R. Grard, D. Klinge, S. Klimov, S. Savin, J. Trotignon
{"title":"火卫一的等离子体波系统","authors":"R. Grard, D. Klinge, S. Klimov, S. Savin, J. Trotignon","doi":"10.1088/0022-3735/22/10/019","DOIUrl":null,"url":null,"abstract":"The Phobos-2 spacecraft has been inserted in a Mars orbit to rendezvous with one of the two Martian satellites, Phobos, in early 1989. The Plasma Wave System (PWS) is part of the scientific payload; this instrument will record, for the first time in a Martian environment, the spectra of natural waves with an electric dipole in the frequency range 0-150 kHz and measure the ionospheric plasma density distribution with a Langmuir probe. In-flight data show that the system performs well and that PWS should meet its scientific goals.","PeriodicalId":16791,"journal":{"name":"Journal of Physics E: Scientific Instruments","volume":"21 1","pages":"656-662"},"PeriodicalIF":0.0000,"publicationDate":"1989-10-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"22","resultStr":"{\"title\":\"The Plasma Wave System on Phobos\",\"authors\":\"R. Grard, D. Klinge, S. Klimov, S. Savin, J. Trotignon\",\"doi\":\"10.1088/0022-3735/22/10/019\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Phobos-2 spacecraft has been inserted in a Mars orbit to rendezvous with one of the two Martian satellites, Phobos, in early 1989. The Plasma Wave System (PWS) is part of the scientific payload; this instrument will record, for the first time in a Martian environment, the spectra of natural waves with an electric dipole in the frequency range 0-150 kHz and measure the ionospheric plasma density distribution with a Langmuir probe. In-flight data show that the system performs well and that PWS should meet its scientific goals.\",\"PeriodicalId\":16791,\"journal\":{\"name\":\"Journal of Physics E: Scientific Instruments\",\"volume\":\"21 1\",\"pages\":\"656-662\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1989-10-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"22\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Physics E: Scientific Instruments\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1088/0022-3735/22/10/019\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Physics E: Scientific Instruments","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1088/0022-3735/22/10/019","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The Phobos-2 spacecraft has been inserted in a Mars orbit to rendezvous with one of the two Martian satellites, Phobos, in early 1989. The Plasma Wave System (PWS) is part of the scientific payload; this instrument will record, for the first time in a Martian environment, the spectra of natural waves with an electric dipole in the frequency range 0-150 kHz and measure the ionospheric plasma density distribution with a Langmuir probe. In-flight data show that the system performs well and that PWS should meet its scientific goals.
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