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Elsevier",{"EN":70,"VI":72},"Cơ sở dữ liệu Scopus thuộc Elsevier","scopus",[75],"SCOPUS","https:\u002F\u002Fwww.scopus.com\u002Fsourceid\u002F15400155600","1978-2023",[79,80],"0c2541d6-7567-4793-aad8-840b3d33f5e0","697fa560-384f-48e0-b639-8db9f902c6c5",{"id":82,"indexDatabase":83,"url":97,"indexYears":20,"academicFieldIds":98,"indexDatabaseRanking":20},"b77bf1fe-a12f-4eaf-8363-150312bb736b",{"id":84,"createTime":85,"updateTime":86,"relativeEntities":87,"label":88,"description":90,"key":93,"publicationTags":94,"standard":20},"88bab0f7-443b-476c-a72a-7fa5222da393","2023-05-22T09:58:31.181+00:00","2025-11-21T10:07:52.271+00:00",[],{"EN":89,"VI":89},"ISI\u002FESCI  - Emerging Sources Citation Index",{"VI":91,"EN":92},"Cơ sở dữ liệu ESCI","ESCI database","esci",[95,96],"ESCI","ISI","https:\u002F\u002Fmjl.clarivate.com\u002Fsearch-results?issn=2037-4909",[99],"0db73426-2364-455f-81a4-efe0f91d712e","https:\u002F\u002Flink.springer.com\u002Fjournal\u002F11543",{"impactFactor":21,"impactFactorByYear":102,"i10Index":21,"i10IndexLast5Year":21,"totalPublication":103,"totalPublicationByYear":104,"totalCitation":21,"totalCitationByYear":105,"totalCitationPerPublication":21,"totalCitationPerPublicationByYear":106,"hindexLast5Year":21,"hindex":21},{},3,{"1992":103},{},{},"JOURNAL",{"meta":109,"data":111},{"total":110},"843",[112,197,265,368,505,620,838,916,1051,1343],{"id":113,"createTime":114,"updateTime":115,"relativeEntities":116,"slug":117,"properties":118,"entityType":127,"verifyStatus":128,"verifyTime":115,"verifyNote":129,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21,"primaryUrl":130,"fullTextUrl":20,"authors":131,"publicationType":159,"publisherRelationship":160,"citationCount":20,"citationInfo":20,"publishDate":194,"publishYear":195,"citationAnalyzeStatus":19,"lastCitationAnalyze":20,"indexDatabases":20,"openAccess":20,"references":20,"isForceReanalyzing":196},"5ed45684-e4b5-46ee-afef-2a4cb8d1ede4","2023-12-06T19:54:56.045+00:00","2025-02-17T23:58:45.628+00:00",[],"The-solar-neutrino-problem-1995",{"references":119,"abstract":121,"title":123,"doi":125},{"VOID":120},"GALLEX Collaboration (P. Anselman et al.),Phys. Lett. B,361 (1995) 235.\nSAGE Collaboration (V. N. Gavrin et al.), talk at theInternational Workshop TAUP-95 (Toledo) 1995.\nInoue K., talk atXXX Rencontres de Moriond, March 12–18, 1995.\nHOMESTAKE Collaboration (B. T. Cleveland et al.),Nucl. Phys. B (Proc. Suppl.),39 (1995) 47.\nBahcall J. N. andPinsonneault M., preprint IASSNS-AST 95\u002F24 to be published inRev. Mod. Phys. (1995).\nBahcall, J. N. andBethe H. A.,Phys. Rev. Lett.,65 (1990) 2233.\nBahcall J. N.,Neutrino Astrophysics (Cambridge University Press, Cambridge) 1989.\nTurck-Chieze S., Däppen W., Fossat E., Provost J., Schatzmann E. andVignaud D.,Phys. Rep.,230 (1993) 57.\nKovetz A. andShaviv G.,Astrophys. J.,426 (1994) 787.\nCastellani V., Degl'Innocenti S. andFiorentini F.,Astron. Astrophys.,271 (1993) 601.\nTurck-Chiese S. andLopes I.,Astrophys. J.,408 (1993) 347.\nBerthomieu G. et al., Astron. Astrophys.,268 (1993) 775.\nGünter D. B. et al., Astrophys. J.,387 (1992), 372.\nChristiansen-Dalsgaard J.:Geophys. Astrophys. Fluid. Dyn.,62 (1992) 123.\nAhrens B., Stix M. andThorn M.,Astron. Astrophys.,264 (1992) 673.\nGuzik J. A. andCox A. N.,Astrophys. J. Lett.,381 (1991) 331.\nProffitt C. R. andCox A. N.,Astrophys. J.,380 (1991) 238.\nSackman I. J., Boothroyd A. I. andFowler W. A.,Astrophys. J.,360 (1990) 727.\nLebreton Y. andDäppen W., inSeismology of the Sun and the Sun-like Stars, edited byV. Domingo andE. J. Rolfe (European Space Agency, Noordwijk) 1988.\nBahcall J. N.,Phys. Rev. Lett.,71 (1993) 2369.