3D Modeling of Magnetic Field Lines using SOHO/MDI Magnetogram Images

被引：0
|
作者：
Colak, Tufan [1 ]
Qahwaji, Rami [1 ]
Ipson, Stan [1 ]
Ugail, Hassan [1 ]
机构：
[1] Univ Bradford, Informat Res Inst, Bradford BD7 1DP, W Yorkshire, England
来源：
RAST 2009: PROCEEDINGS OF THE 4TH INTERNATIONAL CONFERENCE ON RECENT ADVANCES IN SPACE TECHNOLOGIES | 2009年
关键词：
Solar imaging; 3D modeling; Space weather;
D O I：
10.1109/RAST.2009.5158278
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
Solar imaging is currently an active area of research. In this study a 3D modeling technique for magnetic field lines on Sun is provided. Magnetic field foot prints are detected from SOHO (Solar and Heliospheric Observatory) / MDI (Michelson Doppler Imager) Magnetogram images. Using negative and positive footprints possible dipole pairs are found according to their proximity. Then using this data, 3D models are built on bipolar coordinates and placed on detected pairs after transformations.
引用
收藏
页码：685 / 689
页数：5
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