Erratum: Coronal mass ejection geoeffectiveness depending on field orientation and interplanetary coronal mass ejection classification (Journal of Geophysical Research 111 (A05102) DOI:10.1029/2005JA011445);Coronal mass ejection geoeffectiveness depending on field orientation and interplanetary coronal mass ejection classification

Journal of Geophysical Research: Space Physics

Volumn 111, Issue 5, 2006, Pages

  Kang, Seung Mi ^a,b   Moon, Y J ^b   Cho, K S ^b   Kim, Yeon Han ^b   Park, Y D ^b   Baek, Ji Hye ^b   Chang, Heon Young ^a  

^a Kyungpook National University   (South Korea)

^b Korea Astronomy and Space Science Institute (KASI)   (South Korea)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33947707824     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2006JA012018     Document Type: Erratum

References (29)

1. Baek, J.-H., D.-Y. Lee, K. C. Kim, C. R. Choi, Y. D. Park, Y.-J. Moon, and K.-S. Cho (2005), A statistical analysis of solar wind dynamic pressure pulses during geomagnetic storms, J. Astron. Space Sci., 22, 419.
2. Bothmer, V., and D. M. Rust (1997), The field configuration of magnetic clouds and the solar cycle, in Coronal Mass Ejections, Geophys. Monogr. Ser., vol. 99, edited by N. Crooker, J. A. Joselyn, and J. Feynman, pp. 139-146, AGU, Washington, D.C.
3. Bothmer, V., and R. Schwenn (1994), Eruptive prominences as sources of magnetic clouds in the solar wind, Space Sci. Rev., 70, 215.
4. Burlaga, L. F. (1995), Interplanetary Magnetohydrodynamics, Oxford Univ. Press, New York.
5. Burlaga, L. F., R. M. Skoug, C. W. Smith, D. F. Webb, T. H. Zurbuchen, and A. Reinard (2001), Fast ejecta during the ascending phase of solar cycle 23: ACE observations, 1998-1999, J. Geophys. Res., 106, 20,957.
6. Cane, H. V., and I. G. Richardson (2003), Interplanetary coronal mass ejections in the near-Earth solar wind during 1996-2002, J. Geophys. Res., 108(A4), 1156, doi:10.1029/2002JA009817.
7. Cho, K.-S., Y.-J. Moon, M. Dryer, C. D. Fry, Y.-D. Park, and K.-S. Kim (2003), A statistical comparison of interplanetary shock and CME propagation models, J. Geophys. Res., 108(A12), 1445, doi:10.1029/2003JA010029.
8. Fenrich, R. R., and J. G. Luhmann (1998), Geomagnetic reaponse to magnetic clouds of differents polarity, Geophys. Res. Lett., 25, 2999.
9. Fry, C. D., M. Dryer, Z. Smith, W. Sun, C. S. Deehr, and S.-I. Akasofu (2003), Forecasting solar wind structures and shock arrival times using an ensenble of model, J. Geophys. Res., 108(A2), 1070, doi:10.1029/ 2002JA009474.
10. Gopalswamy, N., A. Lara, S. Yashiro, M. L. Kaiser, and R. A. Howard (2001), Predicting the 1-AU arrival times of coronal mass ejections, J. Geophys. Res., 106, 29,207.
11. Gosling, J. T. (1990), Coronal mass ejections and magnetic flux ropesin interplanetary space, in Physics of Magnetic Flux Ropes, Geophys. Monogr. Ser, vol. 58, edited by C. T. Russell, E. R. Priest, and L. C. Lee, pp. 343-364, AGU, Washington, D.C.
12. Jackson, B. V., P. P. Hick, and A. Buffington (2003), Time-dependent tomography of heliosheric structures using IPS and Thomson scattering observations, in Proceedings of ISCS 2003 Symposium on Solar Variability as an Input to the Earth's Environment, ESA SP-535, edited by A. Wilson, p. 823, Eur. Space Agency, Paris.
