A numerical experiment on the formation of the tropopause inversion layer associated with an explosive cyclogenesis: possible role of gravity waves
© Otsuka et al.; licensee Springer. 2014
Received: 7 April 2014
Accepted: 23 August 2014
Published: 30 September 2014
The tropopause inversion layer (TIL) is a persistent layer with high static stability. Although some mechanisms for the formation of the TIL have been proposed, the time evolution of the TIL under realistic conditions especially when factoring in the contribution of small-scale processes such as gravity waves is not well understood. To gain an understanding of this factor, we conducted a numerical experiment on an explosive cyclogenesis in mid-latitudes using a nonhydrostatic regional atmospheric model. Although the TIL in the model is consistent with previous observations in the sense that it is stronger in the negative vorticity areas, the relationship is clear only in the development and mature stages of a cyclone, suggesting that the evolution of the cyclone plays an important role in the formation of the TIL. To ascertain the effects of gravity waves on the TIL, vertical convergence at the tropopause is analyzed. Histograms of maximum buoyancy frequency squared within the TIL show that regions of vertical convergence have higher , in addition to regions with high ∂2 w/∂ z2, implying that waves having downward phase propagation also play an important role in the dynamical formation of the TIL. This tendency is clearer in regions of negative relative vorticity at the tropopause. By taking account of the fact that the gravity wave activities associated with the cyclone and the jet streak are enhanced during the development and mature stages of the cyclone, vertical convergence due to gravity waves associated with synoptic weather systems can be seen to be a key process in the formation of the negative correlation between the strength of the TIL and the local relative vorticity at the tropopause.
KeywordsTropopause inversion layer Extratropical cyclone Gravity wave
The tropopause inversion layer (TIL) is a layer with enhanced static stability just above the tropopause, and it has been extensively studied over the past decade (e.g., Birner et al. ; ). The TIL is observed at all latitudes from the tropics to the polar regions (e.g., Randel et al. ; Tomikawa et al. ; Son et al. ). The TIL exhibits a dependence on the relative vorticity around the tropopause, in that anticyclones exhibit substantially stronger inversion than cyclones (Zängl and Wirth ; Randel et al. . This vorticity dependence has also been reproduced in idealized numerical simulations (e.g., Son and Polvani ). In general, two major mechanisms for TIL formation have been proposed: dynamical formation (e.g., Wirth ) and radiative formation (e.g., Randel et al. ; Randel and Wu ). Wirth (, ) applied a theory of conservative balanced dynamics to axisymmetric cyclonic and anticyclonic vorticies on a mid-latitude f plane to explain the dependence of the TIL on vorticity. Idealized baroclinic life cycle experiments also support the formation of the TIL by dry dynamics (Wirth and Szabo ; Müller and Wirth ; Erler and Wirth ). Birner () reported that a static stability forcing associated with stratospheric residual circulation represents the main cause for the zonal mean TIL in winter mid-latitudes. Erler and Wirth  showed that wave breaking in baroclinic life cycle experiments is important for producing asymmetry between cyclonic and anticyclonic vorticies, resulting in net production of the TIL - even in zonal mean statistics. As for radiative formation, Randel et al.  performed one-dimensional radiative transfer calculations, in which strong gradients in both ozone and water vapor near the tropopause contribute to the formation of the TIL. Randel and Wu  reported that the radiative influence of water vapor provides a primary mechanism for the summer inversion layer in the polar region. These formation processes depend on latitude and season; for example, dynamical formation is considered to be important in winter mid-latitudes, whereas radiative formation is dominant in polar summer (Birner ; Miyazaki et al. [2010b]; Randel and Wu ).
