![Table 6 | The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches | SpringerLink Table 6 | The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches | SpringerLink](https://media.springernature.com/full/springer-static/image/art%3A10.1007%2Fs11207-014-0529-3/MediaObjects/11207_2014_529_Tab6_HTML.gif)
Table 6 | The Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Pipeline: SHARPs – Space-Weather HMI Active Region Patches | SpringerLink
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Three‐dimensional array of strong magnetic field by using cubic permanent magnets - Nishimura - 2021 - Electrical Engineering in Japan - Wiley Online Library
![In magnetic field B=(2hati+3hatj) T, velocity of a charged particle is given in table-1. Corresponding magnetic force is given in table-2. Match the two tables. In magnetic field B=(2hati+3hatj) T, velocity of a charged particle is given in table-1. Corresponding magnetic force is given in table-2. Match the two tables.](https://d10lpgp6xz60nq.cloudfront.net/web-thumb/643188467_web.png)
In magnetic field B=(2hati+3hatj) T, velocity of a charged particle is given in table-1. Corresponding magnetic force is given in table-2. Match the two tables.
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