\nTsytovich V., inSolar Neutrino Problem, edited byV. Berezinksy andE. Fiorini, Vol.1 (1994), p. 238.\nHata N., Bludman S. andLangacker P.,Phys. Rev. D,49 (1994) 3622.\nBerezinsky V.:Commun. Nucl. Part. Phys.,21 (1994) 249.\nRaghavan R. S.:Science,267 (1995) 45.\nBahcall J.,Phys. Lett. B,338 (1994) 276.\nDegl'Innocenti S., Fiorentini G. andLissia M.:Nucl. Phys. B (Proc. Suppl.),43 (1995) 66.\nCastellani V., Degl'Innocenti S., Fiorentini G., Lissia M. andRicci B.,Phys. Rev. D,50 (1994) 4749.\nKwong W. andRosen S. P.,Phys. Rev. Lett.,73 (1994) 369.\nAppessella C. et al., «Borexino at Gran Sasso» (Proposal), edited byG. Bellini andR. Raghavan (INFN, University of Milan) 1991Bellotti E.,Nucl. Phys. B, (Proc. Suppl.),38 (1995) 90.\nKirsten T., invited talk atXVII TEXAS Symposium on Relativistic Astrophysics, Munich, 1994, to be published inAnn. N.Y. Acad. Sci. (1995).\nKirsten T., invited talk at theInternational Conference «Neutrino-94», Nucl. Phys. B (Proc. Suppl.),38 (1995) 68.\nHampel W., talk at the Topical Session«Beryllium Neutrinos: Problem and Detection», Gran Sasso, 1995.\nBerezinsky V.,International Workshop «Neutrino Telescopes», Venice, February 22–24, 1994, edited byM. Baldo Ceolin (1994), p. 239.\nMikheyev S. P. andSmirnov A. Yu.:Yad. Fiz.,42 (1985) 1141;Wolfenstein L.,Phys. Rev. D,17 (1978) 2369.\nPontecorvo B.:Ž. Ėksp. Teor. Fiz.,33 (1953) 549.\nKrastev P. I. andPetcov S. T., preprint SISSA 4\u002F94\u002FEP;Petcov S. T., talk atRencontres de Physique de la Vallee d'Aoste, 1995.\nVoloshin M. B., Vysotsky M. I. andOkun L. B.:Sov. Phys. JETP,64 (1988) 446.\nAkhmedov E. Kh.:Phys. Lett. B,213 (1988) 64;Lim C. S. andMarciano W.,Phys. Rev. D,37 (1988) 1368.\nMikheyev S. P. andSmirnov A. Yu.,Proceedings of Weak and Electromagnetic Interactions in Nuclei (Heidelberg, 1986), edited byH. V. Klapdor (1987), p. 710;Guzzo M., Masiero A. andPetcov S. T.,Phys. Lett. B,260 (1991) 154;Roulet E.,Phys. Rev. D,44 (1991) R935.\nBowles T. J. andGavrin V. N.:Annu. Rev. Nucl. Part. Sci.,43 (1993) 117.\nMotobayashi T. et al., Phys. Rev. Lett.,73 (1994) 2680.\nShi X. andSchramm D. N.:Part. World,3 (1993) 149;Schramm D. N. andShi X.,Nucl. Phys. B, (Proc. Suppl.),35 (1994) 321;Shi X., Schramm D. N. andDearborn D. S.,Phys. Rev. D,50 (1994) 2414.\nDar A. andShaviv G., Preprint Technion, Ph-94-5, (1994);Shaviv G.,Nucl. Phys. B, (Proc. Suppl.),38 (1995) 81.\nBerezinsky V., Fiorentini G. andLissia M., preprint LNGS 95\u002F56, August 1995.\nKrastev P. I. andSmirnov A. Yu.:Phys. Lett. B,338 (1994) 282.\nBerezinsky V., Fiorentini G. andLissia M.:Phys. Lett. B,341 (1994) 38.\nBieber J. W., Seckel D., Stanev T. andSteigman G.:Nature,348 (1990) 407.\nFilippone B. W. andVogel P.:Phys. Lett. B,246 (1990) 546.\nBahcall J. N. andPress W. H.,Astrophys. J.,370 (1991) 730.\nGavryusev V. andGavryuseva E.,Proceedings of the VI International Workshop «Neutrino Telescopes», edited byM. Baldo Ceolin (1994), p. 319.\nStanev T.,Proceedings of the International Workshop «Solar-Neutrino Problem: Astrophysics or Oscillations?», edited byV. Berezinsky andE. Fiorini (1994), Vol.2, p. 51.\nObridko V. N. andRivin Yu. R., to be published inIzv. Russian Acad. Sci., Ser. Phys., Vol.9 (1995).\nOakley D. S. et al., Astrophys. J., L63 (1994) 437.\nSuzuki Y.,Proceedings of the VI International Workshop «Neutrino Telescopes», edited byM. Baldo Ceolin (1994), p. 191.\nTotsuka Y., talk at theInternational Workshop TAUP-95 (1995).\nAkhmedov E. Kh.,Proceedings of the VI International Workshop «Neutrino Telescopes», edited byM. Baldo Ceolin (1994), p. 285.