МОДЕЛИРОВАНИЕ ВЗАИМОДЕЙСТВИЯ ИОНОВ КИСЛОРОДА O+ – O+2 С ДИПОЛИЗАЦИОННЫМИ ФРОНТАМИ В СОПРОВОЖДЕНИИ ЭЛЕКТРОМАГНИТНОЙ ТУРБУЛЕНТНОСТИ В ХВОСТЕ МАГНИТОСФЕРЫ ЗЕМЛИ

Abstract

The paper is devoted to studying processes of plasma particle acceleration in the process of magnetic dipolazations in a current sheet of Earth’s magnetotail. A numerical model is constructed that allows evaluation of oxygen ions O+ – O+2 acceleration in two possible scenarios: (A) Passage of multiple dipolazation fronts; (B) Passage of fronts followed by largescale electromagnetic turbulence. The energy spectra of two types of accelerated particles are obtained: oxygen O+ and O+2. It is shown that, at different time scales, predominant variety acceleration of particle populations occurs in scenarios (A)–(B). Thus the closer the time scale of the field variation to the ions gyroperiod, the more effective is the transfer of energy from fields to particles. Oxygen ions O+2 are accelerated efficiently in multiple dipolazation process (B) and increase energy up to 3 MeV , whereas ions O+ - up to 1.7 МeV. It is shown that accounting for electromagnetic fluctuations, accompanying magnetic dipolazation, may explain the appearance of streams of oxygen ions with energies greater than 3MeV in Earth’s magnetotail.