13. Kim, R.-S., K.-S. Cho, Y.-J. Moon, Y.-H. Kim, Y. Yi, M. Dryer, S.-C. Bong, and Y.-D. Park (2005), Forecast evaluation of the CME geoeffectiveness using halo CMEs from 1997 to 2003, J. Geophys. Res., 110, A11104, doi:10.1029/2005JA011218.
14. Leamon, R. J., R. C. Canfield, and A. A. Pevtsov (2002), Properties of magnetic clouds and geomagnetic storms associated with eruption of coronal sigmoids, J. Geophys. Res., 107(A9), 1234, doi:10.1029/2001JA000313.
15. Manoharan, P. K., N. Gopalswamy, S. Yashiro, A. Lara, G. Michalek, and R. A. Howard (2004), Influence of coronal mass ejection interaction on propagation of interplanetary shocks, J. Geophys. Res., 109, A06109, doi:10.1029/2003JA010300.
16. McAllister, H., and S. F. Martin (2000), The essential role of magnetic reconnection in erupting prominences and CMEs, Adv. Space Res., 26, 469.
17. Moon, Y.-J., K.-S. Cho, M. Dryer, Y.-H. Kim, S.-C. Bong, J. Chae, and Y. D. Park (2005), New geoeffective parameters of very fast halo coronal mass ejections, Astrophys. J., 624, 414.
18. Pevtsov, A. A., and R. C. Canfield (2001), Solar magnetic fields and geomagnetic events, J. Geophys. Res., 106, 25,191.
19. Rust, D. M. (1994), Spawning and shelding helical magnetic fields in the solar atmosphere, Geophys. Res. Lett., 21, 241.
20. Smith, Z., M. Dryer, E. Ort, and W. Murtagh (2000), Performance of interplanetary shock prediction models: STOA and ISPM, J. Atmos. Sol. Terr. Phys., 62, 1265.
21. Song, H., V. B. Yurchyshyn, and H. Wang (2005), Towards real-time automated prediction of geo-magnetic storms based on observations of source regions of halo CMEs, Eos Trans. AGU, 8618, Spring Meet Suppl., Abstract SP23A-01.
22. Wang, Y. M., P. Z. Ye, S. Wang, G. P. Zhou, and J. X. Wang (2002), A statistical study on the geoeffectiveness of Earth-directed coronal mass ejections from March 1997 to December 2000, J. Geophys. Res., 107(A11), 1340, doi:10.1029/2002JA009244.
23. Wu, C. C., and R. P. Lepping (2002a), Effects of magnetic clouds on the occurance of geomagnetic storms: The first 4 years of Wind, J. Geophys. Res., 107(A10), 1314, doi:10.1029/2001JA000161.
24. Wu, C. C., and R. P. Lepping (2002b), Effect of solar wind velocity on magnetic cloud-associated magnetic storm intensity, J. Geophys. Res., 107(A11), 1346, doi:10.1029/2002JA009396.
25. Yurchyshyn, V. B., H. Wang, P. R. Goode, and Y. Deug (2001), Orientation of the magnetic fields in interplanetary flux ropes and solar filaments, Astrophys. J., 563, 381.
26. Yurchyshyn, V. B., H. Wang, and V. Abramenko (2003), How directions and helicity of erupted solar magnetic fields define geoeffectiveness of coronal mass ejections, Adv. Space Res., 32, 10.
27. Yurchyshyn, V. B., H. Wang, and V. Abramenko (2004), Correlation between speeds of coronal mass ejections and the intensity of geomagnetic storms, Space Weather, 2, S02001, doi:10.1029/2003SW000020.
28. Yurchyshyn, V., Q. Hu, and V. Abramenko (2005), Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta, Space Weather, 3, S08C02,doi:10.1029/2004SW000124.
29. Zhang, G., and L. F. Burlaga (1988), Magnetic clouds, geomagnetic disturbances, and cosmic ray decreases, J. Geophys. Res., 93, 2511.