The ATMONSYS lidar is designed as an experimental mobile system for observations of water vapor, aerosol, and temperature profiles throughout the PBL and beyond. The system has been developed with the goal of observing these profiles throughout the entire PBL with sufficiently high quality to resolve turbulent changes in their concentrations and values, especially regarding humidity. Therefore, the water vapor DIAL can be seen as the centerpiece of the ATMONSYS system, which is accompanied by an elastic aerosol backscatter lidar and a temperature rotational Raman lidar. The DIAL technique is advantageous for measuring water vapor for several reasons, most importantly because it is inherently self-calibrating according to its working principle e.g.,. Measurements at two different but nearby wavelengths are performed almost at the same time with the same optical geometry. The only difference in these two measurements is the differential extinction by water vapor along the light path, while all other instrument-dependent parameters cancel out e.g.,. Additionally, the lidar return of the DIAL is backscatter mainly from air molecules (Rayleigh scattering) and aerosols, which is much stronger than the weak inelastic backscatter used in Raman lidars. This allows for short integration times (<10 s) and a full daytime capability over the entire altitude range. A major challenge is the very sophisticated single-mode laser technique, which is mandatory for narrowband water vapor DIALs . All three lidars are housed within the same serial 20” cargo container and therefore easily movable by regular cargo trucks (Fig. a). Major modifications to the container have been made regarding the ceiling and the posts that standard cargo containers normally stand on (Fig. b). In addition to the fixed serial posts, four leveling jacks on all corners allow for mechanical adjustments of the container's height and level by hand – independent of flat ground. Two motor-driven flaps in the ceiling allow the system's periscope to be lifted outside the container.

Stable conditions within the container are vital for proper operation of the laser setup. Ideally, this would mean that there are very low temperature changes within the interior and no vibrations whatsoever. Therefore, the container's room temperature is controlled by a powerful 10 kW air-conditioning/heating system which is placed outside the container during operation to prevent disturbing vibrations. All further components inside the container that cause minor vibration due to fan propellers are mechanically decoupled with slings or rubber stands. Therefore, consequently and very importantly, the optical bench inside the ATMONSYS system is also mechanically decoupled by pneumatic leveling on all four posts of the optical bench. As the ATMONSYS system is not eye-safe, a safety radar is mounted on the container top with an automated interlock for the laser in case of any fly-overs. In addition, sensors for wind and rain are mounted next to the safety radar and are also connected with the laser's interlock in case of unexpected weather changes. A battery-powered uninterruptible power supply guarantees proper shutdown of the system and closing of the ceiling flaps in case of power outage. Also, in the case of a blackout, a block heater protects the system from freezing temperatures inside the container.

As mentioned above, the ATMONSYS lidar consists of three different lidars for the measurements of water vapor, aerosol, and temperature. A sketch of the general optical concept of both the ATMONSYS lidar emitter and receiver is presented in Fig. .

A seeded, diode-pumped, Nd:YAG laser (InnoLas) with a repetition rate of 100 Hz and a maximum average power of P=45W at the wavelength λ=1064nm is used as the main power source for all three lidar laser emissions. The elastic backscatter aerosol channel and the temperature rotational Raman channel can be directly operated with the emission after the second- and third-harmonic generator (532 nm and 355 nm), respectively. The water vapor measurements are performed with the ATMONSYS DIAL, which is operated at two wavelengths in the 817 nm band of water vapor in an alternating sequence. The laser transmission is driven by an in-house developed titanium sapphire (Ti:Sa) laser, which is pumped by a frequency-doubled Nd:YAG laser with ≈ 25 W at λ=532nm. Details on the newly developed transversal pumping configuration and the resonator setup of the Ti:Sa laser as well as its implied advantages are given in . The exact wavelengths of the Ti:Sa are defined by two tunable external cavity-diode lasers (DL1/DL2, Fig. ) which are operated in an injection-seeding procedure with shot-to-shot alternation between λon and λon similar to . Whereas the main focus of the ATMONSYS lidar is set towards high power in the water vapor DIAL channel, the temperature and aerosol channels can be considered a pleasing side product. Therefore, the second-harmonic generator is tuned for maximum power and used as the pump light for the Ti:Sa laser. The third-harmonic generator is also tuned to maximum power at 355 nm but only takes the non-converted light at 1064 nm after the second-harmonic generator. The aerosol channel at 532 nm is then operated only with the unconverted shares from the third-harmonic generator as well. In the end, all pathways of the three different wavelengths (817, 532, 355 nm, all s-polarized) are combined congruently before they leave the ATMONSYS container. The average powers of all lasers can be seen in Table . The option of implementing a beam expander has been omitted due to concerns with changes in polarization as well as chromatic aberrations caused by the three different wavelengths. A possible workaround to this problem would have been the implementation of multiple beam expanders, which, in turn, requires a lot of space and bears the downside of added complexity in their proper adjustment.

For lidar operation, a periscope consisting of two slightly oval receiving mirrors (dmin=64 cm), angled at 45°, is lifted over the container's top. The outgoing laser beams are transmitted by small mirror inlets in the center of the two big mirrors. The periscope has been constructed with the intention of scanning measurement patterns. However, inertial forces related to the high weight of the periscope lead to slight mechanical distortions during movement. Therefore, now, the system is only operated in vertical-stare mode. On the receiving end, the backscattered light is collected by two identical Newtonian telescopes (d=200 mm, f=800 mm). The initial idea of the receiver's design with two telescopes was to establish a near-field channel as well as an identical far-field channel. However, for its use as a boundary layer lidar, one channel is sufficient if the deepest hundred meters above ground are accepted as being blind. It was estimated that an additional near-field receiver would lower the start of the lidar range only by roughly 50 m at most. Instead, the very weak Raman signal return is now taken solely from one telescope in an optically isolated area of the polychromator (Fig.  and abbreviations therein). Taking into the account that Raman scattering by N2 and O2 molecules leads to a depolarization ratio of approximately 3/4 e.g.,, a thin-film polarizer with high reflection for 355 nm p-polarized light is implemented (S3, Fig. b). By this, the polychromator's efficiency for temperature measurements could be improved. The other telescope solely collects the signals for aerosol and water vapor measurements. A dichroic mirror with high transmittance for λ=600–850 nm and high reflectivity at λ=532 nm (LASEROPTIK) is used to split up the signal for aerosol and humidity measurements. For the aerosol channel, a 2 in. filter with the center wavelength of 532.23 nm and a bandwidth of 0.25 nm is used. For water vapor measurements, several filters are available, depending on the chosen absorption line. In the data presented herein we used a filter with 0.5 nm bandwidth and λ0=817.223nm. For completeness, we point out that the Raman section of the polychromator in Fig. b shows a second water vapor detector as well. This channel uses a wider filter width a bandwidth of 2 nm. It has been installed to switch wavelengths without the need for mechanical filter changes. In addition, this allows for using a wider spread of λon and λoff. Also, by this, potential problems with the angle of incidence in the near field could be investigated and reduced . At the focal point of both telescopes, a slit diaphragm (A in Fig. ) defines the actual field of view and allows for the reduction of background light. The field of view ranges from 2.5–5 mrad, depending on the axis of the slit diaphragm. After the telescope's focal point, the light beam is collimated between pairs of f=100mm plano-convex lenses (L1). After passing its respective interference filters and beam splitters within this collimated path, each beam diameter is again reduced (L1) and collimated by f =15 mm plano-convex lenses (L2) directly in front of photomultiplier tubes (PMTs, manufactured by HAMAMATSU).

