the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
| 05 Jun 2024
The impact of QBO disruptions on diurnal tides over the low- and mid-latitude MLT region observed by a meteor radar chain
Abstract. A quasi-biennial oscillation (QBO) disruption is a very rare phenomenon in which QBO westward wind is temporarily interrupted by the occurrence of a band of westward wind in the tropical stratosphere. This phenomenon is important as it could greatly affect the global atmospheric circulation, especially in the mesosphere. Past observational and modelling studies have shown the QBO-varying mesospheric diurnal tide, but the mechanism is still not fully understood. In this study, we report the strong response of mesospheric diurnal tides to the two QBO disruptions that occurred in 2015/16 and 2019/20 and its possible mechanisms. The diurnal tidal winds are observed by a meteor radar chain, consisting of meteor radars located at Kunming (25.6° N, 103.8° E), Wuhan (30.5° N, 114.2° E), Mengcheng (33.4° N, 116.5° E), Beijing (40.3° N, 116.2° E) and Mohe (53.5° N, 122.3° E) in China. These observations provide clear evidence that mesospheric diurnal tides are unusually weakened (by ~-6 m/s) during these QBO disruptions, over Kunming, Wuhan, Mengcheng, and Beijing. By using the Specific Dynamics version of the Whole Atmosphere Community Climate Model with thermosphere and ionosphere extension (SD-WACCM-X) and the European Centre for Medium-Range Weather Forecasts (ECMWF) Reanalysis v5 (ERA5) dataset, the analysis indicates that the QBO wind affects mid-latitude mesospheric diurnal tides by modulating both the solar radiative absorption by subtropical stratospheric ozone (~5 to 0.5 hPa) and the tidal-gravity wave interaction in the mesosphere (~60 to 100 km). Thus, these unexpected QBO disruptions provide an opportunity to better understand the coupling between climate change and middle atmospheric dynamics.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2024-1662', Anonymous Referee #1, 21 Jul 2024
Review on " The impact of QBO disruptions on diurnal tides over the low- and mid-latitude MLT region observed by a meteor radar chain " by Jianyuan Wang, et al.Â
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This paper presents the impact of the QBO and QBO disruptions on diurnal tides in the MLT using meteor radars, ERA5 reanalysis, and SD-WACCM-X. The authors demonstrated that the eastward QBO wind enhances the diurnal tides, while the westward QBO wind suppresses the diurnal tides. This effect is interpreted in terms of the modulation of tidal sources and gravity waves by the QBO.
The investigated problem and the result are no doubt interesting to the community. The manuscript is well-organized and clearly written and the analysis of the relationship between QBO disruption and tidal winds scientifically sounds. I suggest its publication after minor revisions.
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Main: Although QBO disruption is a rare and special phenomenon, the authors should include an explanation of the differences between the impacts of QBO disruption and QBO westward wind on circulation and diurnal tides in the MLT.
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Minors:
Line 25: ‘its possible mechanisms’ should be ‘their possible mechanisms’
Â
Line 35: regions
Â
Line 54: 2003) and the
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Line 59: nightglows
Â
Line 68: Pramitha et al.
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Line 96: coordinates, and observational
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Line 241: It is necessary to explain why the ozone at 15°N is used to compare with the tropical ozone but not the ozone at other latitudes, such as 30°N.
Â
Line 326: the authors seem to think that the role of QBO westward winds and QBO disruptions are the same for the meridional circulation, but in fact, the circulation induced by the QBO disruption is different. Therefore, the impact of the two QBO disruption events on the meridional circulation and the distributions of O3 anomalies should be clearly discussed and explained.
Please also have a look at the references therein (incomplete list):
Diallo, M. A., Ploeger, F., Hegglin, M. I., Ern, M., Grooß, J.-U., Khaykin, S., and Riese, M.: Stratospheric water vapour and ozone response to the quasi-biennial oscillation disruptions in 2016 and 2020, Atmos. Chem. Phys., 22, 14303–14321, https://doi.org/10.5194/acp-22-14303-2022, 2022.
Wang, Y., Rao, J., Lu, Y., Ju, Z., Yang, J., Luo, J.: A revisit and comparison of the quasi-biennial oscillation (QBO) disruption events in 2015/16 and 2019/20, Atmospheric Research, 294, 106970,https://doi.org/10.1016/j.atmosres.2023.106970, 2023.
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Line 367: While the focus of the paper is on the diurnal tides, I think the variation in the background wind is interesting as well. Figure 8 shows the GWs is consistent with the QBO winds, and thus, the background winds may have QBO and QBO disruption signals in the MLT. If yes, then that is an interesting result. It appears that the QBO disruption can affect the MLT via more complex processes.
