the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Is it possible to estimate aerosol optical depth from historic colour paintings?
- 1Institute of Physics, University of Greifswald, Felix-Hausdorff-Str. 6, 17489 Greifswald, Germany
- 2Institute of Art History, Albert-Ludwigs-University of Freiburg, Platz der Universität 3, 79085 Freiburg, Germany
- 3Institute of Environmental Physics, University of Bremen, Otto-Hahn-Allee 1, 28359 Bremen, Germany
- 1Institute of Physics, University of Greifswald, Felix-Hausdorff-Str. 6, 17489 Greifswald, Germany
- 2Institute of Art History, Albert-Ludwigs-University of Freiburg, Platz der Universität 3, 79085 Freiburg, Germany
- 3Institute of Environmental Physics, University of Bremen, Otto-Hahn-Allee 1, 28359 Bremen, Germany
Abstract. The idea of estimating stratospheric aerosol optical thickness from the twilight colours in historic paintings – particularly under conditions of volcanically enhanced stratospheric aerosol loading – is very tantalising, because it would provide information on the stratospheric aerosol loading over a period of several centuries. This idea has in fact been applied in a few studies in order to provide quantitative estimates of the aerosol optical depth after some of the major volcanic eruptions that occurred during the past 500 years. In this study we critically review this approach and come to the conclusion that the uncertainties of the estimated aerosol optical depths are so large that the values have to be considered highly questionable. We show that several auxiliary parameters – which are typically poorly known for historic eruptions – can have a similar effect on the red-green colour ratio as a change in optical depth typically associated with eruptions such as, e.g. Tambora in 1815 or Krakatao in 1883. Among the effects considered here, uncertainties in the aerosol particle size distribution have the largest impact on the colour ratios and hence the aerosol optical depth estimate. For solar zenith angles exceeding 80 degrees, uncertainties in the stratospheric ozone amount can also have a significant impact on the colour ratios. In addition, for solar zenith angles exceeding 90 degrees the colour ratios exhibit a dramatic dependence on solar zenith angle, rendering the estimation of aerosol optical depth essentially impossible.
Christian von Savigny et al.
Status: final response (author comments only)
-
RC1: 'Comment on cp-2022-38', Anders Svensson, 09 Jun 2022
The manuscript is concerned with estimating the uncertainties related to deriving the Aerosol Optical Depth (AOD) from the coloring of the sky in paintings made at the time of large volcanic eruptions. As such, the manuscript provides a critical comment to existing publications that are aiming at deriving such values. Using an atmospheric radiative transfer model, the manuscript presents a number of sensitivity studies by varying a number of parameters that may lead to uncertainties in the color-based AOD estimates. The manuscript is well written and easy to follow and the various uncertainties brought to the table appear relevant.
I do not have comments on the radiative transfer model for which I am not an expert, but I have two suggestions for the authors to consider:
My first point concerns the ‘true’ error related to AOD estimates from paintings. For historical volcanic eruptions, there are ice-core based estimates of the sulfate deposition in both Greenland and Antarctica that provide an independent estimate of the stratospheric sulfate aerosol loading, which in turn can be translated into an stratospheric AOD (Gao et al., 2007;Gao et al., 2008;Sigl et al., 2015). Can those estimates be applied to give an independent estimate of the accuracy of the paintings derived AOD? Of course, the ice-core estimates can be questioned themselves, but a reasonable agreement between the two independent approaches would nevertheless suggest that both methods are providing AOD estimates that are in the right order of magnitude, at least. Likewise, a large disagreement between the two methods would suggest that at least one of them has very large uncertainties. Maybe this comparison has already been done in another study? It seems like a quite obvious comparison to make?
My second point concerns an overall error estimate for the historic color painting method for estimating the stratospheric aerosol optical thickness based on the uncertainties introduced in the present manuscript. In the manuscript, we are provided with numerous figures showing the AOD sensitivity to factors such as particle size distribution, wavelength, solar zenith angle, albedo, azimuth angle, etc. All of those dependencies certainly leave the impression ‘that the uncertainties of the estimated aerosol optical depths are so large that the values have to be considered highly questionable’, as mentioned in the abstract. However, how large are the uncertainties ‘typically’ in a real-case scenario? If we add up all of the uncertainties using a realistic range of values for the parameters discussed in the study, do we then end up with 5% or 50% uncertainty on the final result? If the total uncertainty is in the range below say 50%, the method may still be applicable, eg if there are several paintings of the (sky of the) same eruption that may provide independent evidence. If the final uncertainty estimate is large however, say above 50%, the entire approach of using paintings for estimating the AOD becomes questionable. Therefore, some kind of summary providing a combined uncertainty from all of the discussed parameters would be quite helpful. Also, an estimate of the relative uncertainty contribution from each investigated parameter would be helpful again using a realistic range of parameters. If possible, some uncertainty estimates/ranges could be provided in a table? This may provide some useful guidance for future studies of what knowledge is needed to make constrained AOD estimates from paintings. Maybe, in some cases, there is independent evidence of say the position of the Sun or the time of the day when the picture was painted? Likewise, we may become wiser in the future about what to expect from the particle size distribution related to large volcanic eruptions. Thus - wearing an optimistic hat - it could be that some of the uncertainty ranges discussed in the manuscript could be significantly reduced or even eliminated for specific paintings/eruptions?
