{"title":"负离子等离子体中 (r, q) 分布对离子声波的影响及其在地球电离层中的应用","authors":"Zhong‐Zheng Li, Li‐Qiang Xie, Sheng‐De Liang, Dong‐Ning Gao","doi":"10.1002/ctpp.202400074","DOIUrl":null,"url":null,"abstract":"Ion acoustic waves (IAWs) are theoretically researched in a negative ion plasma (NIP) with warm light ions, cold heavy ions, and distributed electrons. The reductive perturbation method (RPM) is used to simplify two‐fluid plasma equations and the relevant ZK equation and solitary solution of IAWs are derived. Small‐k expansion method is applied to obtained the instability growth rate of IAWs. The flatness and tail parameters modify the amplitude, width, soliton energy, and instability growth rate. It is noted that the increscent flatness and tail parameters result in the increasing amplitude, width, and soliton energy. Increasing flatness and tail parameters lead to the decreasing growth rate. These results will be helpful in understanding the plasma dynamics for NIP system containing distributed electrons in Earth's ionosphere.","PeriodicalId":10700,"journal":{"name":"Contributions to Plasma Physics","volume":"31 1","pages":""},"PeriodicalIF":1.3000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Effect of (r, q) Distribution on Ion Acoustic Waves in a Negative‐Ion Plasma With Application to Earth's Ionosphere\",\"authors\":\"Zhong‐Zheng Li, Li‐Qiang Xie, Sheng‐De Liang, Dong‐Ning Gao\",\"doi\":\"10.1002/ctpp.202400074\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Ion acoustic waves (IAWs) are theoretically researched in a negative ion plasma (NIP) with warm light ions, cold heavy ions, and distributed electrons. The reductive perturbation method (RPM) is used to simplify two‐fluid plasma equations and the relevant ZK equation and solitary solution of IAWs are derived. Small‐k expansion method is applied to obtained the instability growth rate of IAWs. The flatness and tail parameters modify the amplitude, width, soliton energy, and instability growth rate. It is noted that the increscent flatness and tail parameters result in the increasing amplitude, width, and soliton energy. Increasing flatness and tail parameters lead to the decreasing growth rate. These results will be helpful in understanding the plasma dynamics for NIP system containing distributed electrons in Earth's ionosphere.\",\"PeriodicalId\":10700,\"journal\":{\"name\":\"Contributions to Plasma Physics\",\"volume\":\"31 1\",\"pages\":\"\"},\"PeriodicalIF\":1.3000,\"publicationDate\":\"2024-09-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Contributions to Plasma Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.1002/ctpp.202400074\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"PHYSICS, FLUIDS & PLASMAS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Contributions to Plasma Physics","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1002/ctpp.202400074","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, FLUIDS & PLASMAS","Score":null,"Total":0}
Effect of (r, q) Distribution on Ion Acoustic Waves in a Negative‐Ion Plasma With Application to Earth's Ionosphere
Ion acoustic waves (IAWs) are theoretically researched in a negative ion plasma (NIP) with warm light ions, cold heavy ions, and distributed electrons. The reductive perturbation method (RPM) is used to simplify two‐fluid plasma equations and the relevant ZK equation and solitary solution of IAWs are derived. Small‐k expansion method is applied to obtained the instability growth rate of IAWs. The flatness and tail parameters modify the amplitude, width, soliton energy, and instability growth rate. It is noted that the increscent flatness and tail parameters result in the increasing amplitude, width, and soliton energy. Increasing flatness and tail parameters lead to the decreasing growth rate. These results will be helpful in understanding the plasma dynamics for NIP system containing distributed electrons in Earth's ionosphere.