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v5	v6
13	13	Between the photosphere and the dust formation zone, it is the gas opacity ($2\times10^{-4}cm^{2}/g$). The dust formation radii is calculated by
14	14
15		$R_d=\sqrt{\frac{\alpha L \exp{-\tau}}{4 \pi \sigma T_{sub}^{4}}}$
	15	$R_d=\sqrt{\frac{\alpha L \exp{(-\tau)}}{4 \pi \sigma T_{sub}^{4}}}$
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	17	Where $\tau$ is first calculated by assuming there is only gas in the simulation. When the $R_d$ is determined, I update the opacity where there is dust.