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Velocity Dispersion of Solar Energetic Particles in the Turbulent Heliosphere

  • Authors: T. Laitinen, S. Dalla

T. Laitinen and S. Dalla 2026 The Astrophysical Journal Letters 1010 .

  • Provider: AAS Journals

Caption: Figure 2.

The contour shows the simulated proton intensities as a function of inverse of velocity (in light-speed units) and time at Δϕ = 0∘, for the moderate turbulence case. The yellow circles are the onset times determined with Equation (6), and the yellow curve is the fit of the onset times to Equation (1). The blue diamonds, connected with the dashed line, show the arrival time of scatter-free protons along the nominal Parker spiral.

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