aid for different ionosondesen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber513-526en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.05. Wave propagationen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.identifier.doi10.2478/s11600-009-0038-1en
dc.relation.referencesBelehaki, A., L. Cander, B. Zolesi, J. Bremer, C. Juren, I. Stanislawska, D. Dialetis, and M. Hatzopoulos (2005), DIAS Project: The establishment of a European digital upper atmosphere server, J. Atmos. Sol. Terr. Phys., 67, 12, 1092–1099. Belehaki, A., L. Cander, B. Zolesi, J. Bremer, C. Juren, I. Stanisławska, D. Dialetis, and M. Hatzopoulos (2007), Ionospheric specification and forecasting based on observations from European ionosondes participating in DIAS project, Acta Geophys. 55, 3, 398-409. Gajdanskij, V. I., A. L. Karpenko, I. V. Krasheninnikov, N. I. Manaenkova, S. V. Silvestrov, A. A. Smirnov (1996), The Base Network Digital Ionospheric Station “PARUS”, XXVth General Assembly of the International Union of Radio Science, Abstract 360. Gilbert, J. D., and R. W. Smith (1988), A comparison between the automatic ionogram scaling system ARTIST and the standard manual method, Radio Sci., 23, 6, 968–974. Jacobs, L., A. W. V. Poole, and L. A. McKinnel (2004), An analysis of automatically scaled F1 layer data over Grahamstown, South Africa, Adv. Space Res., 34, 1949–1952. Materassi, M., C. N. Mitchell (2005), A simulation study into constructing of the sample space for ionospheric imaging, J. Atmos. Sol. Terr. Phys., 67, 12, 1085–1091. McNamara, L. F. (2006), Quality figures and errors bars for autoscaled Digisonde vertical incidence ionograms, Radio Sci., 41, RS4011, doi:10.1029/2005RS003440. McNamara, L. F., D. T. Decker, J. A. Welsh, D. G. Cole (2007), Validation of the Utah State University Global Assimilation of Ionospheric Measurements (GAIM) model predictions of the maximum usable frequency for a 3000 km circuit, Radio Sci., 42, RS3015, doi:10.1029/2006RS003589. Pezzopane, M., and C. Scotto (2005), The INGV software for the automatic scaling of foF2 and MUF(3000)F2 from ionograms: A performance comparison with ARTIST 4.01 from Rome data, J. Atmos. Sol. Terr. Phys., 67, 12, 1063–1073. Pezzopane, M., and C. Scotto (2007), The Automatic Scaling of Critical Frequency foF2 and MUF(3000)F2: a comparison between Autoscala and ARTIST 4.5 on Rome data, Radio Sci., 42, RS4003, doi:10.1029/2006RS003581. Pezzopane, M., and C. Scotto (2008), A method for automatic scaling of F1 critical frequencies from ionograms, Radio Sci., 43, RS2S91, doi:10.1029/2007RS003723. Pezzopane, M., C. Scotto, I. Stanislawska, and G. Juchnikowski (2008), Autoscala applied at the Ionospheric Station of Warsaw, INAG (Ionosonde Network Advisory Group) bulletin 69, http://www.ips.gov.au/IPSHosted/INAG/web-69/index.html. Reinisch, B.W., and X. Huang (1983), Automatic calculation of electron density profiles from digital ionograms 3. Processing of bottomside ionograms, Radio Sci., 18 (3), 477-492. Scotto, C., in press, Electron density profile calculation technique for Autoscala ionogram analysis, Adv. Space Res.. Scotto, C., and M. Pezzopane (2007), A method for automatic scaling of sporadic E layers from ionograms, Radio Sci., 42, RS2012, doi: 10.129/2006RS003461. Zuccheretti, E., G. Tutone, U. Sciacca, C. Bianchi, and B. J. Arokiasamy (2003), The new AIS-INGV digital ionosonde, Ann. Geophys.-Italy, 46, 4, 647–659.en
dc.description.obiettivoSpecifico1.7. Osservazioni di alta e media atmosferaen
dc.description.obiettivoSpecifico3.9. Fisica della magnetosfera, ionosfera e meteorologia spazialeen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorPezzopane, M.en
dc.contributor.authorScotto, C.en
dc.contributor.authorTomasik, L.en
dc.contributor.authorKrasheninnikov, I.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, 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 Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptSpace Research Center PAS, Warsaw, Poland-
crisitem.author.deptInstitute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation, Russian Academy of Sciences, Troitsk, Moscow Region, Russia-
crisitem.author.orcid0000-0001-5800-2322-
crisitem.author.orcid0000-0002-9437-6775-
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.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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