\nYpsilantis T. et al., preprint LPC-92-31;Bonvicini G.,Nucl. Phys. B, (Proc. Suppl.),35 (1994) 438.",{"EN":122},"The status of the Solar-Neutrino Problem (SNP), as is seen in 1995, is reviewed. Basically, there are two principal solutions to the SNP: i) withstandard neutrino (neutrino of SM of electroweak interactions) and ii) withnon-standard neutrino (neutrino beyond the SM). Actually, one can distinguish three solar-neutrino problems: the deficit of8B neutrinos, the deficit of7Be neutrinos and the HOMESTAKE\u002FKAMIOKANDE conflict. The first problem probably can be solved with small correlated changes of nuclear cross-sections and the change of the central temperature of the Sun. The deficit of7Be neutrinos looks like the key problem. The HOMESTAKE\u002FKAMIOKANDE conflict strongly disfavours or excludes the standard neutrino (nuclear\u002Fastrophysical solution to the SNP). MSW conversion gives a most plausible explanation to the SNP.",{"EN":124},"The solar-neutrino problem, 1995",{"VOID":126},"10.1007\u002FBF02506647","PUBLICATION","VERIFIED","Auto Verify","http:\u002F\u002Flink.springer.com\u002F10.1007\u002FBF02506647",[132],{"id":133,"sortIndex":21,"researcher":20,"roles":134,"affiliations":136,"properties":156},"f9b886a4-bee5-4231-ae76-7e0336d0e4e0",[135],"AUTHOR",[137,145],{"id":20,"sortIndex":21,"affiliation":138,"properties":20},{"id":139,"createTime":140,"updateTime":140,"relativeEntities":141,"slug":20,"properties":142,"entityType":49,"verifyStatus":19,"verifyTime":20,"verifyNote":20,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21},"6affa1ba-cb7f-4cff-95bf-01185bd8193b","2024-01-09T13:42:05.360+00:00",[],{"title":143},{"VI":144},"Laboratori Nazionali del Gran Sasso, INFN, Assergi (AQ), Italy",{"id":146,"sortIndex":147,"affiliation":148,"properties":155},"7afc4bd4-3d98-43f3-9d5c-84ae64ee0759",1,{"id":149,"createTime":150,"updateTime":150,"relativeEntities":151,"slug":20,"properties":152,"entityType":49,"verifyStatus":19,"verifyTime":20,"verifyNote":20,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21},"4b0ae5a0-91a8-4d55-88d3-1df566033529","2023-12-06T19:54:56.066+00:00",[],{"title":153},{"VI":154},"Institute for Nuclear Research of RAN, Moscow, Russia",{},{"title":157},{"VI":158},"V. Berezinsky","ARTICLE",{"url":130,"publisher":161,"properties":189},{"id":6,"createTime":7,"updateTime":8,"relativeEntities":162,"slug":10,"properties":163,"entityType":18,"verifyStatus":19,"verifyTime":20,"verifyNote":20,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21,"subjectFields":167,"manageAffiliations":168,"indexDatabases":169,"url":100,"thumbnailPath":20,"statistic":184,"gsStatistic":20,"type":107,"analyzePriority":20},[],{"issn":164,"eissn":165,"title":166},{"VOID":13},{"VOID":15},{"EN":17},[],[],[170,177],{"id":82,"indexDatabase":171,"url":97,"indexYears":20,"academicFieldIds":176,"indexDatabaseRanking":20},{"id":84,"createTime":85,"updateTime":86,"relativeEntities":172,"label":173,"description":174,"key":93,"publicationTags":175,"standard":20},[],{"EN":89,"VI":89},{"VI":91,"EN":92},[95,96],[99],{"id":63,"indexDatabase":178,"url":76,"indexYears":77,"academicFieldIds":183,"indexDatabaseRanking":20},{"id":65,"createTime":66,"updateTime":67,"relativeEntities":179,"label":180,"description":181,"key":73,"publicationTags":182,"standard":20},[],{"EN":70,"VI":70},{"EN":70,"VI":72},[75],[79,80],{"impactFactor":21,"impactFactorByYear":185,"i10Index":21,"i10IndexLast5Year":21,"totalPublication":103,"totalPublicationByYear":186,"totalCitation":21,"totalCitationByYear":187,"totalCitationPerPublication":21,"totalCitationPerPublicationByYear":188,"hindexLast5Year":21,"hindex":21},{},{"1992":103},{},{},{"volume":190,"pages":192},{"VOID":191},"18",{"VOID":193},"671-684","1995-11-01",1995,false,{"id":198,"createTime":199,"updateTime":200,"relativeEntities":201,"slug":202,"properties":203,"entityType":127,"verifyStatus":128,"verifyTime":200