About: SOLAR VELOCITY FIELDS     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : skos:Concept, within Data Space : foodie-cloud.org, foodie-cloud.org associated with source document(s)

AttributesValues
type
has broader
preferred label
  • SOLAR VELOCITY FIELDS (en)
definition
  • Solar velocity fields are also known as differential rotation. The sun rotates slightly more rapidly at the equator than at the poles. Gases at the equator make about 10 rotations, whiles gases at midlatitudes rotates 9 times and gases at the poles rotates about 7 times. This produces a shear in the gas motions and a pronounced E-W orientation of the magnetic field. (en)
is in scheme
is has narrower of
Faceted Search & Find service v1.16.115 as of Sep 26 2023


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 07.20.3238 as of Sep 26 2023, on Linux (x86_64-generic_glibc25-linux-gnu), Single-Server Edition (252 GB total memory, 112 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2026 OpenLink Software