Simulations of radio-wave anisotropic scattering to interpret type III radio burst data from Solar Orbiter, Parker Solar Probe, STEREO, and Wind

Solar Orbiter First Results (Cruise Phase)

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Fig. 4.

Example of time profiles obtained for photons collected on a sphere of radius 111R_S (where propagation effects become negligible), at different angles θ_P, from the simulations of radio-wave propagation from an emission source at 11R_S and an anisotropy factor or α = 0.30. Dashed vertical lines indicate the peak time for each time profile.

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