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Article

The 50-Year Evolution of the Planetary Boundary Layer in the Southern Part of Romania: Comparison Between the Determinations by the Stull Method and the Reanalysis Data from ERA5

by
Adrian Timofte
1,2,
Diana-Corina Bostan
1,
Cosmina Apetroaie
1,
Ingrid-Mihaela Miclăuș
1 and
Marius-Mihai Cazacu
3,4,*
1
National Meteorological Administration, Bacău Regional Forecast Centre, Timpului Street, No. 3, 600234 Bacău, Romania
2
REXDAN Research Infrastructure (RADO-Galați), Dunărea de Jos University of Galați, 98 George Cosbuc Street, 800008 Galați, Romania
3
Department of Physics, “Gheorghe Asachi” Technical University of Iasi, Dimitrie Mangeron Bld., No. 67, 700050 Iași, Romania
4
INOESY SRL, 8 Fdc. Mestecanis Street, Valea Lupului, 707410 Iași, Romania
*
Author to whom correspondence should be addressed.
Atmosphere 2025, 16(11), 1247; https://doi.org/10.3390/atmos16111247
Submission received: 1 October 2025 / Revised: 25 October 2025 / Accepted: 29 October 2025 / Published: 30 October 2025
(This article belongs to the Section Planetary Atmospheres)

Abstract

The Planetary Boundary Layer (PBL) remains a popular research topic, given its fundamental role in the exchange of energy between the surface and the atmosphere. Understanding the PBL’s mechanisms can improve weather forecasting, climate and air quality modelling. This paper presents a PBL climatology based on 50 years of observations (1973–2023) from the Bucharest Băneasa radio sounding station in Romania (international identifier 15420). The Stull method was used to calculate the PBL height, which was extracted from the sounding at the Bucharest Băneasa observation point and considers virtual potential temperature (θv). This incorporates the effect of humidity on air density. The analysis of climatological seasons (DJF, MAM, JJA and SON) based on PBL height series determined at 00 and 12 UTC using RAOB software revealed that the mixed layer height, as calculated by the Stull method, mainly captures the nocturnal Stable Boundary Layer (SBL) at 00 UTC and highlights the mixed layer (ML) at 12 UTC. ERA5 reanalysis data were also used in parallel.

Graphical Abstract

1. Introduction

The troposphere is the most important layer of the Earth’s atmosphere. The Earth’s atmosphere is 80 percent troposphere, and it is bounded at the top by a layer called the tropopause. This boundary is marked by a temperature inversion in some areas and isothermal conditions in others [1]. Although it extends approximately 11 km [2], with variations in height in the polar and equatorial zones, only 20% of the troposphere is made up of the planetary boundary layer (PBL) [3]. This is the lowest part of the troposphere that is directly influenced by the Earth’s surface, responding in a matter of hours or less to forcing mechanisms. The thickness of the PBL varies over time and space depending on mechanisms including heat transfer, friction force and pollutants, as well as land use and landforms [2,4]. The PBL’s thickness varies with the time of day, involving a diurnal variation in thickness. Since water has a high heat storage and absorption capacity and there are no significant temperature changes, the depth of the PBL varies slowly over seas and oceans during the diurnal cycle. Only large-scale air advection and vertical movement can produce changes in PBL depth over the oceans. The depth of the PBL depends on the pressure regime, both over the oceans and over land. In high-pressure regimes, the PBL is thinner due to downdrafts and subsidence, which are specific to this regime. The situation is different in the case of a low-pressure regime. As a result of upward movements, the PBL can reach high altitudes in the troposphere [2].
Unlike over large bodies of water, the PBL structure over land varies throughout the day. In areas under high pressure, the PBL structure is well-defined during the diurnal cycle [2,3,4,5,6,7,8,9,10]. These are the stable layer, the residual layer and the mixed layer [2,8,9]. During the day, the thickness is influenced by cloud cover and solar radiation [2]. At night, radiative cooling causes the PBL to decrease in thickness, resulting in the layer near the surface remaining stable and forming a stable boundary layer. As the day progresses, the PBL thickness increases due to increased solar radiation and, consequently, convective processes [2,5,6,8]. This is known as the convective boundary layer (CBL), and understanding its structure is important for weather forecasting [7].
Convective processes generate turbulence within the mixed layer, while radiative cooling and surface heat exchange act as additional sources of convection [2,5,7]. In the absence of cold-air advection, turbulent motions weaken after sunset, leading to the formation of a residual layer—the remnant of the daytime convective boundary layer, which persists aloft during the night above the stable surface layer [2,5,8]. As the night progresses, a stable layer develops near the surface, beneath the residual layer, where turbulence becomes very weak and the air remains strongly stratified [2,8].
The structure and dynamics of the planetary boundary layer (PBL) control the processes of dispersion, transport and accumulation of atmospheric pollutants, being an essential element in the assessment of air quality. In the southern region of Lake Baikal, it was found that variations in the concentrations of sulphur and nitrogen oxides are closely dependent on meteorological conditions: precipitation reduces the levels of these pollutants in the warm season, while thermal inversions and frequent calms in winter cause sharp increases [11].
Measurements made with low-cost sensors in the Baikal region have revealed a double seasonality of PM2.5 and PM10 concentrations, with maxima in summer and winter. In summer, convection and high humidity favour the formation of secondary organic aerosols, while in winter, the activity of anthropogenic sources, inversions and the reduction of the PBL thickness limit vertical dispersion [12].
In East China, analysis based on ERA5 data showed that a particular structure of the PBL favours the accumulation of pollutants under conditions of blocked atmospheric circulation. During pollution episodes, wind speed is reduced and temperature and humidity increase over the entire height of the PBL, with a transition height due to dynamic and thermal conditions located around the level of 900 hPa [13].
Extreme PMx concentrations occur under anticyclonic conditions, characterised by weak winds and a stable atmosphere, and changes in wind direction cause rapid decreases in concentrations, highlighting the influence of regional industrial sources. In the Huai River basin, it was observed that annual and seasonal variations in aerosols are dominated by processes in the PBL. The decrease in the extinction coefficient occurred predominantly in the 0–2 km layer, and the aerosol types show a seasonal distribution controlled by the wind regime and the thermodynamic conditions in the lower layer [14].
Therefore, it is found that the PBL parameters—layer height, thermal stability and wind regime—largely determine the level and temporal variability of atmospheric pollution. The integration of boundary layer characteristics in atmospheric chemistry models is an essential condition for improving air quality forecasts [11,12].
There are several methods of determining the height of the PBL, each of which provides different information about it. In 1964, Holzworth conducted a foundational study on the determination of the mixed layer height using radiosonde observations [15]. This was followed by studies that improved and slightly modified his method [2,16,17], which involved adding an excess temperature to the surface temperature to account for measurement uncertainties [15]. One widely used method for determining PBL height from radiosonde data is the parcel method, also known as the Holzworth method [9]. This method does not require the wind profile and is based on the intersection point of the dry adiabatic temperature starting from the surface and the profile temperature. This intersection point is interpreted as the equilibrium level of a rising parcel [9,10]. However, this method is subject to a high degree of uncertainty because it depends on the surface temperature.
Radiosonde data, which is widely used at most stations, is only available at the reference times of 00:00 and 12:00 UTC [6,9]. Therefore, comparisons with model estimations can only be made at these times. The uncertainty associated with this method is related to the nocturnal boundary layer, since no universal correlation has been found between wind, humidity and temperature profiles and turbulence. Several criteria are involved in interpreting the profiles of these parameters. This method can also be expensive [9]. Estimating the PBL height from radiosonde data can be subjective, as it is identified either by a temperature inversion or by a significant reduction in moisture in the profile [2].
Another approach to determining the PBL height is the bulk Richardson number method. This method assumes that the limit is reached when the Richardson number reaches a certain threshold value. The most used thresholds are 0.5 and 0.25 [18]. The bulk Richardson number is highly variable because the PBL is thermally stratified [18]. The bulk Richardson number method is the most suitable for climatological studies [19]. Consequently, many studies use this approach [20,21,22].
The variation in PBL height can also be determined by using aircraft and remote sensing techniques. These techniques have both advantages and disadvantages [23]. For example, aircraft may only be used during the day, but they have the advantage of being able to operate a variety of sensors and cover large areas [9]. Other techniques used include lidar, sonar and Doppler radar/wind profiling [9,23]. Although these methods are expensive, they offer the great advantage of enabling continuous monitoring of height variation over an entire diurnal cycle [9].
Nemuc et al. studied the dynamics of the lower troposphere between May 2008 and February 2009, using multi-wavelength lidar in the Măgurele area [24]. According to Nemuc et al., the mixed layer height determined from lidar measurements at Măgurele was approximately 1300–1500 m during the day, falling below this value after 19:00 UTC, when the atmosphere becomes stable. Comparison with radiosonde profiles indicated the existence of a lower layer located at approximately 700 m, confirming that, under stable conditions, the planetary boundary layer height can drop below 1000 m, below the detection limit of the lidar system. The gradient method was compared with the Richardson number method, obtaining concordant values for the PBL height and the aerosol layers [24].
Ungureanu et al. used the CL-31 ceilometer for the period November 2008–March 2009, finding the predominance of stratiform clouds and a direct correlation between the evolution of low clouds and the PBL structure [25].
Belegante et al. analysed the period 2009–2011, using lidar, radiometric data and numerical models (WRF, GDAS) [26]. The correlation between the measured and modelled PBL height was 0.66 for the entire dataset and 0.73 for the diurnal intervals, highlighting a systematic underestimation of the WRF model in stable nocturnal conditions [26].
Timofte et al. compared lidar, radiometric and radiosonde measurements with the ALARO model, during January–November 2014, for Bucharest and Iași [27]. In the study conducted by Timofte et al. (2015) [27], the average difference between the planetary boundary layer (PBL) height estimated by the ALARO model and that determined by other measurement techniques was below 200 m for both analysed locations (Bucharest and Iași). In the cold season, the ALARO model forecast for Bucharest presented a significant gap compared to the warm season, possibly caused by the overlap of the lidar system, which makes it difficult to detect the PBL for heights lower than 900 m. For the Iași station, the differences between the forecasted and measured values were similar in the summer and winter seasons, indicating a more uniform behaviour of the model in this region [27].
Dandocsi et al. derived the PBL height from lidar measurements (RALI) performed between 9 and 12 July 2012 at Măgurele. The maximum values reached 2265 m, recorded on the warmest day, with a pronounced diurnal variation and an episode of long-range aerosol transport confirmed by HYSPLIT [28].
Cazacu et al. analysed the time series from 5–8 May 2022 in Galați, using a CHM15k ceilometer and an RPG-HATPRO radiometer. By applying the multifractal motion theory, the PBL height (considered the control parameter) was correlated with the radiometric temperature profiles, obtaining good agreement between the theoretical and experimental values [29].
Therefore, studies conducted in Romania indicate a clear seasonal variation in the PBL height between 500 m and 2250 m, dependent on atmospheric stability, the type of layer (convective or stable) and local conditions. The maximum values are recorded in summer, in convective regime, and the minimum values in winter, in stable conditions, confirming the importance of integrating multi-instrumental observations for the characterisation of the planetary boundary layer [24,25,26,27,28,29].
During December 2019–November 2021, the study conducted by Pîrloagă et al. used Doppler wind lidar measurements at Măgurele, highlighting a marked diurnal cycle of wind speed and a seasonal variation in the PBL height, from approximately 500 m during winter nights to 1250 m at noon in summer. The predominant classes of PBL were convective, non-turbulent and intermittent (its pattern is complementary to the Convective and Non turbulent classes, being more pronounced in the top of the mixing layer), with the dominance of the convective regime in the warm season [30].
While previous studies have focused on short periods and local instrumental observations, the present study integrates the long series of aerological data in comparison with the ERA5 reanalysis data, providing for the first time a coherent picture of the multidecadal variation in the planetary boundary layer and the trends associated with the intensification of the duration of sunshine, after 2000 [31,32].

