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The nature of the 760 nm Fraunhofer line in the solar spectrum

PUBLISHED June 14, 2024 (DOI: https://doi.org/10.54985/peeref.2406p3954665)

NOT PEER REVIEWED

Authors

Inna Tkachenko1
  1. Bohdan Khmelnytsky Cherkasy National University

Conference / event

26th All-Ukrainian Scientific Conference for Young Scientists "Topical Problems of Natural Sciences and Humanities in the Studies of Young Scientists", May 2024 (Cherkasy, Ukraine)

Poster summary

This work is devoted to the study of the Fraunhofer line 760 nm origion in the solar spectrum, which is formed as a result of absorption by the Earth’s atmospheric oxygen. The study of the nature of this line is important for the development of atmospheric spectroscopy and the study of physical and chemical processes occurring in the middle and upper layers of the Earth's atmosphere. The results of the study indicate that for a free oxygen molecule the absorption of visible light occurs due to the weak interaction of the magnetic field of the light wave with the spin of the molecule. The Fraunhofer line in the 760 nm region arises from the O2 (1Σg+ – 3Σg-) transition due to spin-orbit coupling between these states being determined by the magnetic dipole transition moment and takes the intensity from the microwave transition between the spin magnetic sublevels 3Σg,0- - 3Σg,1-.

Keywords

Red atmospheric band, Spin-orbit coupling, Magnetic transition moment, Oxygen molecule

Research areas

Chemistry

References

  1. Boris Minaev. Environment friendly spin-catalysis for dioxygen activation. Chemistry & Chemical Technology, 2010, 4 (1), 1-16. DOI: 10.23939/chcht04.01.001.
  2. Boris F. Minaev, Valentina A. Minaeva, Yurij V. Evtuhov. Quantum-Chemical Study of the Singlet Oxygen Emission. Int. J. Quant. Chem., 2008, 109 (3), 500-515. DOI: 10.1002/qua.21783.
  3. Boris Minaev, Olav Vahtras, Hans Ågren. Magnetic phosphorescence of molecular oxygen. A study of the b1Σg+-X3Σg- transition probability using multiconfiguration response theory. Chemical Physics 208 (1996) 299-311.
  4. B.F. Minaev. Solvent induced emission of molecular 1Δg oxygen. Journal of Molecular Structure (Theochem), 183 (1989) 207-214.

Funding

No data provided

Supplemental files

No data provided

Additional information

Competing interests
No competing interests were disclosed.
Data availability statement
The datasets generated during and / or analyzed during the current study are available from the corresponding author on reasonable request.
Creative Commons license
Copyright © 2024 Tkachenko. This is an open access work distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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Cite
Tkachenko, I. The nature of the 760 nm Fraunhofer line in the solar spectrum [not peer reviewed]. Peeref 2024 (poster).
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