the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Estimation of aerosol and cloud radiative heating rate in tropical stratosphere using radiative kernel method
Abstract. A layer of aerosols has been identified in the upper troposphere and lower stratosphere above the Asian summer monsoon region, which is referred to as the Asian Tropopause Aerosol Layer (ATAL). This layer is fed by atmospheric pollutants over South and East Asia lifted to the upper troposphere by deep convection in summer. The radiative effects of this aerosol layer change local temperature, influence thermodynamic stability, and modulate the efficiency of air mass vertical transport near the tropopause. However, quantitative understanding of these effects is still very poor. To estimate aerosol radiative effects in the high atmosphere, a set of radiative kernels is constructed for the tropical upper troposphere and stratosphere to reduce the computational expense of decomposing the different contributions of atmospheric components to anomalies in radiative fluxes. The prototype aerosol kernels in this work are among the first to target vertically resolved heating rates, motivated by the linearity and separability of scattering and absorbing aerosol effects in ATAL. Observationally-derived lower boundary conditions and satellite observations of cloud ice within the upper troposphere and stratosphere are included and simplified in our Tropical Upper Troposphere-Stratosphere Model (TUTSM). Separate sets of kernels are derived and tested for the effects of absorbing aerosols, scattering aerosols, and cloud ice particles on both shortwave (solar) and longwave (thermal) radiative fluxes and heating rates. The results indicate that the kernels we calculated can well reproduce the aerosol radiative effects in ATAL, and these aerosol kernels are also expected to simulate radiative effects of biomass burning and volcanic eruption above troposphere. It has been proved this approach substantially reduces computational expense while achieving good consistency with direct radiative transfer model calculations. It can be applied to models that do not require high precision but have requirements for computing speed and storage space.
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CEC1: 'Comment on egusphere-2024-2815', Juan Antonio Añel, 27 Nov 2024
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Dear authors,
Unfortunately, after checking your manuscript, it has come to our attention that it does not comply with our "Code and Data Policy".
https://www.geoscientific-model-development.net/policies/code_and_data_policy.htmlFirst, in your work you use the RRTMG models, and in the "Code and Data Availability" section you link its webpage. This webpage is not a suitable repository for scientific publication; therefore, it does not comply with our policy. You must store the RRTMG models that you have used in one of the repositories that we accept. I note here that the RRTMG models do not include a license in their webpage, and as a consequence nobody can use them. It is an usual misunderstanding to think that making code available in a web page makes it free to anyone to use it, which is not the case. I recommend you to communicate with the RRTMG developers to make them aware of this, and include with their code a license that allows you and other to use the model, and deposit it in a suitable repository. Then you must reply to this comment with the link and DOi of the new repository containing the RRTMG models code. You should do this as soon as possible, as in its current version your manuscript does not comply with our policy, and we can not accept in Discussions manuscripts that do not do it.
Also, you must include the information on the new repository (DOI an link) in any potentially reviewed version of your manuscript.
Moreover, in your manuscript you state " All other codes are available from the corresponding author on request". First, our policy clearly states that all the code necessary to replicate the work exposed in a manuscript must be published and accessible to anyone at submission time. It is not clear what you mean by "all other codes"; however, we can not accept that it is necessary to contact you to get access to such code. Therefore, you must publish it following the same instructions than for the RRTMG models.
Please, address this issues and reply to this comment as soon as possible. Otherwise, we will have to reject your manuscript for publication because of lack of compliance with the policy of the journal.
Juan A. Añel
Geosci. Model Dev. Executive Editor
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Citation: https://doi.org/10.5194/egusphere-2024-2815-CEC1 -
AC1: 'Reply on CEC1', Jie Gao, 10 Dec 2024
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The RRTMG provide a license at the front of their instruction file (upload as the supplement file in response), I have uploaded the code of model I used and the instruction with license, at https://doi.org/10.5281/zenodo.14357597.The modifications about code availability in manuscript are in Line 508 - Line 510: "And RRTMG models are available at https://doi.org/10.5281/zenodo.14357597 (official website http://rtweb.aer.com/rrtm_frame.html), the license can be found at the front of instruction file.The codes for running RRTMG and calculating radiative kernels are available at https://doi.org/10.5281/zenodo.14359763."
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AC1: 'Reply on CEC1', Jie Gao, 10 Dec 2024
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RC1: 'Comment on egusphere-2024-2815', Hua Zhang, 05 Dec 2024
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This paper estimates the radiative fluxes and heating rates of absorbing aerosols, scattering aerosols, and cloud ice particles in tropical stratosphere using the newly developed radiative kernels. A notable merit of this study is the construction of aerosol kernels, and the application of them has the potential to better understand the radiative effects of aerosols in the upper troposphere and stratosphere.
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Major comments:
Line 221. It seems that the kernels are calculated by perturbing aerosols at each level simultaneously. To my knowledge, previous studies all established kernels (e.g., water vapor, cloud) by perturbing the variable at each level at one time. It is necessary to clarify and justify the choice.
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Line 285. The authors select four reference state boundary conditions for the kernel calculations. It is not clear why these four points are selected and why these points can represent clear-sky, low cloud, middle cloud, and high cloud conditions.
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Line 298. It seems that the changes of water vapor and ozone in the upper troposphere and stratosphere are ignored in the simulations. Any estimate of its impact?
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Line 299. The new kernels are constructed based on several linearity assumptions. However, it is not clear whether the cloud radiative effect varies linearly within a range of COD and whether the total radiative effects of aerosols and cloud ice can be represented as a linear sum of radiative effects associated with AOD and COD. It is necessary to validate these assumptions.
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Figures 2, 3, 5-7, S3. The authors select several months (i.e., January, May, July) to validate the assumptions of kernel calculations. Are these months representative? Are the test results in other months consistent with the results in these months?
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Other comments:
Line 200. Please correct the time range of reference state.
Line 314. “Figure 5 and Fig. 6”. Please use the uniform expression.
Lines 413, 420, 478, 496. Please correct the superscript and subscript.
Table 2. Please add RMSE for the kernel calculation.
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Citation: https://doi.org/10.5194/egusphere-2024-2815-RC1
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