2. Materials and Methods

2.1. ERA5 Reanalysis

The ERA5 reanalysis, developed by the European Centre for Medium-Range Weather Forecasts (ECMWF), is the fifth generation of global atmospheric reanalysis products and forms part of the Copernicus Climate Change Service (C3S). Designed to replace ERA-Interim, this dataset corrects its known limitations and provides a more comprehensive, high-resolution reconstruction of the global climate and atmospheric conditions from 1979 to the present [33]. The improvements are substantial: ERA5 provides hourly output instead of six-hourly; increases horizontal resolution to approximately 31 km; enhances vertical resolution through the use of 137 model levels; assimilates a significantly larger volume of observational data; and introduces uncertainty estimates via ensemble runs [34]. These changes make ERA5 more precise and versatile for a wide range of scientific, operational and societal applications [35]. ERA5 is based on the Integrated Forecast System (IFS), specifically Cycle 41r2, and employs a four-dimensional variational data assimilation (4D-Var) method. This assimilation system integrates various observational data sources with a short-range forecast, known as the background or first guess. Through a cost minimization process, the system constructs an atmospheric analysis that balances observations and model physics over a 12-h assimilation window. Observations are assimilated dynamically, and their biases are corrected in real time using advanced techniques such as variational bias correction (VarBC) [36]. This approach ensures consistency in space and time, as well as improved physical realism compared to older reanalysis.
The volume and diversity of observational data used in ERA5 are unmatched by previous reanalyses. While ERA-Interim assimilated around 750,000 observations per day in 1979, by 2018 ERA5 incorporated more than 24 million daily observations [33]. These include satellite radiance measurements from instruments such as TOVS, AIRS, IASI and AMSU, as well as in situ observations from radiosondes, aircraft, surface stations, ships and buoys. Additional datasets include ocean altimetry, snow depth and soil moisture. The assimilation system applies dynamic bias corrections, particularly to satellite radiances, to ensure consistency over time despite the evolution of the global observing system. ERA5 provides users with highly detailed outputs, offering a horizontal resolution of 0.25 degrees (approximately 31 km), 137 vertical levels extending up to 0.01 hPa (around 80 km in altitude), and an hourly temporal resolution. This represents a significant improvement on the 6-hourly data and coarser resolution of ERA-Interim. Furthermore, ERA5 provides a 10-member ensemble of data assimilations (ERA5-EDA), offering uncertainty estimates every three hours [34]. These ensemble data are particularly valuable in areas with sparse observations or during periods with less reliable data, as they provide users with a quantitative measure of confidence in the reanalysis fields. When validated against independent observations, ERA5 consistently outperforms ERA-Interim. Temperature and wind fields show stronger agreement with radiosonde and aircraft data, and ocean wave heights match buoy measurements more closely. Precipitation fields in ERA5 also correlate better with global observational datasets such as GPCP [35,36]. Furthermore, ERA5 is more successful at capturing extreme weather events, including storms, heatwaves and droughts, offering better temporal and spatial precision. Climate signals, such as tropospheric warming and stratospheric cooling, are preserved more accurately. However, a few known issues persist. For instance, the upper stratosphere shows artificial warming around the year 2000 due to changes in satellite data assimilation. Additionally, mesospheric winds are often overestimated in early periods due to physical limitations in the model [37].
Careful consideration of how the dataset is constructed is required when interpreting ERA5 data. Each analysis field is the result of a synthesis of model dynamics and observational data, with the weighting determined by the level of confidence in each. Therefore, long-term tendency can be affected by changes in the observational system, particularly in the earlier decades when satellite coverage was more limited [38]. Therefore, users must exercise caution when analysing tendencies across decades and ensure that they account for any artificial discontinuities or shifts due to changes in data assimilation. ERA5 provides deterministic estimates as well as ensemble-based measures of uncertainty, which can be used to assess confidence in variables such as wind, temperature or PBL height in data-sparse regions. Differences between ERA5 and other reanalysis products stem from a variety of sources. One key factor is the use of different numerical weather prediction models and physics schemes. For instance, ERA5 turbulence, radiation, and land-surface interaction models are distinct from those used in MERRA-2, JRA-55, or NCEP reanalyses. Additionally, the assimilation systems vary; ERA5 uses 4D-Var, whereas others use 3D-Var or hybrid systems. Other differences arise from the diversity of assimilated observations, differences in spatial and temporal resolution, and distinct bias correction strategies. Even within ERA5, subtle discontinuities can emerge over time due to the addition or removal of satellite instruments or changes in assimilation configuration [39]. Therefore, cross-comparisons between reanalyses must be conducted with attention to methodological compatibility and data lineage. ERA5 has quickly become a foundational dataset for a wide range of scientific and operational domains. It is employed in climate change detection, attribution studies, weather prediction initialization, air quality modelling, renewable energy assessment, hydrological forecasting, and increasingly, machine learning applications in meteorology and climatology. Its combination of high temporal resolution, rich vertical structure and uncertainty quantification makes it an exceptionally useful tool for research and decision-making. Its enhanced depiction of the planetary boundary layer also facilitates research into surface-atmosphere coupling, which is crucial for modelling urban heat, wind energy, pollution dispersion and agricultural productivity.
In summary, ERA5 is a significant improvement on ERA-Interim in almost every respect. It covers a longer period (from 1979 onwards, with extensions planned back to 1950), has finer horizontal and vertical resolution, provides hourly outputs and assimilates a much larger volume of observational data. It also includes ensemble-based uncertainty estimates. These upgrades establish ERA5 as the most advanced and detailed global reanalysis currently available, positioning it as a central resource for understanding the Earth’s atmosphere on weather and climate timescales.

2.2. Planetary Boundary Layer (PBL) in ERA5

One of the key improvements in ERA5 is its enhanced representation of the planetary boundary layer (PBL). The PBL is the lowest portion of the atmosphere and is directly affected by surface processes such as turbulence, heat exchange and moisture fluxes. The PBL in ERA5 has significantly better vertical resolution: around 10 to 15 of the 137 model levels are located within the first two kilometres of the atmosphere. This denser vertical structure enables a more accurate depiction of boundary-layer dynamics, such as the formation of inversion layers or the daily cycle of mixing. ERA5 also uses upgraded turbulence parameterisations and improved coupling with the land surface model (Carbon-Hydrology Tiled ECMWF Forecasts Scheme for Surface Exchanges over Land—CHTESSEL), resulting in more realistic surface-atmosphere interactions [33]. When validated against radiosonde-derived estimates of PBL height, ERA5 performs notably better than previous reanalyses such as MERRA-2 or JRA-55 [40,41]. However, it still exhibits a tendency to underestimate daytime convective PBL heights by approximately 130 metres.
In ERA5, the PBL height is expressed in metres and is provided as a single-level hourly field with a spatial resolution of approximately 0.25 degrees (around 31 km) [33]. Rather than relying on turbulent kinetic energy (TKE), ERA5 determines PBL height using the bulk Richardson number method [42].
The bulk Richardson number is a dimensionless value that compares the stability of the atmosphere, as determined by thermal stratification, with the turbulence generated by wind shear [43]. The process begins by taking the lowest model level—typically around 10 metres above the surface—as the reference point. These model levels represent the atmosphere in a weather model such as ERA5, and are the vertical layers used inside it. These levels follow the terrain near the surface and the pressure levels higher up, enabling detailed calculations, particularly close to the ground [44]. The model then calculates the bulk Richardson number for each level aloft, moving upwards through the atmosphere from this surface level. The PBL top is identified as the lowest model level at which the bulk Richardson number exceeds the critical threshold of 0.25 [45]. If this threshold falls between two model levels, the height is determined by linear interpolation. This threshold is not arbitrary; it stems from empirical findings linking values of the bulk Richardson number below 0.25 to turbulent, well-mixed conditions within the boundary layer and values above 0.25 to stable, stratified layers where turbulence typically ceases [43]. To enhance accuracy, the calculation of the bulk Richardson number incorporates the virtual potential temperature, considering both temperature and humidity [43]. The method is based on physical principles: if the temperature and wind shear gradients are weak, the bulk Richardson number may remain below 0.25 across multiple layers, indicating a deep, well-mixed boundary layer. Conversely, in cases of strong night-time cooling near the surface, the bulk Richardson number can exceed 0.25 within a few hundred metres, resulting in a very shallow nocturnal boundary layer [46].
In practice, ERA5 uses this diagnostic method at each model time step to generate a gridded, hourly output field for boundary layer height. However, it does not store the full Richardson number profile; only the resulting height value is archived. This methodology is based on the ECMWF Integrated Forecasting System (IFS) and PBLH computation occurs during post-processing using the model wind and temperature fields [33,44]. Although the IFS model includes a turbulence closure scheme based on TKE, this is not employed to determine the PBLH in ERA5.
Despite its strengths, the ERA5 PBLH product has certain limitations. It is a diagnostic value, not a direct observation, and the bulk Richardson number method may underperform in situations involving weak shear or complex terrain, where turbulence may persist above 0.25 [46]. Furthermore, estimates of PBL height can vary significantly depending on the diagnostic method employed; while ERA5 relies on the Richardson number approach, other frameworks may use TKE thresholds or buoyancy criteria [45].

