Arge, C. N., Odstrcil, D., Pizzo, V. J., & Mayer, L. R. (2003). Improved method for specifying solar wind speed near the Sun. In M. Velli, R. Bruno, F. Malara, & B. Bucci (Eds.), Solar Wind Ten, (pp. 190). American Institute of Physics.
Burton, R. K., McPherron, R. L., & Russell, C. T. (1975). An empirical relationship between interplanetary conditions and Dst. Journal of Geophysical Research, 80(31), 4204–4214.
Cliver, E. W., & Svalgaard, L. (2004). The 1859 solar-terrestrial disturbance and the current limits of extreme space weather activity. Solar Physics, 224, 407–422. https://doi.org/10.1007/s11207-005-4980-z
Cranmer, S. R., Gibson, S. E., & Riley, P. (2017). Origins of the ambient solar wind: Implications for space weather. Space Science Reviews, 212, 1345. https://doi.org/10.1007/s11214-017-0416-y
Isavnin, A. (2016). FRiED: A novel three-dimensional model of coronal mass ejections. The Astrophysical Journal, 833(2), 278.
Janvier, M., Winslow, R. M., Good, S., Bonhomme, E., Demoulin, P., Dasso, S., Mostl, Ch., Lugaz, N., Amerstorfer, T., Soubrie, E., & Boakes, P.D. (2019). Generic magnetic field intensity profiles of interplanetary coronal mass ejections at Mercury, Venus, and Earth from superposed epoch analyses. Journal of Geophysical Research: Space Physics, 124, 812.
Jaynes, A. N., Baker, D. N., Singer, H. J., Rodriguez, J. V., Loto’aniu, T. M., Ali, A. F., Elkington, S. R., Li, X., Kanekal, S. G., Fennell, J. F., Li, W., Thorne, R. M., Kletzing, C. A., Spence, H. F., & Reeves, G. D. (2015). Source and seed populations for relativistic electrons: Their roles in radiation belt changes. Journal of Geophysical Research: Space Physics, 120, 7240. https://doi.org/10.1002/2015JA021234
Jin, M., Cheung, M.C.M, DeRosa, M.L., Nitta, N.V., & Schrijver, C.J. (2022). Coronal mass ejections and dimmings: A comparative study using MHD simulations and SDO observations. The Astrophysical Journal, 928(2), 154.
Kay, C., Gopalswamy, N., Reinard, A., & Opher, M. (2017). Predicting the magnetic field of Earth-impacting CMEs. The Astrophysical Journal, 835(2), 117. https://doi.org/10.3847/1538-4357/835/2/117
Kay, C., Mays, M., & Verbeke, C. (2020). Identifying critical input parameters for improving drag-based CME arrival time predictions. Space Weather, 18(1), e2019SW002382. https://doi.org/10.1029/2019SW002382
Kilpua, E. K. J., Hietala, H., Turner, D. L., Koskinen, H. E. J., Pulkkinen, T. I., Rodriguez, J. V., Reeves, G. D., Claudepierre, S. G., & Spence, H. E. (2015). Unraveling the drivers of the storm time radiation belt response. Geophysical Research Letters, 42, 3076.
Lavraud, B., & Rouillard, A. (2013). Properties and processes that influence CME geo-effectiveness. Proceedings of the International Astronomical Union, 8, 273.
Linker, J. A., Mikic, Z., Biesecker, D. A., Forsyth, R. J., Gibson, S. E., Lazarus, A. J., Lecinski, A., Riley, P., Szabo, A., & Thompson, B. J. (1999). Magnetohydrodynamic modeling of the solar corona during whole Sun month. Journal of Geophysical Research: Space Physics, 104, 9809. https://doi.org/10.1029/1998JA900159
Manchester, W. B., & Van der Holst, B. (2014). Simulating CME eruptions from active regions. American Geophysical Union, Fall Meeting 2014, abstract id. SH51E-03.
O’Brien, T., & McPherron, R. L. (2000). Forecasting the ring current index Dst in real time. Journal of Atmospheric and Solar-Terrestrial Physics, 62(14), 1295–1299. https://doi.org/10.1016/S1364-6826(00)00072-9
Odstrcil, D., & Pizzo, V. J. (1999). Three-dimensional propagation of CMEs in a structured solar wind flow: 1. CME launched within the streamer belt. Journal of Geophysical Research: Space Physics, 104, 483. https://doi.org/10.1029/1998JA900019
Paulikas, G. A., & Blake, J. B. (1979). Effect of the solar wind on magnetospheric dynamics: Energetic electrons at the synchronous orbit. American Geophysical Union Geophysical Monograph, 21, 180–179.
