Generally speaking, the authors have made a great effort to take into account all the comments to improve the manuscript. However, I still feel the manuscript lacks showing its main brought to the thematic for some of the similar reasons than for the first version of the manuscript. So I've tried to be more detailed on the points that seem to me really essential for this study to be published. The study has good potential, and I think these few changes would really improve the presentation and quality of the paper.
(1) the uncertainties and results lacks of quantification. For example, a quantitative comparison of the errors of L3Bs with the strategy of keeping viewing angles close together and L1As with the strategy of orthorectifying on a home-made DEM is lacking.
It would also be nice to have a quantification of the horizontal displacement errors as a function of viewing angle and DEM error. At present, error is quantified as a function of DEM error for a single viewing angle (Figures 12, and S8).
These elements would enable you to be more trenchant in your discourse, in particular to justify the choice of an appropriate strategy for monitoring slow ground movements.
(2) The flow of the methodology is not easy to follow. The methodology is a succession of small modules, different depending on whether we're dealing with L3B or L1A, I still think it would ease the flow of the reading to have a general Figure presenting this processing chain. At present, it's not easy to follow the general outline when reading the methodology.
(3) It would also be important to discuss the final errors obtained with Planetscope, comparing them with those obtained with other fairly high-frequency satellites (Sentinel-2 or Landsat-8). I have the impression that Sentinel-2 or Landsat-8 always does better, despite its larger pixel size. For instance Sentinel-2 1sigma uncertainty in the Siguas area is around 0.8m (Lacroix et al., 2020). Landsat-8 RMSE is 1.4 m (Lacroix et al., 2019). whereas your study shows an uncertainty of around 1 pixel, (3m). I think it must discussed.
(4) Finally, there are a number of small inaccuracies, which make the explanations not always clear. I've noted them below. I tried to be as precise as possible to help the authors modify their manuscript easily.
Specific comments :
Line 45 : It sounds a bit strange to speak about « latest PSB.SD instruments » without introducing what is PSB.SD. Perhaps you could just explain in brackets that these are the generation of instruments launched since 2020.
Line 70 : ∼ 2 - 12 m/yr. This is not totally true : The Siguas landslide underwent phases of 40m/yr motions.
Figure 1 : the inset showing the locations of the area of study on a regional map is not very clear. It is hard to see that the map is South America and to distinguish between lands and oceans.
Line 130 : there is a small incoherence. It is stated that the relative accuracy is 10m whereas on lines 37 and 136, you state 6m.
Line 198 : remove the « But » at the beginning of the sentence.
Section 3.2 : You could also mention that Lacroix et al., 2023 used a strategy of time-series inversion of displacement field to reduce the global uncertainties, leading to about 0.8 m of errors so about 1/4 pixel.
Line 223 : I think a sentence is lacking at the beginning of this section to explain that correlation is here used only to estimate the quality of the orthorectification. That would ease to understand that the choice of the correlation algorithm is not so important. I would also recommend to change the title of this sub-section to express this. For instance « estimation of the uncertainties ».
Line 245 : « When correlating these scenes, the pixels may be wrongly positioned, but in a similar place. » : this is not really clear. Furthermore, this is true only if there is no ground displacements between the 2 scenes. Please clarify.
A general scheme of the methods used is still lacking. The flow of the methods would really benefit from it.
Line 258 : « Correlation pairs are formed among all scenes within a group that have a temporal baseline of six or more months (180 days). » : this is not clear why you select scenes with large time difference. If your goal is to show the way to better orthorectify images and get rid of the DEM errors, this slow-moving landslide motion estimate should appear as an application of your methods, once you have estimated the quality of your new approach. I suggest displacing all what is related to slow-moving landslide monitoring to a second step.
As it is presented, the flow of the reading is not easy to follow.