2.3. Planetary Boundary Layer (PBL) in RAOB

The radio sounding station was initially located in Mogoșoaia in the 1960s and 1970s, operating until it was relocated to Afumați in 1997–1998. The Afumați Meteorological Station is located approximately 15–17 km away from the former Mogoșoaia location in straight-line (geodesic) distance. At the new location, radiosonde observations are still carried out at synoptic times of 00:00 and 12:00 UTC. To ensure continuity of the time series and avoid interruptions to the observational database initiated in the 1960s and 1970s, the station retained the same international call sign (15420–Bucharest-Băneasa Meteorological Station—see Figure 1). The relocation was carried out in compliance with the norms and recommendations of the World Meteorological Organization (WMO), with the equipment being transferred from north-west to north-east Bucharest [47].
As stated in the internal documentation, the observational series was maintained continuously by taking the same sequence of measurements. However, some of the data were temporarily transmitted under another identifier, other than 15420. This explains their absence from public databases, such as the University of Wyoming archive. It is evident that the observable discrepancies in the series are not attributable to genuine interruptions in the measurement process. Rather, these irregularities are attributed to the modification of the station identifier during the transition period.
According to the literature, researchers are encouraged to define the height of the planetary boundary layer using the methods and instruments available to them [9]. According to the Stull method, the height of the planetary boundary layer (PBL) is defined as the altitude at which the virtual potential temperature of an air parcel lifted adiabatically from the surface becomes equal to the ambient virtual potential temperature profile, thereby marking the upper limit of the convective mixed layer [43,48,49].
The height of the planetary boundary layer (PBL) was determined using the Stull method implemented in the RAOB 7.0 (RAwinsonde OBservations) programme, which provides the PBL’s numerical value and graphical representation on a Skew-T diagram [43,50]. It is also interactive software for analysing atmospheric sounding, capable of decoding and processing data in WMO, BUFR, GRIB and other standardised formats. The programme integrates a wide range of thermodynamic and dynamic algorithms for analysing the vertical structure of the atmosphere. These include modules dedicated to calculating significant levels (LCL, CCL and LFC), instability indices and parameters associated with turbulence and vertical transport [50]. This method was chosen because it is independent of numerical models, is based on direct observational data and provides a more realistic estimate of PBL height in environments with high humidity than other methods. It has also been demonstrated to be applicable in operational meteorology and pollutant dispersion studies.
This method is derived from parcel theory and static stability analysis and is based on the virtual potential temperature (θv) profile.
The RAOB programme can determine the PBL mixing height by several methods (Holzworth, Stull, Heffer, and Q methods). We chose for our study the PBL determination method which uses the standard Theta-based method, “where the surface plot is adiabatically elevated dry until it intersects the sounding profile. If there is a surface inversion, then the PBL height is defined at the top of the surface inversion. If no PBL can be identified and there is a raised inversion, then the PBL height is identified at the base of the raised inversion, as long as it is below a user-defined limit” (4 km, AGL). The Stull method uses the standard method, “but instead uses the plot of the virtual potential temperature of the sounding surface relative to the intersection of the sounding virtual temperature profile” [50].
Thus, determining the PBL height using the Stull method and the RAOB programme provides a robust estimate of the mixed layer depth, as well as solid information for evaluating vertical transport and atmospheric dispersion processes.
Also, in their paper Feron et al. talk about a more realistic assessment of atmospheric stability by the Stull method, because it uses the virtual potential temperature, instead of the virtual temperature (used by the Holzworth method). The results of this study showed that the values obtained by the Stull method are better suited to lidar observations, even there is a slightly larger variance [51].
Also, some conditions described by Seidel et al. were considered [46]. “To avoid mistaking free tropospheric features for the top of the PBL, if the PBL height was not found in the lowest 4000 m, then it was considered missing. Thus, cases of deep convection, which may reach or even penetrate the tropopause, were not captured”. PBL heights are given in metres above ground level (not above mean sea level) [46].
The calculation procedure consists of several steps. First, the virtual potential temperature of the surface is determined from the observed temperature and humidity at ground level. The virtual potential temperature considers the effect of water vapour on air density. Next, the movement of the surface particle along the vertical profile is tracked, assuming an adiabatic rise until it intersects with the ambient medium. The static equilibrium level is then identified as the altitude at which the θv profile of the surface particle is equal to that of the ambient medium. This intersection marks the upper limit of the mixed layer and, consequently, the height of the PBL. Under conditions of convective instability, this method determines the depth of the turbulent layer (mixed layer) between the surface and the intersection level. In situations involving low stable layers or inversions, the method may indicate low PBL values, reflecting inhibited vertical mixing. Compared to the Holzworth method, which uses only potential temperature (θv), the Stull method provides a more realistic estimate of the PBL in humid environments, where the effect of water vapour is significant and neglecting it leads to an underestimation of the mixed layer height.
To filter the data from the 1973–2023 interval, we removed values below 100 m and those above 4000 m, we took into account the station altitude (91 m) and the days in which the programme failed to extract PBL height data were eliminated (the value 76 was displayed, randomly chosen by the programmer).
Fearon M. specifically used the Stull method to compute mixing height values, demonstrating its applicability across different atmospheric conditions [51]. The Stull method is applicable in both cloud and cloudless conditions, as long as there are sounding data that correctly describe the thermodynamic profile. It is true that clouds can affect the interpretation of the result. However, RAOB can simultaneously display cloud layers (RICAPS) and PBL level, allowing the user to correctly interpret the relationship between them (for example, whether the PBL reaches the base of a stratiform cloud layer or remains below it). “RICAPS performs a series of Bottom-Up scans to determine cloud layers. This system is superior to the older, Traditional temperature/dewpoint relationship algorithm, which over-analyses low clouds and under-analyses high clouds. The RICAPS cloud algorithm works with any sounding profile and is completely independent of modelled cloud fields. Cloud algorithms use a combination of temperature, dewpoint, relative humidity, wet-bulb & frostpoint temperatures and their associated lapse-rates. RAOB displays these cloud layers in the same fashion as before, including the Toolbar’s “cloud” analyses” [50,51].

