{"title":"Particle-in-cell Simulation of Electromagnetic Field Structure in the Electron-only Reconnection","authors":"Shi-Hang Hu, Quan-Ming Lu, Yun-Dan Guan, L.U. San","doi":"10.1016/j.chinastron.2025.05.003","DOIUrl":null,"url":null,"abstract":"<div><div>Standard collisionless magnetic reconnection couples with both electron and ion dynamics. Recently, a new type of magnetic reconnection, electron-only magnetic reconnection without ion outflow, has been observed. Using 2.5D particle-in-cell simulation, the electromagnetic field structure in the electron-only reconnection with a strong guide field was studied. At the moment of the maximum reconnection rate, the electron inflow and outflow are observed on either side of the separatrix. The spatial distribution of the electron bulk velocity is approximately symmetric, which generates the nearly symmetrically distributed Hall current, resulting in the quadrupole Hall magnetic field. The Hall magnetic field is not obviously distorted despite the presence of the strong guide field. Meanwhile, the charge separation is caused in the separatrix region, which generates the nearly symmetrically distributed Hall electric field. Besides, the evolution of the spatial distribution of the electron bulk velocity was studied. The equation of motion for the frozen electrons was analytically obtained: <span><math><mrow><msub><mi>v</mi><mrow><mi>e</mi></mrow></msub><mo>=</mo><msub><mi>v</mi><mrow><mrow><mi>e</mi></mrow><mi>y</mi></mrow></msub><mi>B</mi><mo>/</mo><msub><mi>B</mi><mi>y</mi></msub><mo>+</mo><mi>E</mi><mo>×</mo><mrow><mo>(</mo><msub><mi>B</mi><mi>y</mi></msub><msub><mi>e</mi><mi>y</mi></msub><mo>)</mo></mrow><mo>/</mo><msubsup><mi>B</mi><mrow><mi>y</mi></mrow><mn>2</mn></msubsup></mrow></math></span>. According to the equation of motion for the electrons, we divide the electron-only reconnection with a strong guide field into two stages. In the first stage, the <span><math><mrow><mi>E</mi><mo>×</mo><mi>B</mi></mrow></math></span> drift is negligible because of the weaker Hall electric field, and then the electrons flow mainly along the magnetic field line following the equation <span><math><mrow><msub><mi>v</mi><mrow><mi>e</mi></mrow></msub><mo>≈</mo><msub><mi>v</mi><mrow><mrow><mi>e</mi></mrow><mi>y</mi></mrow></msub><mi>B</mi><mo>/</mo><msub><mi>B</mi><mi>y</mi></msub></mrow></math></span>. In the second stage, the Hall electric field is so strong that the motion of electrons is dominated by the <span><math><mrow><mi>E</mi><mo>×</mo><mi>B</mi></mrow></math></span> drift following the equation <span><math><mrow><msub><mi>v</mi><mrow><mi>e</mi></mrow></msub><mo>≈</mo><mi>E</mi><mo>×</mo><mrow><mo>(</mo><msub><mi>B</mi><mi>y</mi></msub><msub><mi>e</mi><mi>y</mi></msub><mo>)</mo></mrow><mo>/</mo><msubsup><mi>B</mi><mrow><mi>y</mi></mrow><mn>2</mn></msubsup></mrow></math></span>. The simulation shows that extremely strong charge separation can be caused in electron-only reconnection, which generates the nearly symmetrically distributed Hall electric field. With a guide field, this Hall electric field leads to the <span><math><mrow><mi>E</mi><mo>×</mo><mi>B</mi></mrow></math></span> drift, which dominates the spatial distribution of the electron bulk velocity. Therefore nearly symmetrically distributed Hall current is formed, which generates the nearly symmetrically distributed quadrupole Hall magnetic field.</div></div>","PeriodicalId":35730,"journal":{"name":"Chinese Astronomy and Astrophysics","volume":"49 2","pages":"Pages 267-279"},"PeriodicalIF":0.0000,"publicationDate":"2025-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy and Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0275106225000335","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"Physics and Astronomy","Score":null,"Total":0}
引用次数: 0
Abstract
Standard collisionless magnetic reconnection couples with both electron and ion dynamics. Recently, a new type of magnetic reconnection, electron-only magnetic reconnection without ion outflow, has been observed. Using 2.5D particle-in-cell simulation, the electromagnetic field structure in the electron-only reconnection with a strong guide field was studied. At the moment of the maximum reconnection rate, the electron inflow and outflow are observed on either side of the separatrix. The spatial distribution of the electron bulk velocity is approximately symmetric, which generates the nearly symmetrically distributed Hall current, resulting in the quadrupole Hall magnetic field. The Hall magnetic field is not obviously distorted despite the presence of the strong guide field. Meanwhile, the charge separation is caused in the separatrix region, which generates the nearly symmetrically distributed Hall electric field. Besides, the evolution of the spatial distribution of the electron bulk velocity was studied. The equation of motion for the frozen electrons was analytically obtained: . According to the equation of motion for the electrons, we divide the electron-only reconnection with a strong guide field into two stages. In the first stage, the drift is negligible because of the weaker Hall electric field, and then the electrons flow mainly along the magnetic field line following the equation . In the second stage, the Hall electric field is so strong that the motion of electrons is dominated by the drift following the equation . The simulation shows that extremely strong charge separation can be caused in electron-only reconnection, which generates the nearly symmetrically distributed Hall electric field. With a guide field, this Hall electric field leads to the drift, which dominates the spatial distribution of the electron bulk velocity. Therefore nearly symmetrically distributed Hall current is formed, which generates the nearly symmetrically distributed quadrupole Hall magnetic field.
期刊介绍:
The vigorous growth of astronomical and astrophysical science in China led to an increase in papers on astrophysics which Acta Astronomica Sinica could no longer absorb. Translations of papers from two new journals the Chinese Journal of Space Science and Acta Astrophysica Sinica are added to the translation of Acta Astronomica Sinica to form the new journal Chinese Astronomy and Astrophysics. Chinese Astronomy and Astrophysics brings English translations of notable articles to astronomers and astrophysicists outside China.