The signal from each of the channel's PMTs in the receiver (Fig. b) is collected by a 12-bit transient digitizer (Licel) with a memory depth of 24 bits, operated at a voltage range of 500 mV. The 24th bit acts as clip flag in the case of signal overflow. However, even if the signal level from a 10 s integration does not indicate overflow, partial overflow due to atmospheric fluctuations can still lead to nonlinear signal behavior of the 10 s integrated signal, even if the clip bit does not indicate overflow. As a rule of thumb, this effect can already occur if the signal level is higher than 50 % of the voltage range (Bernd Mielke, Licel personal communication, 2024). The transient digitizer, connected to the PMT via BNC cables at 50 Ω impedance, operates at a sampling rate of 20 MHz, which equals a spatial resolution of 7.5 m. For technical simplicity, the water vapor DIAL only operates with an analog channel as its focus is set on measurements inside the PBL. Only for the very weak signals of the temperature rotational Raman channel does an adjustable discriminator allow for simultaneous photon counting (FAST-MCS6).

Regarding the retrieval of humidity profiles, much fundamental work has been published on the water vapor DIAL equation, discussing major considerations that have to be respected e.g.,. Based on these detailed publications and adapting the successful implementation as described in , the absolute water vapor molecule concentration NH2O is calculated by using the well-known DIAL equation as follows: 1NH2O=1Δσ↑(r)+Δσ↓(r)-ddrln⁡Son(r)Soff(r)+G(r). Here, Son/off represents the measured signals from the absorbed “online” wavelength λon and the unabsorbed “offline” wavelength λoff. Δσ↑ and Δσ↓ are the effective absorption cross sections of water vapor for the upward path of the narrowband laser light and the downward path, respectively, of the spectrally Doppler-broadened, backscattered light from air molecules. r is the vertical distance from the lidar and G refers to a correction term needed in order to account for the spectral variation of the backscattered light which is molecularly Doppler-broadened see. Therefore, this term is dependent on the water vapor distribution itself as well as the ratio between molecular and particle backscatter. As can be seen in , this term can become relevant in two cases. The first case would be that the molecular backscatter coefficients βM are much higher than the backscatter coefficients βP from aerosols (βM/βM + P≈1) – which is usually not the case for observations within the PBL. The second case in which this term can become relevant is for atmospheric conditions in which there are strong gradients of βM/βM + P – which is indeed the case within the PBL. This effect could principally be reinforced by the occurrence of fluorescing aerosol, caused by the emission of the 355 nm channel, which might act as a masked form of aerosol backscatter coefficients. In the current configuration of very small energies in the 355 nm channel (≈ 1 W), this effect is most probably negligible. Nevertheless, this effect has to be kept in mind in the case of substantially increasing pump lasers. However, after testing the effects of the correction term G, we found that for most heights of the PBL, the error is not dominant as it stays below values of ≈ 2 %. At those altitudes, however, where there are strong gradients of βM/βM + P, the calculation of those is far from being trivial as the calculation of the gradient is very noisy if it is calculated from bin to bin. On the other hand, if the gradient is calculated over multiple bins, the locally very sharp aerosol gradients are artificially broadened and therefore inflict the corrections over a large range of altitudes. This bears the risk of applying a wrong correction at altitudes where G should not play a role. For those reasons, the humidity calculations presented herein omit the correction term G, following the reasoning that an overall small error is preferential over the introduction of artificial errors due to the implementation of a problematic correction term. Recent instrument developments show a method which could potentially circumvent this problem by adding a high-spectral-resolution lidar (HSRL) channel to DIAL systems, providing reliable information on molecular and particle backscatter properties without any dependence on a proper Klett inversion algorithm . Despite the fact that the ATMONSYS has been designed without an additional HSRL channel, following the thoughts of , effects of the Rayleigh–Doppler-broadened signal are minimized if the online frequency is chosen to be near the inflection point of the absorption line as done for this measurement set, taken on a humid summer day. In order to rule out the possibility that Rayleigh–Doppler broadening crosses the absorption line peak, we choose an absorption line under the premise of ensuring a suitable optical depth, resulting in a related wavelength λon in a position further out than the actual inflection point of this absorption line. This, however, comes with the downside of not fully guaranteed minimization of a potential Rayleigh–Doppler error. The online frequency has been chosen to be λon,vac=817.2460nm, which is in the flank of an absorption line centered at λ0,vac=817.2231nm . The offline frequency has been set to λoff,vac=817.3526nm. Further details on the DIAL specifications can also be read in Table . Beyond that, provide a detailed description regarding resonator stabilization, seeding, and spectral characteristics of the laser beams. The calculation of the effective σon/off in both the upward and downward direction is a crucial point within the DIAL equation. In order to account for the Lorentz pressure broadening and the Rayleigh–Doppler broadening, a convolution of those two effects has to be calculated which is described by a Voigt function. This function is dependent on both pressure and temperature over height. Therefore, in order to calculate precise absorption coefficients, additional information on the atmospheric state is needed. More details on both the calculation of the σ profiles and the spectroscopic line characteristics can be found in , or . For all data presented in this paper, the prevailing atmospheric pressure and temperature conditions were taken from radiosonde ascents that are operationally performed by the DWD nearby (Sect. ).

For the numerical inversion of the DIAL equation, Eq. () can be rearranged to 2NH2O=1Δσ↑(r)+Δσ↓(r)-1q(r)ddrq(r)+G(r), avoiding any asymmetric noise behavior caused by the logarithm and where q(r)=Son(r)Soff(r). The numerical solution to the term ddrq(r) is implemented by calculating the slope of a least-squares linear regression line. The regression line at one data point is calculated by using symmetrically distributed neighboring data points. Following the explanations within , this finally leads to the numerical solution 3NH2O(ri)=1Δσ↑(ri)+Δσ↓(ri)×-1q(ri)δi∑(j-i)q(rj)∑(j-i)2+G(ri), where i is the respective bin of interest, k is the number of neighboring points into one direction, ∑=∑j=i-kj=i+k, and δi=ri+1-ri=7.5m. The total linear regression interval length is given as B=2k+1.

The statistical uncertainty of lidar measurements is driven both by electronic noise and disturbing atmospheric noise. For DIAL systems, those statistical uncertainties are calculated by means of Gaussian error propagation, which, in the end, leads to the uncertainty 4σNH2O(ri)=1Δσ↑(ri)+Δσ↓(ri)⋅1q(ri)×a(ri)2q(ri)2σq2(ri)+σa2(ri),witha(ri)=ddrq(ri). Here, σq(ri)=1(2k+1-2)∑(a(ri)rj+b(ri)-q(rj)2 and σa(ri)=σq(ri)δi∑(j-i)2. bi=iδia(ri)+12k+1∑q(ri) denotes the axis intercept of the regression line mentioned above. As can be seen in Eqs. () and (), the total interval length B influences both the spatial resolution of the measurement and the statistical uncertainty. In order to keep a reasonable signal-to-noise ratio (SNR) throughout the PBL, the DIAL retrieval decreases its spatial resolution towards higher altitudes with a step function ∝r2 (Fig. ). The effective vertical resolution of radar and lidar systems is defined by . According to , this equals about a third of the interval width that is chosen for the derivation of the logarithmic signal ratio in the DIAL equation. The parameters for the variable resolution are chosen with the intention of keeping the standard deviation of the calculated water vapor concentrations pretty much constant over height and below 5 %. Due to its measurement principle, the DIAL relative uncertainty is scarcely dependent on the absolute values of specific humidity; further information on the statistical uncertainty of the ATMONSYS measurements will be shown in more detail in Sect. . During some measurement periods, the calculated humidity profiles show an odd artifact of concentrations that are too high at low levels. However, due to the DIAL principle and the instrumental setup, where both signals λon and λoff take the same pathway, which, as a consequence, should cancel out any identical overlap behavior within Eq. (), this cannot be a classic overlap issue. Therefore, we assume that there has been an issue with a detector overload which leads to this artifact, despite the fact that the clip flag has not been set by the transient digitizer. However, as introduced at the beginning of this section, detector overflow could still have taken place without any clear notice. This assumption is supported by the fact that the issue with humidity values that are too high towards ground level is not identical at all times. As the reason for this behavior remains unclear, the presented data have not been modified by any correction function. Therefore, the absolute values below ≈ 0.5 km above ground have to be interpreted with some caution. Their relative changes, however, should not be affected by potential artifacts. The aerosol data shown in Sect.  result from the ATMONSYS elastic backscatter aerosol channel at 532 nm. These data have the same temporal resolution of 10 s but a higher vertical resolution of 7.5 m. The aerosol backscatter coefficients are calculated with the Klett inversion algorithm .

