Please use this identifier to cite or link to this item:
http://hdl.handle.net/2122/1764
DC Field | Value | Language |
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dc.contributor.authorall | De Santis, A.; Istituto Nazionale di Geofisica, Roma, Italy | en |
dc.contributor.authorall | Falcone, C.; Istituto Nazionale di Geofisica, Roma, Italy | en |
dc.contributor.authorall | Lowes, F. J.; Physics Department, Univervità of Newcastle, Upton Tyne, U.K. | en |
dc.date.accessioned | 2006-09-29T10:22:54Z | en |
dc.date.available | 2006-09-29T10:22:54Z | en |
dc.date.issued | 1995-05 | en |
dc.identifier.uri | http://hdl.handle.net/2122/1764 | en |
dc.description.abstract | When 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.extent | 2537835 bytes | en |
dc.format.mimetype | application/pdf | en |
dc.language.iso | English | en |
dc.relation.ispartofseries | 2/38 (1995) | en |
dc.subject | spherical harmonics | en |
dc.subject | orthogonality | en |
dc.subject | geomagnetic spectrum | en |
dc.title | Remarks on the mean-square values of the geomagnetic field and its components | en |
dc.type | article | en |
dc.type.QualityControl | Peer-reviewed | en |
dc.subject.INGV | 04. Solid Earth::04.05. Geomagnetism::04.05.99. General or miscellaneous | en |
dc.subject.INGV | 05. General::05.05. Mathematical geophysics::05.05.99. General or miscellaneous | en |
dc.description.journalType | JCR Journal | en |
dc.description.fulltext | open | en |
dc.contributor.author | De Santis, A. | en |
dc.contributor.author | Falcone, C. | en |
dc.contributor.author | Lowes, F. J. | en |
dc.contributor.department | Istituto Nazionale di Geofisica, Roma, Italy | en |
dc.contributor.department | Istituto Nazionale di Geofisica, Roma, Italy | en |
dc.contributor.department | Physics Department, Univervità of Newcastle, Upton Tyne, U.K. | en |
item.openairetype | article | - |
item.cerifentitytype | Publications | - |
item.languageiso639-1 | en | - |
item.grantfulltext | open | - |
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.dept | Physics Department, University of Newcastle Upon Tyne, NE1 7RU, U.K. | - |
crisitem.author.orcid | 0000-0002-3941-656X | - |
crisitem.author.parentorg | Istituto Nazionale di Geofisica e Vulcanologia | - |
crisitem.classification.parent | 04. Solid Earth | - |
crisitem.classification.parent | 05. General | - |
Appears in Collections: | Annals of Geophysics |
Files in This Item:
File | Description | Size | Format | |
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03 de santis.pdf | 2.48 MB | Adobe PDF | View/Open |
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