Articles | Volume 19, issue 21
https://doi.org/10.5194/amt-19-7071-2026
© Author(s) 2026. This work is distributed under the Creative Commons Attribution 4.0 License.
A multimodal approach to derive cloud microphysics in deep convective clouds from polarized measurements of the cloudbow
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- Final revised paper (published on 06 Nov 2026)
- Preprint (discussion started on 27 Aug 2026)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
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RC1: 'Comment on egusphere-2026-4795', Anonymous Referee #1, 19 Sep 2026
- AC1: 'Reply on RC1', Lea Volkmer, 23 Oct 2026
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RC2: 'Comment on egusphere-2026-4795', Anonymous Referee #2, 22 Sep 2026
- AC2: 'Reply on RC2', Lea Volkmer, 23 Oct 2026
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RC3: 'Comment on egusphere-2026-4795', Anonymous Referee #3, 29 Sep 2026
- AC3: 'Reply on RC3', Lea Volkmer, 23 Oct 2026
Peer review completion
AR – Author's response | RR – Referee report | ED – Editor decision | EF – Editorial file upload
AR by Lea Volkmer on behalf of the Authors (23 Oct 2026)
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ED: Publish subject to technical corrections (26 Oct 2026) by Otto Hasekamp
AR by Lea Volkmer on behalf of the Authors (26 Oct 2026)
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Review of the manuscript
"A multimodal approach to derive cloud microphysics in deep convective clouds from polarized measurements of the cloudbow"
by L. Volkmer, L. Dorfer, and B. Mayer
General comments
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The paper describes a new fitting algorithm for analysis of airborne polarimetric measurements in cloudbow angular range. It assumes up to 3 modes in cloud droplet size distribution (DSD), which is an advantage compared to traditional monomodal retrieval techniques. Another advantage of this method is the extended droplet size range, which allows to characterize drizzle and rain droplets. The algorithm was applied to real airborne observations of clouds, and detailed comparison of its results with those of the existing Rainbow Fourier Transform (RFT) method is provided. The comparison shows good agreement in the RFT's droplet size range (which is shorter, so no rain droplets detected by RFT).
The paper is very detailed and well-written, however, some of its important parts require clarification. I suggest to accept the paper after some minor while mandatory revisions described below in line comments.
Line comments
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l.143
In Eq.10 what does the subscript A in f^_A,i stand for?
l.135
Eq.9 was first introduced by Breon and Goloub (1998), so it would be appropriate to cite that paper here.
l.155
Eq.12 assumes that N = 3 without explicitly stating this, while in all previous equations N can be any number. Please, clarify.
ll.157-159
I don't understand Eq.13 at all. If all A_i are the same, then according to Eq.12 A_tot = N*A_i, and f_A,i = A_i/A_tot = 1/N and does not depend on i (while f^_A,i obviously does). Or what is "general scaling factor" _within_ A_i? Please, explain.
ll.169-173
Denoting droplet number concentration by the same letter N that was already used for the number of DSD's modes is confusing. Please, chose different notation.
1.185
Again yet another parameter is denoted by N. I suggest to use subscripts to avoid confusion.
l.195
Lambda should be 1/(2 r_eff v_eff) to be consistant with Eq.6, since variable in Eq.21 is D = 2 r.
ll.256-262
It is not clear what "adding" another mode means. What information from the previous step is retained? If an actual bimodal distribution has, say, 5 um mode and 15 um modes the monomodal fit would return ~10 um mode, that should be split into two on the next step. But if results of the monomodal fit are not used, the bimodal unconstrained fit would be in the space of 6 parameters (3 for each mode) and is likely to be a very ill-posed problem requiring regularization (that is not included in the presented algorithm). Please, clarify.
Fig.9
Panel (a) is not mentioned in the caption.
ll.448-450 and Figs.12-15
While initial RFT distribution may be noisy and include negative values, these artifacts are removed by mode decomposition. The satellite dataset from PACE HARP-2 instrument does not include the initial RFT curve but only mode decomposition parameters (currently for 2 modes). This also significantly reduces the data volume.
Thus, for "apple to apple" comparison I strongly recommend changing the RFT representation in Figs.12-15 with solid dark-blue curves representing mode decomposition results, while the initial curve may be depicted by light color possibly dashed (or entirely removed).
Actually, comparisons of multimodal-fit distributions with RFT mode decomposition results look quite good, so emphasizing them would only benefit the paper. Of coarse, due to the limited radius range RFT cannot see rain droplets.
Also, RFT mode decomposition algorithm rejects any mode with fraction less then 5% (0.05), while the rain modes retrieved by the fitting technique have fractions around 0.01 and DSD maxima so small that they are visible only on the plot with logarithmic y-axis. However, the rainbow curves in (b) panels are consistent with presence of rain droplets. Are there in situ measurements demonstrating that such weak rain modes are real?
Monomodal curves in Figs.12-15 are plotted in yellow and are barely seen on the white background. I suggest using green instead.