“…Abundant Ca emission lines were observed, including Ca I emission lines at 422.5,429.8,445.4,526.4,558.8,615.6,645.1,714.8,and 720.2 nm;Ca II emission lines at 315.7,317.7,373.5,393.0,396.5,732.3,854.2,and 866.2 nm; and Ca III emission lines at 642.5 and 648.3 nm (Ahmed, Umar, Ahmed, & Baig, 2017;Juvé, Portelli, Boueri, Baudelet, & Yu, 2008;Velioglu, Sezer, Bilge, Baytur, & Boyaci, 2018;Yaroshchyk, Morrison, Body, & Chadwick, 2005). Several signals at 279.3 and 280.0 nm were attributed to Mg II emission lines and those at 382.9 and 383.5 nm represented Mg I emission lines (Abdel-Salam, Al Sharnoubi, & Harith, 2013;Li, Liu, Chen, & Li, 2008;Mansoori et al, 2011;Rai, Zhang, Yueh, Singh, & Weisberg, 2001;Yaroshchyk et al, 2005;Zheng et al, 2008). An Al I emission line was observed at 309.2 nm (Mansoori et al, 2011;Yaroshchyk et al, 2005).…”