3. Results

The data presented in the following figures show the mean PBL height values for each seasonal period (DJF, MAM, JJA and SON) over the 50-year period from 1973 to 2023. The error bars represent the standard error of the mean.
For 12 UTC (see Figure 2 and Figure 3), the average PBL height in the winter season (DJF) is 545 m according to the ERA5 data and 601 m according to the Stull method. In the winter season, both methods indicate low PBL heights. However, the values obtained by the Stull method are higher than those obtained from ERA5.
In spring (MAM), the average PBL height is 1274 m according to the ERA5 data and 1323 m according to the Stull method.
ERA5 data shows an increasing tendency in PBL height for the MAM season, while the Stull method shows similar average values. Predominantly below-average values are observed until the 1990s, after which higher-than-average values predominate.
In summer (JJA), the average PBL height is 1494 m according to the ERA5 data and 1662 m according to the Stull method.
For the warm season, both the ERA5 data and the Stull method indicate a clear intensification of the PBL height, which is correlated with intense warming and convection. ERA5 indicates an increase after 2000. The Stull method shows below-average values until the 1990s, as with the ERA5 values. After this, higher values are observed, but the data are more dispersed.
In autumn (SON), the average PBL height is 936 m according to the ERA5 data and 1021 m according to the Stull method. SON is characterised by moderate average PBL heights. There is a similar value between the two methods, with no clear tendency.
Winter is characterised by generally low values close to the climatological mean, with higher dispersion in the Stull method. ERA5 shows a slight increase in the frequency of years with below-average PBL, but the signal remains modest. The picture is slightly noisier in Stull: above-average values predominate in the 1970s–1980s, followed by a period of decrease in the 1990s and a redistribution with variations around the mean value.
Spring presents a much clearer signal. In ERA5, most years before 2000 have values close to or below average, with a few exceptions. After 2000, however, years with a PBL above the multi-year mean frequently dominate. This increase is particularly evident between 2000 and 2008, suggesting an intensification of convective processes. In Stull, the distribution is more variable, but the general tendency shows a similar shift towards higher values over the past two decades.
Summer is the season with the most pronounced differentiation. In ERA5, below-average values predominated before 2000, but above-climatological values clearly predominated after this year, with notable maxima around 2007 and 2008. This behaviour reflects an increase in the intensity of thermal convection against a background of climate warming. In Stull, the pattern is similar, but with sharper variations, indicating greater methodological sensitivity to extreme years.
Autumn is more balanced: in the ERA5 dataset, an alternating succession of above- and below-average years is observed before 2000. After 2000, the frequency of above-climatological years increases slightly, but without a robust signal. In the Stull method, the variability is high, but the same moderate long-term increasing tendency can be clearly observed after 2000. The Stull method shows a robust positive tendency after 2000, with the strongest increase observed in summer and spring. This suggests an intensification of convective processes on a climatological scale. The ERA5 series at 12 UTC partially confirms this increasing tendency, although with more moderate values and reduced variability.
In spring (MAM), the average PBL height is 308 m according to the ERA5 data and 423 m according to the Stull method. The ERA5 data show moderate variations around the average value that are somewhat symmetrical to it, while the Stull method highlights episodes in which values below the seasonal average predominate.
In the summer season (JJA), the average PBL height value obtained from the ERA5 data is 250 m, while the average PBL height value obtained using the Stull method is 311 m. The ERA5 values show moderate variations around the average, with successive increases and decreases every 10–15 years, while the Stull method predominantly produces above-average values until the 1990s, followed by values lower than the average. The analysed data show that, although ERA5 has lower values than the Stull method, these values are more stable and the tendencies are insignificant. The Stull method reveals greater variability and higher PBL height values, but without a clear tendency.
During the cold season (DIF), the Stull method applied at 00 UTC yields higher mean values than ERA5, albeit with significant inter-annual variability. The significant negative tendencies observed (i.e., height values below the seasonal mean) reflect the deepening of the nocturnal stable layer (SBL), which is determined by persistent thermal inversions and intensified radiative cooling. During the period from the 1970s to the 1990s, there were years when the residual layer (RL) played a more significant role, as the heights were higher than the seasonal mean. It is worth noting that, since the 1990s, the mean values have mostly been below the seasonal mean. ERA5 remains approximately constant throughout this period, showing that the model diagnosis attenuates real variations. At 00 UTC, the residual layer (RL) plays a reduced role and the estimates capture almost exclusively the SBL.
In the transitional months (MAM), the Stull method shows a significant decrease after the 1990s, followed by an upward tendency between 2015 and 2020. Meanwhile, mean height in ERA5 remained relatively constant, with no notable variations. During this season, daytime RL often persists overnight, but the Stull method primarily identifies the depth of the SBL. The difference in values between the Stull method and ERA5 suggests that the reanalysis data does not fully capture the interaction between the RL and the SBL direct estimates, however, highlight greater variability in stratification processes. During the warm season, the Stull method shows a decrease in the mean value after the 1990s, accompanied by a robust negative tendency. ERA5 shows lower values, with a more stable mean over time. Summer is the season with the strongest contrast between the diurnal mixed layer (ML) and the thin SBL formed at night.
During the transition to winter (SON), the Stull method shows clear decreases after the 1990s, whereas ERA5 indicates a slight increase. Autumn is characterised by the contrast between days that are still convective enough for rain-free convection (RFC) and cold nights that favour a persistent surface boundary layer (SBL). Stull estimates show large amplitude and pronounced variability, whereas the ERA5 model reduces these fluctuations.
The data confirm that, at 00 UTC, the Stull method primarily captures the SBL, which shows a noticeable decreasing tendency after the 1990s, followed by stabilisation. Meanwhile, ERA5 maintains a constant and homogeneous regime. Although the residual layer (RL) is present, especially in spring, summer and autumn, it is not directly represented in the 00 UTC series because the applied algorithm prioritises SBL.
When the average values obtained by the Stull method (12 UTC measurements) are compared with those from the ERA5 data (also 12 UTC measurements) for Bucharest-Băneasa, it is found that, for the lowest values of PBL height from the observational data, the values from ERA5 are consistently higher in all months. Conversely, the highest layer height values from the observations are higher than those calculated with ERA5, capturing both the initiation of PBL formation and its maturity phase. There is an increased deviation from March to September (see Table 1 and Table 2).
For 00 UTC (see Figure 4 and Figure 5), the average PBL height in the winter season (DJF) is 312 m according to the ERA5 data and 454.11 m according to the Stull method. While the ERA5 data shows some stability with moderate variations, the Stull method captures larger extremes with higher variability.
Table 1 shows the lowest average value of the planetary boundary layer height (called the mixed layer, or ML) for each month of the year (1973–2023), as determined by the Stull method at 12 UTC. From the ERA5 data, the average value for the respective month in the same year was identified (for example, for January in the period 1973–2023, the lowest average value for the planetary boundary layer height was found in 2015, at 262 m; the ERA5 data showed an average PBL height of 342 m for January 2015). This reasoning was applied to the remaining months.
Table 2 shows the highest average value of the planetary boundary layer height (called the mixed layer, or ML) determined by the Stull method at 12 UTC for each month of the year (1973–2023). From the ERA5 data, the average value for the respective month in the same year was identified (for example, for January in the period 1973–2023, the highest average value for the planetary boundary layer height was in 1978, at 893 m; the ERA5 data showed an average PBL height of 592 m in January 1978). This reasoning was applied to the remaining months.
Table 3 shows the lowest average value of the planetary boundary layer height (Stable Boundary Layer, or SBL) determined by the Stull method at 00 UTC for each month of the year (1973–2023). From the ERA5 data, the average value corresponding to each month was identified (for example, for December in the period 1973–2023, the lowest average value of the planetary boundary layer height was found in 1992, at 150 m; the ERA5 data showed an average PBL height of 341 m in December 1992). This reasoning was applied to the other months.
Table 4 shows the highest average value of the planetary boundary layer height (Stable Boundary Layer, or SBL) for each month of the year (1973–2023), as determined by the Stull method at 00 UTC. From the ERA5 data, the average value corresponding to each month was identified (for example, for December, the highest average value of the planetary boundary layer height was found in 1984, at 781 m; the ERA5 data showed an average PBL height of 298 m in December 1984). This reasoning was applied to the other months.
For the minimum values (see Table 3), the values determined by the Stull method are lower than those in ERA5 in all months. This shows that the reanalysis data tend to overestimate the thickness of the nocturnal stable layer when it is poorly developed. For the maximum values (Table 4), the Stull method consistently yields higher values than ERA5. This suggests that ERA5 underestimates the maximum development of the nocturnal stable layer and only partially captures the intensification of the nocturnal inversion layer.
Therefore, the same tendency observed at 12 UTC is confirmed. ERA5 smooths the extremes, providing higher values at the minimums and lower values at the maximums. This reflects the limitations of the reanalysis data in capturing the true variability of the planetary boundary layer.