,"verifyNote":129,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21,"primaryUrl":212,"fullTextUrl":20,"authors":213,"publicationType":159,"publisherRelationship":229,"citationCount":20,"citationInfo":20,"publishDate":263,"publishYear":264,"citationAnalyzeStatus":19,"lastCitationAnalyze":20,"indexDatabases":20,"openAccess":20,"references":20,"isForceReanalyzing":196},"02c0d51d-7eb3-4975-90c7-6544ae8d216f","2023-12-28T14:46:28.406+00:00","2024-12-27T23:53:02.107+00:00",[],"On-the-relationship-between-the-gradient-and-the-bulk-Richardson-number-for-the-atmospheric-surface-layer",{"references":204,"abstract":206,"title":208,"doi":210},{"VOID":205},"D. Golder:Boundary-Layer Meteorol.,3, 47 (1972).\nN. M. Zoumakis andA. G. Kelessis:Nuovo Cimento C,14, 587 (1991).\nJ. S. Irwin andF. S. Binkowski:Atmos. Environ.,15, 1091 (1981).\nF. S. Binkowski:Atmos. Environ.,9, 453 (1975).\nE. H. Barker andT. L. Baxter:J. Appl. Meteorol.,14, 620 (1975).\nJ. Y. Ku, S. T. Rao andK. S. Rao:Atmos. Environ.,21, 201 (1987).\nJ. F. Louis:Boundary-Layer Meteorol.,17, 187 (1979).\nY. Delage:Boundary-Layer Meteorol.,43, 365 (1988).\nD. W. Byun:J. Appl. Meteorol.,29, 652 (1990).\nN. M. Zoumakis andA. G. Kelessis:The dependence of the bulk Richardson number on stability in the surface layer, to be published inBoundary-Layer Meteorol.\nH. Lettau andB. Davidson:Exploring the Atmosphere's Firts Mile (Pergamon Press, Inc., New York, N.Y., 1957).\nM. Segal andR. A. Pielke:J. Appl. Meteorol.,27, 174 (1988).\nR. R. Draxler:Atmos. Environ.,13, 1559 (1979).\nN. M. Zoumakis andA. G. Kelessis:On the theoretical variation of the Monin-Obukhov stability parameter as a function of the bulk Richardson number, submitted toJ. Appl. Meteorol.\nJ. A. Businger, J. C. Wyngaard, Y. Izumi andE. F. Bradley:J. Atmos. Sci.,28, 181 (1971).\nN. M. Zoumakis andA. G. Kelessis:Boundary-Layer Meteorol.,55, 199 (1991).\nC. H. Huang:Atmos. Environ.,13, 453 (1979).\nJ. S. Irwin:Atmos. Environ.,13, 191 (1979).\nL. Sedefian:J. Appl. Meteorol.,19, 488 (1980).\nH. A. Panofsky andB. Prasad:Int. J. Air Water Pollut.,9, 419 (1965).\nH. A. Panofsky andJ. A. Dutton:Atmospheric Turbulence (Wiley and Sons, 1983), p. 397.",{"EN":207},"Semi-empirical formulations which have been proposed to describe the wind and potential temperature profiles are used to derive relationships between the gradient Richardson number, Ri, the finite-difference layer Richardson number, Rib, the surface layer Richardson number, Ris, and the bulk Richardson number,B, through the atmospheric surface layer. The theoretical analysis for stable conditions indicates that Ri (z\n                3)=Rib, wherez\n                3=(z\n                2−z\n                1)\u002Fln(z\n                2\u002Fz\n                1), andz\n                2;z\n                1=upper and lower levels at which temperature and wind speed are specified. It is also found that, during stable conditions, the wind profile power law exponent,p, is computed at the heightz\n                3, instead of the widely used geometric mean height,z\n                m, between top (z\n                2) and bottom (z\n                1) of the layer considered.",{"EN":209},"On the relationship between the gradient and the bulk Richardson number for the atmospheric surface layer",{"VOID":211},"10.1007\u002FBF02507777","https:\u002F\u002Flink.springer.com\u002Farticle\u002F10.1007\u002FBF02507777",[214],{"id":215,"sortIndex":21,"researcher":20,"roles":216,"affiliations":217,"properties":226},"289d8881-899b-4359-b01b-12b3c2f82c26",[135],[218],{"id":20,"sortIndex":21,"affiliation":219,"properties":20},{"id":220,"createTime":221,"updateTime":221,"relativeEntities":222,"slug":20,"properties":223,"entityType":49,"verifyStatus":19,"verifyTime":20,"verifyNote":20,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21},"5af93cfb-668c-4a14-89e8-b6de1b773390","2023-12-07T19:26:51.914+00:00",[],{"title":224},{"VI":225},"Laboratory