Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/1837
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dc.contributor.authorallChiappini, M.; Istituto Nazionale di Geofisica, Roma, Italyen
dc.contributor.authorallDe Santis, A.; Istituto Nazionale di Geofisica, Roma, Italyen
dc.date.accessioned2006-12-06T11:14:01Zen
dc.date.available2006-12-06T11:14:01Zen
dc.date.issued1994-04en
dc.identifier.urihttp://hdl.handle.net/2122/1837en
dc.description.abstractMost of the magnetic methods used for investigating planetary interiors are based on the reasonable hypothesis that the mechanism for the origin of the field is an Earth-like hydromagnetic dynamo: in this case the planet has an electrically conducting fluid shell within it as in the case of the Earth's core. The present paper describes several techniques of planetary magnetic investigation which give important clues on the internal constitution of planets. Some considerations on the possible mechanisms for maintaining a dynamo and simple concepts with the help of a few non-dimensional numbers are also introduced and discussed. Then some fundamental relationships are given in order to relate the planetary magnetism to other physical parameters, such as angular rotation, core dimensions etc. It finally summarizes some results available for the planets of the Solar System.en
dc.format.extent4751207 bytesen
dc.format.mimetypeapplication/pdfen
dc.language.isoEnglishen
dc.relation.ispartofseries1/37 (1994)en
dc.subjectplanetaty magnetismen
dc.subjectmagnetic probingen
dc.titleMagnetic investigations for studying planetary interiorsen
dc.typearticleen
dc.type.QualityControlPeer-revieweden
dc.subject.INGV01. Atmosphere::01.03. Magnetosphere::01.03.06. Instruments and techniquesen
dc.description.journalTypeJCR Journalen
dc.description.fulltextopenen
dc.contributor.authorChiappini, M.en
dc.contributor.authorDe Santis, A.en
dc.contributor.departmentIstituto Nazionale di Geofisica, Roma, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica, Roma, Italyen
item.openairetypearticle-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.fulltextWith Fulltext-
item.grantfulltextopen-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.orcid0000-0001-7433-9435-
crisitem.author.orcid0000-0002-3941-656X-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
Appears in Collections:Annals of Geophysics
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