Citation: https://doi.org/10.5194/egusphere-2024-1662-RC1 - AC1: 'Reply on RC2', Jianyuan Wang, 27 Sep 2024
- AC2: 'Reply on RC1', Jianyuan Wang, 27 Sep 2024
-
RC2: 'Comment on egusphere-2024-1662', Alan Liu, 21 Aug 2024
Review
This work investigated the anomalous tidal amplitudes in association with the anomaly in QBO. The causes of the tidal anomaly, contributed to anomalous ozone transport and gravity wave filtering, are well explained and demonstrated through observations and modeling. The findings provide new insights of a coupling process between lower and middle/upper atmosphere on the interannual scale. This manuscript is of high scientific merit and high presentation quality.Â
There is one issue that I like to bring to the authors’ attention, which is the calculation of GW forcing on tides. The current method, comparing the phase offset between the tidal tendency and GW forcing to determine whether GW forcing is enhancing or decreasing tidal amplitude is appropriate only when the GW forcing is small relative to the frequency of the tides (1/24 hr). When the GW forcing is large, it changes the resulting tides significantly, both in amplitude and phase.  For example, adding a GW forcing that has 90 deg phase offset with a tide will not change the tide’s amplitude but shift its phase. The resultant tide is then not in 90-deg phase offset with the GW forcing. If one uses the GW-modified tide to compare with the GW forcing, one would find that the GW forcing should change the tidal amplitude (because they are not in 90-deg phase offset) which is incorrect. This issue was described in McLandres (2002) and a correction was described in Liu et al. (2013). Please consider using equation (10) in that paper to obtain a more accurate GW forcing effect on tides.
Â
Minor:
While figures 2,3,5 show meridional tidal amplitudes, Fig.4 shows correlation with zonal diurnal tidal amplitude. Why switching between zonal and meridional amplitudes?
322: ‘mounts’ -> ‘amounts’ ?
323: ‘relatively increases’ -> ‘increases’ ( ‘relatively’ can be associated with ‘larger’ as used in line 322 but not with ‘increase’)
324,325: why give units in the parenthesis? They are not associated with any numbers.
622: (A2) is missing Omega as a coefficient (after taking derivative of A1).Â
625: The meanings of GW_forcing and GW_drag are not described clearly.  It seems GW_drag is the diurnal amplitude of GW forcing, but it’s not stated.
Â
Â
References
McLandress, C. (2002), The seasonal variation of the propagating diurnal tide in the mesosphere and lower thermosphere. Part I: The role of gravity waves and planetary waves, J. Atmos. Sci., 59, 893-906,
Liu, A. Z., X. Lu, S. J. Franke (2013), Diurnal variation of gravity wave momentum flux and its forcing on the diurnal tide, J. Geophys. Res. Atmos., 118, 1668-1678, doi:10.1029/2012JD018653.
Â
Citation: https://doi.org/10.5194/egusphere-2024-1662-RC2 - AC1: 'Reply on RC2', Jianyuan Wang, 27 Sep 2024
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2024-1662', Anonymous Referee #1, 21 Jul 2024
Review on " The impact of QBO disruptions on diurnal tides over the low- and mid-latitude MLT region observed by a meteor radar chain " by Jianyuan Wang, et al.Â
Â
This paper presents the impact of the QBO and QBO disruptions on diurnal tides in the MLT using meteor radars, ERA5 reanalysis, and SD-WACCM-X. The authors demonstrated that the eastward QBO wind enhances the diurnal tides, while the westward QBO wind suppresses the diurnal tides. This effect is interpreted in terms of the modulation of tidal sources and gravity waves by the QBO.
The investigated problem and the result are no doubt interesting to the community. The manuscript is well-organized and clearly written and the analysis of the relationship between QBO disruption and tidal winds scientifically sounds. I suggest its publication after minor revisions.
Â
Main: Although QBO disruption is a rare and special phenomenon, the authors should include an explanation of the differences between the impacts of QBO disruption and QBO westward wind on circulation and diurnal tides in the MLT.
Â
Minors:
Line 25: ‘its possible mechanisms’ should be ‘their possible mechanisms’
Â
Line 35: regions
Â
Line 54: 2003) and the
Â
Line 59: nightglows
Â
Line 68: Pramitha et al.
Â
Line 96: coordinates, and observational
Â
Line 241: It is necessary to explain why the ozone at 15°N is used to compare with the tropical ozone but not the ozone at other latitudes, such as 30°N.
