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Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/9339
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dc.contributor.authorallIppolito, A.; 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.authorallFrancis, M.; IPS Radio & Space Services, Bureau of Meteorology, Level 15, Tower C, 300 Elizabeth Street, Sydney, Australiaen
dc.contributor.authorallSettimi, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallCesaroni, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2015-02-23T13:02:00Zen
dc.date.available2015-02-23T13:02:00Zen
dc.date.issued2015-03-15en
dc.identifier.urihttp://hdl.handle.net/2122/9339en
dc.description.abstractWe present an algorithm for the identification of trace characteristics of oblique ionograms allowing determination of the Maximum Usable Frequency (MUF) for communication between the transmitter and receiver. The algorithm automatically detects and rejects poor quality ionograms. We performed an exploratory test of the algorithm using data from a campaign of oblique soundings between Rome, Italy (41.90 N, 12.48 E) and Chania, Greece (35.51 N, 24.01 E) and also between Kalkarindji, Australia (17.43 S, 130.81 E) and Culgoora, Australia (30.30 S, 149.55 E). The success of these tests demonstrates the applicability of the method to ionograms recorded by different ionosondes in various helio and geophysical conditions.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofAdvances in space researchen
dc.relation.ispartofseries6/55 (2015)en
dc.subjectIonosphereen
dc.subjectElectron densityen
dc.subjectOblique ionogramsen
dc.subjectMUFen
dc.titleAutomatic interpretation of oblique ionogramsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber1624-1629en
dc.identifier.URLhttp://www.sciencedirect.com/science/article/pii/S0273117714008011en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneousen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.04. Plasma Physicsen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.06. Instruments and techniquesen
dc.subject.INGV05. General::05.01. Computational geophysics::05.01.99. General or miscellaneousen
dc.subject.INGV05. General::05.01. Computational geophysics::05.01.03. Inverse methodsen
dc.subject.INGV05. General::05.01. Computational geophysics::05.01.05. Algorithms and implementationen
dc.identifier.doi10.1016/j.asr.2014.12.025en
dc.relation.referencesCesaroni, C., Scotto, C., Ippolito, A., 2013. An automatic quality factor for Autoscala foF2 values. Adv. Space Res., 51 (12), 2316-2321, doi: 10.1016/j.asr.2013.02.009. Galkin, I. A., Khmyrov, G. M., Kozlov, A. V., Reinisch, B. W., Huang, X., Paznukhov, V. V., 2008. The ARTIST 5. In: Radio Sounding and Plasma Physics, AIP Conf. Proc., 974, 150–159, doi:10.1063/1.2885024. Galkin, I. A., Reinisch, B. W., Huang, X., Bilitza, D., 2012. Assimilation of GIRO data into a real-time IRI. Radio Sci., 47 (4), RS0L07 [10 pages], doi:10.1029/2011RS004952. Gilbert, J. D., Smith, R. W., 1988. A comparison between the automatic ionogram scaling system ARTIST and the standard manual method. Radio Sci., 23 (6), 968–974, doi: 10.1029/RS023i006p00968. Huang, X., Reinisch, B. W., Kuklinski, W. S., 1996. Mid-point electron density profiles from oblique ionograms. Ann. Geophys. - Italy, 49 (4), 757-761, doi: 10.4401/ag-4012. Norman, R. J., and Cannon, P. S., 1999. An evaluation of a new two-dimensional analytic ionospheric ray-tracing technique: Segmented method for analytic ray tracing (SMART). Radio Sci., 34 (2), 489-499, doi: 10.1029/98RS01788. Pezzopane, M., Scotto, C., 2007. Automatic scaling of critical frequency foF2 and MUF (3000) F2: A comparison between Autoscala and ARTIST 4.5 on Rome data. Radio Sci., 42 (4), RS4003 [17 pages], doi:10.1029/2006RS003581. Piggott, W. R., Rawer, K., 1972. U.R.S.I. Handbook of Ionogram Interpretation and Reduction. U.S. Department of Commerce National Oceanic and Atmospheric Administration-Environmental Data Service, Asheville, North Carolina, USA. Reinisch, B. W., Huang, X., 1983. Automatic calculation of electron density profiles from digital ionograms: 3. Processing of bottomside ionograms. Radio Sci., 18 (3), 477–492, doi: 10.1029/RS018i003p00477. Scotto, C., 2009. Electron density profile calculation technique for Autoscala ionogram analysis. Adv. Space Res., 44 (6), 756-766, doi: 10.1016/j.asr.2009.04.037. Scotto, C., Pezzopane, M., 2002. A software for automatic scaling of foF2 and MUF(3000)F2 from ionograms. URSI XXVII General Assembly (http://www.ursi.org/Proceedings/ProcGA02/papers/p1018.pdf). Scotto, C., Pezzopane, M., 2004. Software for the automatic scaling of critical frequency f0F2 and MUF(3000) F2 from ionograms applied at the Ionospheric Observatory of Gibilmanna. Ann. Geophys. - Italy, 47 (6), 1783–1790, doi: 10.4401/ag-3375. Stankov, S. M., Jodogne, J. C., Kutiev, I., Stegen, K., Warnan R., 2012. Evaluation of automatic ionogram scaling for use in real-time ionospheric density profile specification: Dourbes DGS-256/ARTIST-4 performance. Ann. Geophys. - Italy, 55 (2), 283-291, doi: 10.4401/ag-4976.en
dc.description.obiettivoSpecifico2A. Fisica dell'alta atmosferaen
dc.description.journalTypeJCR Journalen
dc.description.fulltextpartially_openen
dc.relation.issn0273-1177en
dc.relation.eissn1879-1948en
dc.contributor.authorIppolito, A.en
dc.contributor.authorScotto, C.en
dc.contributor.authorFrancis, M.en
dc.contributor.authorSettimi, A.en
dc.contributor.authorCesaroni, C.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
dc.contributor.departmentIPS Radio & Space Services, Bureau of Meteorology, Level 15, Tower C, 300 Elizabeth Street, Sydney, Australiaen
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.deptIPS Radio & Space Services, Bureau of Meteorology, Level 15, Tower C, 300 Elizabeth Street, Sydney, Australia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0003-3823-127X-
crisitem.author.orcid0000-0002-9437-6775-
crisitem.author.orcid0000-0002-9487-2242-
crisitem.author.orcid0000-0003-2268-4389-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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.classification.parent05. General-
crisitem.classification.parent05. General-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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