Skip to main content
SpringerLink
Log in

Changes in the solar wind’s isotope component, due to interaction between solar flare particles and the photosphere

  • Proceedings of the 34th All-Russian Conference on Cosmic Rays
  • Published:
Bulletin of the Russian Academy of Sciences: Physics Aims and scope

Abstract

Possible mechanisms responsible for changes in the solar wind’s isotope component caused by interaction between solar flare protons and helium isotopes with photospheric nuclei are considered. Depth profiles of the rates of 6Li, 7Li, 7Be, 14C production in the solar atmosphere are simulated using the GEANT4 software package. It is concluded that anomalous isotopic compositions of the solar wind relative to the average values can form during the coronal mass ejections.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Similar content being viewed by others

References

  1. Chaussidon, M., et al., Nature, 1999, vol. 402, p. 270.

    Article  ADS  Google Scholar 

  2. Jull, T., et al., Geochim. Cosmochim. Acta, 1998, vol. 62, p. 3025.

    Article  ADS  Google Scholar 

  3. Asplund, M., et al., Annu. Rev. Astron. Astrophys., 2009, vol. 47, p. 481.

    Article  ADS  Google Scholar 

  4. Ramaty, R., et al., Astrophys. J. Lett., 2000, vol. 534, p. L207.

    Article  ADS  Google Scholar 

  5. Kotov, Yu.D., et al., Astrophys. J., 1996, vol. 473, p. 514.

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Ioffe Institute, Russian Academy of Sciences, St. Petersburg, 194021, Russia

    G. I. Vasilyev & A. K. Pavlov

  2. St. Petersburg State Polytechnic University, St. Petersburg, 195251, Russia

    V. M. Ostryakov, A. K. Pavlov & M. E. Chakchurina

Authors
  1. G. I. Vasilyev
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. V. M. Ostryakov
    View author publications

    You can also search for this author in PubMed Google Scholar

  3. A. K. Pavlov
    View author publications

    You can also search for this author in PubMed Google Scholar

  4. M. E. Chakchurina
    View author publications

    You can also search for this author in PubMed Google Scholar

Corresponding author

Correspondence to G. I. Vasilyev.

Additional information

Original Russian Text © G.I. Vasilyev, V.M. Ostryakov, A.K. Pavlov, M.E. Chakchurina, 2017, published in Izvestiya Rossiiskoi Akademii Nauk, Seriya Fizicheskaya, 2017, Vol. 81, No. 2, pp. 162–164.

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Vasilyev, G.I., Ostryakov, V.M., Pavlov, A.K. et al. Changes in the solar wind’s isotope component, due to interaction between solar flare particles and the photosphere. Bull. Russ. Acad. Sci. Phys. 81, 143–145 (2017). https://doi.org/10.3103/S1062873817020435

Download citation

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.3103/S1062873817020435

Search

Navigation