of Atmospheric Physics, Technological Education Institute (T.E.I.), Thessaloniki, Greece",{"title":227},{"VI":228},"N. M. Zoumakis",{"url":212,"publisher":230,"properties":258},{"id":6,"createTime":7,"updateTime":8,"relativeEntities":231,"slug":10,"properties":232,"entityType":18,"verifyStatus":19,"verifyTime":20,"verifyNote":20,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21,"subjectFields":236,"manageAffiliations":237,"indexDatabases":238,"url":100,"thumbnailPath":20,"statistic":253,"gsStatistic":20,"type":107,"analyzePriority":20},[],{"issn":233,"eissn":234,"title":235},{"VOID":13},{"VOID":15},{"EN":17},[],[],[239,246],{"id":82,"indexDatabase":240,"url":97,"indexYears":20,"academicFieldIds":245,"indexDatabaseRanking":20},{"id":84,"createTime":85,"updateTime":86,"relativeEntities":241,"label":242,"description":243,"key":93,"publicationTags":244,"standard":20},[],{"EN":89,"VI":89},{"VI":91,"EN":92},[95,96],[99],{"id":63,"indexDatabase":247,"url":76,"indexYears":77,"academicFieldIds":252,"indexDatabaseRanking":20},{"id":65,"createTime":66,"updateTime":67,"relativeEntities":248,"label":249,"description":250,"key":73,"publicationTags":251,"standard":20},[],{"EN":70,"VI":70},{"EN":70,"VI":72},[75],[79,80],{"impactFactor":21,"impactFactorByYear":254,"i10Index":21,"i10IndexLast5Year":21,"totalPublication":103,"totalPublicationByYear":255,"totalCitation":21,"totalCitationByYear":256,"totalCitationPerPublication":21,"totalCitationPerPublicationByYear":257,"hindexLast5Year":21,"hindex":21},{},{"1992":103},{},{},{"volume":259,"pages":261},{"VOID":260},"15",{"VOID":262},"111-114","1992-01-01",1992,{"id":266,"createTime":267,"updateTime":268,"relativeEntities":269,"slug":270,"properties":271,"entityType":127,"verifyStatus":128,"verifyTime":268,"verifyNote":129,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":280,"primaryUrl":281,"fullTextUrl":20,"authors":282,"publicationType":159,"publisherRelationship":334,"citationCount":20,"citationInfo":20,"publishDate":367,"publishYear":195,"citationAnalyzeStatus":19,"lastCitationAnalyze":20,"indexDatabases":20,"openAccess":20,"references":20,"isForceReanalyzing":196},"bc2b2998-c52b-4405-aba8-77ea2e1432cc","2023-12-05T14:34:07.346+00:00","2025-02-10T23:51:45.558+00:00",[],"An-application-of-neural-nets-to-the-Rome-precipitation-series-1782-1989-",{"references":272,"abstract":274,"title":276,"doi":278},{"VOID":273},"Vinnikov K. Y., Groisman P. Y. andLugina K. M.,J. Climate,3 (1990) 662.\nElsner J. B. andTsonis A. A.,Bull. Am. Meteorol. Soc.,73 (1992) 49.\nCamuffo D., Bernardi A. andOngaro A.,Memorie della Società Geografica Italiana,46 (1991) 363 (in Italian).\nRich E. andKnight K.,Artificial Intelligence (Mc Graw Hill, New York, N.Y.) 1991.\nAnthes R. A.,Predictability of mesoscale meteorological phenomena, inPredictability of Fluid Motions, edited byG. Holloway andB. J. West (American Institute of Physics) 1984, p. 247.\nTrevisan, V.,Meteorologia romana. La serie delle osservazioni al Collegio Romano (1782–1978), inCollana del Progetto Finalizzato «Promozione della Qualità dell’Ambiente», CNR AQ\u002F5\u002F28 (1980) (in Italian).\nMangianti F. andSorrenti A.,Aggiornamento della serie storica delle osservazioni al Collegio Romano (1979–1989), UCEA Pubblicazione Interna (1990) (in Italian).\nEredia F.,Il clima di Roma (Bertero, Roma) 1911 (in Italian).\nColacino M. andPurini R.,Theor. Appl. Clim.,37 (1986) 90.\nKatsoulis B. D. andKambetzidis H. D.,Climatic Change,14 (1989) 263.