4. Discussion

In the analysed interval for Bucharest, the lowest monthly PBL height values in ERA5, measured at 12 UTC, are found in January and December. This is because the average number of sunny days in these months is three, with the remaining days being partially or fully cloudy, which limits the PBL height. If the height is relatively uniform in December, lower values appear in January. The most notable of these were in 1985 (when 16 consecutive days with negative temperatures were recorded in Bucharest and it was declared the coldest winter in 40 years), 1990, 2002 and 2011, when the PBL height slightly exceeded 300 m.
Some discrepancies between the Bucharest radiosonde observations and ERA5 grid-cell averages are expected, particularly due to urbanisation and heterogeneous terrain. The literature indicates that such differences are consistent with the inherent representativeness limitations of point observations relative to gridded products [52,53,54]. Therefore, the observed deviations are interpreted in light of these spatial constraints, and the representativeness radius of ~50–100 km is applied when comparing radiosonde and ERA5 profiles.
The highest value was 775 m in January 2022. According to the European Union’s Climate Change Service, Copernicus, temperatures higher than climatological averages were recorded throughout Europe, including Romania, that month. According to this report, “globally, January 2022 was 0.28 °C warmer than the average January in the 1991–2020 reference period and the sixth warmest January recorded to that date. At the European level, average temperature anomalies are generally larger and more variable than at the global level, the average temperature in January 2022 was 0.79 °C above the average of the 1991–2020 reference period” [50].
In Bucharest, the month began with temperatures over 10 degrees Celsius and sunny days.
The height of the PBL varies depending on the surface temperature and humidity. It increases when the surface temperature is high and humidity is low. In these conditions, sensible heat fluxes dominate latent heat fluxes, leading to an increase in buoyancy. As expected, the mixing depth begins to increase in March, a month generally characterised by changeable weather, with cold, wet days alternating with warm, sunny ones. This continues until October, with the most significant increases occurring from May to August in the first 25 years analysed (1973 to 2002). The year 1994 (with an average value of 1258 m recorded in March) was extraordinarily warm and amazed climatologists at the time. Few would have thought that there would be warmer years in the following 30 years. Significant warming began to be felt after 2002, when droughts and heatwaves became increasingly frequent. In the following 25 years, there were significant increases in PBL height in all summer months (June 2007: 2031 m; July 2007: 2258 m; August 2008: 2067 m). Moreover, these increases extend from the beginning of spring and continue until late autumn (March to September inclusive).
The increasing tendency for PBL heights to rise in September can be attributed to heatwaves that persist at the end of summer and affect Southeastern Europe. These heat waves, characterised by sunny days and high temperatures, have become more frequent and intense, as seen in 2007, 2012, 2015, 2017, 2020 and 2022.
In 2007, the maximum PBL values corresponded to three prolonged heatwaves: one in June (19–27 June), with an average value of 2031 m; one in July (15–25 July), with an average value of 2258 m, during which there was an uninterrupted heatwave; and one in August (23–25 August), with an average value of 1610 m. In 2012, the maximum PBL value in July (1906 m) can be interpreted as the result of advection of tropical warm air of North African origin, which was present over south-eastern Europe from the beginning of the month until 16 July. From June to September in 2015, there were five heatwaves, two of which covered most of July (between the 6th and 9th and the 16th and 30th) with values between 1600 and 1700 metres. In 2017, two heatwaves in August (at the beginning and end of the month) led to an increase in the PBL height in both August and September (with values between 1300 and 1600 m).
The summer of 2020 saw record temperatures, even in September, with an average value of 1510 m, when heatwaves reached as far as Russia, with temperatures of 30 °C in Moscow. The PBL depth remained high from April (with an average value of 2063 metres) until early October, reaching its maximum in July, August and September (with values between 1500 and 1900 metres, and an average value of 1962 metres in August).
According to the report published by the European Copernicus Climate Change Service, the summer of 2022 was declared the warmest ever recorded in Europe since the beginning of meteorological measurements. This dethroned the summer of 2021, which had previously been recorded as the hottest summer to that date (with values between 1600 and 1900 m, and an average value of 1974 m in July).
From 2008 to 2023, August was often warmer than July, although July was generally warmer than the following month.
Bucharest is a metropolis located inland, far from the influences of water, in contrast to other European cities used as observation points in the literature on the analysed topic. These other cities are located in the vicinity of large bodies of water (Mediterranean Sea: Brindisi, Trapani, Cagliari, Gibraltar; Bay of Biscay: Bordeaux; Atlantic Ocean: Valencia) [1]. The temperate climate of Bucharest is dictated by its geographical location in the Carpathian-Balkan basin, respectively, in the Romanian Plain [2], and the Afumați Meteorological Station is located at an elevation of 91 m (with an indicative 15420 from Bucharest-Băneasa, as we explained why this convention was made). These cumulative aspects influence the local climate peculiarities.
Tumanov et al. even discuss differences in the main meteorological parameters within the metropolis, taking the meteorological stations at Băneasa and Filaret into account in their analysis [55]. In their study, they observed a noticeable difference in cloudiness between the two stations. The presence of stratiform clouds at the meteorological station in the northern part of the city is attributed to the influence of the lake and the forest in that area. This phenomenon is said to occur more frequently in the mornings at the Băneasa meteorological station than at the Filaret meteorological station. The author also analysed a case of a frontal passage on 17 April 1994. A compact system that was expected to pass over the city broke up as it passed over, regrouping after crossing the city [2].
The particularities induced by the local geography, in all its aspects, along with influences at the synoptic scale, are reflected in the climatology of the planetary boundary layer height above Bucharest. The temporal and spatial variability of this parameter can be clearly represented using heatmap graphs, which facilitate a complex yet consolidated analysis of the climatology of the planetary boundary layer height. As can be seen in Figure 6, which shows the PBL height resulting from ERA5 calculations, the months in the cold semester indeed present the lowest heights, ranging from 219 m to 368 m (average values). January is the month when the PBL reaches its lowest heights. In January, the northern half of the continent experiences tighter barometric gradients due to the deepening of the Icelandic Low. This leads to an intensification of atmospheric circulation in the north. In contrast, the south and the Romanian Plain typically see greater stability of the air masses. This is due to the formation of an anticyclonic belt, brought about by the union of the Siberian and Azores high-pressure systems.
