{"title":"普通恒星发出的闪光","authors":"B. Schaefer","doi":"10.1086/167162","DOIUrl":null,"url":null,"abstract":"The characteristics of flashes from 24 normal stars are presented and discussed. Rate estimates are made for the flashes and possible mechanisms for them are considered. The consequences for the earth of solar flashes of varying intensities are examined.","PeriodicalId":9423,"journal":{"name":"Bulletin of the American Astronomical Society","volume":"211 1","pages":"1023"},"PeriodicalIF":0.0000,"publicationDate":"1989-02-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"43","resultStr":"{\"title\":\"Flashes from normal stars\",\"authors\":\"B. Schaefer\",\"doi\":\"10.1086/167162\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The characteristics of flashes from 24 normal stars are presented and discussed. Rate estimates are made for the flashes and possible mechanisms for them are considered. The consequences for the earth of solar flashes of varying intensities are examined.\",\"PeriodicalId\":9423,\"journal\":{\"name\":\"Bulletin of the American Astronomical Society\",\"volume\":\"211 1\",\"pages\":\"1023\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1989-02-15\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"43\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Bulletin of the American Astronomical Society\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1086/167162\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Bulletin of the American Astronomical Society","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1086/167162","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The characteristics of flashes from 24 normal stars are presented and discussed. Rate estimates are made for the flashes and possible mechanisms for them are considered. The consequences for the earth of solar flashes of varying intensities are examined.
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