Transition Layers for $P_\mathrm{min}<P_\mathrm{c}<P_\mathrm{max}$ {#sec:zp large}
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In the ZP solutions, the mass flux is determined so that the CNM is connected with the WNM. Here, we consider the condensation front $(j<0)$. What happen if the mass flux is larger than $|j_\mathrm{ZP}|$?

### Classification of Solutions

![image](fig2.eps){width="13.0cm"}

It is found that solutions for larger mass flux can be divided by four type solutions: C-U-o, C-U, C-c, and C-C. We describe the property of each solution below.

[*C-U-o Solutions.*]{} For the case with $j=3j_\mathrm{ZP}$, the solution does not reaches the saddle point of the WNM but approaches the spiral point of the unstable phase (see the first row of figure \[fig:j0\]b). From the second row of figure \[fig:j0\](b), one can see the oscillation of the temperature profile that corresponds to the spiral motion in the phase diagram. The third row shows the trajectory of the solution in the $(n,P)$ plane. The solution truncates at the heating-dominated region before arriving at the WNM. The truncation point corresponds to the peak of the temperature in the second row of figure \[fig:j0\](b). Since the mass flux is still low, the pressure is almost constant. This type solutions already has been found in @Eetal92 under 