Skip to main content
Log in

Investigation of the Geoeffectiveness of CMEs Associated with IP Type II Radio Bursts

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

We perform a statistical analysis of the geoeffectiveness of coronal mass ejections (CMEs) that are associated with interplanetary (IP) type II bursts in Solar Cycle 23 during the period 1997 – 2008. About 47 % (109 out of 232) of IP type II bursts are found to be associated with geomagnetic storms. Of these 47 %, 27 % are associated with moderate, 14 % with intense, and 6 % with severe geomagnetic storms. We find that the IP type II bursts and their corresponding end frequencies can be used as indicators of CME geoeffectiveness: the lower the type II burst end frequency, the higher the possibility of having a stronger storm. In addition, we show that various combinations of CME remote-sensing and IP type II parameters can be used to improve geomagnetic storm forecasting.

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.

Figure 1
Figure 2
Figure 3
Figure 4
Figure 5
Figure 6

Similar content being viewed by others

Notes

  1. http://cdaw.gsfc.nasa.gov/CME_list/radio/waves_type2.html .

  2. http://cdaw.gsfc.nasa.gov/CME_list/index.html .

  3. http://www.ngdc.noaa.gov/stp/space-weather/solar-data/solar-features/solar-flares/x-rays/goes/ .

  4. http://wdc.kugi.kyoto-u.ac.jp/dst_final/index.html .

References

  • Bougeret, J.-L., Kaiser, M.L., Kellogg, P.J., Manning, R., Goetz, K., Monson, S.J., Monge, N., Friel, L., Meetre, C.A., Perche, C., Sitruk, L., Hoang, S.: 1995, Waves: The radio and plasma wave investigation on the wind spacecraft. Space Sci. Rev. 71, 231. DOI . ADS .

    Article  ADS  Google Scholar 

  • Burlaga, L., Sittler, E., Mariani, F., Schwenn, R.: 1981, Magnetic loop behind an interplanetary shock – Voyager, Helios, and IMP 8 observations. J. Geophys. Res. 86, 6673. DOI . ADS .

    Article  ADS  Google Scholar 

  • Chen, Y., Du, G., Feng, L., Feng, S., Kong, X., Guo, F., Wang, B., Li, G.: 2014, A solar type II radio burst from coronal mass ejection-coronal ray interaction: Simultaneous radio and extreme ultraviolet imaging. Astrophys. J. 787, 59. DOI . ADS .

    Article  ADS  Google Scholar 

  • Dumbović, M., Devos, A., Vršnak, B., Sudar, D., Rodriguez, L., Ruždjak, D., Leer, K., Vennerstrøm, S., Veronig, A.: 2015, Geoeffectiveness of coronal mass ejections in the SOHO era. Solar Phys. 290, 579. DOI . ADS .

    Article  ADS  Google Scholar 

  • Gilbert, H.R., Holzer, T.E., Burkepile, J.T., Hundhausen, A.J.: 2000, Active and eruptive prominences and their relationship to coronal mass ejections. Astrophys. J. 537, 503. DOI . ADS .

    Article  ADS  MATH  Google Scholar 

  • Gonzalez, W.D., Joselyn, J.A., Kamide, Y., Kroehl, H.W., Rostoker, G., Tsurutani, B.T., Vasyliunas, V.M.: 1994, What is a geomagnetic storm? J. Geophys. Res. 99, 5771. DOI . ADS .

    Article  ADS  MATH  Google Scholar 

  • Gopalswamy, N., Yashiro, S., Akiyama, S.: 2007, Geoeffectiveness of halo coronal mass ejections. J. Geophys. Res. 112, 6112. DOI . ADS .

    Article  Google Scholar 

  • Gopalswamy, N., Yashiro, S., Kaiser, M.L., Howard, R.A., Bougeret, J.-L.: 2001, Characteristics of coronal mass ejections associated with long-wavelength type II radio bursts. J. Geophys. Res. 106, 29219. DOI . ADS .

    Article  ADS  Google Scholar 

  • Gopalswamy, N., Aguilar-Rodriguez, E., Yashiro, S., Nunes, S., Kaiser, M.L., Howard, R.A.: 2005a, Type II radio bursts and energetic solar eruptions. J. Geophys. Res. 110, 12. DOI . ADS .

    Google Scholar 

  • Gopalswamy, N., Lara, A., Manoharan, P.K., Howard, R.A.: 2005b, An empirical model to predict the 1-AU arrival of interplanetary shocks. Adv. Space Res. 36, 2289. DOI . ADS .

