{"title":"白矮星和中子星","authors":"S. Shapiro, S. Teukolsky","doi":"10.1017/9781108181914.019","DOIUrl":null,"url":null,"abstract":"A modulation contrast microscope employs a closely wound lamp filament of a rectangular configuration as an illuminating source. The image of the filament is registered on a Fourier plane to which plane a modulator is located which serves to render phase gradients in phase objects visible by functioning to provide light amplitude differences in accordance with modifying the amplitude of the light beam relatively about a given region in both a greater and lesser intensity.","PeriodicalId":348488,"journal":{"name":"Stars and Stellar Processes","volume":"64 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2019-02-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"17","resultStr":"{\"title\":\"White Dwarfs and Neutron Stars\",\"authors\":\"S. Shapiro, S. Teukolsky\",\"doi\":\"10.1017/9781108181914.019\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"A modulation contrast microscope employs a closely wound lamp filament of a rectangular configuration as an illuminating source. The image of the filament is registered on a Fourier plane to which plane a modulator is located which serves to render phase gradients in phase objects visible by functioning to provide light amplitude differences in accordance with modifying the amplitude of the light beam relatively about a given region in both a greater and lesser intensity.\",\"PeriodicalId\":348488,\"journal\":{\"name\":\"Stars and Stellar Processes\",\"volume\":\"64 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2019-02-07\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"17\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Stars and Stellar Processes\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1017/9781108181914.019\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Stars and Stellar Processes","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1017/9781108181914.019","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
A modulation contrast microscope employs a closely wound lamp filament of a rectangular configuration as an illuminating source. The image of the filament is registered on a Fourier plane to which plane a modulator is located which serves to render phase gradients in phase objects visible by functioning to provide light amplitude differences in accordance with modifying the amplitude of the light beam relatively about a given region in both a greater and lesser intensity.
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