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Updated: Jun 29, 2026

Probing the Structure and Dynamics of Interfacial Water with Scanning Tunneling Microscopy and Spectroscopy
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Probing the Structure and Dynamics of Interfacial Water with Scanning Tunneling Microscopy and Spectroscopy

Published on: May 27, 2018

銀河間媒介におけるイオン化されたヘリウムの構造を,遠紫外線スペクトロスコピクエクスプローラーで解明した

G A Kriss1, J M Shull, W Oegerle

  • 1Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA. gak@stsci.edu

Science (New York, N.Y.)
|August 11, 2001
PubMed
まとめ

初期の宇宙の構造は,中性水素 (H I) とイオン化されたヘリウム (He II) の吸収によって明らかになる. 観測により,He II ライマンアルファ吸収が示され,ほとんどの特徴にはH Iの対称性があり,低密度地域でも構造を示しています.

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Sample Preparation and Transfer Protocol for In-Vacuum Long-Wavelength Crystallography on Beamline I23 at Diamond Light Source10:32

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