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We also tabulated the distribution of shower and bath length and frequency in control mothers (Additional file 1: Table S1).
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Using weekday data only, we derived probability distributions of the starting time for showers (Figure 4) and low volume usages (Figure 5). Figure 4 The probability distribution of the shower starting time.
Our regimen was simplified from that of Tan et al. (2006), who used a pulsed water intake and a distribution for shower start time.
The distributions of rain showers (say, their frequency in 1-month interval over a given DCP) as well as rain duration (how long a shower lasts) were generated by uniform distributions.
In 1937 he and his colleague Otto Zeiller arrayed nine counters in a circle to determine the angular distribution of a cosmic ray shower.
We present here the salient features of GRAPES-3 experiment and some details of muon multiplicity distributions (MMDs) observed with a 560 muonuon detector as a function of shower size (Ne) fro analysis of 560 days of data.
The measured distribution of Nμ of cosmic ray air showers can then be analysed, in conjunction with measurements of Xmax from fluorescence detectors, to put constraints on the cosmic ray composition and hadronic interaction models.
Within each shower interval, however, the distribution of tipping time intervals was modeled by Eq. 1.
number of shower heads used: 150.
To characterize exposure, shower water and aerosol of shower have been sampled.
These factors include water temperature and flow rate, shower duration, volume of shower enclosure, air exchange rates, and showerhead type.
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