Abstract

Abstract. We examine sunsets painted by famous artists as proxy information for the aerosol optical depth after major volcanic eruptions. Images derived from precision colour protocols applied to the paintings were compared to online images, and found that the latter, previously analysed, provide accurate information. Aerosol optical depths (AODs) at 550 nm, corresponding to Northern Hemisphere middle latitudes, calculated by introducing red-to-green (R / G) ratios from a large number of paintings to a radiative transfer model, were significantly correlated with independent proxies from stratospheric AOD and optical extinction data, the dust veil index, and ice core volcanic indices. AODs calculated from paintings were grouped into 50-year intervals from 1500 to 2000. The year of each eruption and the 3 following years were defined as "volcanic". The remaining "non-volcanic" years were used to provide additional evidence of a multidecadal increase in the atmospheric optical depths during the industrial "revolution". The increase of AOD at 550 nm calculated from the paintings grows from 0.15 in the middle 19th century to about 0.20 by the end of the 20th century. To corroborate our findings, an experiment was designed in which a master painter/colourist painted successive sunsets during and after the passage of Saharan aerosols over the island of Hydra in Greece. Independent solar radiometric measurements confirmed that the master colourist's R / G ratios which were used to model his AODs, matched the AOD values measured in situ by co-located sun photometers during the declining phase of the Saharan aerosol. An independent experiment was performed to understand the difference between R / G ratios calculated from a typical volcanic aerosol and those measured from the mineral aerosol during the Hydra experiment. It was found that the differences in terms of R / G ratios were small, ranging between −2.6% and +1.6%. Also, when analysing different parts of cloudless skies of paintings following major volcanic eruptions, any structural differences seen in the paintings had not altered the results discussed above. However, a detailed study on all possible sources of uncertainties involved (such as the impact of clouds on R / G ratios) still needs to be studied. Because of the large number of paintings studied, we tentatively propose the conclusion that regardless of the school, red-to-green ratios from great masters can provide independent proxy AODs that correlate with widely accepted proxies and with independent measurements.

Highlights

  • The typical size and vertical profile of the Saharan aerosols differ from the volcanic ones, their effect on solar irradiance and R / G close to sunset was proved to be significant because of their relative high values of Aerosol optical depths (AODs) (∼ 0.25 at 500 nm)

  • The AOD values observed at Hydra, for the most part, can be attributed to the presence of the Saharan dust aerosol and follow the temporal evolution depicted by the dust simulations shown in Fig. 6, from which we see higher AOD values on 19 June and lower on the day at Hydra

  • A series of paintings by master painters have been revisited and comparisons between digital images of paintings from lower resolution vs. high resolution, derived from high precision protocols, showed similar results, as far as the R / G ratios measured at sunsets are concerned

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Summary

Introduction

Digital images from 554 paintings were downloaded from the websites of several art galleries and museums These images were processed to derive ratios between the intensities of monochromatic colours. The study by Zerefos et al (2007) concluded that regardle4ss oFf itghuere 1 school or the style of the painter, the R / G ratios at low solar elevation angles, correlated well to the modelled aer5osol optical depth (AOD) values following large volcanic eruptions. In this work we provide new evidence that our earlier results, based on R / G ratios to estimate and model AODs in paintings are robust, a hypothesis which is supported using the following three methods: firstly, by correlating the available R / G ratios from the above-mentioned public websites with the same ratios from their respective high quality colour profile protocols.

Comparison between high and low quality digital images of paintings
A live case: the Hydra experiment
Experiment organization and instrumentation
Experimental Results and discussion
Figure 8
Conclusions
Figure 9
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Full Text
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