I. On a gas showing the spectrum of helium, the reputed cause of D3, one of the lines in the coronal spectrum. Preliminary note

@article{RamsayIOA,
  title={I. On a gas showing the spectrum of helium, the reputed cause of D3, one of the lines in the coronal spectrum. Preliminary note},
  author={William Ramsay},
  journal={Proceedings of the Royal Society of London},
  volume={58},
  pages={65 - 67}
}
  • W. Ramsay
  • Geology
  • Proceedings of the Royal Society of London
In the course of investigations on argon, some clue was sought for, which would lead to the selection of one out of the almost innumerable compounds with which chemists are acquainted, with which to attempt to induce argon to combine. A paper by W. F. Hillebrand, “On the Occurrence of Nitrogen in Uraninite, &c.” (‘Bull, of the U. S. Geological Survey,’ No. 78, p. 43), to which M r. Miers kindly directed my attention, gave the desired clue. In spite of Hillebrand’s positive proof that the gas he… 

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