References:
Gao, C. C., Robock, A., and Ammann, C.: Volcanic forcing of climate over the past 1500 years: An improved ice core-based index for climate models, Journal of Geophysical Research-Atmospheres, 113, D23111, 10.1029/2008jd010239, 2008.
Gao, C. H., Oman, L., Robock, A., and Stenchikov, G. L.: Atmospheric volcanic loading derived from bipolar ice cores: Accounting for the spatial distribution of volcanic deposition, Journal of Geophysical Research-Atmospheres, 112, 10.1029/2006jd007461, 2007.
Sigl, M., Winstrup, M., McConnell, J. R., Welten, K. C., Plunkett, G., Ludlow, F., Büntgen, U., Caffee, M., Chellman, N., Dahl-Jensen, D., Fischer, H., Kipfstuhl, S., Kostick, C., Maselli, O. J., Mekhaldi, F., Mulvaney, R., Muscheler, R., Pasteris, D. R., Pilcher, J. R., Salzer, M., Schüpbach, S., Steffensen, J. P., Vinther, B. M., and Woodruff, T. E.: Timing and climate forcing of volcanic eruptions for the past 2,500 years, Nature, 523, 543-549, 10.1038/nature14565, 2015.
-
AC1: 'Reply on RC1', Christian von Savigny, 31 Aug 2022
The comment was uploaded in the form of a supplement: https://cp.copernicus.org/preprints/cp-2022-38/cp-2022-38-AC1-supplement.pdf
-
AC1: 'Reply on RC1', Christian von Savigny, 31 Aug 2022
-
RC2: 'Comment on cp-2022-38', Anonymous Referee #2, 12 Jul 2022
The manuscript challenges the notion that historical paintings can be used to quantitively assess the amount of stratospheric sulphate aerosols following major volcanic eruptions, based in particular on a series of sensitivity tests with an atmospheric radiative transfer model.
In general the manuscript is clear and well written, and it could be of interest to Climate of the Past readers.
I think that already in the introduction the authors should clarify the premises of this study, as the readers may not be familiar with all the background facts, for instance by concisely but explicitly addressing the following issues:
Why do you focus on near-horizon radiance (e.g. evenings)?
Why do you focus on the red/green ratio?
How do you know that the painting is depicting the evening?
How do you know that the painter’s style was realistic in reproducing the colors?
How do you know that pigment conservation allows for estimating the original colors faithfully?Specific comments
9) Krakatoa?
55) “The troposphere was assumed to be free of aerosols”. This appears to be a strong assumption. Was there a basic sensitivity test at least, to justify this? No reference is provided either, of why this assumption should hold.
Table 1) If I interpreted the parameter values correctly, the central case is that of painters reproducing on canvas what they see in front of them, just before sunset, while giving their back to the setting sun. Is that correct? Maybe it’s worth spelling this out.
59) Since the red/green ratio is relevant here, and the application of tristimulus values implies using specific wavebands, it would be worth seeing a curve of RI vs wavelength
85) Why not showing a plot of the tristimulus values wavelength dependence?
-
AC2: 'Reply on RC2', Christian von Savigny, 31 Aug 2022
The comment was uploaded in the form of a supplement: https://cp.copernicus.org/preprints/cp-2022-38/cp-2022-38-AC2-supplement.pdf
-
AC2: 'Reply on RC2', Christian von Savigny, 31 Aug 2022
-
RC3: 'Comment on cp-2022-38', Anonymous Referee #3, 12 Jul 2022
This study raises a number of important uncertainties that were not considered in the Zerefos et al., 2007 and 2014 methodology, in particular regarding the particle size distribution and stratospheric ozone concentration. It acts as an interesting and useful continuation of research on the question of whether historical paintings encode quantitative environmental information. However, I have four major comments that question the conclusion that “quantitative determination of the AOD from colours in paintings is generally not possible” — while agreeing that error quantification of the Zerefos methodology is an important next step.
Major comments
1) More justification for the choice of parameters used in the sensitivity studies should be provided. Having a sense of how these perturbations compare to values in a typical volcanic eruption would help contextualize the magnitude of the resulting errors.
