{"title":"A Unified Phenomenology of Ion Heating in Low-$β$ Plasmas: Test-Particle Simulations","authors":"Zade Johnston, Jonathan Squire, Romain Meyrand","doi":"arxiv-2409.07015","DOIUrl":null,"url":null,"abstract":"We argue that two prominent theories of ion heating in low-$\\beta$\ncollisionless plasmas -- stochastic and quasi-linear heating -- represent\nsimilar physical processes in turbulence with different normalized cross\nhelicities. To capture both, we propose a simple phenomenology based on the\npower in scales at which critically balanced fluctuations reach their smallest\nparallel scale. Simulations of test ions interacting with turbulence confirm\nour scalings across a wide range of different ion and turbulence properties,\nincluding with a steep ion-kinetic transition range as relevant to the solar\nwind.","PeriodicalId":501423,"journal":{"name":"arXiv - PHYS - Space Physics","volume":"8 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Space Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.07015","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We argue that two prominent theories of ion heating in low-$\beta$
collisionless plasmas -- stochastic and quasi-linear heating -- represent
similar physical processes in turbulence with different normalized cross
helicities. To capture both, we propose a simple phenomenology based on the
power in scales at which critically balanced fluctuations reach their smallest
parallel scale. Simulations of test ions interacting with turbulence confirm
our scalings across a wide range of different ion and turbulence properties,
including with a steep ion-kinetic transition range as relevant to the solar
wind.