In addition to these processes, Müller and Wirth () stated that gravity waves, turbulence, and deep convection may be important for the formation of the TIL. Of these processes, however, the effect of gravity waves on the formation of the TIL is not well understood yet. Previous studies focused on idealized theories (Wirth , ), and researchers performed numerical experiments using idealized systems (e.g., Erler and Wirth ; Müller and Wirth ; Son and Polvani ; Wirth and Szabo ), and analyzed them from a global point of view (e.g., Birner ; Miyazaki et al. [2010b]; Randel et al. ). Thus, time-dependent small-scale processes around the TIL are not fully understood yet. Gravity wave activity around the TIL is considered to be important in terms of mixing. Miyazaki et al. [2010a] reported that the degree of mixing around the TIL due to small-scale processes is high, and the local Richardson number tends to be less than 0.25, indicating higher possibilities of gravity wave breaking around the TIL. Mixing around the tropopause leads to material exchange between the stratosphere and the troposphere.
Motivated by these studies, the objective of this work is as follows. The first question is how the TIL evolves in a realistic life cycle of an extratropical cyclone in winter mid-latitudes, in which dynamical formation mechanisms seem to be dominant. The second question is how small-scale processes such as gravity waves contribute to the TIL. To address these questions, a case study on a realistic explosive extratropical cyclogenesis is conducted using a mesoscale regional atmospheric model. Although this case study provides only limited statistics on the small-scale processes around the TIL, it will fill in the gap in previous studies.
The rest of this paper is organized as follows. The ‘Methods’ section describes the numerical model. The ‘Results’ section gives the results of the numerical experiment and analyses for the TIL. In the ‘Discussion’ section, implications of the results are discussed, and the ‘Conclusions’ section provides our conclusions.
The cumulus parameterization scheme is a modified Kain-Fritsch. The cloud microphysics scheme is a 6-class bulk microphysics. The GSM0412 radiation scheme ([Yabu et al. 2005]) and an improved Mellor-Yamada Level-3 planetary boundary layer scheme ([Nakanishi and Niino 2004]; ) are used. The time constant for the nonlinear diffusion term is 1,200 s and that for the linear diffusion term is 600 s. The National Centers for Environmental Prediction (NCEP) Global Tropospheric Analyses (final analyses, FNL) with a horizontal resolution of 1°×1° and a time interval of 6 h are used as the initial and boundary conditions of the model.
Water vapor and ozone are important species for the radiative formation of the TIL as noted in the ‘Background’ section. In our experiment, water vapor is a prognostic variable in the model and contributes to the formation of the TIL. The ozone distribution is taken from three-dimensional monthly mean climatology interpolated in time and does not follow the temporal change of the local tropopause.
The two horizontal axes of the model domain are denoted by x (almost eastward) and y (almost northward). Note that the zonal wind u in this paper denotes the wind component in the x direction, and the meridional wind v denotes that in the y direction.
3.1 Synoptic evolution
This subsection presents an overview of the cyclogenesis during the period of the experiment. Figure 1a,b,c,d,e shows the horizontal distributions of temperature (color) and geopotential height (contour) at 950 hPa for the entire computational domain at 12-h intervals. The explosive cyclogenesis is captured by this simulation as follows. At t=12 h, a cyclone starts to develop over Japan. The horizontal gradient of temperature becomes steeper, leading to frontogenesis. At t=36 h, the cyclone moves to the east of Hokkaido Island, at which time the central pressure drops to the lowest in the cyclone’s life. At t=48 h, the cyclone moves to the east of the Kamchatka Peninsula, and the sharp core of the cyclone starts to decay. The model domain covers the cyclone throughout the period of the experiment. The domain also covers an anticyclone to the east of the cyclone until t=24 h and another anticyclone to the west from t=24 h. Asymmetry between the cyclone and the anticyclones is large; the cyclone is deeper and compact, and the anticyclones are wider. Although this asymmetry may create some bias in domain-averaged statistics on the TIL, the main purpose of the paper is to describe the time evolution of the TIL with fine-scale structures, and global or zonal mean statistics are beyond the scope of this study.
