Author:
Blessy W. Hannah,Rahman A. Mujiber,Inbanathan S. S. R.,Prasad Pa. Gokhula
Reference15 articles.
1. Anna Lakshmi, M., Umapathy, S., Prakash, O., and Vasanth, V., Studies on some properties of coronal mass ejections based on angular width, Astrophys. Space Sci., 2011, vol. 335, pp. 373–378.
2. Bidhu, S.S., Iren, S.N., and, Dickson, B.A., CME speed and angular width distribution during 23 and 24 solar cycle maximum, J. Space Explor., 2017, vol. 6, no. 1, p. 122.
3. Brueckner, G.E., Delaboudiniere, J.-P., Howard, R.A., Paswaters, S.E., St. Cyr, O.C., Schwenn, R., Lamy, P., Simnett, G.M., Thompson, B., and Wang, D., Geomagnetic storms caused by coronal mass ejections (CMEs): March 1996 through June 1997, Geophys. Res. Lett., 1998, vol. 25, no. 15, pp. 3019–3022.
4. Cremades, H. and St. Cyr, O.C., Coronal mass ejections: Solar cycle aspects, Adv. Space Res., 2007, vol. 40, no. 7, pp. 1042–1048.
5. Gilbert, H.R., Holzer, T.E., and Burkepile, J.T., and Hundhausen, A.J., Active and eruptive prominences and their relationship to coronal mass ejections, Astrophys. J., 2000, vol. 537, no. 1, p. 503.