Line 279 : « used for newer PSB.SD scenes », can you precise what you mean by « newer »
All along the text, you use the terms offset, disparity, displacement for the same measure. Also you sometimes use X,Y sometimes EW, NS, dx, dy. Please be consistent
Line 313-320 : I am not sure to understand these sentences. Do you mean you iteratively refine the DEM coregistration by minimizing the mean/median horizontal disparities in X and Y between an image mapprojected using the reference DEM and the same image mapprojected using the PlanetScope DEM ?
Please clarify.
What about the Z shift of the DEM ? Do you also correct for a mean vertical shift of your Planetscope DEM ?
Line 339 : do you mean the values of X, Y and Z are normalized to obtain new variables between 0 and 1 ? The « maxima » term is not clear : are you creating new variable X/Xmax, Y/Ymax, Z/Zmax ? In this case the variables are not between 0 and 1. Or are you normalizing by (X-Xmin)/(Xmax-Xmin)… ?
Line 353 : « stereo correlation » : do you mean image correlation ?
Line 360 : I disagree with the choice of the quality metric : « As a quality metric, we utilized the mean velocity of stable terrain which we refer to as all pixels outside the landslide mask. ». Indeed, you have forced the displacement fields to be centered on 0 (section 4.4). Therefore, the mean velocity should also be zero. You would better have to use the standard deviation or IQR as you mention in the section 5.4.
Line 363 : can you show on a map where is situated the stable area ?
Line 368-370 : It is not clear what are the disparities you are estimating and why are you using 2 different images ? To me, to evaluate the effect of the DEM error you better have to estimate the disparities between the same image projected onto the 2 different DEMs. This would help you to also evaluate the effect of the viewing angle together with the DEM error on the dx and dy disparities (see also my comments on section 5.3).
Line 370 : can you refer to the corresponding figure ?
Line 373-405 : I would have really appreciate a quantitative comparison of the 2 approaches, rather than purely qualitative. Could you estimate the IQR for all the image correlation of L3B images of the same groups (and short temporal baselines) and the image correlation of the same dates but L1B-orthorectified with the Planetscope DEM ?
Section 5.3
It is really not clear what are you evaluating (see my comment from the lines 368-370).
Also the origin of your conclusions on the different errors in x and y directions is not really clear. To me the difference between the 2 directions must be caused by the orientation of the acquisition, right ? I think it is required to show what is the viewing angle of the satellite in Figure 12, and also to evaluate not only the horizontal error as a function of the DEM error (Figure 12 and Figure S8), but also as a function of the viewing angle.
Line 419 : « For all correlation pairs, the IQR was reduced to the sub-pixel range (< 3m). » It is not really true for the dy in Siguas.
Section 5.5
This is relatively important section, as it shows the main brought of the developed method for the landslide thematic. Either, the methods could have been developed on any areas without landslides. That’s why I have the feeling that this section could be more developed.
For instance, I have the feeling that we can observe a seasonal variation of the velocity on the Del Medio landslide. Do you agree ? Is it also what we expect related to a seasonal forcing from the precipitations ?
On the Siguas landslide you observe a deceleration of the landslide over 3 years. Could it still be the similar decay following the material supply from 2016 (Lacroix et al., 2019) ? In this latter study, authors show that the material transient acceleration last few weeks. So why should the landslide velocity decrease over 3 years ? Drainage ? Morphological barriers at the toe of the landslide ? Decrease of the irrigation ?
Section 6.1 : This section is not really informative. I am wondering about its utility ?
Section 6.3 : A quantitative comparison of the 2 approaches is still lacking. Figures S9 and S10 are dealing about that, but a metric (IQR ? Standard deviation?) would be very useful to quantify this error for the 2 approaches for different scenes. See also my previous comment on the line 373-405.
Line 519-520 : « a few meter per year » : This is not really quantitative.
A sensitivity analysis of the effect of DEM error together with viewing angle on the horizontal displacement is lacking (see also my comment on section 5.3).
The results in terms of uncertainties would be nice to be compared with other open-source sensors like Sentinel-2 or Landsat8, to see the validity of Planetscope data compared to other open-source sensors. |