{"title":"望远镜流星的实际星等和视星等","authors":"C. Wylie","doi":"10.1111/J.1945-5100.1951.TB00162.X","DOIUrl":null,"url":null,"abstract":"Six (6) dual observations of meteors, made with the naked eye and with a telescope or binoculars, are discussed. It is found that one (1) was a “point” meteor. Two (2) were “line” meteors seen with the telescope or binoculars before being noticed with the naked eye and at below-the-naked-eye magnitude. Three (3) were “line” meteors, for which the binocular and the naked-eye observers recorded essentially the same real magnitudes.","PeriodicalId":294885,"journal":{"name":"Contributions of the Meteoritical Society","volume":"9 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1900-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"The Real and Apparent Stellar Magnitudes of Telescopic Meteors\",\"authors\":\"C. Wylie\",\"doi\":\"10.1111/J.1945-5100.1951.TB00162.X\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Six (6) dual observations of meteors, made with the naked eye and with a telescope or binoculars, are discussed. It is found that one (1) was a “point” meteor. Two (2) were “line” meteors seen with the telescope or binoculars before being noticed with the naked eye and at below-the-naked-eye magnitude. Three (3) were “line” meteors, for which the binocular and the naked-eye observers recorded essentially the same real magnitudes.\",\"PeriodicalId\":294885,\"journal\":{\"name\":\"Contributions of the Meteoritical Society\",\"volume\":\"9 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"1900-01-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Contributions of the Meteoritical Society\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1111/J.1945-5100.1951.TB00162.X\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Contributions of the Meteoritical Society","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1111/J.1945-5100.1951.TB00162.X","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
The Real and Apparent Stellar Magnitudes of Telescopic Meteors
Six (6) dual observations of meteors, made with the naked eye and with a telescope or binoculars, are discussed. It is found that one (1) was a “point” meteor. Two (2) were “line” meteors seen with the telescope or binoculars before being noticed with the naked eye and at below-the-naked-eye magnitude. Three (3) were “line” meteors, for which the binocular and the naked-eye observers recorded essentially the same real magnitudes.
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