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Summary
| Description |
English: Mathematical model of artificial magnetosphere for a spacecraft with a field source operating in a plasma environment (pe) with effective wind velocity upe illustrating the magnetospheric bubble enclosed by a magnetopause that creates a bow shock and an effective sail area S with radius equal to the characteristic length L. Under certain conditions, the standoff between wind pressure pw and magnetic pressure pB transfers the plasma wind force Fw to a propulsive force on the spacecraft Fsc. |
| Date | |
| Source | Own work |
| Author | Dmcdysan |
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File history
Click on a date/time to view the file as it appeared at that time.
| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 19:43, 28 October 2023 | | 1,008 × 755 (141 KB) | Dmcdysan | Changed font size to 14 pt. |
| 20:30, 7 July 2022 |  | 1,308 × 995 (183 KB) | Dmcdysan | Aligned notation with text in Magnetic sail article. | |
| 17:58, 5 July 2022 |  | 1,308 × 991 (172 KB) | Dmcdysan | Changed color density to match Artificial Magnetospheric Model. Added F_loss | |
| 03:17, 30 June 2022 |  | 1,279 × 991 (164 KB) | Dmcdysan | Higher resolution version. | |
| 03:11, 30 June 2022 |  | 307 × 238 (23 KB) | Dmcdysan | Uploaded own work with UploadWizard |
File usage
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