Thus, cyclonic activity in the Mediterranean Basin weakens and circulation becomes less intense [3]. The transitional seasons (MAM and SON) exhibit similarities with regard to the height of the planetary boundary layer. In March, values range from 609 m to 1671 m, with the lowest value recorded in 2018. April is the month when the height has exceeded 2000 m on two occasions in the analysed data series (2063 m in 2020 and 2017 m in 2007). The lowest height was recorded in 2016 at 990 m, while May is characterised by values exceeding 1500 m. The maximum height was recorded in 1986 at 1865 m, and the minimum value does not drop below 1100 m, with an average value of 1144 m in 1980. As the Northern Hemisphere warms, the anticyclonic belt shifts northwards, the Icelandic Low weakens and the depression over Asia Minor becomes more influential. Consequently, the southern part of the continent experiences more intense circulation than the northern part [3]. During the warm season, the highest PBL height values are recorded, with July 2007 standing out from the other years in the analysed period with a maximum value of 2258 m.
The lowest height, 1011 m, is observed in June 1991. Starting in June, evident changes to the baric field are observed at continental level. The thermal low over Asia Minor deepens while the Siberian High weakens. The Icelandic Low weakens over the North Atlantic, resulting in weaker winds over northern Europe [3]. From September onwards, the values gradually decreased, with November showing the most homogeneous PBL height values across the entire analysed period, ranging from 409 m to 832 m.
November is the most stable month of the year due to the extension of the Siberian High ridge, which reaches as far as the western Alps. The ridges of the Azores High and the Siberian High merge to form a high-pressure belt positioned further south over the continent during the cold season than during the warm season. This configuration blocks circulation from the Mediterranean Sea towards Romania [3].
The heatmaps in Figure 6 and Figure 7, which are based on measurements from the observation point at Meteorological Station Afumați (15420 Bucharest Băneasa), also show a clear seasonal variability, with the highest PBL heights occurring during the summer months. This is a result of thermal convection that induces intense turbulence [4]. The greatest homogeneity is observed during the cold and transitional months. In the warm months, however, although there is a clear upward tendency in PBL height, year-to-year homogeneity is observed to decrease. The highest PBL height was recorded in July 2007, with average values of 2258 m and 2794 m from ERA5 and the Stull method, respectively. The increase in PBL height is related to changes in other meteorological parameters in the Bucharest area, which influence the local climate. In his study, Tumanov S. et al. report a decrease in the number of foggy days and rainy days, a reduction in wind speed and an increase in relative humidity at the Băneasa and Filaret stations in the period 1961–1990 [55].
The ERA5 data (Figure 8) show a relatively uniform evolution of the boundary layer at night, with moderate height values (the multiannual monthly average is approximately 240–330 m, with seasonal variations). These values are typical of a stable nocturnal boundary layer (SBL), which develops through the radiative cooling of the surface. It is characterised by shallow depth and weak turbulence. The limited interannual variations suggest that the ERA5 reanalysis tends to ‘smooth out’ extremes and provide robust climatological averages. At the same time, higher values occasionally appear (above 500–600 m; for example, 540 m in October 2004 and 617 m in March 2002), which are interpreted as residual layers (RLs) formed during the day that did not dissipate completely after sunset. This behaviour indicates that ERA5 effectively captures both the SBL typical of calm and cold nights, and episodes of persistent RL, particularly during the transitional months of spring and autumn.
Estimates based on Stull’s method (Figure 9) show much greater variability in PBL height at night, with values ranging from a few hundred metres (multiannual monthly averages between 300 and 510 m) to over 1000 metres (1116 metres in March 1984). This behaviour indicates that the method is more sensitive to local conditions (atmospheric circulation, stratification and mechanical forcing). The high values (800–1200 m; specifically, 951 m in February 1984; 1116 m in March 1984; 897 m in October 1987; and 974 m in November 1975) suggest that the method retains the signal of a strongly developed residual layer (RL) during the day, which dominates the nocturnal structure. In contrast, low values (200–400 m) correspond to a classic SBL formed under conditions of radiative cooling and stable stratification. Compared to ERA5, the Stull method accentuates these differences, providing a clearer distinction between the shallow SBL and the persistent RL. This is an important aspect for case studies and the evaluation of residual vertical transport events (e.g., pollutants and aerosols).
After 2000, sunshine duration in Europe increased significantly, confirming a consistent positive trend in surface solar radiation. Data from the ESOTC 2024 report show that after 2006, positive anomalies in sunshine duration have persisted almost every year, with only one notable deviation in 2010, higher and lower solar radiation [31].
The evolution of cloudiness was inversely correlated with that of solar radiation. After 2000, satellite data show a gradual decrease in average cloud cover in Central and Eastern Europe, while moderate increases in cloudiness were observed in the west of the continent. In 2024, these contrasts were accentuated: anomalies of −10% over the Balkans and +10% in the west (France), with minimum values up to −50% in September (eastern Europe), associated with a persistent anticyclonic regime and drought conditions.
In parallel, the intensification of solar radiation and the reduction in cloudiness in south-eastern Europe have favoured a constant increase in extreme temperatures and the number of hot days. Since the 2000s, a clear increase in the frequency of heat waves, days with severe heat stress and tropical nights (minimum temperature below 20 °C) has been observed. The average number of such nights has increased, and the continental area affected by at least one tropical night has risen from 20% in the 1970s to over 35% in the 2020s. In 2024, south-eastern Europe recorded 66 days with severe heat stress, the highest number in the observational series, and 23 tropical nights, exceeding previous records. Copernicus analyses show that, after 2000, it showed an accelerated increase in the frequency and intensity of heat days, a greater persistence of heat values and an increase in the annual variability of summer rainy days, which amplifies the effects of drought [31,32].
During the period 2000–2003, the temperature anomaly at the 850 hPa level was analysed and studied for each year, compared to the period 1991–2020. Except for the period 2003–2006 and 2011, where the anomalies are negative, the entire interval had positive anomalies, above the observation point [31,32,56].
The climatological results obtained for the period 1973–2023 are consistent with previously reported observations for Romania, which describe a clear seasonal variation in the PBL height between 500 m and 2250 m, dependent on atmospheric stability, layer type and local conditions. Studies carried out with lidar and ceilometer systems at Măgurele [24,25,28,30] have revealed maximum values of the convective layer between 1300 and 2265 m during summer and minimum values below 800 m in stable nocturnal regime, similar to our multi-annual averages obtained by the Stull method and ERA5. Belegante et al. and Timofte et al. showed that numerical models tend to underestimate the PBL under certain stability conditions, and the differences between measured and simulated values are frequently below 200 m, which corresponds to our observation of the underestimation of ERA5 compared to the survey determinations, especially for the maximum diurnal values [26,27].
Compared to these studies, the present work makes an essential contribution through its climatological character, covering a period of five decades and providing a systematic analysis of the evolution of the PBL in southern Romania.

