Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/8103
DC FieldValueLanguage
dc.contributor.authorallScotto, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallSettimi, A.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.date.accessioned2012-10-09T09:06:22Zen
dc.date.available2012-10-09T09:06:22Zen
dc.date.issued2013en
dc.identifier.urihttp://hdl.handle.net/2122/8103en
dc.description.abstractThe results of this paper demonstrate that the effect of collisions on the group refraction index is small, when the ordinary ray is considered. If, however, in order to improve the performance of a system for automatic interpretation of ionograms, the information contained in ordinary and extraordinary traces is combined, the effect of collisions between the electrons and neutral molecules should be taken into account for the extraordinary ray. The magnitude of these differences is generally very small and must be compared with the resolution in the virtual vertical height of the ionosonde, resolution which is typically of the order of few kilometers.en
dc.language.isoEnglishen
dc.publisher.nameElsevier Science Limiteden
dc.relation.ispartofAdvances in space researchen
dc.relation.ispartofseries/51 (2013)en
dc.subjectIonogram inversionen
dc.subjectEarth's magnetic fielden
dc.subjectelectron-neutral molecule collisionsen
dc.subjectordinary and extraordinary rayen
dc.subjectphase and group refraction indexen
dc.titleThe effect of collisions in ionogram inversionen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber697-701en
dc.identifier.URLhttp://www.sciencedirect.com/science/article/pii/S0273117712006230?v=s5en
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.04. Plasma Physicsen
dc.subject.INGV01. Atmosphere::01.02. Ionosphere::01.02.05. Wave propagationen
dc.subject.INGV05. General::05.01. Computational geophysics::05.01.03. Inverse methodsen
dc.identifier.doi10.1016/j.asr.2012.09.033en
dc.relation.referencesBudden, K. G. Radio waves in the ionosphere. Cambridge University Press, Cambridge, United Kingdom, 1961. Davies, K., Ionospheric Radio, Peter Peregrinus Ltd. (ed.), London, UK, 1990. Huang, X., Reinisch, B. W. Vertical Electron density profiles from the digisonde network. Adv. Space Res. 18 (6) , 121-(6)129, 1996. Pezzopane, M., Scotto, C. Software for the automatic scaling of critical frequency foF2 and MUF(3000)F2 from ionograms applied at the Ionospheric Observatory of Gibilmanna. Ann. Geophysics, 47, 1783-1790, 2004. Scotto, C. Electron Density profile calculation technique for Autoscala ionogram analysis. Adv. Space Res. 44, 756-766, 2009. Scotto, C., Pezzopane, M. A software for automatic scaling of foF2 and MUF(3000)F2 from ionograms. Proceedings of URSI 2002, Maastricht, 17-24 august, 2002 (on CD). Scotto, C., Pezzopane, M. and Zolesi, B. Estimating the vertical electron density profile from an ionogram: On the passage from true to virtual heights via the target function method. Radio Scie.Vol. 47, RS1007, 6 PP., 2012, doi:10.1029/2011RS004833. Shinn, D. H. and Whale H. A. Group velocities and group heights from magnetoionic theory. J. Atmos. Terr. Phys. 2, 85-105, 1952. Titheridge, J. E. Ionogram analysis with the generalised program POLAN. World Data Center A for Solar-Terrestrial Physics, Boulder, CO (USA), Technical Report PB-89-152482/XAB UAG-93, 204 pp., 1985.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.fulltextrestricteden
dc.relation.issn0273-1177en
dc.relation.eissn1879-1948en
dc.contributor.authorScotto, C.en
dc.contributor.authorSettimi, A.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.grantfulltextrestricted-
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.orcid0000-0002-9437-6775-
crisitem.author.orcid0000-0002-9487-2242-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent01. Atmosphere-
crisitem.classification.parent05. General-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
Appears in Collections:Article published / in press
Files in This Item:
File Description SizeFormat Existing users please Login
1-s2.0-S0273117712006230-main.pdfMain article569.16 kBAdobe PDF
Show simple item record

WEB OF SCIENCETM
Citations

2
checked on Feb 10, 2021

Page view(s) 20

365
checked on Apr 24, 2024

Download(s)

35
checked on Apr 24, 2024

Google ScholarTM

Check

Altmetric