Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/1764
DC FieldValueLanguage
dc.contributor.authorallDe Santis, A.; Istituto Nazionale di Geofisica, Roma, Italyen
dc.contributor.authorallFalcone, C.; Istituto Nazionale di Geofisica, Roma, Italyen
dc.contributor.authorallLowes, F. J.; Physics Department, Univervità of Newcastle, Upton Tyne, U.K.en
dc.date.accessioned2006-09-29T10:22:54Zen
dc.date.available2006-09-29T10:22:54Zen
dc.date.issued1995-05en
dc.identifier.urihttp://hdl.handle.net/2122/1764en
dc.description.abstractWhen considering functions on the Earth's (spherical) surface, mean-square values are often used to indicate their (relative) magnitude. If a function is separated into it, (essentially) spherical harmonic components then, provided these individual harmonic components are orthogonal over the surface, the concept of spatial power spectrum can be introduced, with each harmonic contributing separately to the total mean square value; this is true for the geomagnetic field vector B, its horizontal component vector H, and its vertical component z. However, because of the lack of orthogonality this concept is not applicable to the horizontal X and y components individually; problems which arise from this are discussed.en
dc.format.extent2537835 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofseries2/38 (1995)en
dc.subjectspherical harmonicsen
dc.subjectorthogonalityen
dc.subjectgeomagnetic spectrumen
dc.titleRemarks on the mean-square values of the geomagnetic field and its componentsen
dc.typearticleen
dc.type.QualityControlPeer-revieweden
dc.subject.INGV04. Solid Earth::04.05. Geomagnetism::04.05.99. General or miscellaneousen
dc.subject.INGV05. General::05.05. Mathematical geophysics::05.05.99. General or miscellaneousen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorDe Santis, A.en
dc.contributor.authorFalcone, C.en
dc.contributor.authorLowes, F. J.en
dc.contributor.departmentIstituto Nazionale di Geofisica, Roma, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica, Roma, Italyen
dc.contributor.departmentPhysics Department, Univervità of Newcastle, Upton Tyne, U.K.en
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.deptPhysics Department, University of Newcastle Upon Tyne, NE1 7RU, U.K.-
crisitem.author.orcid0000-0002-3941-656X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.classification.parent05. General-
Appears in Collections:Annals of Geophysics
Files in This Item:
File Description SizeFormat
03 de santis.pdf2.48 MBAdobe PDFView/Open
Show simple item record

Page view(s)

162
checked on Apr 17, 2024

Download(s) 5

1,203
checked on Apr 17, 2024

Google ScholarTM

Check