Magnetostatic Boundary Conditions
Magnetic Field Lines
Divergence and Curl of Magnetic Field
Potential Due to a Magnetized Object
Plane Electromagnetic Waves II
Magnetic Field due to Moving Charges
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Updated: May 25, 2026

Spectral and Angle-Resolved Magneto-Optical Characterization of Photonic Nanostructures
Published on: November 21, 2019
Akira Hasegawa1, Bruce T Tsurutani
1Osaka University, Yamadaoka 2-1, Suita, Japan.
Observed mirror modes in planetary magnetosheaths are larger than predicted. A Bohm diffusion process explains this by shifting wave numbers as modes move away from their source, matching observations across multiple celestial bodies.
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