At Lindenberg, DWD has operated the autonomous Raman lidar for atmospheric moisture sensing (RAMSES) since 2005. After several extensions, RAMSES has evolved into a spectrometric fluorescence and Raman lidar with several receiver units, including three spectrometers. Unfortunately, due to maintenance on its air-conditioning system, RAMSES did not operate continuously during the ATMONSYS deployment in Lindenberg. However, it was possible to have a small temporal overlap in which both systems operated, which is sufficient to allow for a comparison of the measured data. For the case study presented here, data from the discrete detection channels of the near- and far-range receivers , and from the UVA spectrometer (378–458 nm) , which is a subsystem of the near-range receiver, are analyzed. Because of its complex receiving system, RAMSES possesses duplicate measurement capability for most measured quantities. For instance, to obtain optimum measurements of water vapor mixing ratio, data from the near-range receiver (discrete detection channels before and UVA spectrometer after sunset, respectively) below 2 km and the far-range receiver (discrete detection channels) above are merged. In contrast, the particle backscatter coefficient and depolarization ratio are calculated using only data from the discrete detection channels in the far-range receiver. The fluorescence backscatter coefficient in the cyan wavelength range is determined by integrating the fluorescence spectrum measured with the UVA spectrometer (nighttime operation only) between 455 and 535 nm. In this study, 240 s of lidar data are integrated for each profile. The vertical resolution of the raw data is 60 m, and signal profiles are smoothed with a sliding average length of 3 and 5 height bins between 1 and 2.5 km and above 2.5 km, respectively. With these settings, statistical measurement errors of the water vapor mixing ratio are typically between 5 % and 15 %.

Towards the end of FESSTVaL, an additional water vapor Raman lidar was set up at Lindenberg. The Atmospheric Raman Temperature and Humidity Sounder (ARTHUS) lidar system is the noncommercial precursor of the Raman lidars from Purple Pulse Lidar Systems S.L. It measures water vapor throughout the PBL during nighttime and daytime conditions at a sampling rate of at least 10 s. Although it was not directly involved in the FESSTVaL campaign, we could benefit from the synchronous measurement. This gives us the advantage of an intercomparison between all three water vapor lidar systems. The ARTHUS data have been obtained with a vertical sampling of 3.75 m at a temporal resolution of 10 s. The signal has been smoothed by a vertical sliding average of 26 bins, resulting in an effective vertical resolution of ≈ 100 m. The statistical uncertainty of the ARTHUS measurements is determined by applying error propagation to the measured photon counts (or virtual photon counts for analog signals) . This method accounts for shot noise, the primary source of error in Raman lidar signals. To obtain the total statistical uncertainty, an autocorrelation analysis is performed on a time series of the measured parameter fluctuations . This approach distinguishes between uncorrelated noise and correlated atmospheric fluctuations, enabling the simultaneous retrieval of total noise uncertainty profiles and higher-order moment profiles of atmospheric fluctuations, along with their associated uncertainties.

Measurements of vertical fluxes with lidar systems depend on the combination of vertical thermodynamic profiles with vertical wind information. Therefore, vertical-staring Doppler wind lidars with a very high temporal resolution are needed. At MOL-RAO, we operated a Streamline XR Doppler lidar (Halo Photonics). The instrument has a range gate length, and therefore vertical resolution, of 48 m while using a maximum of 125 range gates, which, under good meteorological conditions, leads to a maximum vertical range of 6000 m. The Doppler lidar measured with 20 000 pulses per ray and a sampling rate of ≈ 3 s. The system has a pulse width of 330 ns, a pulse repetition frequency of 10 kHz, and a wind velocity statistical measurement uncertainty of 0.1 ms-1. We removed the data with a high noise level by filtering with a relatively low signal-to-noise ratio (SNR) + 1 threshold of 1000 to keep the data availability high as in. The SNR values are used as a quality indicator of the radial velocity measurements and are generally output by the Doppler lidar. The system calculates the SNR values by comparing the sensor's internal noise level with the intensity of the backscattered light from the system's emitted pulsed laser beams. As the spatial variability inside the PBL is known to be quite high, we situated the Doppler lidar as close as possible to the ATMONSYS DIAL at a horizontal distance of <5 m. By this, both lidars should measure mostly the same air volume, with small discrepancies due to differing beam divergence. This setup was realized only for a selected time period as the Doppler wind lidar was operated at different sites and in different scan configurations during the campaign.

At MOL-RAO, DWD conducts four daily routine ascents of Vaisala RS41-SGP radiosondes per day. During the time of FESSTVaL, additional ascents were conducted in cases of promising atmospheric conditions regarding the campaign goals of FESSTVaL. The release site of the radiosondes was in close proximity to the ATMONSYS container within a distance of ≈ 200 m. Detailed information on the technical specifications of the radiosondes is given directly by the manufacturer (https://docs.vaisala.com/v/u/B211444EN-J/en-US, last access: 9 September 2025). For measurements of relative humidity, a sounding uncertainty of 4 % and temperature-dependent response times of <0.3 s (20 °C) and <10 s (-40 °C) are claimed. These data are available for the entire time period in which ATMONSYS was operating .

All data presented in this paper were collected during 18 July 2021. This specific day has been chosen for two reasons. First, it has the advantage that all of the instruments introduced above were operating simultaneously and at the very same location. Second, the prevailing weather on this day led to representative conditions of a typical convective summer day. Figure  gives a broad overview of the atmospheric conditions and development during the second half of this specific day. This overview graphic has been generated with data from the continuously running RAMSES lidar at a temporal resolution of 4 min. Already at this temporal resolution, frequent changes between high and low humidity concentrations within the lowest 2 km reveal convective behavior (Fig. a). Also, a typical moistening of the PBL during day can be observed with a simultaneous increase in the PBL height – visually defined by strong vertical humidity gradients, vertical gradients in the particle backscatter coefficients (Fig. b), and partly by the particle depolarization ratio (Fig. c). However, it has to be stressed that the determination of the PBL height is somehow tricky and strongly dependent on the method being used e.g.,and references therein. Definitions of aerosol- and humidity-gradient-based PBL heights do not necessarily coincide with thermodynamic or kinetic energy definitions of the PBL top. Therefore, as additional information, data from the available radiosonde ascents have been used to calculate the PBL top (Table ) defined by the bulk Richardson number as described in and . At least for high noon, those values show to be in good agreement with the visual perception of humidity and aerosol backscatter gradients. A Doppler wind lidar at a nearby site was measuring horizontal wind speeds by doing velocity–azimuth display (VAD) scans. Based on the measured values for the horizontal wind speed maximum, showing the nose of the low-level jet (and therefore the PBL height), the PBL top can be confirmed to be at altitudes of 1500 ma.g.l. during high noon.

