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Earth, Planets and Space
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The working of the IGRF 2000 Task Force

descriptionPublicationkeyboard_double_arrow_right Article 24 Jun 2014 English Publisher:Springer Science and Business Media LLCJournal:Earth, Planets and Space, volume 52, pages 1,171-1,174 (eissn: 1880-5981, Copyright policy )
Authors: Lowes, F. J.;

doi: 10.1186/bf03352348

The working of the IGRF 2000 Task Force

Abstract

At its meeting in July 1999, the IAGA Working Group for Analysis of the Global and Regional Geomagnetic Field and Secular Variation (WG V-8) felt unable to decide on a main-field model to use for IGRF 2000. It therefore set up a small Task Force with the remit to produce a model by the end of the year. This paper is the Chairman’s report of the working of that Task Force, outlining the various stages involved, and giving the background to the various decisions. He also makes some retrospective personal comments.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
8
Average
Top 10%
Top 10%
Published in a Diamond OA journal