Nuclear-Chemical Processes in the Solar Atmosphere

Timashev Serge

doi:doi:10.11648/j.ijass.20140206.12

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Nuclear-Chemical Processes in the Solar Atmosphere

Timashev Serge

Published in International Journal of Astrophysics and Space Science (Volume 2, Issue 6)

Received: 10 December 2014 Accepted: 19 December 2014 Published: 27 December 2014

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Abstract

The ideas put forward earlier about the initiation of nuclear processes in a low-temperature plasma as a result of interaction between electrons of high (on chemical scales) energies and nuclei are demonstrated to be helpful in clearing some debatable issues concerning the synthesis of light elements in the solar atmosphere. Specifically the case in point is one of the puzzles associated with the radioactive isotope beryllium-7 whose abundance in the solar atmosphere exceeds the concentration of the stable isotope lithium-7 that is formed from beryllium-7, too, upon K-electron capture with a half-life of 53 days.

Published in	International Journal of Astrophysics and Space Science (Volume 2, Issue 6)
DOI	10.11648/j.ijass.20140206.12
Page(s)	88-92
Creative Commons	This is an Open Access article, distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution and reproduction in any medium or format, provided the original work is properly cited.
Copyright	Copyright © The Author(s), 2014. Published by Science Publishing Group

Keywords

Nuclear-Chemical Processes, Synthesis of Elements in the Solar Atmosphere

References

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Timashev Serge. (2014). Nuclear-Chemical Processes in the Solar Atmosphere. International Journal of Astrophysics and Space Science, 2(6), 88-92. https://doi.org/10.11648/j.ijass.20140206.12

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ACS Style

Timashev Serge. Nuclear-Chemical Processes in the Solar Atmosphere. Int. J. Astrophys. Space Sci. 2014, 2(6), 88-92. doi: 10.11648/j.ijass.20140206.12

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AMA Style

Timashev Serge. Nuclear-Chemical Processes in the Solar Atmosphere. Int J Astrophys Space Sci. 2014;2(6):88-92. doi: 10.11648/j.ijass.20140206.12

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@article{10.11648/j.ijass.20140206.12,
  author = {Timashev Serge},
  title = {Nuclear-Chemical Processes in the Solar Atmosphere},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {2},
  number = {6},
  pages = {88-92},
  doi = {10.11648/j.ijass.20140206.12},
  url = {https://doi.org/10.11648/j.ijass.20140206.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20140206.12},
  abstract = {The ideas put forward earlier about the initiation of nuclear processes in a low-temperature plasma as a result of interaction between electrons of high (on chemical scales) energies and nuclei are demonstrated to be helpful in clearing some debatable issues concerning the synthesis of light elements in the solar atmosphere. Specifically the case in point is one of the puzzles associated with the radioactive isotope beryllium-7 whose abundance in the solar atmosphere exceeds the concentration of the stable isotope lithium-7 that is formed from beryllium-7, too, upon K-electron capture with a half-life of 53 days.},
 year = {2014}
}

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TY  - JOUR
T1  - Nuclear-Chemical Processes in the Solar Atmosphere
AU  - Timashev Serge
Y1  - 2014/12/27
PY  - 2014
N1  - https://doi.org/10.11648/j.ijass.20140206.12
DO  - 10.11648/j.ijass.20140206.12
T2  - International Journal of Astrophysics and Space Science
JF  - International Journal of Astrophysics and Space Science
JO  - International Journal of Astrophysics and Space Science
SP  - 88
EP  - 92
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20140206.12
AB  - The ideas put forward earlier about the initiation of nuclear processes in a low-temperature plasma as a result of interaction between electrons of high (on chemical scales) energies and nuclei are demonstrated to be helpful in clearing some debatable issues concerning the synthesis of light elements in the solar atmosphere. Specifically the case in point is one of the puzzles associated with the radioactive isotope beryllium-7 whose abundance in the solar atmosphere exceeds the concentration of the stable isotope lithium-7 that is formed from beryllium-7, too, upon K-electron capture with a half-life of 53 days.
VL  - 2
IS  - 6
ER  -

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Author Information

Timashev Serge

Karpov Institute of Physical Chemistry, Moscow, Russia

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APA Style

Timashev Serge. (2014). Nuclear-Chemical Processes in the Solar Atmosphere. International Journal of Astrophysics and Space Science, 2(6), 88-92. https://doi.org/10.11648/j.ijass.20140206.12

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ACS Style

Timashev Serge. Nuclear-Chemical Processes in the Solar Atmosphere. Int. J. Astrophys. Space Sci. 2014, 2(6), 88-92. doi: 10.11648/j.ijass.20140206.12

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AMA Style

Timashev Serge. Nuclear-Chemical Processes in the Solar Atmosphere. Int J Astrophys Space Sci. 2014;2(6):88-92. doi: 10.11648/j.ijass.20140206.12

Copy | Download

@article{10.11648/j.ijass.20140206.12,
  author = {Timashev Serge},
  title = {Nuclear-Chemical Processes in the Solar Atmosphere},
  journal = {International Journal of Astrophysics and Space Science},
  volume = {2},
  number = {6},
  pages = {88-92},
  doi = {10.11648/j.ijass.20140206.12},
  url = {https://doi.org/10.11648/j.ijass.20140206.12},
  eprint = {https://article.sciencepublishinggroup.com/pdf/10.11648.j.ijass.20140206.12},
  abstract = {The ideas put forward earlier about the initiation of nuclear processes in a low-temperature plasma as a result of interaction between electrons of high (on chemical scales) energies and nuclei are demonstrated to be helpful in clearing some debatable issues concerning the synthesis of light elements in the solar atmosphere. Specifically the case in point is one of the puzzles associated with the radioactive isotope beryllium-7 whose abundance in the solar atmosphere exceeds the concentration of the stable isotope lithium-7 that is formed from beryllium-7, too, upon K-electron capture with a half-life of 53 days.},
 year = {2014}
}

Copy | Download

TY  - JOUR
T1  - Nuclear-Chemical Processes in the Solar Atmosphere
AU  - Timashev Serge
Y1  - 2014/12/27
PY  - 2014
N1  - https://doi.org/10.11648/j.ijass.20140206.12
DO  - 10.11648/j.ijass.20140206.12
T2  - International Journal of Astrophysics and Space Science
JF  - International Journal of Astrophysics and Space Science
JO  - International Journal of Astrophysics and Space Science
SP  - 88
EP  - 92
PB  - Science Publishing Group
SN  - 2376-7022
UR  - https://doi.org/10.11648/j.ijass.20140206.12
AB  - The ideas put forward earlier about the initiation of nuclear processes in a low-temperature plasma as a result of interaction between electrons of high (on chemical scales) energies and nuclei are demonstrated to be helpful in clearing some debatable issues concerning the synthesis of light elements in the solar atmosphere. Specifically the case in point is one of the puzzles associated with the radioactive isotope beryllium-7 whose abundance in the solar atmosphere exceeds the concentration of the stable isotope lithium-7 that is formed from beryllium-7, too, upon K-electron capture with a half-life of 53 days.
VL  - 2
IS  - 6
ER  -

Copy | Download