Besides a general idea of the PBL development, the particle backscatter coefficient shows the development of convective clouds passing over the lidar from 12:00 to 16:00 UTC. Starting around 20:00 UTC, dense clouds develop underneath an elevated aerosol layer which is located at ≈ 2.5 km. Furthermore, the combination of Fig. b–d reveals valuable information about the dynamical situation of aerosol concentrations during the second half of this day. From 12:00 until 20:00 UTC, the particle depolarization ratio shows increased values between ≈ 2 and 4 km, hinting towards elevated concentrations of dust particles. Between 20:00 and 24:00 UTC, the already mentioned enhanced particle backscatter coefficients at ≈ 2.5–3.5 km show almost no particle depolarization ratio. However, the fluorescence backscatter coefficient of this layer is significant with very high vertical gradients. Based on those features, the origin of this aerosol layer can be connected with wildfires. Section  already discussed the potential issue with fluorescence backscatter in the 817 nm DIAL channel, which could be caused by strong emission power at 355 nm. Although the ATMONSYS system does not operate with such high power at this wavelength, Fig. d impressively shows very steep fluorescent backscatter coefficient gradients.

All ATMONSYS DIAL data presented within this publication have been recorded at a sampling rate of 10 s. This is the highest temporal resolution at which the system has been operated so far. Though somehow arbitrary, this value is a trade-off decision in order to allow for observations of turbulent transport processes while, at the same time, keeping a good SNR and, therefore, reliable measurements over a high range of altitude. With the very same intention towards signal quality and vertical range, the DIAL retrieval decreases its spatial resolution as already shown in Sect. .

On 18 July 2021, this resulted in a maximum vertical range for the water vapor DIAL of ≈ 3.2 km under clear-sky conditions even around the time of the daily apex of the sun's motion (Fig. a). This maximum range value naturally changes mostly with the prevailing atmospheric conditions. In this particular case it can be seen that 3.2 km corresponds to an altitude with a thin layer of nearly zero aerosol concentration. The aerosol layer lying above with slightly higher particle backscatter coefficients, at least in the presented case, does not lead to a reasonable DIAL signal anymore (Fig. b). Furthermore, at an altitude between ≈ 2 and 2.5 km, Fig. b shows a very significant wave pattern which is not that apparent within Fig. a. The reasons for this “wave-like” structure are not clearly attributable. The presented time period has been chosen as it is (mostly) free of small convective clouds and constantly allows for smooth values over the full height. Regardless of the fact that there is enhanced aerosol up to a height of at least 3.2 km, it has to be stressed that the PBL top is situated much lower in this specific case, as already indicated by Table . The application of an automated boundary layer height detection algorithm to the aerosol data similar to determines the PBL top to a height of ≈ 1.2 km. This altitude of steepest gradients can easily be confirmed by eye for both aerosol and humidity distribution. However, as discussed earlier, a humidity- and/or aerosol-gradient-based estimation of the PBL top does not necessarily coincide with its thermodynamic definition, leading to differing numbers in comparison to Table .

Over the presented time period of 1 h, structures of alternating moisture concentrations can clearly be observed throughout the entire PBL in the form of darker plumes (e.g., at ≈ 11:48 UTC) which are surrounded by drier time periods with lighter color shading. Those changes can also be studied in more detail within Fig. a. As the structure of those humidity plumes is non-periodic, we can attribute this behavior to convection. However, the direct linkage between convective updrafts and changes in humidity is not always straightforward as can be seen in the following. For an exemplary purpose, in order to visualize correlations in changes of humidity and aerosol concentration with convective phases, their changing structures can be highlighted by calculating absolute and relative changes to the median in each height level: 5Δxrel=xx̃-1,Δxabs=x-x̃. Here, x can be either absolute humidity or aerosol backscatter coefficients. x̃ is the median of the respective measure at each single height level over the entire time period that is plotted in Fig. . In contrast, to directly show the actual vertical movement of the air parcels, Fig. c visualizes the measured absolute vertical wind velocity. By this formula, positive values show an overall increase in concentrations compared to the prevailing median and vice versa for negative values. These changes (Fig. a and b) can be compared with the prevailing vertical winds measured by the Doppler wind lidar positioned directly next to the ATMONSYS system (Fig. c). For the changes in humidity, one has to keep in mind that the absolute values of humidity as observed in Fig. a drop above the PBL. This allows for several insights. First, the changes of absolute humidity (Fig. a) are slightly larger above the PBL than within the PBL, whereas the relative changes are substantially larger above the PBL. In our understanding, this can be attributed to turbulent mixing inside the PBL, which becomes apparent in constant vertical humidity concentrations inside the PBL e.g.,. Above the PBL, on the other hand, lacking turbulence and entrainment processes lead to much more horizontal heterogeneity, which is advected by free-tropospheric winds, therefore leading to larger relative changes of moisture concentrations over time. At the same time, a statistical SNR feature cannot be ruled out as the absolute humidity concentrations above the PBL become lower, which can increase the relative deviation as well. Nevertheless, the behavior of increasing relative moisture variability over height is apparent in other observations as well e.g., but at much lower temporal resolution. This can at least partially be attributed to the fact that the upper edge of the PBL is a mixing layer, where turbulent mixing of humid air from the PBL and dry air from the free troposphere takes place. This potentially results in a very heterogeneous water vapor distribution in this altitude region, which streams through the probed volume with the synoptic wind. The attribution of vertical variability will be discussed in more detail in Sect. . Second, we can ascertain that the correlation between moisture and aerosol concentration on the sub-minute timescale (Fig. a and b) is quite complex and not at all straightforward. As can be seen, e.g., around 12:00 and 12:18 UTC and especially around the PBL top, there are times in which high moisture values coincide with high aerosol concentrations and vice versa for low values. This could be explained by a common source of aerosol particles and moisture at Earth's surface. Also, although there is a lot of noise in the moisture changes above the PBL, one can interpret quite similar sinusoidal patterns for both moisture and aerosol concentration. A simple temporal moving average for the humidity data, which is not included here, denoises the patterns. Nevertheless, this does not change the general picture of some identical patterns, which are, however, not always temporally and spatially consistent with the aerosol pattern. Therefore, a general and straightforward correlation between aerosol and humidity changes is not apparent. The same observation can be stated if one includes the vertical winds (Fig. c). Again, there are phases in which, e.g., the sinusoidal pattern of the aerosol changes at ≈ 1.8–2.3 km above ground level (a.g.l.) coincide with respective upwinds and downwinds. However, the connections are not always obvious. Finally, the very same observation is also true if one compares the changes of humidity with vertical wind speed. Again, it can be seen by eye that enhanced moisture concentrations do not always coincide with a certain direction of vertical motion. This shows that the horizontal advection by large eddies and mean horizontal wind plays a major role and has to be considered. Especially above the PBL, we consider horizontal advection to be the most dominant source of inhomogeneity, which should lead to a certain decoupling of moisture and aerosol changes to the vertical wind velocity. As can be seen, the combination of data in Fig.  contains a lot of potential. We expect that an in-depth analysis of correlations and causalities between humidity, aerosol concentration, and vertical winds over multiple days is of high interest in terms of convection initiation and cloud formation. However, the much more detailed analysis of potential coherence between those measures is beyond the focus of this paper.

