Skip to main content
SpringerLink
Log in

Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24

  • Published:
Bulletin of the Lebedev Physics Institute Aims and scope Submit manuscript

Abstract

The interaction of the interplanetary coronal mass ejection (ICME) and the high-speed solar wind flux (HSSWF) associated with the coronal hole (CH) is considered. By the examples of two events at the maximum of solar cycle 24 from June 4 to June 16 and from June 30 to July 10, 2012 it is shown that the temperature-dependent parameters of the SW ionic composition appear closer to the values in the HSSWF than in the ICME due to mixing of fluxes in the corona when the ICME source is near the CH boundary.

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. ENLIL Solar Wind Prediction–URL: http://helioweather.net/

  2. A. A. Mohamed, N. Gopalswamy, S. Yashiro, et al., J. Geophys. Res. 117, A01103 (2012).

    Article  Google Scholar 

  3. B. E. Wood, C.-C. Wu, A. P. Rouillard, et al., Astrophys. J. 755, 43 (2012).

    Article  ADS  Google Scholar 

  4. N. Gopalswamy, P. Mäkelä, H. Xie, et al., J. Geophys. Res. 114, A00A22 (2009).

    ADS  Google Scholar 

  5. P. Mäkelä, N. Gopalswamy, H. Xie, et al., Solar Phys. 284, 59 (2013).

    Article  ADS  Google Scholar 

  6. Near-Earth Interplanetary Coronal Mass Ejections Since January 1996, compiled by Ian Richardson and Hilary Cane–URL: http://www.srl.caltech.edu/ACE/ASC/DATA/level3/icmetable2.htm

  7. H. V. Cane and I. G. Richardson, J. Geophys. Res. 108, SSH 6–1 (2003).

    Google Scholar 

  8. I. G. Richardson and H. V. Cane, Solar Phys. 264, 189 (2010).

    Article  ADS  Google Scholar 

  9. N. Gopalswamy, P. Mäkelä, S. Akiyama, et al., Solar Phys. 284, 17 (2013).

    Article  ADS  Google Scholar 

  10. CDAWData Center. SOHO LASCO CME CATALOG–URL: http://cdaw.gsfc.nasa.gov/CME−list/

  11. George Mason University Space Weather Lab. Solar Eruptive Event Detection System–URL: http://helio.gmu.edu/seeds/secchi.php

  12. Solar Dynamics Observatory. AIA/HMI Browse Data–URL: http://sdo.gsfc.nasa.gov/

  13. A software package for “Computer Aided CME Tracking” (CACTUS)–URL: http://sidc.oma.be/cactus/

  14. U. Feldman, E. Landi, and N. A. Schwadron, J. Geophys. Res.: Space Phys. 110, A07109 (2005).

    Article  ADS  Google Scholar 

  15. The ACE Science Center (ASC). ACE Level 2 (Verified) Data–URL: http://www.srl.caltech.edu/ACE/ASC/level2/index.html

  16. U. Feldman, Physica Scripta 46, 202 (1992).

    Article  ADS  Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Lebedev Physical Institute, Russian Academy of Sciences, Leninskii pr. 53, Moscow, 119991, Russia

    D. G. Rodkin & V. A. Slemzin

  2. Skobeltsyn Institute of Nuclear Physics, Moscow State University, Moscow, 119991, Russia

    Yu. S. Shugai & V. A. Veselovskii

Authors
  1. D. G. Rodkin
    View author publications

    You can also search for this author in PubMed Google Scholar

  2. Yu. S. Shugai
    View author publications

    You can also search for this author in PubMed Google Scholar

  3. V. A. Slemzin
    View author publications

    You can also search for this author in PubMed Google Scholar

  4. V. A. Veselovskii
    View author publications

    You can also search for this author in PubMed Google Scholar

Corresponding author

Correspondence to D. G. Rodkin.

Additional information

Original Russian Text © D.G. Rodkin, Yu.S. Shugai, V.A. Slemzin, I.S. Veselovskii, 2016, published in Kratkie Soobshcheniya po Fizike, 2016, Vol. 43, No. 9, pp. 44–49.

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Rodkin, D.G., Shugai, Y.S., Slemzin, V.A. et al. Interaction of high-speed and transient fluxes of solar wind at the maximum of solar cycle 24. Bull. Lebedev Phys. Inst. 43, 287–290 (2016). https://doi.org/10.3103/S1068335616090062

Download citation

  • Received:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.3103/S1068335616090062

Keywords

Search

Navigation