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592.] [Footnote 574: He died in London, November 20, 1898.] [Footnote 575: _Bull. Acad. St. Petersbourg_, t. vi., p. 253.] [Footnote 576: W. H. Wesley, _Phil. Trans._, vol. cxc, p. 204.] [Footnote 577: _Lick Reports on Eclipse of January 1, 1889_, p. 204.] [Footnote 578: _Astroph. Jour._, vol. xi., p. 226.] [Footnote 579: _Observatory_, vol. xxi., p. 157.] [Footnote 580: _The Indian Eclipse_, 1898, p. 114.] [Footnote 581: _Science_, June 22, 1900; _Astroph. Jour._, vol. xii., p. 370.] [Footnote 582: _Ann. der Physik_, Bd. xlviii., p. 528. See also Wood, _Physical Review_, vol. iv., p. 191, 1896.] [Footnote 583: _Science_, August 3, 1900.] [Footnote 584: _Lick Observatory Bulletin_, No. 9.] [Footnote 585: _Observatory_, vol. xxiv., pp. 321, 375.] [Footnote 586: _Lick Report on Eclipse of December 22, 1889_, p. 47; _Month. Not._, vol. l., p. 372.] [Footnote 587: _Lick Obs. Bull._, No. 9.] [Footnote 588: _Bull. de l'Acad. St. Petersbourg_, t. iv., p. 289.] [Footnote 589: _The Solar Corona discussed by Spherical Harmonics_, Smithsonian Institution, 1889.] [Footnote 590: Bakerian Lecture, _Proc. Roy. Soc._, vol. xxxix.] [Footnote 591: _Astr. and Astrophysics_, vol. xi., p. 483.] [Footnote 592: _Ibid._, vol. xii., p. 804.] [Footnote 593: _Am. Journ. of Science_, vol. xi., p. 253, 1901.] [Footnote 594: See Huggins, _Proc. Roy. Soc._, vol. xxxix., p. 108; Young, _North Am. Review_, February, 1885, p. 179.] [Footnote 595: Professor W. A. Norton, of Yale College, appears to have been the earliest formal advocate of the Expulsion Theory of the solar surroundings, in the second (1845) and later editions of his _Treatise on Astronomy_.] CHAPTER IV _SOLAR SPECTROSCOPY_ The new way struck out by Janssen and Lockyer was at once and eagerly followed. In every part of Europe, as well as in North America, observers devoted themselves to the daily study of the chromosphere and prominences. Foremost among these were Lockyer in England, Zoellner at Leipzig, Spoerer at Anclam, Young at Hanover, New Hampshire, Secchi and Respighi at Rome. There were many others, but these names stood out conspicuously. The first point to be cleared up was that of chemical composition. Leisurely measurements verified the presence above the sun's surface of hydrogen in prodigious volumes, but showed that sodium had nothing to do with the o
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