In the previous section, Fig. a already visualized the variability of calculated absolute humidity values over height and time. The amplitude of relative deviations from the median value at each respective altitude was shown to be considerably lower inside the PBL and much higher in the lower free troposphere. However, purely based on the previously discussed graphics (Figs.  and ), it is unclear where to attribute the reasons for this pattern as several causalities are plausible. On the one hand, decreasing signal strengths from higher altitudes proportional to 1/r2 and overall lower humidity concentrations lead to much lower SNR values and therefore higher statistical noise. This physical restriction is reflected in an increased profile-to-profile variance which can be misinterpreted as atmospheric variability. This issue, however, can be exacerbated by increasing the spatial interval length for the linear regression inside the DIAL algorithm (Eq. ), leading to lower spatial resolution but also lower statistical noise. On the other hand, changes in concentrations of water vapor in the lower free troposphere are much more related to horizontal advection by substantially stronger winds than they are inside the PBL. Different sources of origin and less turbulent mixing can therefore lead to substantial differences in atmospheric humidity concentrations rolling by the lidar's vertical measuring column. Therefore, it is not possible to directly attribute the observed deviation fluctuations to issues with signal strength or actual atmospheric conditions. As a consequence, a quantification of uncertainties based on all single 10 s profiles from the very same time period as before (11:36–12:36 UTC, ≈ 360 profiles) is presented in the following (Fig. ). For this quantification of uncertainties, dense cloud-inflicted profiles that show unrealistic, strongly oscillating values are ignored above the clouds and therefore not included in the statistics. They are detected based on their simple feature of reaching negative values at an altitude in which humidity is far from zero. The negative values occur due to the fact that, in the event of clouds in the laser pathway, the stronger signal for λoff reaches a saturated nonlinear response first near the cloud base. As a consequence, afterwards, ddrln⁡Son(r)Soff(r) changes its sign above the cloud base due to a further increase in λon, leading to negative values of the retrieved water vapor concentration. Accordingly, the filtering is done in the simple way that we look for the respective cloud-influenced profiles that reach values less than zero within the lowest 3 km. This proved to be a straightforward and at the same time reliable method, at least under the weather conditions at the instrument site for the presented data. The spread of values for all single profiles within the respective time period is presented by the dashed gray lines in Fig. a. At first glance, it is obvious that the spread of values above ≈ 3.2 km is too high for reliable humidity values. This has already been seen directly in the time series (Fig. ). Below that altitude, the spread is reduced and reveals several characteristics. For a better visualization of the majority of measurements, the gray shaded area shows all values between the p10 and p90 percentiles. By this, single extreme outliers which can be caused by atmospheric disturbances (e.g., insects, condensation) or lowered laser performance (e.g., mode hop/reset of the seeding device) do not influence the overall distribution. The absolute width between p90 and p10 is visualized on the right side of the same graphic (Fig. b, gray line). According to our expectations, the spread of values is the lowest for the lowermost altitudes, which is at least partially fostered by a high SNR. Above the PBL, especially at ≈ 1.3–2 km, the calculated values show a larger spread than below. Interestingly, the p90–p10 width is reduced again at around ≈ 2.5 km, almost reaching the values from the lowermost measurement altitude. This can be understood as direct proof that at least a significant portion of the wider spread of humidity concentrations at altitude levels of ≈ 1.3–2 km is caused by actual atmospheric variability and not by a decreasing SNR. This argumentation is reinforced by the relative standard deviation, which is directly calculated out of the linear regression during the DIAL retrieval . The respective blue line in Fig. b is relatively constant over height, always staying below values of 5 % relative standard deviation. As already described, this behavior is due to the dynamic spatial resolution over height (Sect. ). It shows that, with this configuration, the ATMONSYS DIAL stays within the aforementioned criteria for observation uncertainties <5 %. In addition to the standard deviation that can be determined from the linear regression inside the retrieval algorithm, Fig. b also shows the profile-to-profile relative standard deviation (red line). This means that the standard deviation is calculated with respect to the mean of all values inside the selected time period.

What can be seen directly from both the red and the blue line is that there is a maximum of values at ≈ 1.5–1.7 km. This is again an indication for the position of the PBL top. As dry air parcels from the free troposphere are entrained into the moist PBL and vice versa, the variance is the highest in the region of the PBL top, although the relative standard deviations lead to maxima at higher altitudes compared with the strong gradient of humidity. From the comparison of the profile-to-profile standard deviation (Fig. b, red line) with the standard deviation of the DIAL algorithm (Fig. b, blue line) we can deduce information on the spatial scale of the humidity variations. This is enabled by the fact that the prevailing moisture concentration within a chosen interval length dr defines the slope of the term ddrln⁡Son(r)Soff(r) (Eq. ). Therefore, under the assumption of constant humidity throughout this interval length, the slope of this term would be constant and, hence, the standard deviation of the linear regression would be low. As a consequence, if the interval length is large enough to include different humidity regimes, the standard deviation of the DIAL algorithm increases and, thus, can be misinterpreted as statistical uncertainty. As the integration length of the DIAL retrieval algorithm in this region is about 150 m we conclude that there are humidity variations on a smaller scale. A higher level of standard deviation in the DIAL algorithm might also be induced due to less humidity and therefore lower values of ddrln⁡Son(r)Soff(r) or low SNR values. Nevertheless, this influence is not dominant as the standard deviation decreases towards higher altitudes despite a further decrease in humidity. Above this layer, the values drop for both uncertainty estimators, similar to the previously described p90–p10 width (gray line), but stay at higher levels than inside the PBL. From the difference between the blue and the red line (Fig. b), we can also give an estimation of the atmospheric variability, which is related to the residual of the measured variations after subtraction of the instrumental uncertainties. Within the PBL, it covers values from 5 % at the lowermost altitudes that grow with height up to ≈ 30 % in the area of the PBL top. This increase in variability with height shows that both horizontal advection by eddies and vertical entrainment into the PBL lead to much higher humidity variability than is generated by the ground-dependent heterogeneity of evaporation at the surface level. Both the magnitude of variance values and the described behavior of increasing values over height can be confirmed by humidity measurements at several levels on very high towers (e.g., the Park Falls tower – data available at https://flux.aos.wisc.edu/fluxdata, last access: 9 September 2025). Above the boundary layer top, the atmospheric relative variability has values around ≈ 20 % or more. Again, above 3 km the backscatter from aerosols diminishes, which leads to very high uncertainties that, in contrast to lower altitudes, have to be attributed to instrumental noise caused by low SNR values.

A first impression of how the absolute values and their median from that time period compare to the in situ RS41 radiosonde measurements is given by the red line in Fig. a. This is, however, only a coarse intercomparison as the starting time of the radiosonde was at 10:45 UTC and it only needed about 10 min to reach a height level of 3 km above ground. Additionally, the radiosonde drifts with horizontal winds and does not probe the same volume. Nevertheless, the general vertical humidity distribution is still well represented by the sonde as there were not any major meteorological changes within the time difference of less than an hour. As already mentioned in the previous section, the time period around the ascent of the radiosonde is afflicted by sporadic occurrences of shreds of clouds. Nevertheless, Sect.  will show an intercomparison between cloud-free radiosonde profiles and the lidar measurements at the best possible temporal overlaps. The absolute deviations between the humidity, measured by the radiosonde and DIAL, especially within the PBL, will be discussed there in more detail.

