Carolina SM, Karl L, Gerard T (2017). Microwave radio emission as a proxy for coronal mass ejection arrival speed in predictions of interplanetary coronal mass ejections at IAU. Space Weather Space Climate J. 7:A2.
Crossref

Cheng L, Shen YZ, Bin A, Ye MP, Wang S (2014). Full Halo coronal mass ejections arrival at the earth. 

View

Cyr OC, Raymond JC, Thompson BJ, Gopalswamy NK, Kahler SK, Lara N, claravella A, Romol N, Oneal R (2000). SOHO and Radio observation of CME shock Wave. Geophys. Res. Letters J. 27(10):1439-1442.
Crossref

Gopalswamy N, Lara A, Lepping RP, Kaiser ML, Berdichevsky D, Cyr OC (2000). Interplanetary acceleration of coronal mass ejections. Geophys. Res. Lett. J. 27:145.
Crossref

Gopalswamy N, Alejandro L, Russel A H (2001). Predicting the I-AU arrival times of coronal mass ejections. Geophys. Res. J. 106(A12):29, 207-209, 217.

Gopalswamy N, Alejandro L, Yashiro S, Kaiser ML, Howard RA (2005). An empirical model to predict the 1-AU arrival of interplanetary shocks. Adv. space res. J. 36(12):2289-2294.

Mishra AP, Tripathi RM (2005). Characteristics features of CMEs with respect to their source region. Proceeding of the 29th International Cosmic Ray Conference, Pune, India 1:149.

Mostl CK, Amla JR, Hall PC, Liewer EM, Jong RC, Colaninno AM, Galvin AB (2014). Connecting speeds , directions and arrival time of 22 Coronal Mass Ejection from the Sun to 1AU. Astrophysi. J. V5/2/11.
Crossref

Okeke FN, Okpala KC, Akaogu V (2011). Predictions of the arrival time of Coronal Mass Ejection (CME) and its contributions to major Geomagnetic storms. Nig. J. Space Res. 10:217-230.

Owens M, Cargil P (2004). Predictions of the arrival time of Coronal Mass Ejection at IAU: an analysis of the causes of errors.

Sheeley NR, Wang YM, Hawley SH, Bruckner GE, Dere, KP, Howard RA, Koomen MJ, Korendyke CM, Michels DJ, Paswaters SE, Socker DG, St. Cyr OC, Wang D, Lamy PL, Liberia A, Schwenn R, Simnett GH, Plunkett S Biesecker DA (1997). Measurements of the flow speed in the corona between 2 and 30 rs. Astrophys. J. 484:472.
Crossref

Tong S, Yikang W, Linfeng W, Xin C, Mingde D, Jie Z (2015). Predicting the arrival time of coronal mass ejection with the graduated cylindrical shell and drag force model. Astrophys. Res. letters J. 806:2.

Vrsnak B, Gopalswamy N (2002). Influence of aerodynamic drag on the motion interplanetary ejecta. J. Geophys. Res. 107:10.1029/2001/JA 000120.

Yashiro SN, Gopalswamy GM, Cyr OC, Plunkett SP, Rich NB, Howard RA (2001). A catalog of white light coronal mass ejections observed by the SOHO Spacecraft. J. Geophys. Res. 109(A):7105.

Zhang J, Wang T, Zhang C, Liu Y, Nitta N, Slater GL, Wang J (2001). Flare-CME events association with a super activeregion recent insight into the Physics of the Sun and heliosphere: Highlights from SOHO and other space missions. Pal Brekke (Eds), Proceedings of IAU Symposium. P 203.