{"title":"地球极区极光弧和极光洞场向静电势的空间等离子体沉淀和排斥过程","authors":"Masafumi Hirahara , Yusuke Ebihara , Takeshi Sakanoi","doi":"10.1016/j.asr.2025.06.037","DOIUrl":null,"url":null,"abstract":"<div><div>Electric fields along local magnetic field line are one of effective mechanisms for accelerating space plasmas, as represented by the cases of neutron stars and planetary auroras. In the terrestrial polar regions, anti-earthward electrostatic fields along geomagnetic field lines can accelerate electrons in space plasmas into the Earth’s upper atmosphere, generating bright and dynamic auroras characterized by arcs, curtains, curls, etc. One of the acceleration mechanisms producing “inverted V”-shaped features in energy-time/latitude distributions of precipitating auroral electrons, as observed in low-altitude space missions, is due to anti-earthward parallel electrostatic fields. The field-aligned electrostatic potentials, ranging from tens of volts to tens of kilo volts, are a consequence of the dynamo process generated in the dynamically changing magnetosphere. Our satellite instruments observed clear ion flux depletion in the energy range corresponding to localized field-aligned electrostatic potential above the satellite, which was coincidental with the electron precipitation forming the inverted-Vs. With advanced instruments onboard a microsatellite in low-altitude polar orbit, we detected recurring ion precipitation signatures accelerated by earthward parallel electrostatic fields, coinciding with electron flux depletion in the energy range smaller than the electrostatic potential. These precipitating ion signatures were observed in aurora-void regions, which we call “auroral holes” here, a conception newly defined after “coronal hole” of the Sun. These signatures provide persuasive double clues for the earthward electrostatic fields that accelerate ions toward the Earth and prevent electrons from penetrating the upper atmosphere although results in the past satellite missions might show the similar signatures.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"76 4","pages":"Pages 2249-2264"},"PeriodicalIF":2.8000,"publicationDate":"2025-06-18","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Space plasma precipitation and repelling processes by field-aligned electrostatic potential in auroral arc and hole in the terrestrial polar regions\",\"authors\":\"Masafumi Hirahara , Yusuke Ebihara , Takeshi Sakanoi\",\"doi\":\"10.1016/j.asr.2025.06.037\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>Electric fields along local magnetic field line are one of effective mechanisms for accelerating space plasmas, as represented by the cases of neutron stars and planetary auroras. In the terrestrial polar regions, anti-earthward electrostatic fields along geomagnetic field lines can accelerate electrons in space plasmas into the Earth’s upper atmosphere, generating bright and dynamic auroras characterized by arcs, curtains, curls, etc. One of the acceleration mechanisms producing “inverted V”-shaped features in energy-time/latitude distributions of precipitating auroral electrons, as observed in low-altitude space missions, is due to anti-earthward parallel electrostatic fields. The field-aligned electrostatic potentials, ranging from tens of volts to tens of kilo volts, are a consequence of the dynamo process generated in the dynamically changing magnetosphere. Our satellite instruments observed clear ion flux depletion in the energy range corresponding to localized field-aligned electrostatic potential above the satellite, which was coincidental with the electron precipitation forming the inverted-Vs. With advanced instruments onboard a microsatellite in low-altitude polar orbit, we detected recurring ion precipitation signatures accelerated by earthward parallel electrostatic fields, coinciding with electron flux depletion in the energy range smaller than the electrostatic potential. These precipitating ion signatures were observed in aurora-void regions, which we call “auroral holes” here, a conception newly defined after “coronal hole” of the Sun. These signatures provide persuasive double clues for the earthward electrostatic fields that accelerate ions toward the Earth and prevent electrons from penetrating the upper atmosphere although results in the past satellite missions might show the similar signatures.</div></div>\",\"PeriodicalId\":50850,\"journal\":{\"name\":\"Advances in Space Research\",\"volume\":\"76 4\",\"pages\":\"Pages 2249-2264\"},\"PeriodicalIF\":2.8000,\"publicationDate\":\"2025-06-18\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Advances in Space Research\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S0273117725006490\",\"RegionNum\":3,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Advances in Space Research","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0273117725006490","RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
Space plasma precipitation and repelling processes by field-aligned electrostatic potential in auroral arc and hole in the terrestrial polar regions
Electric fields along local magnetic field line are one of effective mechanisms for accelerating space plasmas, as represented by the cases of neutron stars and planetary auroras. In the terrestrial polar regions, anti-earthward electrostatic fields along geomagnetic field lines can accelerate electrons in space plasmas into the Earth’s upper atmosphere, generating bright and dynamic auroras characterized by arcs, curtains, curls, etc. One of the acceleration mechanisms producing “inverted V”-shaped features in energy-time/latitude distributions of precipitating auroral electrons, as observed in low-altitude space missions, is due to anti-earthward parallel electrostatic fields. The field-aligned electrostatic potentials, ranging from tens of volts to tens of kilo volts, are a consequence of the dynamo process generated in the dynamically changing magnetosphere. Our satellite instruments observed clear ion flux depletion in the energy range corresponding to localized field-aligned electrostatic potential above the satellite, which was coincidental with the electron precipitation forming the inverted-Vs. With advanced instruments onboard a microsatellite in low-altitude polar orbit, we detected recurring ion precipitation signatures accelerated by earthward parallel electrostatic fields, coinciding with electron flux depletion in the energy range smaller than the electrostatic potential. These precipitating ion signatures were observed in aurora-void regions, which we call “auroral holes” here, a conception newly defined after “coronal hole” of the Sun. These signatures provide persuasive double clues for the earthward electrostatic fields that accelerate ions toward the Earth and prevent electrons from penetrating the upper atmosphere although results in the past satellite missions might show the similar signatures.
期刊介绍:
The COSPAR publication Advances in Space Research (ASR) is an open journal covering all areas of space research including: space studies of the Earth''s surface, meteorology, climate, the Earth-Moon system, planets and small bodies of the solar system, upper atmospheres, ionospheres and magnetospheres of the Earth and planets including reference atmospheres, space plasmas in the solar system, astrophysics from space, materials sciences in space, fundamental physics in space, space debris, space weather, Earth observations of space phenomena, etc.
NB: Please note that manuscripts related to life sciences as related to space are no more accepted for submission to Advances in Space Research. Such manuscripts should now be submitted to the new COSPAR Journal Life Sciences in Space Research (LSSR).
All submissions are reviewed by two scientists in the field. COSPAR is an interdisciplinary scientific organization concerned with the progress of space research on an international scale. Operating under the rules of ICSU, COSPAR ignores political considerations and considers all questions solely from the scientific viewpoint.