Articles | Volume 18, issue 19
https://doi.org/10.5194/amt-18-5037-2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.Comparison of total ozone measurements in Melbourne, Australia, performed with a low-cost micro spectrometer and a Brewer MK-III
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- Final revised paper (published on 02 Oct 2025)
- Preprint (discussion started on 17 Feb 2025)
Interactive discussion
Status: closed
Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor
| : Report abuse
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RC1: 'Comment on egusphere-2025-87', Anonymous Referee #1, 11 Mar 2025
- AC1: 'Reply on RC1', Kåre Edvardsen, 06 Jun 2025
- AC2: 'Reply on RC2', Kåre Edvardsen, 06 Jun 2025
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RC2: 'Comment on egusphere-2025-87', Anonymous Referee #2, 19 Mar 2025
- AC2: 'Reply on RC2', Kåre Edvardsen, 06 Jun 2025
- AC1: 'Reply on RC1', Kåre Edvardsen, 06 Jun 2025
Peer review completion
AR: Author's response | RR: Referee report | ED: Editor decision | EF: Editorial file upload
AR by Kåre Edvardsen on behalf of the Authors (06 Jun 2025)
Author's response
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ED: Referee Nomination & Report Request started (10 Jun 2025) by Mark Weber
RR by Anonymous Referee #2 (10 Jul 2025)
ED: Publish as is (17 Jul 2025) by Mark Weber
AR by Kåre Edvardsen on behalf of the Authors (11 Aug 2025)
Review of
Comparison of total ozone measurements in Melbourne, Australia, performed with a low-cost micro spectrometer and a Brewer MK-III
Kåre Edvardsen, Matt Tully, Steve Rhodes
Submitted to https://doi.org/10.5194/egusphere-2025-87 Preprint. Discussion started: 17 February 2025
General comments:
This paper provides a description of the methods to derive total column ozone (TCO) from a very low-cost instrument measuring global ultra-violet irradiance. The paper is well written, well structured and the methods are clearly described. It is recommended for publication after addressing the comments below.
The paper focuses rather on the method of TCO retrial rather than a sound analysis of the performance of TCO compared to a reference instrument. Therefore, the general comments are divided into two following parts:
Method:
Commonly, TCO is derived best by direct sun measurements. The paper uses global UV measurements, which implicate parameters of uncertainty such as clouds in front of the sun, clouds in the sky, effective albedo from the surrounding terrain and cosine response of the diffusor. All these effects would not occur when using direct sun measurements. The authors argue that in many places worldwide cloud coverage hinder direct sun measurement for TCO. Are there so many places with such conditions? Maybe the performance of the low-cost instrument would be much better when using direct sun measurements. Has this ever been tested with the instrument?
The method includes many parametrizations based on empirical functions. I have lost the overview. Maybe the authors can provide a summary of all the empirical parametrizations, the number of measurements needed for the parametrization and, if possible, an estimation of the uncertainty of the parametrization and its implication of TCO.
The parametrization also arises the question if the method is also suitable for other placed world wide, once it has “calibrated” with a Brewer at a specific site. Or must the method be “calibrated” for each location worldwide separately with a Brewer?
Performance:
It is not clear if the authors have compared daily averages with quasi synchronous measurements for STS GI and Brewer DS. I suggest comparing synchronous measurements within e.g. 10 minutes intervall and also show the individual measurements to indicate the variation of TCO.
Commonly these small low cost spectrometers suffer from straylight, which biases TCO at low solar zenith angles or high ozone slant columns. In order to assess the performance of the instrument the comparison between the Brewer and STS GI depending on ozone slant column (airmass * TCO) should be provided.
Temperature dependency. Indeed, the dependency of the small array spectroradiometer is a crucial issue of these instruments. Ambient temperature causes wavelength shifts, linearity and detectability problems (signal to noise ratio etc.). I am surprised that a simple parametrization (Eq. 2) can account for that. It would be worthful to calculate the uncertainty of TCO based on the parametrization and its applicability for other instruments and other locations.
Furthermore, the model includes the ozone absorption cross section, which depends on the effective ozone temperature (basically stratospheric temperature). How sensitive is the algorithm and resulting TCO on effective ozone temperature?
Specific comments:
Page 2: line 32: How significant is the fraction of the price of the Brewer. To my estimate it is about 10% of a Brewer, which is already low cost.
Page 2, line 47: Is the MK II Brewer a double monochromator with insignificant stray light impact?
Page 2, line 60: Can the method be described as a cloud correction?
Page 3 line 89: The reference is missing
Page 4 line 95: What is the slit function and full width half maximum of the instrument, resulting from 25 micron slit?
Page 5 line 126: Do you mean ozone slant column (=airmass * TCO) - > see comment above.
Page 5: 132: and EQ 1 is this parametrization also applicable at other locations
Page 5, line 146. Again, what is the full width half maximum of the slit function?
Table 1: It would be worthful to indicate the performance in percent
Caption Figure 2: SZ -> ZS
Figure 4. The ratio between Brewer and STS would be more helpful
Page 11 line 280: Why is TCO increasing with temperature? Wavelength shift?:
Page 11 line 286: I suggest using quasi simultaneous measurements.
Page 12 line 310: At what conditions is STS comparable to the Brewer? What are the limitations?
Page 13: line 324. The conclusion should not end with a bullet list. Maybe a closing sentence would help.