Citation: | Xie Yanqiong, Zhang Ying, Du Dan. Predicting whether an interplanetary shock will encounter the Earth by using solar and interplanetary parameters[J]. Chinese Journal of Space Science, 2014, 34(1): 11-23. doi: 10.11728/cjss2014.01.011 |
[1] |
Feng Xueshang, Xiang Changqing, Zhong Dingkun. The state-of-art of three-dimensional numerical study for corona-interplanetary process of solar storms[J]. Sci. China: D, 2011, 41(1):1-28. In Chinese (冯学尚, 向长青, 钟鼎坤. 太阳风暴的日冕行星际过程三维数值研究进展[J]. 中国科学: D, 2011, 41(1):1-28)
|
[2] |
Fry C D, Dryer M, Smith Z, et al. Forecasting solar wind structures and shock arrival times using an ensemble of models[J]. J. Geophys. Res., 2003, 108(A2):1070, doi: 10.1029/2002JA009474
|
[3] |
McKenna-Lawlor S M P, Dryer M, Kartalev M D, et al. Near realtime predictions of the arrival at Earth of flare-related shocks during Solar Cycle 23[J]. J. Geophys. Res., 2006, 111, A11103, doi: 10.1029/2005JA011162
|
[4] |
Smith Z K, Dryer M, McKenna-Lawlor S M P, et al. Operational validation of HAFv2's predictions of interplanetary shock arrivals at Earth: Declining phase of Solar Cycle 23[J]. J. Geophys. Res., 2009, 114, A05106, doi: 10.1029/2008JA013836
|
[5] |
Zhao X H, Feng X S, Wu C C. Characteristics of solar flares associated with interplanetary shock or nonshock events at Earth[J]. J. Geophys. Res., 2006, 111, A09103, doi: 10.1029/2006JA011784
|
[6] |
Zhao X H, Feng X S, Wu C C. Influence of solar flare's location and heliospheric current sheet on the associated shock's arrival at Earth[J]. J. Geophys. Res., 2007, 112, A06107, doi: 10.1029/2006JA012205
|
[7] |
Yermolaev Y I, Yermolaev M Y, Zastenker G N, et al. Statistical studies of geomagnetic storm dependencies on solar and interplanetary events: a review[J]. Planet. Space Sci., 2005, 53:189-196
|
[8] |
Cane H V, Richardson I G, Cyr O C St. Coronal mass ejections, interplanetary ejecta and geomagnetic storms[J]. Geophys. Res. Lett., 2000, 27(21):3591-3594
|
[9] |
Wang Y M, Ye P Z, Wang S, et al. A statistical study on the geoeffectiveness of Earth-directed coronal mass ejections from March 1997 to December 2000[J]. J. Geophys. Res., 2002, 107(A11): 1340, doi: 10.1029/2002JA009244
|
[10] |
Srivastava N, Venkatakrishnan P. Solar and interplanetary sources of major geomagnetic storms during 1996—2002[J]. J. Geophys. Res., 2004, 109, A10103, doi: 10.1029/2003JA010175
|
[11] |
Gopalswamy N, Yashiro S, Akiyama S. Geoeffectiveness of halo coronal mass ejections[J]. J. Geophys. Res., 2007, 112, A06112, doi: 10.1029/2006JA012149
|
[12] |
Moon Y J, Cho K S, Dryer M, et al. New geoeffective parameters of very fast halo coronal mass ejections[J]. Astrophys. J., 2005, 624:414-419
|
[13] |
Kang S M, Moon Y J, Cho K S, et al. Coronal mass ejection geoeffectiveness depending on field orientation and interplanetary coronal mass ejection classification[J]. J. Geophys. Res., 2006, 111, A05102, doi: 10.1029/2005JA011445
|
[14] |
Shen C L, Wang Y M, Gui B, et al. Kinematic Evolution of A Slow CME in Corona Viewed by STEREO-B on October 8, 2007[J]. Solar Phys., 2011, 269:389-400
|
[15] |
Song H, Yurchyshyn V, Yang G, et al. The automatic predictability of super geomagnetic storms from Halo CMEs associated with large solar flares[J]. Solar Phys., 2006, 238:141-165
|
[16] |
Hu Y Q, Jia X Z. Interplanetary shock interaction with the heliospheric current sheet and its associated structures[J]. J. Geophys. Res., 2001, 106:29299-29304
|
[17] |
Wei F S, Dryer M. Propagation of solar flare-associated interplanetary shock waves in the heliospheric meridional plane[J]. Solar Phys., 1991, 132:373-394
|
[18] |
Xie Y Q, Wei F S, Xiang C Q, et al. The effect of heliospheric current sheet on interplanetary shocks[J]. Solar Phys., 2006, 238(2):377-390
|
[19] |
Gopalswamy N, Makela P, Xie H, et al. CME interactions with coronal holes and their interplanetary consequences[J]. J. Geophys. Res., 2009, 114, A00A22, doi: 10.1029/2008JA013686
|
[20] |
Gopalswamy N, Xie H, Makela P, et al. Interplanetary shocks lacking type Ⅱ radio bursts[J]. Astrophys. J., 2010, 710:1111-1126
|
[21] |
Xie H, Gopalswamy N, Cyr O C St. Near-Sun flux rope structure of CMEs[J]. Solar Phys., 2013, 284(1):47-58
|
[22] |
Mohamed A A, Gopalswamy N, Yashiro S, et al. The relation between coronal holes and coronal mass ejections during the rise, maximum, and declining phases of Solar Cycle 23[J]. J. Geophys. Res., 2012, 117, 1103, doi: 10.1029/2011JA016589
|
[23] |
Smart D F, Shea M A. A simplified model for timing the arrival of solar flare-initiated shocks[J]. J. Geophys. Res., 1985, 90(A1):183-190
|
[24] |
Smith Z K, Dryer M. The interplanetary shock propagation model: A model for predicting solar-flare-caused geomagnetic sudden impulses based on the 2-1/2D MHD numerical simulation results from the interplanetary global model[R]. NOAA-TM-ERL-SEL-89, 1995
|
[25] |
Fry C D, Sun W, Deehr C S, et al. Improvements to the HAF solar wind model for space weather predictions[J]. J. Geophys. Res., 2001, 106:20985-21002
|
[26] |
Feng X S, Zhang Y, Yang L P, et al. An operational method for shock arrival time prediction by one-dimensional CESE-HD solar wind model[J]. J. Geophys. Res., 2009, 114, A10103, doi: 10.1029/2009JA014385
|
[27] |
Feng X S, Zhang Y, Sun W, et al. A practical database method for predicting arrivals of average interplanetary shocks at Earth[J]. J. Geophys. Res., 2009, 114, A01101, doi: 10.1029/2008JA013499
|
[28] |
Qin G, Zhang M, Rassoul H K. Prediction of the shock arrival time with SEP observations[J]. J. Geophys. Res., 2009, 114, A09104, doi: 10.1029/2009JA014332
|
[29] |
Zhang J, Dere K P, Howard R A, et al. Identification of solar sources of major geomagnetic storms between 1996 and 2000[J]. Astrophys. J., 2003, 582:520-533
|