    Article  ADS  Google Scholar 

  • Gopalswamy, N., Yashiro, S., Michalek, G., Stenborg, G., Vourlidas, A., Freeland, S., Howard, R.: 2009, The SOHO/LASCO CME catalog. Earth Moon Planets 104, 295. DOI . ADS .

    Article  ADS  MATH  Google Scholar 

  • Gosling, J.T.: 1993, The solar flare myth. J. Geophys. Res. 98, 18937. DOI . ADS .

    Article  ADS  Google Scholar 

  • Gosling, J.T.: 1997, Coronal mass ejections: An overview. In: Crooker, N., Joselyn, J.A., Feynman, J. (eds.) Coronal Mass Ejections, AGU Geophys. Monograph 99, 9. DOI . ADS .

    Chapter  Google Scholar 

  • Gosling, J.T., McComas, D.J., Phillips, J.L., Bame, S.J.: 1991, Geomagnetic activity associated with Earth passage of interplanetary shock disturbances and coronal mass ejections. J. Geophys. Res. 96, 7831. DOI . ADS .

    Article  ADS  Google Scholar 

  • Hudson, H.S., Lemen, J.R., St. Cyr, O.C., Sterling, A.C., Webb, D.F.: 1998, X-ray coronal changes during halo CMEs. Geophys. Res. Lett. 25, 2481. DOI . ADS .

    Article  ADS  Google Scholar 

  • Kong, X., Chen, Y., Guo, F., Feng, S., Wang, B., Du, G., Li, G.: 2015, The possible role of coronal streamers as magnetically closed structures in shock-induced energetic electrons and metric type II radio bursts. Astrophys. J. 798, 81. DOI . ADS .

    Article  ADS  MATH  Google Scholar 

  • Lara, A., Gopalswamy, N., Nunes, S., Muñoz, G., Yashiro, S.: 2003, A statistical study of CMEs associated with metric type II bursts. Geophys. Res. Lett. 30, 8016. DOI . ADS .

    Article  ADS  Google Scholar 

  • Leblanc, Y., Dulk, G.A., Bougeret, J.-L.: 1998, Tracing the electron density from the corona to 1 AU. Solar Phys. 183, 165. DOI . ADS .

    Article  ADS  Google Scholar 

  • Loewe, C.A., Prölss, G.W.: 1997, Classification and mean behavior of magnetic storms. J. Geophys. Res. 102, 14209. DOI . ADS .

    Article  ADS  Google Scholar 

  • Ma, S., Raymond, J.C., Golub, L., Lin, J., Chen, H., Grigis, P., Testa, P., Long, D.: 2011, Observations and interpretation of a low coronal shock wave observed in the EUV by the SDO/AIA. Astrophys. J. 738, 160. DOI . ADS .

    Article  ADS  Google Scholar 

  • Michalek, G., Gopalswamy, N., Lara, A., Yashiro, S.: 2006, Properties and geoeffectiveness of halo coronal mass ejections. Space Weather 4, 10003. DOI . ADS .

    Article  ADS  Google Scholar 

  • Reiner, M.J., Kaiser, M.L.: 1999, High-frequency type II radio emissions associated with shocks driven by coronal mass ejections. J. Geophys. Res. 104, 16979. DOI . ADS .

    Article  ADS  Google Scholar 

  • Schwenn, R., dal Lago, A., Huttunen, E., Gonzalez, W.D.: 2005, The association of coronal mass ejections with their effects near the Earth. Ann. Geophys. 23, 1033. DOI . ADS .

    Article  ADS  Google Scholar 

  • Srivastava, N., Gonzalez, W.D., Gonzalez, A.L.C., Masuda, S.: 1998, On the solar origins of intense geomagnetic storms observed during 6 – 11 March 1993. Solar Phys. 183, 419. DOI . ADS .

    Article  ADS  MATH  Google Scholar 

  • Sterling, A.C., Hudson, H.S., Thompson, B.J., Zarro, D.M.: 2000, Yohkoh SXT and SOHO EIT observations of sigmoid-to-arcade evolution of structures associated with halo coronal mass ejections. Astrophys. J. 532, 628. DOI . ADS .

    Article  ADS  Google Scholar 

  • Valach, F., Bochníček, J., Hejda, P., Revallo, M.: 2014, Strong geomagnetic activity forecast by neural networks under dominant southern orientation of the interplanetary magnetic field. Adv. Space Res. 53, 589. DOI . ADS .

    Article  ADS  Google Scholar 

  • Vasanth, V., Umapathy, S.: 2013, A statistical study on CMEs associated with DH-type-II radio bursts based on their source location (Limb and disk events). Solar Phys. 282, 239. DOI . ADS .

