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Web14 dec. 2024 · A variety of kinetic electrostatic and electromagnetic waves develop in the solar wind and the relationship between these waves and larger scale structures, such … WebSolution. The wave function of the ball can be written. Ψ ( x, 0) = A cos ( k x) ( − L / 2 < x < L / 2), where A is the amplitude of the wave function and k = 2 π / λ is its wave number. … Web30 nov. 2024 · The Parker Solar Probe (PSP) has observed primarily magnetic-field-aligned flows and outward (or antisunward) propagating Alfvén waves in its first four orbits, with … css name 指定の仕方