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    <title>IIAP Repository Collection: John Evershed (1911 - 1923)</title>
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    <title>The Channel Image</title>
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    <title>The problem of the red shift in the solar spectrum (Reply to S.M. Sulaiman)</title>
    <link>http://hdl.handle.net/2248/4039</link>
    <description>Title: The problem of the red shift in the solar spectrum (Reply to S.M. Sulaiman)&lt;br/&gt;&lt;br/&gt;Authors: Evershed, John&lt;br/&gt;&lt;br/&gt;Description: Open Access</description>
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    <title>The Einstein effect in the solar spectrum</title>
    <link>http://hdl.handle.net/2248/4038</link>
    <description>Title: The Einstein effect in the solar spectrum&lt;br/&gt;&lt;br/&gt;Authors: Evershed, John&lt;br/&gt;&lt;br/&gt;Description: Open Access</description>
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    <title>The positive-on-negative method of measuring spectra</title>
    <link>http://hdl.handle.net/2248/4037</link>
    <description>Title: The positive-on-negative method of measuring spectra&lt;br/&gt;&lt;br/&gt;Authors: Evershed, John&lt;br/&gt;&lt;br/&gt;Description: Open Access</description>
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    <title>Recollections of seventy years of scientific work</title>
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    <description>Title: Recollections of seventy years of scientific work&lt;br/&gt;&lt;br/&gt;Authors: Evershed, John&lt;br/&gt;&lt;br/&gt;Abstract: This article records some of the researches in solar physics undertaken during my life. These have included the following: prominence observations covering sixteen years; spectroheliograph work with a direct vision prism; experiments on the radiation of heated gases; eclipse expeditions in 1898 and 1900; studies of the relation between emission and absorption spectra, and of the continuous spectrum of hydrogen. In India (1906–1923) my work included: the discovery of radial motion and the estimate of pressure in sunspots; a study of the exceptional observing conditions in Kashmir; measurements of the red-shift in connection with Einstein's prediction; great magnetic storms during flares; the motion in the tail of Halley's comet and its transit over the Sun; observations of novae. At Ewhurst (1923–1954) I was concerned with: high-dispersion work with liquid prisms; the study of the Zeeman effect and the discovery of a particularly sensitive line for its determination; measurements of minute line-shifts due to horizontal motions; and the decrease of wavelength of solar lines. Reference is made to scientific men I have met and to whom I am indebted for interest and encouragement.&lt;br/&gt;&lt;br/&gt;Description: Restricted Access</description>
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