We present the interim results of simultaneous time monitoring observations of SiO v=1, 2, J =1-0, $^{29}SiO$ v=0, J =1-0, and $H_2O$ $6_{16}-5_{23}$ maser lines toward about 60 relatively strong SiO and/or H2O maser sources using the single dishes of the Korean VLBI Network from 2009 September to 2012 June. These monitoring sources are composed of representative semiregular variables, Miras, water fountain sources, preplantary nebulae and SiO maser sources of star forming regions etc. The variations of intensity ratios between SiO and $H_2O$ masers and velocity structures are investigated according to stellar optical phases and observational epochs. Several individual sources which show an interesting feature will be presented here.