Figure 1f shows a time series of minimum sea level pressure within the computational domain. As the cyclone develops, the pressure starts to decrease from t=10 h. The pressure becomes the lowest, 965 hPa, at around t=36 h and then starts to increase. The pressure decreases nearly 35 hPa in 24 h between 35 and 45°N, which satisfies the criterion for a ‘bomb’ cyclone by put forward by Sanders and Gyakum (). As the position and the central pressure of the cyclone at t=36 h are almost the same as those in the JMA analysis ([Japan Meteorological Agency 2009]), we consider that the model simulates the cyclone realistically. In this paper, we define the development stage of the cyclone as the period from 10 to 36 h; its typical snapshot is at t=24 h, and the mature stage is at t=36 h.
Figure 3b shows the vertical component of relative vorticity at Z TP (hereafter ζ TP) at t=36 h. Horizontal winds at Z TP are also shown by arrows. A spiral pattern of positive and negative vorticities associated with the cyclone is discernible. The highest ζ TP is obtained around 145 to 150°E, 40 to 45°N, which is located to the north of the jet exit region and to the east of the surface cyclone. The lowest ζ TP is obtained around 160 to 165°E, 45°N. The region of ζ TP>0 along the northern edge of the jet streak (southern edge of the analysis region) is caused by the horizontal wind shear of the jet streak. A spiral band of ζ TP>0 extending to the northwestern corner of the domain coincides with the northeastern edge of strong westerlies at the tropopause level. Within the analysis region, the area of positive ζ TP is greater than that of negative ζ TP. Thus, data are binned by ζ TP and normalized by the sample size to ensure that the conclusions are not biased by the difference of positive and negative ζ TP areas.
3.2 Relationship between TIL and relative vorticity at tropopause
Figure 4b is the same as Figure 4a but for the buoyancy frequency squared (N2). The tropospheric N2 (4 km below the tropopause) is about 1.5×10−4 s −2, whereas the stratospheric N2 (4 km above the tropopause) is about 3 to 4×10−4 s −2. The profiles for ζ TP<0 show a sharp local maximum just above the tropopause and a sharp local minimum just below the tropopause (except for −5×10−5≤ζ TP<0 s −1), whereas the profiles for ζ TP>0 show a smooth transition from the troposphere to the stratosphere without sharp peaks. As ζ TP increases, the sharpness of the N2 profiles decreases. Following [Birner et al. (2006]), the maximum N2 within the temperature inversion (denoted by ) is used as a measure of the strength of the TIL in the following analyses. In this study, is searched for within 4 km above the local tropopause.
The horizontal map of at t=36 h is shown in Figure 3c. Regions with high are located to the north of the surface cyclone, whereas regions with low are located around the south edge of the analysis region. The distribution of around the cyclone is similar to that in the idealized simulation with dry dynamics by [Wirth and Szabo (2007]) (their Figure three), implying common mechanisms between these two simulations. A comparison of Figure 3b,c shows that regions with high (low) coincide with negative (positive) ζ TP. Thus, in general, a negative correlation exists between ζ TP and in the horizontal distributions at t=36 h. However, the regions of ζ TP<0 in the eastern part of the domain coincide with greater than 8×10−4 s −2 (red regions in Figure 3c), whereas those with similar negative values of ζ TP in the western part coincide with less than 7×10−4 s −2 (green and blue regions in Figure 3c), implying the existence of other factors that determine .
From t=24 to 42 h, a clear negative correlation between ζ TP and is obtained with a correlation coefficient of about −0.7. The linear regressions of as functions of ζ TP (black lines in Figure 5) show steeper slopes, and the regressed values become about 7×10−4 s −2 around ζ TP=−1×10−4 s −2, and about 5 × 10−4 s −2 around ζ TP>2 × 10−4 s −1. The proportionality coefficient between ζ TP and the mean for ζ TP<0 is about −1, which is somewhat smaller than that for the reference run in [Erler and Wirth (2011]), presumably due to the coarser spatial resolution of our model. The deviations from the regression lines are partly due to small-scalel disturbances such as gravity waves, which will be discussed in the following subsections.