As one example, regarding the claim that the particle size distribution is a strong confounding variable, it would be useful to provide more justification for the choice of 350 and 450 nm as perturbed parameters. A study is cited of observed values > 400 nm after Pinatubo. The authors do mention a number of other uncertainties regarding the particle size distribution and this sensitivity test, e.g., whether the distribution is log-normal, what are reasonable median values, whether the median scales with the strength of the volcanic eruption, how the distribution depends on the observation geometrics. Another issue appears to be how the median value varies as a function of altitude and latitude (cf. Figure 1b in Bingen et al., 2004). Given these various uncertainties, it is not clear to me whether median particle size can be considered a systematic source of error.
A related specific issue concerns that Pinatubo was a large eruption (VEI 6), and similarly VEI 6 eruptions (between years 1500-1900) in the Zerefos study have AODs around 0.4-0.6, which is outside the range of AODs shown in Fig. 2 (going to 0.3). It would be useful to include the curves for an AOD value of 0.5 or 0.6 to show how the uncertainty introduced by particle size distribution compares with the full range spanned by AOD values considered in Zerefos et al., 2007 (e.g., their Fig 6).
Similarly, justification for the choice of ozone parameters would also be helpful. It seems that the influence of volcanic aerosols on stratospheric ozone is not yet fully understood. The different perturbations in this study could, moreover, co-vary, which has not been considered. For instance, it could, conceivably, be that a larger volcanic eruption does indeed increase the median particle size, but decreases the stratospheric ozone concentration, such that these two errors cancel to some extent. Some research indicates that stratospheric ozone could decrease if there is a natural (biogenic) source of bromine or hydrogen halides (e.g., Klobas et al., 2017, Ming et al., 2020). The large uncertainties, both in the individual processes and possible interactions/compensations among different factors also introduce substantial uncertainty in the sensitivity tests shown here that is not yet discussed.
2) As a continuation of the points raised in 1), it would be useful to have a synthesized error estimate – that is, jointly considering the influence of the various sensitivity studies. Such error bounds would allow for a like-for-like comparison with the Zerefos results (e.g., as a function of AOD and zenith angle, as in Zerefos et al., 2007 Tables 2 and 3). Such an overall error estimate would also give a sense of how the uncertainties involved in this methodology compare with uncertainties present in other methodologies to estimate historical volcanic AODs, such as from ice cores.
That said, an overall error bound seems difficult to estimate, given a lack of knowledge of how these error sources combine: additively? some compensation as discussed in 1)? It is not clear whether the error sources would combine to yield iid observational error, adding noise to the estimates of the paintings. In that case, that a signal in the R/G ratios can nevertheless be extracted, despite the noise, is surprising and would point to a strength, rather than a weakness, in the methodology.
In conclusion, it seems that overall error bounds are necessary before one can make the argument that a quantitative estimate of volcanic AOD from historical paintings is not possible.
3) The art historical analysis in Sec. 4.1 focuses only on a single painter, Caspar David Friedrich, who was known to be more spiritual and less empirical than many of his contemporaries, such as John Constable, JMW Turner, or Johan Christian Dahl. As one example, the German thinker Johann Wolfgang von Goethe became aware of Luke Howard’s cloud studies and expounded them in intellectual circles in Germany. As described in Richard Hamblyn’s The Invention of Clouds: How an Amateur Meteorologist Forged the Language of the Skies, whereas many painters, such as Constable and Dahl actively engaged with these scientific ideas, Friedrich was an exception in categorically dismissing scientific ideas as incompatible with his artistic practice (e.g., refusing Goethe’s request to provide illustrations for Goethe’s 1817 essay on Howard, saying the project would ‘undermine the whole foundation of landscape painting, Hamblyn, p. 221).
It is understood that this section is not an exhaustive art historical analysis. Yet the balance of this section needs improvement. It could note the general spirit of empiricism and greater overlap between the arts and sciences that was present in the period considered from 1500-1900 – rather than simply selecting one painter to make the point that artwork does not contain quantitative environmental information. Environment is, of course, not the only factor that influences artwork, but there is evidence that painters do depict the environment with some sort of fidelity. This evidence can be qualitative (e.g., the Turner quote at the end of Zerefos et al., 2007, Paul Cézanne’s critique of Monet that he was “only an eye…But my God!... what an eye!”), but also more quantitative (e.g., Olson et al., 2003, Aragon et al., 2006, Fikke et al., 2017).
4) My fourth major comment relates to the ‘tone’ of the manuscript, which gives the impression of dismissing any quantitative skill of the Zerefos et al. methodology (e.g., that the Zerefos results “have to be considered highly questionable”). The uncertainties mentioned in points 1) and 2), however, imply that the ultimate magnitude of the error is far from certain. It therefore appears somewhat misleading and unfortunate to entirely disregard this methodology, especially given the paucity of records of historical volcanic AOD.
