| 1. | Applying the Amp�re-Maxwell equation to surface " S 1 " we find:
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| 2. | This is a big difference with Maxwell equations that require only charge conservation.
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| 3. | So we cannot naively formulate expectations based on the Maxwell equations in this frame.
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| 4. | The microscopic Maxwell equations have universal applicability but may be infeasible to calculate with.
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| 5. | The direct space time formulations make manifest that the Maxwell equations are relativistically invariant.
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| 6. | By the NP formalism of Einstein-Maxwell equations, one has
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| 7. | This theory gives the solutions to the Maxwell equations for prolate and oblate spheroidal particles.
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| 8. | It states that any spherically symmetric solution of the source-free Maxwell equations is necessarily static.
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| 9. | He is best known for his stories The Maxwell Equations ( 1963 ) and Iva.
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| 10. | That is, the current density on the right side of the Amp�re Maxwell equation is:
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