Nonlinear Processes in the Heliosphere and Their Effect on Spectral Index and Particle Energization (P45)

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The main objective of this talk would be to use the scientific data of various space missions (present and past related to IHY) and use them to understand the basic phenomenon that is responsible for transporting the energy of the sun (source) in the form of solar wind turbulence in the earth magnetosphere. What is the spectral index of this turbulence and on what parameters/factors it depends? With the help of computer simulated results, the evolution process will be illustrated in space and time in the heliospheric regions. In the second part of this talk, the coupling of this energy to the heliospheric particles and other nonlinear waves will be discussed. Specifically, the solar energetic particles generation and their energy distribution functions will be presented.

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