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Part VII ›
Plasmas and Magnetohydrodynamics
Plasmas and Magnetohydrodynamics
phenomena owed owes (derived) owes (derived) owes (derived) owes (derived) phenomenon 66.1: Collective oscillation at the plasma frequency 66.1 Collective oscil… phenomenon 66.2: Sunspots are strongly magnetized 66.2 Sunspots are str… phenomenon 66.3: The ionosphere reflects radio waves below a critical
frequency 66.3 The ionosphere r… phenomenon 66.4: Waves damp in a collisionless plasma 66.4 Waves damp in a… phenomenon 66.5: Magnetic trapping: the radiation belts 66.5 Magnetic trappin… phenomenon 66.6: Alfvén waves 66.6 Alfvén waves phenomenon 66.7: Magnetic reconnection 66.7 Magnetic reconne… phenomenon 66.8: The solar wind 66.8 The solar wind pending : ch:09-plasmas-mhd@pending-1 pending pending : ch:09-plasmas-mhd@pending-2 pending pending : ch:09-plasmas-mhd@pending-3 pending pending : ch:09-plasmas-mhd@pending-4 pending pending : ch:09-plasmas-mhd@pending-5 pending The chain of Plasmas and Magnetohydrodynamics: 13 of 13 objects, read left to right from what the chapter assumes to what tests it. Solid lines are declared logical edges, dashed ones were inferred from the structure of the source. Click any node to open its own chain.