From t=42 to 48 h, the negative correlation between ζ TP and becomes weaker, and the correlation coefficient becomes about −0.6 at t=48 h. The linear regression slope becomes gentler. In summary, the negative correlation between ζ TP and is clearer during the development and mature stages of the cyclone, whereas it is unclear before and after that period.
3.3 Analysis of gravity waves around the tropopause
The arc-shaped waves are robustly simulated in sensitivity experiments with different horizontal resolutions (15 and 20 km), vertical resolutions (50 layers and 210 layers), numerical integration time steps (10 and 20 s), time constants for nonlinear numerical diffusion (1,200 and 2,400 s), or time constants for linear numerical diffusion (600 and 2,400 s). If the number of vertical layers is reduced to 50, the amplitude of the arc-shaped waves in ∂ w/∂ z becomes slightly weaker, and the associated peak in also becomes smaller (not shown). The resolution dependency of the peak is consistent with the results of the idealized experiment by Müller and Wirth (). On the other hand, the weakening of the TIL around the center of the cyclone also becomes gentle. Although the small-scale structures are different, the time evolution of the arc-shaped waves and the negative correlation between ζ TP and does not change much.
3.3.1 Vertically propagating disturbances
If the phase propagation is downward (m/ω<0), N2 and ∂2 w/∂ z2 become in phase. For simplicity, the feedback from the changes in N2 to the dispersion relation of the wave is considered to be free from the variation in N2 in this paper. Nonlinearity in the TIL (e.g., Miyazaki et al. [2010a]) is beyond the scope of this paper, which focuses on a diagnosis of linear wave propagation.
3.3.2 Stationary disturbances
In this case, −∂ w/∂ z and N2 are in phase.
gives an intrinsic frequency – 4.1×10−4 s −1, or a period of about 2.5– 3.7×102 minutes. Here, ω denotes the frequency in a fixed frame of reference, k and l are the wavenumbers along the x and y directions, respectively, and k≡(k,l,m). We assume k>0, l<0, and m<0 from the phase lines in Figures 6 and 7. Substituting environmental wind speeds of of about (2.8×10, 3.2×10, 1.8×10−2) m s −1, ω becomes −5.4 to −4.0×10−4 s −1 or a period of about 1.9 to 2.6×102 min. In the model, the period at a fixed point is about 2.0×102 min with northward phase propagation, or ω=−5.2×10−3 s −1, which is close to the value estimated from Equation 11. Thus, this wave satisfies the dispersion relation for an inertia-gravity wave.
From a hodograph analysis of high-pass filtered horizontal winds, it is also confirmed that the wave is an inertia-gravity wave that has a downward phase speed (not shown). Although detailed analysis of gravity waves is beyond the scope of this paper, several discussions will be presented later.
3.4 Relationship between TIL and gravity waves
In this subsection, the relationship between the TIL and the gravity waves is further examined to ascertain if the vertical convergence shown in Figure 7 is the dominant factor in the strengthening of the TIL during the development and mature stages of the cyclone.
In Figure 7, ∂ w/∂ z is in quadrature with N2 in the stratosphere; the local maxima of N2 are located between the local maxima of ∂ w/∂ z above and the local minima below. From Equations 6 to 7, this implies that the wave pattern for N2 is produced by the downward propagating wave disturbance of w, which is consistent with the analysis in the previous subsection that indicated that the wave with a downward phase speed is an inertia-gravity wave. These high- N2 regions are detected as TILs.
It is important to confirm that the amplitudes of the wave patterns in N2 and w are consistent with each other. From Equation 6, the amplitude of N2 becomes A m N2/ω. In Figure 7, the amplitude of ∂ w/∂ z, which becomes Am, is about 5×10−5 s −1. Substituting A m=5×10−5 s −1, N2=5×10−4 s −2, and ω=3.1×10−4 s −1 into Equation 6, the amplitude of the wave pattern of N2 is estimated to be 8.3×10−5 s −2, whereas the actual amplitude in Figure 7 is about 10−4 s −2. These are the same order of magnitude as each other. As the amplitude of the wave pattern for N2 is proportional to N2, the wave pattern is clearly seen only within the TIL (Figure 7).
