Dear colleagues, Combined with time-series observations which were kindly sent by Nyrola team and B. Martin and ours, the light curve of V344 Ori on January 16 -- 19 shows gradual decline with a rate of 0.08mag/day which is reminiscent of a plateau stage during a superoutburst. The humps, which I previously mentioned in [vsnet-alert 5569], are however not similar to ordinary superhumps as reported by T. Vanmusnter in [vsnet-alert 5574]. Their amplitudes are highly variable and irregular between ~0.02 and ~0.1 mag, but their peaks seem to appear rather periodically. Our PDM analysis yields candidates of the period of ~0.04 day, with which we see an average light curve with single peak, and ~0.12 day, with multiple peaks. If 0.04d is a superhump period, it is well below the "minimum period" of hydrogen-rich cataclysmic variables. Follow-up time-series observations are urgently needed to determine whether these modulations are due to superhumps or a kind of quasi-periodic oscillations, or another. We will keep nightly time-series photometry for 9 hours during this outburst in fine nights. Regards, Makoto Uemura, Taichi Kato and Ryoko Ishioka