\nMennella C.,Il clima d’Italia (Fratelli Conte Editori, Napoli) 1967.",{"EN":275},"In a recent paper Elsner and Tsonis (1992) have demonstrated the feasibility of short-term prediction of climatic data by means of neural nets. In this paper, the same technique has been applied to the rather long (208 years) Rome precipitation series. At first, some examples of artificially generated time series, ranging from analytical functions to a mathematical model, have been used to test the capability of the method. Then the neural net has been applied to the annual and quarterly amounts of precipitation recorded in Rome. 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Teggi:Misure di temperatura superficiale su specchi d'acqua, TN no. 105, CNR-ISDGM-Venezia (1987).",{},{"id":20,"text":496,"url":20,"identifiers":497},"L. Richard andS. Pritchard:Algorithm for Correcting the VHRRImagery for Geometric Distorsions Due to the Earth Curvature, Earth Rotation, and Spacecraft Roll Attitude Errors, NOAA Tech. Mem. NESS 77 (1976).",{},{"id":20,"text":499,"url":20,"identifiers":500},"P. Frontero, L. Lombroso andS. Pugnaghi:G. Fis., Vol. XXIX, No. 2-3 Aprile-Settembre (1988).",{},{"id":20,"text":502,"url":20,"identifiers":503},"K. B. 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Bavassano, U. Villante, L. F. Burlaga andN. F. Ness:J Geophys. Res.,83, 5161 (1978).\nF. Mariani, U. Villante, R. Bruno, B. Bavassano andN. F. Ness:Solar Phys.,63, 411 (1979).\nL. F. Burlaga, N. F. Ness, F. Mariani, B. Bavassano, U. Villante, H. Rosenbauer, R. Schwenn andJ. Harvey:J. Geophys. Res.,83, 5167 (1978).\nU. Villante, F. Mariani, N. F. Ness andL. F. Burlaga:Nuovo Cimento C,1, 539 (1978).\nU. Villante, F. Mariani, R. Bruno, L. F. Burlaga andN. F. Ness:J. Geophys. Res.,84, 6641 (1979).\nL. F. Burlaga, A. J. Hundhausen andZhao Xue-Pu:J. Geophys. Res.,86, 8893 (1981).\nU. Villante andR. Bruno:J. Geophys. Res.,87, 607 (1982).\nU. Villante, F. Mariani andP. Francia:J. Geophys. Res.,87, 249 (1982).\nR. Bruno, L. F. Burlaga andA. J. Hundhausen:J. Geophys. Res.,87, 10331 (1982).\nG. Scearce, S. Cantarano, N. F. Ness, F. Mariani, R. Terenzi andL. F. Burlaga: NASA\u002FGSFC Technical Report, X-692-112 (1975).\nB. 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Bernardi, R. Cecchi, F. Costa, G. Ghermandi andS. Vazzoler:Inquinamento,28, 46 (1986).",{},{"id":20,"text":771,"url":20,"identifiers":772},"C. Avanzi, V. Fossato, P. Gatto, R. Rabagliati, P. Rosa Salva andA. Zitelli:Ripristino, conservazione ed uso dell'ecosistema lagunare (Venezia, 1983), Chapt. 3 byG. Rallo, p. 77.",{},{"id":20,"text":774,"url":20,"identifiers":775},"F. Nyffeler, R. Dazzi, B. Hirel andL. Alberotanza: ISDGM-CNR, Venezia, TR 86 (1975).",{},{"id":20,"text":777,"url":20,"identifiers":778},"Reparto Misure Ambientali: ISDGM-CNR, Venezia, TR 120 (1982).",{},{"id":20,"text":780,"url":20,"identifiers":781},"M. Meneghin andG. Zamperoni:Idrotecnica,1, 21 (1984).",{},{"id":20,"text":783,"url":20,"identifiers":784},"Reparto Misure Ambientali: ISDGM-CNR, Venezia, TN 100.",{},{"id":20,"text":786,"url":20,"identifiers":787},"A. Rusconi:Il comune marino a Venezia, Publ. No. 157, Ufficio Idrografico del Magistrato alle Acque (MLP), Venezia (1983).",{},{"id":20,"text":789,"url":20,"identifiers":790},"Reparto Misure Ambientali: ISDGM-CNR, Venezia, TN 102.",{},{"id":20,"text":792,"url":20,"identifiers":793},"H. Elderfield andA. Hepworth:Mar. Pollut. Bull.,6, 85 (1975).",{"doi":794},"10.1016\u002F0025-326X(75)90149-6",{"id":20,"text":796,"url":20,"identifiers":797},"D. E. Walling andB. W. Webb:Mar. Pollut. Bull.,16, 488 (1985).",{"doi":798},"10.1016\u002F0025-326X(85)90382-0",{"id":20,"text":800,"url":20,"identifiers":801},"R. Capelli, V. Contardi, V. U. Fossato andR. Frache:Metodologie analitiche per lo studio della qualità dell'ambiente marino (Genova, 1983), p. 65.",{},{"id":20,"text":803,"url":20,"identifiers":804},"R. Chester andF. G. Voutsinou:Mar. Pollut. Bull.,12, 84 (1981).",{"doi":805},"10.1016\u002F0025-326X(81)90198-3",{"id":20,"text":807,"url":20,"identifiers":808},"G. Aprilesi, R. Cecchi, G. Ghermandi, G. Magnoni andR. Santangelo:Nucl. 