Contribution to Solar Physics. I. a Popular Account of Inquiries Into the Physical Constitution of the Sun, With Special Reference to Recent Spectroscopic Researches; Ii. Communication to the Royal Society of London, And the French Academy of Sciences, Wi
The book Contribution to Solar Physics. I. a Popular Account of Inquiries Into the Physical Constitution of the Sun, With Special Reference to Recent Spectroscopic Researches; Ii. Communication to the Royal Society of London, And the French Academy of Sciences, Wi was written by author Lockyer, Norman, Sir, 1836-1920 Here you can read free online of Contribution to Solar Physics. I. a Popular Account of Inquiries Into the Physical Constitution of the Sun, With Special Reference to Recent Spectroscopic Researches; Ii. Communication to the Royal Society of London, And the French Academy of Sciences, Wi book, rate and share your impressions in comments. If you don't know what to write, just answer the question: Why is Contribution to Solar Physics. I. a Popular Account of Inquiries Into the Physical Constitution of the Sun, With Special Reference to Recent Spectroscopic Researches; Ii. Communication to the Royal Society of London, And the French Academy of Sciences, Wi a good or bad book?
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Such great advances have been made that it will be necessary for me to split up the subject, in order that the different lines of research may be the better understood, and that my own 1 Revised from the short-hand notes of two lectures delivered before the Literary and Philosophical Society of Newcastle-upon-Tyne, in October 1872. 382 SOLAR PHYSICS. chap. work will be the easier, for I quite feel the difficulties con- ' nected with the giving of such a general resume of entirely in the spectru...m new work over so large a field. Looking at the new results, then, from the spectrum point of view — that is, arranging them as the spectrum is affected by the various solar phenomena with which the new method has familiarized us, we may group it as follows : — Changes i. Variations in the positions of lines in the solar spec- trum (changes of wave-length), connected with changes in the lines from dark to bright. 2. Variations in the thickness of spectral lines (selec- tive radiation and absorption), and in the amount of con- tinuous absorption.
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