5. Conclusions

At 12 UTC, both the Stull method and the ERA5 reanalysis data capture the convective mixed layer (CML), with values in the order of kilometres for the warm and transitional seasons. The Stull method reveals greater extremes and variability, whereas the ERA5 provides a more consistent diagnosis with lower maximum limits.
The Stull series shows positive tendencies after 2000, which are particularly significant during the warm seasons (JJA and SON). This suggests an intensification of diurnal convection. By contrast, the ERA5 data only shows moderate increases until the 2000s, after which it stabilises.
The results suggest an increase in ML height after 2000, which is probably associated with an intensification of convection and a change in the regional energy regime. The differences between the Stull method and the ERA5 reanalysis data reflect methodological limitations: the Stull method is more sensitive to local and extreme processes, whereas the ERA5 data are less variable.
At 00 UTC, the values obtained by the Stull method primarily reflect the stable night-time layer (SBL). These values demonstrate significant variability and a tendency to decrease below average in all seasons. In contrast, ERA5 provides a more consistent diagnosis without any robust climatological signals currently.
The pronounced increases observed in the Stull method at 00 UTC during the 1970s–1990s disappear, indicating a possible change in the nocturnal stability regime. After 2000, the at 12 UTC tendencies are positive, especially during the warm seasons, suggesting an intensification of diurnal convection.
In terms of the differences between the methods, the Stull method produces estimates that reach higher maximum values than ERA5 but also exhibit much greater dispersion. In contrast, ERA5 limits extremes and smooths variability. This structural difference between the two methods is a key factor in interpreting the results.
Regarding the connection between the 00 and 12 UTC observations, the following can be stated: inter-annual correlations are weak or negative, particularly in summer. This confirms that the PBL height at 00 UTC cannot be used as a proxy for the residual layer (RL). The diurnal amplitude between the 00 and 12 UTC observations is primarily determined by the ML depth rather than the nocturnal structure.
The results emphasise that the processes governing the diurnal PBL (convection) and the nocturnal PBL (radiative cooling and inversions) are fundamentally different. The climatological analysis must therefore treat these regimes separately. To characterise the RL, other dedicated methods that explicitly distinguish between the SBL and the RL must also be applied.
Summarising the above, our conclusions regarding the evolution of the PBL height are consistent with the measured meteorological parameters. After 2000, Europe experienced an increase in sunshine duration and ground radiation, especially in the east and southeast of the continent, a reduction in cloudiness in the same regions, and an intensification of extreme temperatures, with records of torrid days and tropical nights in Southeast Europe.

