Evaluation of the candidate Main Field model for IGRF 2000 derived from preliminary Orsted data

被引:7
作者
Lowes, FJ [1 ]
Bondar, T
Golovkov, VP
Langlais, B
Macmillan, S
Mandea, M
机构
[1] Univ Newcastle Upon Tyne, Dept Phys, Newcastle Upon Tyne NE1 7RU, Tyne & Wear, England
[2] IZMIRAN, Troitsk 142092, Moscow Region, Russia
[3] Inst Phys Globe, Lab Geomagnetisme, F-75252 Paris, France
[4] British Geol Survey, Edinburgh EH9 3LA, Midlothian, Scotland
来源
EARTH PLANETS AND SPACE | 2000年 / 52卷 / 12期
关键词
Candidate Model; Scalar Data; Earth Planet Space; Repeat Station; Longitude Sector;
D O I
10.1186/BF03352350
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
On this occasion the selection of the IGRF for 2000 was left to a small Task Force. Before it was accepted by the Task Force as IGRF 2000, the final candidate model (a truncated version of Orsted(10c/99)) was compared with a comprehensive set of independent surface and satellite data. The method, data selection, and results of this comparison are described.
引用
收藏
页码:1183 / 1186
页数:4
相关论文
共 6 条
[1]   An IGRF candidate main geomagnetic field model for epoch 2000 and a secular variation model for 2000-2005 [J].
Langlais, B ;
Mandea, M .
EARTH PLANETS AND SPACE, 2000, 52 (12) :1137-1148
[2]  
LANGLAIS B, 1999, OERSRP00000031IPG CN
[3]   The working of the IGRF 2080 Task Force [J].
Lowes, FJ .
EARTH PLANETS AND SPACE, 2000, 52 (12) :1171-1174
[4]   THE K-DERIVED PLANETARY INDEXES - DESCRIPTION AND AVAILABILITY [J].
MENVIELLE, M ;
BERTHELIER, A .
REVIEWS OF GEOPHYSICS, 1991, 29 (03) :415-432
[5]   Determination of the IGRF 2000 model [J].
Olsen, N ;
Sabaka, TJ ;
Toffner-Clausen, L .
EARTH PLANETS AND SPACE, 2000, 52 (12) :1175-1182
[6]  
Wessel P., 1991, EOS T AGU, V72, P441, DOI [DOI 10.1029/90E000319, 10.1029/90EO00319]