Vyacheslav Pilipenko , Shufan Zhao , Natalia Savelieva , Nikolay Mazur , Evgeniy Fedorov , Zhenhui Ma
{"title":"CSES 卫星探测到的 ZEVS 发射器在顶层电离层的 ELF 发射","authors":"Vyacheslav Pilipenko , Shufan Zhao , Natalia Savelieva , Nikolay Mazur , Evgeniy Fedorov , Zhenhui Ma","doi":"10.1016/j.asr.2024.07.074","DOIUrl":null,"url":null,"abstract":"<div><div>The extremely-low-frequency (ELF) response in the upper ionosphere to ground large-scale transmitter ZEVS on the Kola Peninsula has been detected by low-Earth orbiting satellite CSES (<span><math><mrow><mo>∼</mo></mrow></math></span>500 km altitude). When the satellite was in the vicinity of the ZEVS transmitter above the White Sea (horizontal distance <span><math><mrow><mo>∼</mo></mrow></math></span>400–900 km), the electric and magnetic sensors detected a narrowband 82 Hz emission with amplitudes <span><math><mrow><mi>E</mi><mo>≃</mo><mn>1</mn><mo>-</mo><mn>3</mn></mrow></math></span> <span><math><mrow><mi>μ</mi></mrow></math></span>V/m and <span><math><mrow><mi>B</mi><mo>≃</mo><mn>0.5</mn><mo>-</mo><mn>1.0</mn></mrow></math></span> pT. We modeled the ELF wave field spatial structure in the upper ionosphere excited by an oscillating 82 Hz linear current with the 60 km length suspended above a high-resistive ground. Realistic altitudinal profiles of the plasma parameters during events under study have been reconstructed with the use of the IRI ionospheric model. The modeled amplitudes of electromagnetic response of the upper ionosphere are in reasonable agreement with the 82-Hz emission power recorded by the CSES satellite for a typical transmitter current intensity <span><math><mrow><mo>></mo><mn>100</mn></mrow></math></span> A.</div></div>","PeriodicalId":50850,"journal":{"name":"Advances in Space Research","volume":"74 10","pages":"Pages 4937-4947"},"PeriodicalIF":2.8000,"publicationDate":"2024-08-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"ELF emission in the topside ionosphere from the ZEVS transmitter detected by CSES satellite\",\"authors\":\"Vyacheslav Pilipenko , Shufan Zhao , Natalia Savelieva , Nikolay Mazur , Evgeniy Fedorov , Zhenhui Ma\",\"doi\":\"10.1016/j.asr.2024.07.074\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><div>The extremely-low-frequency (ELF) response in the upper ionosphere to ground large-scale transmitter ZEVS on the Kola Peninsula has been detected by low-Earth orbiting satellite CSES (<span><math><mrow><mo>∼</mo></mrow></math></span>500 km altitude). When the satellite was in the vicinity of the ZEVS transmitter above the White Sea (horizontal distance <span><math><mrow><mo>∼</mo></mrow></math></span>400–900 km), the electric and magnetic sensors detected a narrowband 82 Hz emission with amplitudes <span><math><mrow><mi>E</mi><mo>≃</mo><mn>1</mn><mo>-</mo><mn>3</mn></mrow></math></span> <span><math><mrow><mi>μ</mi></mrow></math></span>V/m and <span><math><mrow><mi>B</mi><mo>≃</mo><mn>0.5</mn><mo>-</mo><mn>1.0</mn></mrow></math></span> pT. We modeled the ELF wave field spatial structure in the upper ionosphere excited by an oscillating 82 Hz linear current with the 60 km length suspended above a high-resistive ground. Realistic altitudinal profiles of the plasma parameters during events under study have been reconstructed with the use of the IRI ionospheric model. The modeled amplitudes of electromagnetic response of the upper ionosphere are in reasonable agreement with the 82-Hz emission power recorded by the CSES satellite for a typical transmitter current intensity <span><math><mrow><mo>></mo><mn>100</mn></mrow></math></span> A.</div></div>\",\"PeriodicalId\":50850,\"journal\":{\"name\":\"Advances in Space Research\",\"volume\":\"74 10\",\"pages\":\"Pages 4937-4947\"},\"PeriodicalIF\":2.8000,\"publicationDate\":\"2024-08-02\",\"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/S0273117724007932\",\"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/S0273117724007932","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}
ELF emission in the topside ionosphere from the ZEVS transmitter detected by CSES satellite
The extremely-low-frequency (ELF) response in the upper ionosphere to ground large-scale transmitter ZEVS on the Kola Peninsula has been detected by low-Earth orbiting satellite CSES (500 km altitude). When the satellite was in the vicinity of the ZEVS transmitter above the White Sea (horizontal distance 400–900 km), the electric and magnetic sensors detected a narrowband 82 Hz emission with amplitudes V/m and pT. We modeled the ELF wave field spatial structure in the upper ionosphere excited by an oscillating 82 Hz linear current with the 60 km length suspended above a high-resistive ground. Realistic altitudinal profiles of the plasma parameters during events under study have been reconstructed with the use of the IRI ionospheric model. The modeled amplitudes of electromagnetic response of the upper ionosphere are in reasonable agreement with the 82-Hz emission power recorded by the CSES satellite for a typical transmitter current intensity A.
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.