Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/1964
DC FieldValueLanguage
dc.contributor.authorallBarducci, A.; Istituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.contributor.authorallBenvenuti, M.; Istituto di Biometeorologia (IBIMET), CNR, Firenze, Italyen
dc.contributor.authorallCastagnoli, F.; Centro di Studi per l’Applicazione dell’Informatica in Agricoltura (CeSIA), Accademia dei Georgofili, Firenze, Italyen
dc.contributor.authorallGuzzi, D.; Istituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.contributor.authorallMarcoionni, P.; Istituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.contributor.authorallPippi, I.; Istituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.date.accessioned2006-12-07T14:39:10Zen
dc.date.available2006-12-07T14:39:10Zen
dc.date.issued2006-02en
dc.identifier.urihttp://hdl.handle.net/2122/1964en
dc.description.abstractindustries. In this paper we introduce the results from a remote sensing campaign performed in September 2001 at night time. For the first time nocturnal light pollution was measured at high spatial and spectral resolution using two airborne hyperspectral sensors, namely the Multispectral Infrared and Visible Imaging Spectrometer (MIVIS) and the Visible InfraRed Scanner (VIRS-200). These imagers, generally employed for day-time Earth remote sensing, were flown over the Tuscany coast (Italy) on board of a Casa 212/200 airplane from an altitude of 1.5-2.0 km. We describe the experimental activities which preceded the remote sensing campaign, the optimization of sensor configuration, and the images as far acquired. The obtained results point out the novelty of the performed measurements and highlight the need to employ advanced remote sensing techniques as a spectroscopic tool for light pollution monitoring.en
dc.format.extent2753932 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofseries1/49 (2006)en
dc.subjectlight pollution monitoringen
dc.subjectline emissionen
dc.subjecthyperspectral remote sensingen
dc.subjectairborne imaging spectrometersen
dc.subjectdata processingen
dc.titleHyperspectral remote sensing for light pollution monitoringen
dc.typearticleen
dc.type.QualityControlPeer-revieweden
dc.subject.INGV05. General::05.09. Miscellaneous::05.09.99. General or miscellaneousen
dc.relation.referencesBARDUCCI, A. and I. PIPPI (2001): Analysis and rejection of systematic disturbances in hyperspectral remotely sensed images of the Earth, Appl. Opt., 40, 1464-1477. BARDUCCI, A., P. MARCOIONNI, I. PIPPI and M. POGGESI (2002): Development of a solar spectro-irradiometer for the validation of remotely sensed hyperspectral images, in Observing our Environment from Space: New Solutions for a New Millennium, edited by G. BEGNI, Proceedings of 21st EARSeL Symposium, 14-16 May 2001, Paris (France), (A.A. Balkema Publishers), 197-202. CATANZARO, G. and F.A. CATALANO (2000): Measurements of the night sky brightness at the Catania astrophysical observatory, Men. S.A.It., 71, 211-220. CINZANO, P., F. FALCHI and C.D. ELVIDGE (2001): Nakedeye star visibility and limiting magnitude mapped from DMSP-OLS satellite data, Mon. Not. R. Astron. Soc., 323, 34-46. GARSTANG, R.H. (1989): Night-sky brightness at observatories and sites, Publ. Astron. Soc. Pac., 101, 306-329. GARSTANG, R.H. (1991): Dust and light pollution, Publ. Astron. Soc. Pac., 103, 1109-1116. GARSTANG, R.H. (2000): Light pollution at Mount Wilson: the effects of population growth and air pollution, Men. S.A.It., 71, 71-81. ISOBE, S. (1998): Bilateral agreements, zoning, international protocol to preserve astronomical windows, Astron. Soc. Pac. Conf. Ser., 139, 119-123. ISOBE, S. and S. HAMAMURA (1998): Ejected city light of Japan observed by a defense meteorological satellite program, Astron. Soc. Pac. Conf. Ser., 139, 19-199. ISOBE, S. and H. KOSAI (1998): Star watching observations to measure night sky brightness, Astron. Soc. Pac. Conf. Ser., 139, 175-184. WALKER, M.F. (1973): Light pollution in California and Arizona, Publ. Astron. Soc. Pac., 85, 508-519.en
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorBarducci, A.en
dc.contributor.authorBenvenuti, M.en
dc.contributor.authorCastagnoli, F.en
dc.contributor.authorGuzzi, D.en
dc.contributor.authorMarcoionni, P.en
dc.contributor.authorPippi, I.en
dc.contributor.departmentIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.contributor.departmentIstituto di Biometeorologia (IBIMET), CNR, Firenze, Italyen
dc.contributor.departmentCentro di Studi per l’Applicazione dell’Informatica in Agricoltura (CeSIA), Accademia dei Georgofili, Firenze, Italyen
dc.contributor.departmentIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.contributor.departmentIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
dc.contributor.departmentIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italy-
crisitem.author.deptIstituto di Biometeorologia (IBIMET), CNR, Firenze, Italy-
crisitem.author.deptCentro di Studi per l’Applicazione dell’Informatica in Agricoltura (CeSIA), Accademia dei Georgofili, Firenze, Italy-
crisitem.author.deptIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italy-
crisitem.author.deptIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italy-
crisitem.author.deptIstituto di Fisica Applicata «Nello Carrara» (IFAC), CNR, Firenze, Italy-
crisitem.classification.parent05. General-
Appears in Collections:Annals of Geophysics
Files in This Item:
File Description SizeFormat
34 Barducci.pdf2.69 MBAdobe PDFView/Open
Show simple item record

Page view(s) 50

230
checked on Apr 17, 2024

Download(s) 5

757
checked on Apr 17, 2024

Google ScholarTM

Check