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J. de Groot, W. Salomons andE. Allersma:Estuarine Chemistry (London, 1976), p. 131.",{},{"id":20,"text":832,"url":20,"identifiers":833},"Reparto Misure Ambientali: ISDGM-CNR, Venezia, TN 103.",{},{"id":20,"text":835,"url":20,"identifiers":836},"P. S. Roy andE. A. Crawford:Estuarine, Coastal Shelf Sci.,19, 341 (1984).",{"doi":837},"10.1016\u002F0272-7714(84)90030-1",{"id":839,"createTime":840,"updateTime":841,"relativeEntities":842,"slug":843,"properties":844,"entityType":127,"verifyStatus":128,"verifyTime":841,"verifyNote":129,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21,"primaryUrl":853,"fullTextUrl":20,"authors":854,"publicationType":159,"publisherRelationship":882,"citationCount":20,"citationInfo":20,"publishDate":915,"publishYear":264,"citationAnalyzeStatus":19,"lastCitationAnalyze":20,"indexDatabases":20,"openAccess":20,"references":20,"isForceReanalyzing":196},"cb52dc55-37aa-455e-96c6-e61db6ec7241","2024-01-17T14:17:55.092+00:00","2025-01-06T23:45:31.177+00:00",[],"An-algorithm-for-the-automatic-detection-of-anomalous-temperature-variations-at-ground-level-its-application-to-the-METEOSAT-2-satellite",{"references":845,"abstract":847,"title":849,"doi":851},{"VOID":846},"ESA:Introduction to the Meteosat System, MDMD-ESOC.\nN.P. Slater:Remote Sensing: Optics and Optical Systems (Reading, 1980), p. 15.\nV. Cappellini:Elaborazione numerica delle immagini (Torino, 1985), p. 107.\nG.M. Lechi andA. Zandonella:Alcune considerazioni sulla entropia delle immagini, Atti IV Convegno S.I.TE., 1982.\nK.R. Castleman:Digital Image Processing (Prentice Hall Inc., Englewood Cliffs, 1979).\nS. Corda: Tesi, Dipartimento di Fisica, Università di Cagliari (1989).\nESA:Meteosat High Resolution Image Dissemination, Vol. 9, Meteosat System Guide.\nM. Jones:Use of Meteosat High Resolution Format Interpretation Data, Report, MDMD-ESOC.\nM. Jones andJ. Morgan:Adjustment of METEOSAT-1 radiometer response by ground processing, Preliminary report, MDMD-ESOC (1979).\nS. Campbell:Vicarious Calibration of Meteosat’s Infrared Sensors, ESA Journal,6, 151 (1982).",{"EN":848},"The algorithm, starting from techniques typical of image processing and information theory, is an instrument for the detection of anomalous variations in any physical parameter measured by remote sensing. Within a software system capable of checking the validity of such a measurement, comparing it with extant historical data and reporting it, the algorithm acts as a filter able to amplify the anomaly. The aim of this work is to see if it possible to detect anomalous temperature variations in some way connected with fire at ground level by means of the sensors in the infrared heat band of the METEOSAT-2 satellite. The choice of this geostationary satellite was made because, despite low spatial resolution (at the latitude of Sardinia pixels are about 7 km square), it has good time resolution (one slot every 30 minutes).",{"EN":850},"An algorithm for the automatic detection of anomalous temperature variations at ground level: its application to the METEOSAT-2 