Pomoell, J., & Poedts, S. (2018). EUHFORIA: European heliospheric forecasting information asset. Journal of Space Weather and Space Climate, 8(27), A35. https://doi.org/10.1051/swsc/2018020
Riley, P., & Ben-Nun, M. (2021). On the sources and sizes of uncertainty in predicting the arrival time of interplanetary coronal mass ejections using global MHD models. Space Weather, 19, e02775. https://doi.org/10.1029/2021SW002775
Sabri, S., & Poedts, S. (2024a). Frontiers in astronomy and space science. Frontiers in Astronomy and Space Sciences, 11.
Sabri, S., & Poedts, S. (2024b). Magnetoacoustic wave propagation in the solar corona and filament dynamics. Scientific Reports, 14, 30723.
Sabri, S., & Poedts, S. (2025a). The investigation of June 21 and 25, 2015 CMEs using EUHFORIA. EGU General Assembly, under review.
Sabri, S., & Poedts, S. (2025b). June 21 and 25, 2015 CMEs interaction's results on Earth's ionosphere and magnetosphere. EGU General Assembly, under review.
Sabri, S., Ebadi, H., & Poedts, S. (2020). Plasmoids and resulting blobs due to the interaction of magnetoacoustic waves with a 2.5D magnetic null point. The Astrophysical Journal, 902(1), 11.
Sabri, S., Ebadi, H., & Poedts, S. (2021). Alfvén wave propagation and induced perturbations in the vicinity of a 3D magnetic null-point. The Astrophysical Journal, 924(2), 126.
Sabri, S., Ebadi, H., & Poedts, S. (2021). Plasma flow generation due to the nonlinear Alfvén wave propagation around a 3D magnetic null point. The Astrophysical Journal, 922(2), 123.
Sabri, S., Ebadi, H., & Poedts, S. (2022). Propagation of the Alfvén wave and induced perturbations in the vicinity of a 3D proper magnetic null point. The Astrophysical Journal, 924(2), 126.
Sabri, S., Poedts, S., & Ebadi, H. (2019). Plasma heating by magnetoacoustic wave propagation in the vicinity of a 2.5D magnetic null-point. Astronomy & Astrophysics, 623, A81.
Sabri, S., Poedts, S., & Ebadi, H. (2023). How nonlinearity changes different parameters in the solar corona. The Astrophysical Journal, 944(2), 72.
Sabri, S., Vasheghani Farahani, S., Ebadi, H., & Poedts, S. (2020). How Alfvén waves induce compressive flows in the neighborhood of a 2.5D magnetic null-point. Scientific Reports, 10, 15603.
Savani, N. P., Vourlidas, A., Szabo, A., Mays, M. L., Richardson, I. G., Thompson, B. J., Pulkkinen, A., Evans, R., & Nieves-Chinchilla, T. (2015). Predicting the magnetic vectors within coronal mass ejections arriving at Earth: 1. Initial architecture. Space Weather, 13, 374. https://doi.org/10.1002/2015SW001171
Schwenn, R. (2006). Space weather: The solar perspective. Living Reviews in Solar Physics, 3, 2. https://doi.org/10.12942/lrsp-2006-2
Scolini, C., Winslow, R. M., Lugaz, N., et al. (2022b). Causes and consequences of magnetic complexity changes within interplanetary coronal mass ejections: A statistical study. The Astrophysical Journal, 927(2), 102.
Siscoe, G. (2007). Space weather forecasting historically viewed through the lens of meteorology. Space Weather, 5(6), 6003.
Siscoe, G., Crooker, N. U., & Clauer, C. R. (2006). Dst of the Carrington storm of 1859. Advances in Space Research, 38, 173–179.
Toth, G., De Zeeuw, D.L., Gombosi, T.I., Manchester, W.B., Ridley, A.J., Sokolov, I.V., & Roussev, I.I. (2007). Sun-to-thermosphere simulation of the 28–30 October 2003 storm with the Space Weather Modeling Framework. Space Weather, 5(6), 6003.
Winslow, R. M., Lugaz, N., Scolini, C., & Galvin, A. B. (2021a). On the importance of investigating CME complexity evolution during interplanetary propagation. The Astrophysical Journal, 916(2), 94.
Zhao, X., & Dryer, M. (2014). Current status of CME/shock arrival time prediction. Space Weather, 12, 448–469. https://doi.org/10.1002/2014SW001060
Zheng, Y. (2013). Improving CME forecasting capability: An urgent need. Space Weather, 11, 641.