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An Improved Seeding Algorithm of Magnetic Flux Lines Based on Data in 3D Space Cover

An Improved Seeding Algorithm of Magnetic Flux Lines Based on Data in 3D Space

By: ,   and    
Open Access
|May 2015

Figures & Tables

Figure 1

Plane S with its sub-planes.

Figure 2

The domain of subdivision along axis X and axis Y.

Figure 3

The variations of magnetic flux caused by the errors.

Figure 4

The distribution of magnetic flux lines from dipole field on the magnetic equatorial plane.

Figure 5

The distribution of seed points from the equivalent magnetic flux algorithm.

Table 1

The accuracies of the traditional and improved algorithms with the same number of grids using different subdivisions.

4/9x4/9 subdomain A5/9x5/9 subdomain B7/9x7/9 subdomain C
18x1827x2736x3618x1827x2736x3618x1827x2736x36
N30.121130.119730.1192N43.698843.697343.6967N74.220174.218974.2185
ε (%)7.57547.57057.5688ε (%)1.62511.62161.6204ε (%)0.29750.29590.2953
9x369x8118x729x369x8118x729x369x8118x72
N'30.113630.112830.1174N'43.690343.689543.6946N'74.213474.212774.2168
ε' (%)7.54867.54587.5621ε' (%)1.60531.60341.6155ε' (%)0.28840.28740.2931
Table 2

The accuracies of the traditional and improved algorithms with a different numbers of grids using different subdivisions.

4/9x4/9 subdomain A5/9x5/9 subdomain B7/9x7/9 subdomain C
18x1827x2736x3618x1827x2736x3618x1827x2736x36
N30.121130.119730.1192N43.698843.697343.6967N74.220174.218974.2185
ε (%)7.57547.57057.5688ε (%)1.62511.62161.6204ε (%)0.29750.29590.2953
9x1818x2727x369x1818x2727x369x1818x2727x36
N'30.116530.118930.1189N'43.693743.696343.6964N'74.216074.218274.2183
ε' (%)7.55927.56757.5677ε' (%)1.61321.61941.6196ε' (%)0.29190.29490.2950
Language: English
Page range: 6 - 6
Published on: May 22, 2015
Published by: Ubiquity Press
In partnership with: Paradigm Publishing Services
Publication frequency: 1 issue per year

© 2015 Jia Zhong, Xiaoyan Hu, Ziming Zou, published by Ubiquity Press
This work is licensed under the Creative Commons Attribution 4.0 License.