The PBL is the atmospheric layer that is directly influenced by the Earth's surface. Thermal convection and surface-induced friction cause both vertical and horizontal wind shear, which in consequence leads to the formation of eddies and, therefore, turbulence. From a starting point, these eddies are driven by stronger winds in the free troposphere, which, as a consequence of the friction, lead to eddies with big diameters that can even equal the PBL height. Depending on the apparent season, local weather conditions, time of day, and surface properties, the PBL height can vary from <100m up to ≈ 3 km. For the specific time period of investigation, judging from strong humidity and aerosol gradients as well as wind and bulk Richardson number (Sect. ), the PBL height is >≈1.2–1.5 km. Over time, these big eddies decay into multiple smaller ones with diameters less than 1 m, leading to eddies of multiple diameters e.g.,. The decay from larger to smaller eddies means a simultaneous energy decline. Inside the PBL and within isotropic turbulence conditions (≈ 0.01–5 Hz), this decline of energy follows the so-called “Kolmogorov -5/3 law” . This law stipulate that a decline of energy density by the factor 5 is directly intertwined with an increase in frequency by the factor 3. The applicability of this law to real-world measurements has been demonstrated many times by multiple studies e.g.,, but only rarely for humidity lidar measurements. Throughout the last three decades, a small collection of such turbulence investigations developed with DIAL measurements has been made with, at that time, lower spatiotemporal resolution , a methodological focus on the treatment of statistical high-order moments for high-resolution DIAL measurements , and high-resolution Raman humidity lidars .

Following this theorem, instruments can be tested on their capability to resolve turbulence, which is frequently done e.g.,. In the logic of this theory, only within spectral ranges where the turbulence spectra of the instrument show the -5/3 correlation is the measuring instrument capable of resolving turbulence. The application of this theory is bound to the assumption of isotropic turbulence and only refers to the inertial sub-range. The methodology of this procedure is described, e.g., by and is based on the Fourier-transformed turbulence spectra of the measurements. For turbulence spectra, Fourier-transformed always refers to the fluctuation of the mean value according to the Reynolds decomposition. This means that every measured value, here in the case of absolute humidity q, can be decomposed into the mean value q‾ and its fluctuation q′ in the following manner: q=q‾+q′.

In the following, we present turbulence spectra over a time interval of 2 h for the ATMONSYS DIAL humidity measurements q′ and for the Doppler wind lidar standing next to it, delivering vertical wind values w′ (w=w‾+w′). In addition, the co-spectra from vertical humidity and wind measurements are shown as well. For the co-spectra, one has to keep in mind that the Kolmogorov dependency for the energy decay in the inertial sub-range changes from -5/3 to -7/3 e.g.,. In order to get reliable results from those co-spectra, the time series of measurements have to be carefully prepared so that they match each other in the best possible way. As already described, the DIAL measurements have a temporal resolution of 10 s. The Doppler wind lidar was running with a higher temporal resolution of Δt=3s. In order to have similar resolutions, the wind data have been block-averaged to the identical resolution of Δt=10s. Outliers from both time series are removed in an iterative way in which the standard deviation σ is calculated individually for each height level of the time series. In a next step, all median-subtracted values that exceed a range of 5σ are removed. Then, the next iteration starts with a newly calculated median and σ. This is done until no more data points are removed. Removed values are replaced by interpolated values. If the number of outliers exceeds a threshold of 10 %, the entire time series is neglected. The time series is detrended by the application of a linear regression. Finally, the data are high-pass-filtered with a boundary frequency of 30 min.

The comparison of the turbulence spectra for both humidity q and vertical wind w (Fig. ) reveals several features. First, the wind spectra for w′ are visually in good agreement with Kolmogorov's law from ≈ 1.5–5 ×10-2 Hz at all presented heights. At the frequency of ≈ 1.5 ×10-2 Hz, a drop towards lower energies is visible at all heights – although the spectra still show parallel behavior to the dashed Kolmogorov line down to ≈ 6 ×10-3 Hz. For all three altitudes, but most dominantly for the spectrum line at 500m, a second drop of energies towards lower energy can be observed at ≈ 9 ×10-3 Hz. Similar, but not identical, structures can be observed for the humidity spectra. Here, agreement with the Kolmogorov spectrum is obvious in the frequency range of ≈ 2–3 ×10-2 Hz across all altitudes. However, the spectrum of q′ does not always follow the dashed Kolmogorov line. Horizontal “energy plateaus” can be seen almost simultaneously at all three altitudes, e.g., from ≈ 1.5–2 ×10-2 Hz and ≈ 3–4 ×10-2 Hz. Nevertheless, at both lower and higher frequencies, the spectra change again from plateaus to a decline of energy, parallel to the dashed line of the Kolmogorov spectrum. Even at the highest frequencies of the DIAL (≈ 4–5 ×10-2 Hz), where white noise would be expected the most, the spectra at all three altitudes are parallel to the Kolmogorov line. Interestingly, at least the q spectra for 358 and 500 m show agreement with Kolmogorov even towards lower frequencies (≈ 4 ×10-3 Hz), as this is the case for the w′ spectra. This would imply that turbulence is more relevant for the local moisture variation at lower frequencies than it is for vertical winds. An atmospheric reasoning for such differences could be multifaceted. However, it seems plausible that external drivers such as solar radiation at the surface due to clouds in combination with horizontal advection can lead to a decoupling of the behavior of q and w in their accordance with Kolmogorov's law – especially over heterogeneous terrain.

The co-spectrum (Fig. ) is the spectrum of the product q′w′. The latent heat flux is defined as QE=ρ(p,T)Lv(T)⋅q′w′, where ρ is the persisting pressure- and temperature-dependent air density and Lv the latent heat of water vaporization. Thus, the co-spectra can be seen as test frequency spectra, giving an answer to the question of whether or not the instrument combination can ultimately lead to a proper determination of the latent heat flux. The actual calculation of those vertical fluxes, however, is not part of this publication.

Looking at the co-spectra, it becomes apparent that the spectra of q′ and w′ do not always follow the same behavior, as the co-spectra can show different features compared to the single spectra. Especially at the altitude level of 500 m, the co-spectrum consistently follows the Kolmogorov -7/3-relation for higher frequencies (>2.5×10-2Hz). However, similar to the single spectra, the co-spectra also show frequency bands with almost constant energy levels. In contrast to the single spectra, the frequency bands in which deviations from the Kolmogorov law appear are now non-identical for the shown altitudes. From the analysis of more altitude levels, which are not included here, it could be observed that the intervals with strict accordance with the dashed Kolmogorov line do change their frequency range non-systematically over height. Therefore, we conclude that those features are not the result of any systematic error. The co-spectra of all altitudes flatten towards lower frequencies, the lowest around < 5 ×10-3 Hz, which is in agreement with a similar behavior that could be seen for low frequencies in the DIAL humidity and mostly the Doppler wind turbulence spectra and, therefore, does not indicate a general DIAL deficiency at low frequencies. As a consequence of the observed flattening of the co-spectra, first of all, we conclude that the variations in vertical latent heat flux slower than 5×10-3Hz are not generated by the decay of larger eddies but represent the initial variability by the first order of large eddies or advected horizontal inhomogeneity. As the co-spectra do not show identical structures as within the initial spectra of w′ and q′ towards lower frequencies, we secondly conclude that the variations slower than 5×10-3Hz are independent and decoupled for w′ and q′ and have different origins. This hints towards the hypothesis that the variability of q, at least in high PBL altitudes, is in large part a result of the horizontal advection of inhomogeneous air masses, while the variability of w is dominated by convective dynamics. However, looking at the highest frequencies of the co-spectra, agreement with Kolmogorov's law is apparent at all altitudes, despite minor differences in the frequency range of good agreement. This is true even besides the general point that spatial averaging of the lidar data leads to losses of the high-frequency contributions of very small eddies . The advantage of co-spectra is that the noise of w′ and the noise of q′ are not dependent on each other. This has the pleasing effect that higher noise levels from one instrument can be partly compensated for by another instrument with better high-frequency quality.