Â
Line 326: the authors seem to think that the role of QBO westward winds and QBO disruptions are the same for the meridional circulation, but in fact, the circulation induced by the QBO disruption is different. Therefore, the impact of the two QBO disruption events on the meridional circulation and the distributions of O3 anomalies should be clearly discussed and explained.
Please also have a look at the references therein (incomplete list):
Diallo, M. A., Ploeger, F., Hegglin, M. I., Ern, M., Grooß, J.-U., Khaykin, S., and Riese, M.: Stratospheric water vapour and ozone response to the quasi-biennial oscillation disruptions in 2016 and 2020, Atmos. Chem. Phys., 22, 14303–14321, https://doi.org/10.5194/acp-22-14303-2022, 2022.
Wang, Y., Rao, J., Lu, Y., Ju, Z., Yang, J., Luo, J.: A revisit and comparison of the quasi-biennial oscillation (QBO) disruption events in 2015/16 and 2019/20, Atmospheric Research, 294, 106970,https://doi.org/10.1016/j.atmosres.2023.106970, 2023.
Â
Line 367: While the focus of the paper is on the diurnal tides, I think the variation in the background wind is interesting as well. Figure 8 shows the GWs is consistent with the QBO winds, and thus, the background winds may have QBO and QBO disruption signals in the MLT. If yes, then that is an interesting result. It appears that the QBO disruption can affect the MLT via more complex processes.
Citation: https://doi.org/10.5194/egusphere-2024-1662-RC1 - AC1: 'Reply on RC2', Jianyuan Wang, 27 Sep 2024
- AC2: 'Reply on RC1', Jianyuan Wang, 27 Sep 2024
-
RC2: 'Comment on egusphere-2024-1662', Alan Liu, 21 Aug 2024
Review
This work investigated the anomalous tidal amplitudes in association with the anomaly in QBO. The causes of the tidal anomaly, contributed to anomalous ozone transport and gravity wave filtering, are well explained and demonstrated through observations and modeling. The findings provide new insights of a coupling process between lower and middle/upper atmosphere on the interannual scale. This manuscript is of high scientific merit and high presentation quality.Â
There is one issue that I like to bring to the authors’ attention, which is the calculation of GW forcing on tides. The current method, comparing the phase offset between the tidal tendency and GW forcing to determine whether GW forcing is enhancing or decreasing tidal amplitude is appropriate only when the GW forcing is small relative to the frequency of the tides (1/24 hr). When the GW forcing is large, it changes the resulting tides significantly, both in amplitude and phase.  For example, adding a GW forcing that has 90 deg phase offset with a tide will not change the tide’s amplitude but shift its phase. The resultant tide is then not in 90-deg phase offset with the GW forcing. If one uses the GW-modified tide to compare with the GW forcing, one would find that the GW forcing should change the tidal amplitude (because they are not in 90-deg phase offset) which is incorrect. This issue was described in McLandres (2002) and a correction was described in Liu et al. (2013). Please consider using equation (10) in that paper to obtain a more accurate GW forcing effect on tides.
Â
Minor:
While figures 2,3,5 show meridional tidal amplitudes, Fig.4 shows correlation with zonal diurnal tidal amplitude. Why switching between zonal and meridional amplitudes?
322: ‘mounts’ -> ‘amounts’ ?
323: ‘relatively increases’ -> ‘increases’ ( ‘relatively’ can be associated with ‘larger’ as used in line 322 but not with ‘increase’)
324,325: why give units in the parenthesis? They are not associated with any numbers.
622: (A2) is missing Omega as a coefficient (after taking derivative of A1).Â
625: The meanings of GW_forcing and GW_drag are not described clearly.  It seems GW_drag is the diurnal amplitude of GW forcing, but it’s not stated.
Â
Â
References
McLandress, C. (2002), The seasonal variation of the propagating diurnal tide in the mesosphere and lower thermosphere. Part I: The role of gravity waves and planetary waves, J. Atmos. Sci., 59, 893-906,
Liu, A. Z., X. Lu, S. J. Franke (2013), Diurnal variation of gravity wave momentum flux and its forcing on the diurnal tide, J. Geophys. Res. Atmos., 118, 1668-1678, doi:10.1029/2012JD018653.
Â
Citation: https://doi.org/10.5194/egusphere-2024-1662-RC2 - AC1: 'Reply on RC2', Jianyuan Wang, 27 Sep 2024
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Jianyuan Wang
Iain Reid
Jianfei Wu
Hailun Ye
Jian Li
Zonghua Ding
Jinsong Chen
Guozhu Li
Yaoyu Tian
Boyuan Chang
Jiajing Wu
Lei Zhao
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(2199 KB) - Metadata XML