References
- Armstrong JW, Coles WA, Analysis of three-station interplanetary scintillation, J. Geophys. Res. 77, 4602-4610 (1972). https://doi.org/10.1029/ja077i025p04602
- Brueckner GE, Howard RA, Koomen MJ, Korendyke CM, Michels DJ, et al., The large angle spectroscopic coronagraph (LASCO) visible light coronal imaging and spectroscopy, Solar Phys. 162, 357-402 (1995). https://doi.org/10.1007/bf00733434
- Cane HV, Richardson IG, Interplanetary coronal mass ejections in the near-Earth solar wind during 1996-2002, J. Geophys. Res. 108, 1156 (2003). https://doi.org/10.1029/2002JA009817
- Chen J, Theory of prominence eruption and propagation: interplanetary consequences, J. Geophys. Res. 101, 27499-27519 (1996). https://doi.org/10.1029/96JA02644
- Choi KC, Park MY, Kim JH, Auto-detection of halo CME parameters as the initial condition of solar wind propagation, J. Astron. Space Sci. 34, 315-330 (2017). https://doi.org/10.5140/JASS.2017.34.4.315
- Coles WA, Kaufman JJ, Solar wind velocity estimation from multi-station IPS, Radio Sci. 13, 591-597 (1978). https://doi.org/10.1029/rs013i003p00591
- Dryer M, Interplanetary studies: propagation of disturbances between the Sun and the magnetosphere, Space Sci. Rev. 67, 363-419 (1994). https://doi.org/10.1007/BF00756075
- Gapper GR, Hewish A, Purvis A, Duffett-Smith PJ, Observing interplanetary disturbances from the ground, Nature 296, 633-636 (1982). https://doi.org/10.1038/296633a0
- Gonzalez-Esparza JA, Carrillo A, Andrade E, Enriquez RP, Kurtz S, The MEXART interplanetary scintillation array in Mexico, Geofis. Int. 43, 61-73 (2004).
- Gopalswamy N, Lara A, Yashiro S, Kaiser ML, Howard RA, Predicting the 1-AU arrival times of coronal mass ejections, J. Geophys. Res. 106, 29207-29217 (2001). https://doi.org/10.1029/2001JA000177
- Gosling JT, Coronal mass ejections and magnetic flux ropes in interplanetary space, in Physics of Magnetic Flux Ropes, eds. Russell CT, Priest ER, Lee LC (American Geophysical Union, Washington, DC, 1990). https://doi.org/10.1029/GM058p0343
- Iwai K, Shiota D, Tokumaru M, Fujiki K, Den M, Kubo Y, Development of a coronal mass ejection arrival time forecasting system using interplanetary scintillation observations, Earth Planets Space. 71, 39 (2019). https://doi.org/10.1186/s40623-019-1019-5
- Jackson BV, Hick PL, Kojima M, Yokobe A, Heliospheric tomography using interplanetary scintillation observations: 1. combined Nagoya and Cambridge data, J. Geophys. Res. 103, 12049-12067 (1998). https://doi.org/10.1029/97ja02528
- Kim JH, Chang HY, Association between solar variability and teleconnection index, J. Astron. Space Sci. 36, 149-157 (2019). https://doi.org/10.5140/JASS.2019.36.3.149
- Kim KH, Moon YJ, Cho KS, Prediction of the 1-AU arrival times of CME-associated interplanetary shocks: evaluation of an empirical interplanetary shock propagation model, J. Geophys. Res. 112, A05104 (2007). https://doi.org/10.1029/2006JA011904
- Kim RS, Cho KS, Kim KH, Park YD, Moon YJ, et al., CME earthward direction as an important geoeffectiveness indicator, Astrophys. J. 677, 1378-1384 (2008). https://doi.org/10.1086/528928
- Kim RS, Cho KS, Moon YJ, Kim YH, Yi Y, et al., Forecast evaluation of the coronal mass ejection (CME) geoeffectiveness using halo CMEs from 1997 to 2003, J. Geophys. Res. 110, A11104 (2005). https://doi.org/10.1029/2005JA011218
- Kim RS, Gopalswamy N, Cho KS, Moon YJ, Yashiro S, Propagation characteristics of CMEs associated with magnetic clouds and ejecta, Solar Phys. 284:77-88 (2013). https://doi.org/10.1007/s11207-013-0230-y
- Kojima M, Kakinuma T, Solar cycle dependence of global distribution of solar wind speed, Space Sci. Rev. 53, 173-222 (1990). https://doi.org/10.1007/BF00212754
- Manoharan PK, Gopalswamy N, Yashiro S, Lara A, Michalek G, et al., Influence of coronal mass ejection interaction on propagation of interplanetary shocks, J. Geophys. Res. 109, 6109 (2004). https://doi.org/10.1029/2003JA010300
- Manoharan PK, Subrahmanya CR, Chengalur JN, Space weather and solar wind studies with OWFA, J. Astrophys. Astron. 38, 16 (2017). https://doi.org/10.1007/s12036-017-9435-z
- Moon YJ, Dryer M, Smith Z, Park YD, Cho KS, A revised shock time of arrival (STOA) model for interplanetary shock propagation: STOA-2, Geophys. Res. Lett. 29, 1390 (2002). https://doi.org/10.1029/2002GL014865
- Morgan JS, Macquart JP, Chhetri R, Ekers RD, Tingay SJ, et al., Interplanetary scintillation with the Murchison Widefield Array V: an all-sky survey of compact sources using a modern low-frequency radio telescope, Publ. Astron. Soc. Aust. 36, E002 (2019). https://doi.org/10.1017/pasa.2018.40
- Mostl C, Isavnin A, Boakes PD, Kilpua EKJ, Davies JA, et al., Modeling observations of solar coronal mass ejections with heliospheric imagers verified with the Heliophysics System Observatory, Space Weather 15, 955-970 (2017). https://doi.org/10.1002/2017SW001614
- Odstrcil D, Modeling 3-D solar wind structure, Adv. Space Res. 32, 497-506 (2003). https://doi.org/10.1016/S0273-1177(03)00332-6
- Rollett T, Mostl C, Isavnin A, Davies JA, Kubicka M, et al., ElEvoHI: a novel CME prediction tool for heliospheric imaging combining an elliptical front with drag-based model fitting, Astrophys. J. 824, 131 (2016). https://doi.org/10.3847/0004-637X/824/2/131
- Tokumaru M, Kojima M, Fujiki K, Yamashita M, Yokobe A, Toroidal-shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000, J. Geophys. Res. 108, 1220 (2003). https://doi.org/10.1029/2002JA009574
- Tokumaru M, Kojima M, Fujiki K, Yokobe A, Three-dimensional propagation of interplanetary disturbances detected with radio scintillation measurements at 327 MHz, J. Geophys. Res. 105, 10435-10453 (2000). https://doi.org/10.1029/2000ja900001