    Article  ADS  Google Scholar 

  • Vasanth, V., Umapathy, S., Vršnak, B., Anna Lakshmi, M.: 2011, Characteristics of type-II radio bursts associated with flares and CMEs. Solar Phys. 273, 143. DOI . ADS .

    Article  ADS  Google Scholar 

  • Verbanac, G., Živković, S., Vršnak, B., Bandić, M., Hojsak, T.: 2013, Comparison of geoeffectiveness of coronal mass ejections and corotating interaction regions. Astron. Astrophys. 558, A85. DOI . ADS .

    Article  ADS  Google Scholar 

  • Wang, Y.M., Ye, P.Z., Wang, S., Zhou, G.P., Wang, J.X.: 2002, A statistical study on the geoeffectiveness of Earth-directed coronal mass ejections from March 1997 to December 2000. J. Geophys. Res. 107, 1340. DOI . ADS .

    Article  Google Scholar 

  • Webb, D.F.: 2002, CMEs and the solar cycle variation in their geoeffectiveness. In: Wilson, A. (ed.) From Solar Min to Max: Half a Solar Cycle with SOHO, ESA SP 508, 409. ADS .

    Google Scholar 

  • Wild, J.P., McCready, L.L.: 1950, Observations of the spectrum of high-intensity solar radiation at metre wavelengths. I. The apparatus and spectral types of solar burst observed. Aust. J. Sci. Res., Ser. A 3, 387. ADS .

    ADS  Google Scholar 

  • Yashiro, S., Gopalswamy, N., Michalek, G., St. Cyr, O.C., Plunkett, S.P., Rich, N.B., Howard, R.A.: 2004, A catalog of white light coronal mass ejections observed by the SOHO spacecraft. J. Geophys. Res. 109, 7105. DOI . ADS .

    Article  Google Scholar 

  • Yermolaev, Y.I., Yermolaev, M.Y.: 2006, Statistic study on the geomagnetic storm effectiveness of solar and interplanetary events. Adv. Space Res. 37, 1175. DOI . ADS .

    Article  ADS  Google Scholar 

  • Zarro, D.M., Sterling, A.C., Thompson, B.J., Hudson, H.S., Nitta, N.: 1999, SOHO EIT observations of extreme-ultraviolet “Dimming” associated with a halo coronal mass ejection. Astrophys. J. Lett. 520, L139. DOI . ADS .

    Article  ADS  Google Scholar 

  • Zhang, G., Burlaga, L.F.: 1988, Magnetic clouds, geomagnetic disturbances, and cosmic ray decreases. J. Geophys. Res. 93, 2511. DOI . ADS .

    Article  ADS  Google Scholar 

  • Zhang, J., Dere, K.P., Howard, R.A., Bothmer, V.: 2003, Identification of solar sources of major geomagnetic storms between 1996 and 2000. Astrophys. J. 582, 520. DOI . ADS .

    Article  ADS  Google Scholar 

  • Zhang, J., Richardson, I.G., Webb, D.F., Gopalswamy, N., Huttunen, E., Kasper, J.C., Nitta, N.V., Poomvises, W., Thompson, B.J., Wu, C.-C., Yashiro, S., Zhukov, A.N.: 2007, Solar and interplanetary sources of major geomagnetic storms (\(\mathrm{Dst} \leq-100~\mbox{nT}\)) during 1996 – 2005. J. Geophys. Res. 112, 10102. DOI . ADS .

    Article  Google Scholar 

Download references

Acknowledgements

The authors gratefully acknowledge the various online data centers of NOAA and NASA for providing the data. We express our thanks to the Wind/WAVES teams for providing the Type II catalog, and the LASCO CME catalog we used is generated and maintained by the Center for Solar Physics and Space Weather, The Catholic University of America in cooperation with the Naval Research Laboratory and NASA. We also express our thanks to the world data center in Kyoto for minimum Dst Values and NSSDCs OMNI web services for interplanetary magnetic field data. This work was supported by grants NSBRSF 2012CB825601, NNSFC 41274175, 41331068, U1431103 and Natural Science Foundation of Shandong Province (ZR2014DQ001).

Author information

Authors and Affiliations

Authors

Corresponding author

Correspondence to Y. Chen.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Vasanth, V., Chen, Y., Kong, X.L. et al. Investigation of the Geoeffectiveness of CMEs Associated with IP Type II Radio Bursts. Sol Phys 290, 1815–1826 (2015). https://doi.org/10.1007/s11207-015-0713-0

Download citation

  • Received:

  • Accepted:

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1007/s11207-015-0713-0

Keywords

Navigation