First, differences due to the sign of ζ TP are examined (Figure 8a). The peak for ζ TP<0 appears at s −2, whereas that for ζ TP≥0 appears at s −2. This result is consistent with the negative correlation between ζ TP and in Figures 4 to 5.
It is not a straightforward task to test the statistical significance of spatially correlated samples with appropriate estimates of correlation scales. Thus, we have adopted the moving block bootstrap method ([Künsch 1989]) to test the statistical significance of the differences in mean . Because the optimum block size is unknown, we choose block sizes of 10×10×5, 20×20×10, and 40×40×10 grid points (or, equivalently 200 km × 200 km × 5 h, 400 km × 400 km × 10 h, and 800 km × 800 km × 10 h) in the x, y, and t directions. We obtained 10,000 bootstrap observations each. As a result, the differences in the means in Figure 8a,c are significant to levels higher than 99% except for Figure 8c with the largest block size (see the values at the top left of each figure). The difference in the means in Figure 8b is not as significant as that in other pairs of data except the smallest block size. Statistical tests for Figures 9 and 10 are more difficult to construct, and will not be shown in this paper.
In our experiment, the TIL is formed as the cyclone develops. During the development and mature stages of the cyclone, the negative correlation between ζ TP and becomes clearer (Figure 5). In particular, for negative ζ TP increases, whereas for positive ζ TP decreases. This is consistent with the results of idealized simulations by [Wirth and Szabo (2007]) and [Erler and Wirth (2011]), in which the TIL becomes sharper as baroclinically unstable disturbances develop, and the TIL decays as the cyclone decays. Our experiment confirms that the TIL shows a similar time evolution in a realistic life cycle of an extratropical cyclone.
From Equations 6 to 10, it is expected that a steady disturbance of ∂ w/∂ z produces a pattern of N2 that is in phase with −∂ w/∂ z, whereas a downward-propagating wave produces a pattern of N2 that is in phase with ∂2 w/∂ z2. As shown in Figure 8, has a negative correlation with ∂ w/∂ z, whereas has a positive correlation with ∂2 w/∂ z2. From these two facts, it is concluded that the TIL in our model result is strongly controlled by the dynamical processes. In particular, inertia-gravity waves, which have not been investigated in depth in previous studies on the TIL, play a significant role. Note that the western half of the analysis region is dominated by nearly stationary patterns of ∂ w/∂ z by the synoptic disturbances and the mountain waves, whereas the eastern half is dominated by the effect of vertically propagating gravity waves. Although both the western and eastern sides contribute to the negative correlation between ζ TP and , the eastern side exhibits both the highest and the lowest values. The lowest appears around the center of the cyclone and the highest is produced by the arc-shaped wave packet. This fact also implies that the development of the cyclone and the radiation of the gravity waves are important for the development of the negative correlation.
Radiation of inertia-gravity waves from synoptic systems has been investigated by several groups using numerical experiments (e.g., O’Sullivan and Dunkerton ; Plougonven and Snyder ; Zhang ; Zülicke and Peters ). For example, [Plougonven and Snyder (2007]) simulated two types of wave packets generated around the tropopause region in a so-called LC2-type baroclinic life cycle experiment. The arc-shaped packet of the inertia-gravity waves shown in Figure 6 is similar to that in previous studies and can be considered a representative feature associated with developing baroclinic disturbances. Under the assumption that gravity waves of this type are ubiquitous around synoptic systems in the extratropics, the enhancement of the TIL by gravity waves may have an impact on the climatology of the TIL. Furthermore, gravity waves generated at the exit region of jet streaks tend to experience ‘wave capture’ (e.g., McIntyre ), staying within the same region relative to the synoptic disturbances. Thus, these gravity waves may not be just linear and transient features, but could be more persistent forcings to the tropopause region through nonlinear interactions. This may be the reason the negative correlation between ζ TP and is clearer during the development and mature stages of the cyclone. Thus, this relationship among gravity waves, ζ TP, and could be a general feature associated with extratropical cyclones. Proving the statistical significance of the effect of gravity waves radiated from synoptic disturbances is a subject we plan to investigate in the future using a regional atmospheric model.
