Particle Acceleration Mechanisms
Alexandr Afanasiev; Rami Vainio
Particle Acceleration Mechanisms
Alexandr Afanasiev
Rami Vainio
Springer
Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2021042720257
https://urn.fi/URN:NBN:fi-fe2021042720257
Tiivistelmä
This chapter provides a short tutorial review on particle acceleration in dynamic electromagnetic fields under scenarios relevant to the problem of particle acceleration in the solar corona and solar wind during solar eruptions. It concentrates on fundamental aspects of the acceleration process and refrains from presenting detailed modeling of the specific conditions in solar eruptive plasmas. All particle acceleration mechanisms (in the solar corona) are related to electric fields that can persist in the highly conductive plasma: either electrostatic (or potential) or inductive related to temporally variable magnetic fields through Faraday’s law. Mechanisms involving both kinds of fields are included in the tutorial.
Kokoelmat
- Rinnakkaistallenteet [19207]