As a result, the co-spectra are shown to be able to resolve turbulent structures down to the level of 5×10-2Hz or 20 s, which is the Nyquist frequency for measurements with Δt=10s. Nevertheless, the unexpected behavior of almost constant energy levels over frequency remains of interest. As already indicated, in general, constant levels of energy in the co-spectra are interpreted as white noise and hint towards increased noise in the data – hindering the adequate detection of turbulence. Typically, and under the assumption that the highest frequencies are still within the inertial sub-range, this white noise becomes apparent at the highest frequency range of the spectra where the measurements reach their SNR limit. Measurements with instruments at higher temporal resolution e.g., show that the assumption of an inertial sub-range is valid up to much higher frequencies than the maximum of 5×10-2Hz presented herein. For the case presented herein, however, both the single spectra and the co-spectra again match the Kolmogorov co-spectrum well for the highest frequencies at all altitudes. Therefore, we conclude that the observed “energy plateaus” are not necessarily due to insufficient instrument performance – which, however, also cannot be ruled out categorically. Previous studies showed that surface heterogeneity can lead to perturbations of the expected turbulent state e.g.,. As a consequence, the imprint of surface heterogeneity on vertical fluxes is highly dependent on the structure of the surface heterogeneity itself . Therefore, one possible explanation for the observed “energy plateaus” in the spectra could be the imprint of surrounding heterogeneity on vertical fluxes of, especially, latent heat that is advected towards the lidar. The “blending height” concept , describing a gradual, vertical decrease in influence from heterogeneous surfaces due to mixing and increasing eddy diameters, would be contradictory to this assumption. However, as shown by , influences by heterogeneous surfaces can indeed propagate throughout the entire PBL.

Translating the interval borders of the “energy plateaus” in the co-spectra from frequencies into time, the “non-Kolmogorov” range reaches from ≈ 25–33 s for the upper- and lowermost altitude (3–4 ×10-2 Hz) and ≈ 40–66 s (1.5–2.5 ×10-2 Hz) for the plateau at lower frequencies at the upper altitudes. As can be seen from the single spectra within Fig. , those plateaus arise mainly from the spectra of q′ – although the spectra of w′ also show the previously described energy jumps but much less pronounced. Therefore, it can be assumed that there is much less advection of surface heterogeneity in the wind field. In the respective time period, wind data from the DWD site at MOL-RAO at 10 m above ground show a mean horizontal wind velocity of ≈ 3 m s⁻¹ at northerly wind directions from ≈ 340–20° (not shown here). Therefore, corresponding surface heterogeneities, which could potentially cause the non-Kolmogorov behavior, would be of the order of ≈ 75–100 and ≈ 120–200 m. With a rough scale estimation for vertical wind speeds of ≈ 1 m s⁻¹, such an input of surface heterogeneity would be in a horizontal distance of ≈ 1 km (lowest altitude), ≈ 1.5 km (middle altitude), and ≈ 3 km (highest altitude). The naturally non-homogeneous horizontal and vertical wind field leads of course to alterations of this estimation. As the wind speed increases over height, the horizontal extent of surface-induced energy perturbations therefore most probably corresponds to larger horizontal inhomogeneities for higher altitudes. In order to evaluate the influence of the surrounding heterogeneity on the co-spectra, Fig.  shows the surrounding surface conditions at MOL-RAO in Lindenberg. Sentinel-2 L2A satellite mosaic images from 15–25 July 2021, with the least cloud coverage used as the mosaicking order, are used to show the normalized difference moisture index (NDMI, Fig. a) and the RGB highlighting optimized natural colors (Fig. c). NDMI delivers information on the water content in leaves and is therefore taken as a proxy for the evaporative potential. The RGB channel shows both the current state of vegetation and visually an estimation on the prevailing surface albedo. Figure b shows the surface height in the region as taken from an image-based digital surface model (bDOM2022) by the local land surveying office LGB (Landesvermessung und Geobasisinformation Brandenburg) with a spatial resolution of 0.2 m.

As can be seen, especially the NDMI map, which is probably the most relevant one in order to explain the energy plateau in the q spectra, shows a large surface fragmentation in the region where the winds come from. For this measure, which does not provide information on the surface moisture itself, surface heterogeneities on the scale of <50 m to >2 km are indeed apparent. On an even larger scale (not shown by the maps), changing patterns of lakes and urban areas with horizontal extent >3 km are apparent within the wider surrounding area of Lindenberg – potentially introducing non-typical energy contributions at even lower frequencies as well. A direct attribution of a specific surface pattern to the observed energy plateau is not possible as the wind field changes in both speed and direction vertically. In order to better investigate whether surrounding surface heterogeneity really is the causal link to the observed energy roll-offs in the turbulence spectra, more measurements at the same location have to be taken and investigated. If comparable behavior could be seen more often and, ideally and hypothetically, by different sensors, the analysis of humidity turbulence spectra could offer a new approach to better understanding PBL humidity transport processes. Nevertheless, keeping in mind that the co-spectra w′q′ can depend on several surface features, it seems plausible that the observed energy plateaus are not caused by white noise but by real atmospheric turbulent transport processes. Therefore, we conclude that the measurement of vertical turbulent fluxes of latent heat with the presented combination of instruments is most probably possible down to at least a frequency of 0.05Hz.

Figure  shows an intercomparison of the median ATMONSYS DIAL profile with a radiosonde ascent. However, the temporal overlap is not given as the radiosonde started at 10:45 UTC and the median was calculated for a time span of ≈ 70 min and at a slightly later point in time. To achieve a more spatiotemporally representative intercomparison, free of any potential diurnal humidity development between the analyzed time intervals, we now show all single lidar profiles and their median for the same restricted time period of a bit more than 11 min. This period starts from the ascent time of the same radiosonde until it reaches an altitude of ≈ 3.5 km (Fig. ).

Within this short and accurate time comparison, the profile-to-profile variance is shown to be roughly of the same magnitude as it was in Fig. . Again, there are altitudes up to 3 km at which the DIAL measurements show significantly lower variability than below. Therefore, we assume that the enhanced variability of humidity at ≈1.2–2 and ≈2.3–2.7 km is real atmospheric variability, which is captured by the DIAL and is not related to a temporal trend over the previously shown time span of more than 1 h. The relative vertical distribution of moisture between the DIAL median and the radiosonde data is very similar. However, despite the temporal overlap, the DIAL median mostly shows lower humidity concentrations compared to the radiosonde. Only a few profiles show humidity values as high as the sonde, whereas there are even altitudes (e.g., ≈ 1.2 km) at which not a single profile reached the humidity values by the radiosonde, not even within the statistical uncertainty of 4 % for the radiosonde measurements themselves. As Fig.  and Fig.  do not show a systematic issue of humidity profiles that are too low, there is no obvious system-dependent explanation for this absolute deviation of humidity concentrations. Keeping in mind the substantial short-time fluctuations that can be seen within the DIAL data, as well as the measurement's low statistical uncertainty, those mismatches could principally be due to real temporal atmospheric variability. As a matter of fact, former studies have shown that humidity intercomparisons can be heavily dependent on both temporal and spatial overlap – even on very small scales e.g.,. For sonde–lidar intercomparisons, such spatiotemporal overlap mismatches cannot be avoided. Therefore, the following subsection will show an extended intercomparison with the inclusion of ARTHUS and RAMSES lidar data during their overlap of operation in close proximity to each other.

