About: Geomagnetic secular variation     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : owl:Thing, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/c/3uWkFFoNxA

Geomagnetic secular variation refers to changes in the Earth's magnetic field on time scales of about a year or more. These changes mostly reflect changes in the Earth's interior, while more rapid changes mostly originate in the ionosphere or magnetosphere.

AttributesValues
rdfs:label
  • Variación secular geomagnética (es)
  • Geomagnetic secular variation (en)
rdfs:comment
  • Geomagnetic secular variation refers to changes in the Earth's magnetic field on time scales of about a year or more. These changes mostly reflect changes in the Earth's interior, while more rapid changes mostly originate in the ionosphere or magnetosphere. (en)
  • La variación secular geomagnética se refiere a cambios en el campo magnético de la Tierra en escalas de tiempo de aproximadamente un año o más. Estos cambios reflejan principalmente cambios en el interior de la Tierra, mientras que los cambios más rápidos se originan principalmente en la ionosfera o magnetosfera.​ (es)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Earth_Magnetic_Field_Declination_from_1590_to_1990.gif
  • http://commons.wikimedia.org/wiki/Special:FilePath/Geomagnetic_axial_dipole_strength.svg
dct:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
Link from a Wikipage to an external page
sameAs
dbp:wikiPageUsesTemplate
thumbnail
has abstract
  • Geomagnetic secular variation refers to changes in the Earth's magnetic field on time scales of about a year or more. These changes mostly reflect changes in the Earth's interior, while more rapid changes mostly originate in the ionosphere or magnetosphere. The geomagnetic field changes on time scales from milliseconds to millions of years. Shorter time scales mostly arise from currents in the ionosphere and magnetosphere, and some changes can be traced to geomagnetic storms or daily variations in currents. Changes over time scales of a year or more mostly reflect changes in the Earth's interior, particularly the iron-rich core. These changes are referred to as secular variation. In most models, the secular variation is the amortized time derivative of the magnetic field , . The second derivative, is the secular acceleration. (en)
  • La variación secular geomagnética se refiere a cambios en el campo magnético de la Tierra en escalas de tiempo de aproximadamente un año o más. Estos cambios reflejan principalmente cambios en el interior de la Tierra, mientras que los cambios más rápidos se originan principalmente en la ionosfera o magnetosfera.​ El campo geomagnético cambia en escalas de tiempo de milisegundos a millones de años. Las escalas de tiempo más cortas surgen principalmente de las corrientes en la ionosfera y la magnetosfera, y algunos cambios pueden atribuirse a tormentas geomagnéticas o variaciones diarias en las corrientes. Los cambios en escalas de tiempo de un año o más reflejan principalmente cambios en el interior de la Tierra, particularmente el núcleo rico en hierro. Estos cambios se conocen como variación secular.​ (es)
prov:wasDerivedFrom
page length (characters) of wiki page
foaf:isPrimaryTopicOf
is Link from a Wikipage to another Wikipage of
is Wikipage redirect of
is foaf:primaryTopic of
Faceted Search & Find service v1.17_git147 as of Sep 06 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3331 as of Sep 2 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 63 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software