In total, 99 temperature profiles having local tropopauses below 14 km are selected at 35 stations from 0000 UTC 20 to 0000 UTC 21 February, 2009, and is computed for each profile. Figure 11c shows the scatter diagram between the observed (the horizontal axis) and model (the vertical axis) at the same time and place. The model values are linearly interpolated to the corresponding observation sites. The correlation coefficient between the observed and simulated is 0.59. The mean in the model is 5.3×10−4 s −2, whereas that in the observation is 5.9×10−4 s −2, indicating that the model underestimates the strength of the TILs. Overall, it is concluded that the model reproduced the observed reasonably well.
In summary, the difference between our results and previous studies is that the effect of gravity waves has been explicitly taken into account in our analyses. As synoptic disturbances develop, gravity wave activities also increase in a specific region relative to the synoptic systems. The inertia-gravity waves are robustly reproduced with a range of model resolutions and parameters. Both synoptic-scale wave breaking and gravity wave activity seem to contribute to the time evolution of . Although we have presented a single case study on TIL formation associated with extratropical explosive cyclogenesis, it is well known that explosive cyclogenesis occurs frequently in the mid-latitude storm tracks from autumn to spring (e.g., Sanders and Gyakum ). Furthermore, our result is consistent with the fact that the dynamical TIL formation is considered to be dominant in winter mid-latitudes (e.g., Birner ; Miyazaki et al. [2010b]; Randel and Wu ).
We conducted a numerical experiment using a regional atmospheric model with realistic configurations to investigate the formation of the extratropical TIL associated with a realistic synoptic disturbance in mid-latitudes. The model successfully reproduced the TIL associated with an explosive cyclogenesis that occurred from 19 to 21 February, 2009 over Japan. The model also reproduced the negative correlation between the strength of the TIL (measured by the maximum buoyancy frequency squared in the TIL, ) and the relative vorticity near the tropopause (ζ TP), which has been reported by observations (e.g., Randel et al. ) and previous model studies (e.g., Son and Polvani ). However, the negative correlation was clear only during the development and mature stages of the cyclogenesis. This suggests that the evolution of the cyclone plays an important role in the formation of the TIL.
To ascertain the dynamical formation of the TIL including the effects of gravity waves, the relationship between and the vertical divergence, ∂ w/∂ z, and its vertical derivative, ∂2 w/∂ z2, were analyzed. Histograms of showed that regions of vertical convergence (∂ w/∂ z<0) correspond to higher as well as regions of ∂2 w/∂ z2>0 (Figure 8). The former indicated the effect of the dynamical formation by large- to synoptic-scale motions (e.g., Wirth ; Birner ), whereas the latter indicated the effect of small-scale waves with downward phase propagation. This tendency was clearer in the regions of negative relative vorticities at the tropopause.
By taking account of the fact that the gravity wave activity associated with the cyclone and the jet streak seem to be enhanced during the development and mature stages of the cyclone, the vertical convergence by gravity waves associated with synoptic weather systems could be a key element in the formation of the negative correlation between the strength of the TIL and the local relative vorticity at the tropopause.
The authors thank the two anonymous reviewers for their helpful comments. This work was supported by JSPS KAKENHI (S) Grant Number 24224911 and Kyoto University’s Global COE Program ‘Sustainability/Survivability Science for a Resilient Society Adaptable to Extreme Weather Conditions’ for FY 2009–13. The figures were produced by the GFD-DENNOU Library.
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