Skip to main content
Log in

Suprathermal ions in solar-wind outflows from coronal holes at 1 AU

  • Published:
Astronomy Reports Aims and scope Submit manuscript

Abstract

The energy spectra and relative abundances of 3He, 4He, C, O, and Fe ions with energies of ~0.04–2 MeV/nucleon are studied using data from the ULEIS instrument on board the ACE spacecraft obtained during quiescent periods in 2006–2012. During the unique, prolonged minimum between cycles 23 and 24, 35 quiescent periods were distnguished, during which solar-wind flows from near-equatorial coronal holes (CHs) were detected. It is shown that the C/O and Fe/O ratios for suprathermal ions correspond to the relative abundances of the corresponding thermal ions in the fast and slow (Maxwellian) solar wind (SWICS/ACE), while the 4He/O ratio exceeds the corresponding ratio in the solar wind by a factor of two. The intensities of the 3He, 4He, C, O, and Fe suprathermal ions in outflows from CHs grow with the speed of the solar wind. This indicates that, in periods ofminimumsolar activity, suprathermal ions from CHs represent a high-temperature “tail” of the solar wind. An additional flux of suprathermal helium ions may also be contributed by other external sources.

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

Access this article

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

Instant access to the full article PDF.

Similar content being viewed by others

References

  1. U. Feldman and K. G. Widing, Space Sci. Rev. 107, 665 (2003).

    Article  ADS  Google Scholar 

  2. U. Feldman and K. G. Widing, Space Sci. Rev. 130, 115 (2007).

    Article  ADS  Google Scholar 

  3. L. A. Fisk and G. Gloeckler, Space Sci. Rev. 130, 139 (2007).

    Article  ADS  Google Scholar 

  4. R. von Steiger, N. A. Schwadron, L. A. Fisk, J. Geiss, G. Gloeckler, S. Hefti, B. Wilken, R. F. Wimmer-Schweingruber, and T. H. Zurbuchen, J. Geophys. Res. 105, 27217 (2000).

    Article  ADS  Google Scholar 

  5. R. A. Mewaldt, C. M. S. Cohen, G. M. Mason, A. C. Cummings, M. I. Desai, R. A. Leske, J. Raines, E. C. Stone, M. E. Wiedenbeck, T. T. von Rosenvinge, and T. H. Zurbuchen, Space Sci. Rev. 130, 207 (2007).

    Article  ADS  Google Scholar 

  6. D. V. Reames, Space Sci. Rev. 90, 413 (1999).

    Article  ADS  Google Scholar 

  7. G. M. Mason, M. E. Wiedenbeck, J. A. Miller, J. E. Mazur, E. R. Christian, C. M. S. Cohen, A. C. Cummings, J. R. Dwyer, R. E. Gold, S. M. Krimigis, R. A. Leske, R. A. Mewaldt, P. L. Slocum, E. C. Stone, and T. T. von Rosenvinge, Astrophys. J. 574, 1039 (2002).

    Article  ADS  Google Scholar 

  8. G. Gloeckler and J. Geiss, Space Sci. Rev. 130, 139 (2007).

    Article  ADS  Google Scholar 

  9. G. M. Mason, R. A. Leske, M. I. Desai, C. M. S. Cohen, J. R. Dwyer, J. E. Mazur, R. A. Mewaldt, R. E. Gold, and S. M. Krimigis, Astrophys. J. 678, 1458 (2008).

    Article  ADS  Google Scholar 

  10. S.W. Kahlerý, A. J. Tylka, and D. V. Reames, Astrophys. J. 701, 561 (2009).

    Article  ADS  Google Scholar 

  11. M. I. Desai, G. M. Mason, J. E. Mazur, and J. R. Dwyer, Astrophys. J. 645, L81 (2006).

    Article  ADS  Google Scholar 

  12. M. I. Desai, G. M. Mason, R. E. Gold, S.M. Krimigisý, C. M. S. Cohen, R. A. Mewaldt, J. E. Mazur, and J. R. Dwyer, Astrophys. J. 649, 470 (2006).

    Article  ADS  Google Scholar 

  13. M.I.Desai, M.A.Dayeh, and G.M.Mason, in Proceedings of the 31st International Cosmic Ray Conference, Lodz, Poland, July 7–15, 2009, paper ID 0061.

  14. M. A. Dayeh, M. I. Desai, J. R. Dwyer, H. K. Rassoul, G. M. Mason, and J. E. Mazur, Astrophys. J. 693, 1588 (2009).

    Article  ADS  Google Scholar 

  15. M. A. Zel’dovich, Yu. I. Logachev, and G. M. Surova, Astron. Rep. 55, 374 (2011).

    Article  ADS  Google Scholar 

  16. M. A. Zel’dovich, V. N. Ishkov, Yu. I. Logachev, and K. Kecskemety, Bull. Russ. Acad. Sci.: Phys. 75, 776 (2011).

    Article  Google Scholar 

  17. V. N. Ishkov, M. A. Zeldovich, K. Kecskemety, and Yu. I. Logachev, Adv. Space Res. 50, 757 (2012).

    Article  ADS  Google Scholar 

  18. M. A. Zel’dovich, Yu. I. Logachev, G.M. Surova, and K. Kecskemetý, Astron. Rep. 58, 399 (2014).

    Article  ADS  Google Scholar 

  19. G. M. Mason, R. E. Gold, S. M. Krimigis, J. E. Mazur, G. B. Andrews, K. A. Daley, J. R. Dwyer, K. F. Heuerman, T. L. James, M. J. Kennedy, T. Lefevere, E. H. Malcolm, B. Tossman, and P.H. Walpole, Space Sci. Rev. 86, 409 (1998).

    Article  ADS  Google Scholar 

  20. G. Gloeckler, Space Sci. Rev. 86, 497 (1998).

    Article  ADS  Google Scholar 

  21. L. Zhao, T. H. Zurbuchen, and L. A. Fisk, Geophys. Res. Lett. 36, L14104 (2009).

    Article  ADS  Google Scholar 

  22. S. T. Lepri, E. Landi, and T.H. Zurbuchen, Astrophys. J. 768, 94 (2013).

    Article  ADS  Google Scholar 

  23. Y. K. Ko, K. Muglach, Y. M. Wang, P. R. Young, and S. T. Lepri, Astrophys. J. 787, 121 (2014).

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to M. A. Zel’dovich.

Additional information

Original Russian Text © M.A. Zel’dovich, Yu.I. Logachev, G.M. Surova, K. Kecskemety, I.S. Veselovskii, 2016, published in Astronomicheskii Zhurnal, 2016, Vol. 93, No. 7, pp. 675–681.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Zel’dovich, M.A., Logachev, Y.I., Surova, G.M. et al. Suprathermal ions in solar-wind outflows from coronal holes at 1 AU. Astron. Rep. 60, 687–693 (2016). https://doi.org/10.1134/S1063772916070106

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1134/S1063772916070106

Navigation