File:Magnetic dipole force MHD and kinematic models.jpg

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Description
English: The figure shows MHD and kinematic models for force generated in the solar wind by a magnetic dipole versus characteristic length L, the green line showing the value of ion gyroradius rg ≈ 72 km and the black line showing force FMHD from the Magnetohydrodynamic (MHD) model. Kinematic models apply for L < rg. A coefficient of drag numerical model from Fujita04 shows the reduced force and percentage thrust lost in the solid and dashed blue lines, respectively. Results from Ashida14 show similar reduced force and percentage thrust lost in the solid and dashed red lines, respectively. Additional simulation results from Hajiwara15 are shown for the MHD and kinematic model as single data points. All models are in close agreement. The results show that choice of a magnetic sail radius L much less than the ion gyroradius rg would result in significant lost thrust as compared with the MHD model.
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Author Dmcdysan

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Magnetic dipole force: MHD and kinematic models

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20 July 2022

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Date/TimeThumbnailDimensionsUserComment
current20:04, 28 October 2023Thumbnail for version as of 20:04, 28 October 2023855 × 727 (108 KB)DmcdysanChanged font size to 14 pt.
22:05, 20 July 2022Thumbnail for version as of 22:05, 20 July 20222,408 × 2,000 (397 KB)DmcdysanEdited axis number styles, added T_loss to secondary axis.
20:46, 20 July 2022Thumbnail for version as of 20:46, 20 July 20222,475 × 1,991 (408 KB)DmcdysanUploaded own work with UploadWizard

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