Author Contributions

Conceptualization, D.-C.B., A.T. and M.-M.C.; methodology, D.-C.B., I.-M.M., C.A., A.T. and M.-M.C.; software, I.-M.M., C.A., A.T. and M.-M.C.; validation, D.-C.B., A.T. and M.-M.C.; formal analysis, D.-C.B., I.-M.M., C.A., A.T. and M.-M.C.; investigation, D.-C.B., I.-M.M., C.A., A.T. and M.-M.C.; resources, D.-C.B., I.-M.M., C.A., A.T. and M.-M.C.; data curation, D.-C.B., I.-M.M., C.A., A.T. and M.-M.C.; writing—original draft preparation, C.A., A.T. and M.-M.C.; writing—review and editing, D.-C.B., A.T. and M.-M.C.; visualisation, D.-C.B., I.-M.M., C.A., A.T. and M.-M.C.; supervision, D.-C.B., A.T. and M.-M.C.; project administration, D.-C.B., A.T. and M.-M.C. All authors have read and agreed to the published version of the manuscript.

Funding

This work was financed by Smart Growth, Digitization and Financial Instruments Program (PoCIDIF) 2021–2027, Action 1.3 Integration of the national RDI ecosystem in the European and international Research Space, project “Supporting the operation of facilities in Romania within the ACTRIS ERIC research infrastructure”, SMIS code 309113.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

The raw data supporting the conclusions of this article will be made available by the authors without undue reservation. Due to licence restrictions, the source code of CHTESSEL cannot be made publicly available.

Acknowledgments

Marius Mihai Cazacu would like to thank the CEEPUS mobility programme (CIII-Freemover-2425-196985) for its scientific support.

Conflicts of Interest

Marius-Mihai Cazacu is employed by INOESY SRL. The paper reflects the views of the scientists and not the company. The authors declare no conflicts of interest. The company had no role in the design of the study; in the collection, analysis, or interpretation of data; in the writing of the manuscript; or in the decision to publish the results.

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Figure 1. Geographical location of the observation point.
Figure 1. Geographical location of the observation point.
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Figure 2. Distribution of PBL height from ERA5 12 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
Figure 2. Distribution of PBL height from ERA5 12 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
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Figure 3. Distribution of PBL height from Stull Method 12 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
Figure 3. Distribution of PBL height from Stull Method 12 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
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Figure 4. Distribution of PBL height from ERA5 00 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
Figure 4. Distribution of PBL height from ERA5 00 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
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Figure 5. Distribution of PBL height from Stull Method 00 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
Figure 5. Distribution of PBL height from Stull Method 00 UTC, with error bars, by seasons DJF, MAM, JJA, SON, for the period 1973–2023.
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Figure 6. Heat map of average PBL height values [m] from ERA5 reanalysis at 12 UTC for the period 1973–2023.
Figure 6. Heat map of average PBL height values [m] from ERA5 reanalysis at 12 UTC for the period 1973–2023.
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Figure 7. Heat map of average PBL height values [m], derived using the Stull method at 12 UTC, for the period 1974–2023.
Figure 7. Heat map of average PBL height values [m], derived using the Stull method at 12 UTC, for the period 1974–2023.
Atmosphere 16 01247 g007
Figure 8. Heat map of average PBL height values [m] from ERA5 reanalysis at 00 UTC for the period 1973–2023.
Figure 8. Heat map of average PBL height values [m] from ERA5 reanalysis at 00 UTC for the period 1973–2023.
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Figure 9. Heat map of average PBL height values [m], derived using the Stull method at 00 UTC, for the period 1973–2023.
Figure 9. Heat map of average PBL height values [m], derived using the Stull method at 00 UTC, for the period 1973–2023.
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Table 1. The minimum average values (m) of the PBL at 12 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
Table 1. The minimum average values (m) of the PBL at 12 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
MonthYear
(Specific to Stull Method)
Minimum Mean Value (m) of PBL at 12 UTC from Stull MethodMean Value of PBL (m) at 12 UTC from ERA5, from the Same Year
January2015262342
February1991278413
March1981577869
April19814761313
May19787511279
June19817231305
July19879981292
August19849391436
September19877041256
October1979760841
November1983378582
December1989282504
Table 2. The maximum average values (m) of the PBL at 12 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
Table 2. The maximum average values (m) of the PBL at 12 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
MonthYear
(Specific to Stull Method)
Maximum Mean Value (m) of PBL at 12 UTC from Stull MethodMean Value of PBL (m) at 12 UTC from ERA5, from the Same Year
January1978893592
February19951288798
March202215821493
April200721622017
May201820411486
June200723842031
July200727942258
August199527741564
September201920291662
October197414401165
November19741148625
December1985779385
Table 3. The minimum average values (m) of the SBL at 00 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
Table 3. The minimum average values (m) of the SBL at 00 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
MonthYear
(Specific to Stull Method)
Minimum Mean Value (m) of PBL at 00 UTC from Stull MethodMean Value of PBL (m) at 00 UTC from ERA5, from the Same Year
January2015223276
February2016256330
March2000227296
April1995185215
May2018200265
June2021176203
July2013172253
August2011171266
September2020194341
October2012184218
November1995203289
December1992150341
Table 4. The maximum average values (m) of the SBL at 00 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
Table 4. The maximum average values (m) of the SBL at 00 UTC determined by the Stull method and the average values of the PBL height extracted from ERA5, corresponding to the specific years of the minimum average values determined by the Stull method.
MonthYear
(Specific to Stull Method)
Maximum Mean Value (m) of PBL at 00 UTC from Stull MethodMean Value of PBL (m) at 00 UTC from ERA5, from the Same Year
January1980788299
February1984851405
March19841116424
April1974788457
May1980700349
June1980550223
July1990686257
August1983612217
September1987759222
October1987897338
November1975974402
December1984781298
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Timofte, A.; Bostan, D.-C.; Apetroaie, C.; Miclăuș, I.-M.; Cazacu, M.-M. The 50-Year Evolution of the Planetary Boundary Layer in the Southern Part of Romania: Comparison Between the Determinations by the Stull Method and the Reanalysis Data from ERA5. Atmosphere 2025, 16, 1247. https://doi.org/10.3390/atmos16111247

AMA Style

Timofte A, Bostan D-C, Apetroaie C, Miclăuș I-M, Cazacu M-M. The 50-Year Evolution of the Planetary Boundary Layer in the Southern Part of Romania: Comparison Between the Determinations by the Stull Method and the Reanalysis Data from ERA5. Atmosphere. 2025; 16(11):1247. https://doi.org/10.3390/atmos16111247

Chicago/Turabian Style

Timofte, Adrian, Diana-Corina Bostan, Cosmina Apetroaie, Ingrid-Mihaela Miclăuș, and Marius-Mihai Cazacu. 2025. "The 50-Year Evolution of the Planetary Boundary Layer in the Southern Part of Romania: Comparison Between the Determinations by the Stull Method and the Reanalysis Data from ERA5" Atmosphere 16, no. 11: 1247. https://doi.org/10.3390/atmos16111247

APA Style

Timofte, A., Bostan, D.-C., Apetroaie, C., Miclăuș, I.-M., & Cazacu, M.-M. (2025). The 50-Year Evolution of the Planetary Boundary Layer in the Southern Part of Romania: Comparison Between the Determinations by the Stull Method and the Reanalysis Data from ERA5. Atmosphere, 16(11), 1247. https://doi.org/10.3390/atmos16111247

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