Simulation of Atmospheric Ozone Layer Formation and Study on the Influence of Equatorial Atmospheric Vertical Motion on the Ozone Layer
Abstract. Stratospheric ozone is crucial for protecting terrestrial ecosystems and maintaining climate stability by absorbing solar ultraviolet radiation. Its distribution is jointly determined by photochemical reactions and atmospheric dynamic processes. Equatorial vertical motion, as a key component of global circulation, profoundly influences ozone production and depletion by regulating precursor transport, photolysis rates, and temperature fields. Based on the Chapman mechanism and catalytic reaction theory, this study establishes a photochemical-dynamic coupled numerical model covering the surface to 500 km, simulating the formation process of the equatorial ozone layer. Through multiple controlled experiments, the effects of vertical motions with different intensities are systematically quantified. Results demonstrate that vertical motion significantly reshapes the steady state and structure of the ozone layer: stronger motion leads to reduced ozone layer thickness, elevated concentration peak altitude, and a transition from multi-peak to nearly single-peak vertical distribution. Notably, the simulations reveal for the first time that in the absence of external dynamic forcing apart from Earth’s revolution around the Sun and its rotation, the ozone system itself exhibits an intrinsic oscillation period of approximately 31 months. Based on this finding, we propose a novel scientific hypothesis: this intrinsic period may serve as a "baseline frequency anchor" that facilitates research on the periods of the stratospheric Quasi-Biennial Oscillation (QBO) and the Tropospheric Biennial Oscillation (TBO). This suggests that the ozone layer may not be merely a passive responder within the climate system, but rather an active component with autonomous oscillation capability capable of modulating atmospheric circulation through radiative feedbacks. This study provides new numerical evidence and theoretical perspectives for understanding the spatiotemporal evolution of the ozone layer and stratosphere-troposphere interactions.
This paper attempts to study the ozone layer formation and the influence of vertical model on ozone. This paper does not meet the standards I would expect of a credible scientific work submitted to ACP as a preprint.
Main criticisms:
- The experimental design section does not include enough detail for this study to be reproducible.
- The results section consists of a series of poorly formatted bullet points and low resolution figures. The references have not been checked. I.P. Gibel is not the correct author for the paper listed.
- The model top is at 500 km with 47 vertical levels. Ozone concentrations peak at about 40 km. There is little justification for studying beyond ~100 km (conventional definition of the edge of space).
- Many values seem to be off by an order of magnitude. For example, the authors claim that " Vertical velocities in the stratosphere typically range from 0.3–2 cm/s". Typical upwelling values are in the range 0.2 to 0.5 mm/s [1]. With no vertical motion, the total column ozone in their model is ~2500 DU. Observed global mean total column ozone is around 300 DU [2]. The model appears to need unrealisticaly high stratospheric upwelling to produce realistic ozone values of ~270 DU.
References:
[1] Butchart, N. (2014), The Brewer-Dobson circulation, Rev. Geophys., 52, doi:10.1002/2013RG000448.
[2] Chipperfield, M. P. and Bekki, S.: Opinion: Stratospheric ozone – depletion, recovery and new challenges, Atmos. Chem. Phys., 24, 2783–2802, https://doi.org/10.5194/acp-24-2783-2024, 2024.