Yes, it is indeed the case that you can get lost very quickly here.
But, it can be very helpful to see filmic not as a styling element, but as a module with which you can create the optimal conditions for modifying the photo in further steps. The filmic is excellently suited for this and in most cases - under this condition - very easy to use.
Let’s take your example for that.
We push the exposure up until everything is “optimally” illuminated. “Optimal” is a personal assessment and depends on what you see in the photo as the main subject.
I have increased it here to 3 EV because I still want to see the details in shadows:
As you can see in the histogram, the highlights are hard on the edge of overexposure. So, my goal now will be, with the help of filmic, to expand this margin, i.e. - to compress the highlights and to see that the details in the shadows do not disappear into the black. In filmic, I increase the white relative exposure and black relative exposure until I have enough room for further processing.
The fact that the photo now looks very flat and low-contrast doesn’t interest me at this moment. Note also the values in the histogram:
Now I have, so to speak, “set the scene” and can concentrate on the processing. This also means that most of what happens now happens in the pixel pipe after the filmic.
Specifically, I now want to increase lost contrast again and there are countless possibilities. In this case I will simply - after the filmic - use a new instance of the exposure module with multyply (or multiply reverse) blend mode for this. Let’s see how it looks like:
Now I have again a nice contrast with all the parts I want to have: the shadows are not too dark (you can still see the details) and highlights also show the nice transitions and even there the details are still clearly visible (look at the brown bark of the tree in the middle).
I can now use Tone equalizer to subtly lighten the shadow areas and that’s it:
I could now play a bit more with saturation and colors, but that is not necessary for this demonstration.
_DSF1845.RAF.xmp (9,2 KB)
darktable 3.5.0~git1357.578d3ffa7-1