satellite",{"VOID":852},"10.1007\u002FBF02511737","https:\u002F\u002Flink.springer.com\u002Farticle\u002F10.1007\u002FBF02511737",[855,870],{"id":856,"sortIndex":147,"researcher":20,"roles":857,"affiliations":858,"properties":867},"dab8bd8d-27d2-4f02-a137-82798908311a",[135],[859],{"id":20,"sortIndex":21,"affiliation":860,"properties":20},{"id":861,"createTime":862,"updateTime":862,"relativeEntities":863,"slug":20,"properties":864,"entityType":49,"verifyStatus":19,"verifyTime":20,"verifyNote":20,"syncStatus":19,"languages":20,"translateLanguages":20,"viewCount":21},"3061a0e0-8038-46b9-81cf-a2fd87fb4fd0","2024-01-17T14:17:55.188+00:00",[],{"title":865},{"VI":866},"Astronomical Observatory of Cagliari, Cagliari, Italy",{"title":868},{"VI":869},"E. 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Weber:Phys. Rev. Lett.,18, 498 (1967).\nG. W. Gibbons andS. W. Hawking:Phys. Rev. D,4, 2191 (1971).\nJ. L. Levine andR. L. Garwin:Phys. Rev. Lett.,31, 173 (1973).b)D. Bramanti, K. Maischberger andD. Parkinson:Lett. Nuovo Cimento,7, 665 (1973).\nP. Bonifazi, V. Ferrari, S. Frasca, G. V. Pallottino andG. Pizzella:Nuovo Cimento C,1, 465 (1978).\nP. F. Michelson andR. C. Taber:J. Appl. Phys.,52, 4313 (1981).\nW. Johnson, Bu-Xin Xu, B. Price andW. O. Hamilton:Digital filters for bar antennas, International Symposium on GW Signal Analysis, Amalfi, 1988.\nA. Papoulis:Probability, Random Variables, and Stochastic Process (McGraw-Hill, New York, N.Y., 1991).\nA. D. Whalen:Detection of Signals in Noise (Academic Press, New York, N.Y., 1971).\nP. Astone, P. Bonifazi, S. Frasca, G. V. Pallottino andG. Pizzella:Nuovo Cimento C,15, 447 (1992).\nB. F. Schutz:Data processing, analysis and storage for interferometric antennas, inThe Detection of Gravitational Waves, edited byD. G. Blair (Cambridge University Press, Cambridge, 1991), pp. 406–452.\nS. Frasca, G. V. Pallottino andG. Pizzella:Spectral domain data analysis for a gravitational wave antenna, inSignal Processing III: Theories and Applications, edited byI. T. Young (North-Holland, Amsterdam, 1986), pp. 597–600.\nP. Astone, M. Bassan, P. Bonifazi, P. Carelli, M. G. Castellano, G. Cavallari, E. Coccia, C. Cosmelli, V. Fafone, S. Frasca, E. Majorana, I. Modena, G. V. Pallottino, G. Pizzella, P. Rapagnani, F. Ricci andM. Visco:Phys. Rev. D,47, 362 (1993).\nG. V. Pallottino andG. Pizzella:Data analysis and algorithms for GW antennas, inData Analysis in Astronomy III, edited byV. Di Gesù (Plenum Press, New York, N.Y., 1989), pp. 361–390.\nG. V. Pallottino andG. Pizzella:Nuovo Cimento C,4, 237 (1981).\nR. Giffard:Phys. Rev. D,14, 2478 (1976).\nS. Frasca:Discrete time Gauss-Markov processes: theory and application to gravitational antenna signals simulation and filtering, Internal report 732, Institute of Physics, University of Rome, July 13, 1979.\nH. J. Paik:J. Appl. Phys.,47, 1168 (1976).\nG. L. Turin:IEEE Trans. Inf. Theory, IT-6, 311 (1960).\nB. M. Dwork:Proc. IRE,38, 771 (1950).\nG. C. Newton, L. A. Gould andJ. F. Kaiser:Analytical Design of Linear Feedback Controls (Wiley, New York, N.Y., 1957).\nD. R. White:IEEE Trans. Instrum. Meas.,IM-38, 1036 (1989).\nP. Astone, P. Bonifazi andG. V. Pallottino:Rev. Sci. Instrum.,61, 3899 (1990).",{"EN":925},"We report on the application of Wiener filters to the data of Weber-type gravitational-wave antennas, with particular reference to data processed by means of lock-in amplifiers driven at the frequencies of the modes of the detector. After a review of some basic results concerning the filtering of the data, we briefly examine the relationship between Wiener filters and matched filters. The discussion that follows is centred on various aspects related to the practical application of Wiener filters as well as on their limitations, also addressing the dependence of their performance on the values of their parameters. 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