Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/7315
DC Field | Value | Language |
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dc.contributor.authorall | Scotto, C.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
dc.date.accessioned | 2012-01-17T09:33:49Z | en |
dc.date.available | 2012-01-17T09:33:49Z | en |
dc.date.issued | 2011 | en |
dc.identifier.uri | http://hdl.handle.net/2122/7315 | en |
dc.description.abstract | An algorithm is proposed for evaluation of the probability of occurrence of an F1 layer or L condition, based on tables. Observations independent of the tables database are used for comparison between the estimated probability of occurrence, the formulation used at present in IRI, and the occurrence actually observed. The importance of the inclusion of L condition in the electron density profile model is shown. | en |
dc.language.iso | English | en |
dc.publisher.name | Alsevier | en |
dc.relation.ispartof | Advances in Space Research | en |
dc.relation.ispartofseries | /48 (2011) | en |
dc.subject | Ionosphere, F1 layer, Electron density profile models | en |
dc.title | Estimation of probability of occurrence of F1 layer or L condition using tables and electron density profile models | en |
dc.type | article | en |
dc.description.status | Published | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.description.pagenumber | 2053-2056 | en |
dc.identifier.URL | http://www.sciencedirect.com/science/article/pii/S0273117711006156 | en |
dc.subject.INGV | 01. Atmosphere::01.02. Ionosphere::01.02.99. General or miscellaneous | en |
dc.identifier.doi | 10.1016/j.asr.2011.08.019 | en |
dc.relation.references | Du Charme, E.D., and L. E. Petrie, A method for predicting the F1 layer critical frequency based on the Zurich smoothed sunspot number, Radio Sci., 8, 837, 1973. Reinisch, B. W., Huang, X. Redefining the IRI F1 Layer Profile, Adv. Space Res. 25, 81-88, 2000. Scotto, C., M.M. de Gonzalez, S.M. Radicella and B. Zolesi, On the prediction of F1 ledge and critical frequency, Adv. Space Res., 20, 1773-1775, 1997. Scotto, C:, S.M. Radicella, and Zolesi B, An improved probability function to predict the F1 layer occurrence and L condition, Radio Sci., 33, 1763-1765, 1998. Cardinali, F. “Probabilità di occorrenza dello strato ionosferico F1 e condizione L”, Thesis work for the degree of “Laurea in Fisica” (in Italian), 2001. Scotto, C., Pezzopane, M., A software for automatic scaling of foF2 and MUF(3000)F2 from ionograms, Proceeding of URSI XXVIIth General Assembly, 17-24 August 2002, Maastricht, Holland. Scotto, C., , The probability of occurrence of F1 layer or L condition estimated by tables, Adv. Space Res., 29, 987-992, 2002. Pezzopane, M., Scotto, C. , “The INGV software for the automatic scaling of foF2 and MUF(3000)F2 from ionograms: A performance comparison with ARTIST from Rome data” J. Atmos Sol Terr Phys., vol. 67, pp. 1063-1073, 2005. Scotto C. “Electron density profile calculation technique for Autoscala ionogram analysis “Adv. Space Res., vol. 44, pp. 756-766, 2009. | en |
dc.description.obiettivoSpecifico | 3.9. Fisica della magnetosfera, ionosfera e meteorologia spaziale | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | reserved | en |
dc.contributor.author | Scotto, C. | en |
dc.contributor.department | Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italia | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | restricted | - |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | Istituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia | - |
crisitem.author.orcid | 0000-0002-9437-6775 | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 01. Atmosphere | - |
crisitem.department.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
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ASR_F1_Tables_Profile.pdf | 555.05 kB | Adobe PDF |
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