Charged Particle Transport in the Interplanetary Medium
: Angels Aran, Neus Agueda, Alexandr Afanasiev, Blai Sanahuja
: Olga E. Malandraki, Norma B. Crosby
: 2018
: Solar Particle Radiation Storms Forecasting and Analysis: The HESPERIA HORIZON 2020 Project and Beyond
: Astrophysics and Space Science Library
: 444
: 63
: 78
: 978-3-319-60050-5
: 978-3-319-60051-2
: 0067-0057
DOI: https://doi.org/10.1007/978-3-319-60051-2_4
: https://link.springer.com/chapter/10.1007/978-3-319-60051-2_4
: https://research.utu.fi/converis/portal/detail/Publication/36896333
The scenario and fundamentals of the physics of charged particle interplanetary transport are briefly introduced. Relevant characteristics of solar energetic particle (SEP) events and of the interplanetary magnetic field are described. Next, the motion of a charged particle and the main assumptions leading to the description of the focused and diffusive particle transport equations utilised in the next chapters are discussed. Finally, two different models are applied to interpret SEP events.