Lidar to radiosonde data comparisons, as shown in the previous subsection and e.g.,, are a convenient method to evaluate the lidar data quality. Often, it is the only way to test the lidar data against in situ. However, even if the measurements of radiosonde and lidar show good agreement, a certain degree of uncertainty remains. The spatial drifting of the radiosonde remains a relevant factor, and horizontal homogeneity cannot always be assumed from lidar data showing similar results to the radiosonde. Especially in the convective boundary layer during daytime, turbulent fluctuations cause significant sampling differences between the vertically pointing lidar instruments, with diameters of the laser beams of a few centimeters, and radiosondes, which drift horizontally while moving upwards at only a few meters per second. These instrumental sampling differences naturally cause differences in the measured data. So we cannot expect perfect agreement even if the uncertainties of each of the instruments are zero. Therefore, coinciding intercomparisons between multiple lidars and radiosondes are of great advantage in order to better understand deviations between radiosondes and lidars. At least to our knowledge, such intercomparisons have rarely or never been carried out with high-power boundary layer humidity lidars. Within the FESSTVaL campaign we had the opportunity to make such comparisons. In Fig. , we show an intercomparison between all three humidity lidars (ATMONSYS, RAMSES, ARTHUS) that have been operating in close proximity to each other at Lindenberg and radiosondes from the same location. Besides their proximity (Fig. ), instrumental differences between the three lidars remain. One aspect is the difference in their power aperture products. This product of laser power and telescope area gives an idea of how much signal one can expect from the different lidars based on their optical setup (Table ). Higher-aperture products thereby potentially lead to higher signal levels and better signal quality if the background noise caused by larger telescopes can be reduced in an appropriate manner. However, it has to be acknowledged that the different measurement techniques of DIAL and Raman lead to differences in the magnitude of β(r) (Eq. ) and therefore a different instrumental behavior. Another difference between the instruments is their way of calibration and the calibration data they refer to. Whereas the DIAL data are free of any calibration, the Raman lidars have been calibrated against radiosonde measurements in Lindenberg. The RAMSES measurements use the same calibration parameters for the entire second half of the respective month, therefore referring to a radiosonde from ≈ 2 weeks earlier. The ARTHUS system, on the other hand, uses calibration parameters referring to the 00:00 UTC radiosonde on 18 July 2021. Figure  shows two radiosonde ascents and the median values of all three lidars around the corresponding time of ascent. Note that the temporal resolution of the RAMSES lidar is 4 min, whereas the temporal resolution of the ATMONSYS and ARTHUS is 10 s. Also, the vertical resolutions are different for all three lidars (Sect. ). For the 18:00 UTC radiosonde (starting time 16:45 UTC, Fig. a), the comparison time for all lidars has been shifted to slightly before the start of the radiosonde due to data gaps. Nevertheless, all four systems show good agreement in the lowest 2 km above ground. Besides DIAL values that are too high at the lowest altitudes, both the DIAL and ARTHUS values are in good agreement within their respective statistical uncertainties. The reason for the steep humidity increase in the DIAL data towards the ground might be detector issues, which will be discussed later within this subsection. The RAMSES profile reveals smoother data due to longer integration times and, at the same time, the highest humidity values from ≈ 0.6–1.5 km. Whereas the agreement between the radiosonde data and all three lidars is quite good at ≈ 0.6–1.1 km, there is also an altitude range (≈ 1.3–1.7 km) in which the radiosonde shows substantially lower values than the three lidar systems. At ≈ 1.7 km, a steep gradient in humidity can be observed within both the radiosonde and the lidar data – with some minor differences. ATMONSYS and RAMSES measure the gradient with almost identical steepness. ARTHUS, on the other hand, also shows the gradient but at higher altitudes and consistent with the radiosonde. For the radiosonde, possible explanations for increased humidity measurements towards higher altitudes could be hysteresis effects stemming from a wet balloon surface or spatial mismatch. This, however, does not explain the differences between the ARTHUS data and the data measured by RAMSES and DIAL.

Overall, starting from ≈ 1.8 km, it can be seen that during daylight conditions, ARTHUS measurements show a substantial increase in noise and statistical uncertainties. This behavior can be attributed to the physical constraints of the Raman technique during daylight conditions at this high sampling frequency. Above an altitude of ≈ 2.7 km, ATMONSYS measurements show lower humidity concentrations which are not seen by RAMSES or the radiosonde, indicating the maximum range for the DIAL measurements under the given conditions. Beyond this altitude, only the RAMSES data show realistic humidity values in good agreement with the radiosonde.

The second intercomparison is chosen for the midnight radiosonde ascent (starting time 22:47 UTC, Fig.  b). As already discussed in Sect. , an aerosol layer of different origin and dense clouds was present during that night and also directly at the time of the radiosonde ascent. In order to capture more profiles without any cloud influence, the lidar comparison time has been shifted to a time period almost 40 min later than the radiosonde starting time. Especially during night, the lack of convection generally leads to more continuous humidity structures, justifying this temporal shift. On first sight, very good agreement between RAMSES and the radiosonde can be observed over the entire range of altitude, with measurement differences mostly within the respective statistical uncertainty. Interestingly, both ATMONSYS and ARTHUS see lower humidity concentrations than RAMSES and the radiosonde at lower altitudes, outside the statistical uncertainties. In comparison, the DIAL data show the lowest humidity values, including a small humidity minimum at 1.6 km due to unfiltered wisps of clouds. In contrast to Fig. a, the issue of unrealistically increasing humidity concentrations at the lowest altitudes is not so apparent at this point in time, indicating problems with nonlinear signal behavior mostly during daylight conditions and thin clouds. In the case of optically dense clouds, causing a detector overload, the corresponding data are flagged by the transient digitizer within the ATMONSYS data processing routine. Such clip flags have not been set by the transient digitizer in the corresponding time. However, the PMT detectors in photon-counting mode already show nonlinear behavior before full saturation (deadtime issue). But, also in analog mode, the pre-amplifiers of the transient digitizer can show a nonlinear behavior already at 50 % of the clipping threshold caused by atmospheric fluctuations in single shots (B. Mielke, Licel, priv. comm.). A closer look at the DIAL raw data (which are not shown within this publication) revealed nonlinear-looking structures in some signals. Therefore, we conclude that the false maxima of humidity concentration in this special case as well as the overestimation of humidity at the lowest altitudes within Fig. a are due to signal levels that were not high enough to entirely saturate the detector but already led to signal distortions. However, at least in comparison to the humidity values of the radiosonde and ARTHUS, there is still a more pronounced increase in the ATMONSYS humidity towards the lowest altitudes within Fig. b. Therefore, it seems plausible that this feature is not necessarily caused only by daylight background but could also be partly caused by stray light from the outgoing laser pulse. Apart from this deficiency, all three lidars, and also the radiosonde, prove to be very consistent with each other at altitudes ≈ 2–2.5 km. This good agreement and the fact that measurements below those altitudes were in much better agreement 7 h earlier justify the assumption that those deviations are partly a matter of different temporal averaging, and therefore atmospheric variability, rather than having a systematic nature. This calls for the analysis of a larger intercomparison dataset, which, unfortunately, was not possible to collect at that point in time.

Despite good agreement between the sensors at changing altitudes and times, deviations between the four measurements of ≈ 1–3 gm-3 at all heights, corresponding to relative deviations of ≈ 10 % or more, remain. In the case of the DIAL measurements, statistical uncertainties are shown to be lower – hinting towards atmospheric variability on both small temporal and spatial scales. This, in conclusion, highlights the valuable additional information which can be provided by humidity lidars at high spatiotemporal resolutions. Up to now, only very sparse information on the extent of short-term humidity fluctuations in the middle and upper PBL exist. Future humidity measurements at 10 s resolution and less, such as introduced here for the ATMONSYS DIAL, will therefore deepen our understanding of turbulent exchange processes and the energy budget throughout the PBL.