Perhaps the total errors will someday be shown to be too large such that the Zerefos methodology does not have any quantitative skill, but it is premature to make this conclusion given uncertainties in 1) the perturbed parameters in the sensitivity studies and 2) potential compensations among the different factors considered here. Instead, the authors could consider changing the language to say that uncertainties considered are avenues for further research. Reducing uncertainty about these important issues would allow for better constraining volcanic AOD from historical images.
Minor comments
1) The authors might consider including a schematic illustrating the key radiative processes and quantities, e.g., diffuse downward radiation vs. near-horizon radiance, solar zenith angle, to increase readability for a broader audience. In such a schematic, it could also be worthwhile to show a sunset with bluer sky towards the zenith and increasingly red colors towards the horizon to illustrate the issue of irradiance vs. near-horizon radiance.
2) Zerefos et al., 2007 say that there are large errors when the zenith angle exceeds 90 degrees: “In our calculations we used the diffuse irradiance over the whole hemisphere at the given wavelengths. However if we calculate the R/G ratios shown in Figs. 1 and 2 using the integral of the calculated radiances within 20 degree azimuth, around the setting sun and for zenith angles 70–90deg, then we would be able to simulate with the model the paintings’ ratios even better. We note here that the radiative transfer solver included in libRadtran is only a pseudo-spherical and not a fully spherical code, and therefore its accuracy for radiance calculations is limited at high SZAs.”. The current manuscript says, “One issue is that they did not calculate the radiance ratio for a near-horizon viewing geometry, but calculated the ratio of the diffuse downward fluxes at the two wavelengths, although the near-horizon radiance would be the correct quantity in this context.” I found this discrepancy hard to understand. Could the authors please clarify why Zerefos et al., 2007 wrote that the accuracy of radiance calculations is limited at high solar zenith angles, but it is no longer a problem – have the models improved since 2007 to eliminate this issue? They also seem to address the concern of diffuse downward fluxes vs. near-horizon radiance in their manuscript and find that it little influences results (as cited above), so I was surprised to see this difference so prominently highlighted.
3) Typo ‘Krakatoa’ line 9 in abstract
4) Lines around 85, a reference could perhaps be given for the CIE colour matching functions?
References:
Aragón, J.L., Naumis, G.G., Bai, M., Torres, M. and Maini, P.K., 2008. Turbulent luminance in impassioned van Gogh paintings. Journal of Mathematical Imaging and Vision, 30(3), pp.275-283.
Bingen, C., Fussen, D. and Vanhellemont, F., 2004. A global climatology of stratospheric aerosol size distribution parameters derived from SAGE II data over the period 1984–2000: 1. Methodology and climatological observations. Journal of Geophysical Research: Atmospheres, 109(D6).
Fikke, S.M., Kristjánsson, J.E. and Nordli, Ø., 2017. Screaming clouds. Weather, 72(5), pp.115-121.
Hamblyn, R., 2002. The invention of clouds: How an amateur meteorologist forged the language of the skies. Pan Macmillan.
Klobas, E. J., Wilmouth, D.M., Weisenstein, D.K., Anderson, J.G. and Salawitch, R.J., 2017. Ozone depletion following future volcanic eruptions. Geophysical Research Letters, 44(14), pp.7490-7499.
Ming, A., Winton, V.H.L., Keeble, J., Abraham, N.L., Dalvi, M.C., Griffiths, P., Caillon, N., Jones, A.E., Mulvaney, R., Savarino, J. and Frey, M.M., 2020. Stratospheric ozone changes from explosive tropical volcanoes: Modeling and ice core constraints. Journal of Geophysical Research: Atmospheres, 125(11), p.e2019JD032290.
Olson, D.W., Doescher, R.L. and Olson, M.S., 2003. Dating Van Gogh's" Moonrise".
-
AC3: 'Reply on RC3', Christian von Savigny, 31 Aug 2022
The comment was uploaded in the form of a supplement: https://cp.copernicus.org/preprints/cp-2022-38/cp-2022-38-AC3-supplement.pdf
-
AC3: 'Reply on RC3', Christian von Savigny, 31 Aug 2022
- EC1: 'Comment on cp-2022-38', Denis-Didier Rousseau, 22 Jul 2022
Christian von Savigny et al.
Christian von Savigny et al.
Viewed
| HTML | XML | Total | BibTeX | EndNote | |
|---|---|---|---|---|---|
| 446 | 113 | 19 | 578 | 2 | 3 |
- HTML: 446
- PDF: 113
- XML: 19
- Total: 578
- BibTeX: 2
- EndNote: 3
Viewed (geographical distribution)
| Country | # | Views | % |
|---|
| Total: | 0 |
| HTML: | 0 |
| PDF: | 0 |
| XML: | 0 |
- 1