| 11. | After all, if one taps the magnetic field energy, the particle is breaked ( see Lenz's law ).
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| 12. | The orbit of the planet would warp the field lines until the instability released magnetic field energy as a flare.
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| 13. | Force field energy evaluation are most often used to select energetically reasonable conformations, but knowledge-based methods have also been used.
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| 14. | When this happens, an extra drain is seen on the transmitter, resulting from the reactive near-field energy that is not returned.
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| 15. | Sometimes one can assume that the field energy of any electromagnetic field is so small that its gravitational effects can be neglected.
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| 16. | The magnetic field energy and the inductance of the second system thus are twice as large as that of the first system.
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| 17. | But this has to be taken with a grain of salt because the " energy " here doesn't include gravitational field energy.
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| 18. | The total field energy for this disk is infinite, and so this G = 0 limit does not solve the problem of infinite self-energy.
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| 19. | The domains keep dividing into smaller domains until the energy cost of creating an additional domain wall is just equal to the field energy saved.
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| 20. | :: : Yes, a charged particle has kinetic energy and magnetic field energy when moving, and so it takes " more " energy to accelerate it.
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