Can liquid cloud microphysical processes be used for vertically pointing cloud radar calibration?
- 1Cooperative Institute for Research in Environmental Sciences (CIRES), University of Colorado Boulder, Boulder, Colorado, USA
- 2NOAA Earth System Research Laboratory (ESRL), Physical Sciences Division, Boulder, Colorado, USA
- 3NOAA Earth System Research Laboratory (ESRL), Chemical Sciences Division, Boulder, Colorado, USA
- 4Brookhaven National Laboratory, Upton, New York, USA
Correspondence: Maximilian Maahn (firstname.lastname@example.org)
Cloud radars are unique instruments for observing cloud processes, but uncertainties in radar calibration have frequently limited data quality. Thus far, no single robust method exists for assessing the calibration of past cloud radar data sets. Here, we investigate whether observations of microphysical processes in liquid clouds such as the transition of cloud droplets to drizzle drops can be used to calibrate cloud radars. Specifically, we study the relationships between the radar reflectivity factor and three variables not affected by absolute radar calibration: the skewness of the radar Doppler spectrum (γ), the radar mean Doppler velocity (W), and the liquid water path (LWP). For each relation, we evaluate the potential for radar calibration. For γ and W, we use box model simulations to determine typical radar reflectivity values for reference points. We apply the new methods to observations at the Atmospheric Radiation Measurement (ARM) sites North Slope of Alaska (NSA) and Oliktok Point (OLI) in 2016 using two 35 GHz Ka-band ARM Zenith Radars (KAZR). For periods with a sufficient number of liquid cloud observations, we find that liquid cloud processes are robust enough for cloud radar calibration, with the LWP-based method performing best. We estimate that, in 2016, the radar reflectivity at NSA was about 1±1 dB too low but stable. For OLI, we identify serious problems with maintaining an accurate calibration including a sudden decrease of 5 to 7 dB in June 2016.
Due to their profiling capabilities, millimeter wavelength cloud radars are one of the most important tools for cloud remote sensing. Their measurements are used for process studies as well as for long-term monitoring of hydrometeor properties. Although maintaining an accurate radar calibration is absolutely crucial to avoid biases and false trends in observational data sets, calibrating cloud radars accurately is a challenging and long-standing problem. In this study, we investigate the potential for using observations of liquid cloud microphysical processes for radar calibration.
Radar calibration is quantified by the “radar calibration constant”. Despite the name constant, the constant can actually change due to the aging of components, temperature fluctuations, or hardware defects. Therefore, we have to not only determine the initial calibration constant of a system but also monitor the calibration constant for changes. For example, waveguide corrosion of the MilliMeter wavelength Cloud Radar (MMCR) of the US Department Of Energy (DOE) Atmospheric Radiation Measurement (ARM) program at the North Slope of Alaska (NSA) site in Utqiaġvik (Barrow), Alaska, caused a 9.8 dB calibration offset in 2008 (Protat et al., 2011). Also, a liquid film on the radome or radar antenna caused by precipitation can temporarily lead to up to 4 dB of additional two-way attenuation (Frech, 2009). From an engineering perspective, radar calibration is complicated by the fact that radar returns span several orders of magnitude in power and – particularly for pulsed radars – the span between the transmitted and received power is even larger.
The community has multiple approaches for calibrating cloud radars but none are applicable to all situations. Most commonly, a budget calibration is done wherein all components are calibrated separately and the individual calibration constants are summed (Chandrasekar et al., 2015). A budget calibration can also be combined with a receiver calibration by observing a reference target emitting microwave radiation. For example, Whiton et al. (1977) proposed pointing a scanning radar into the sun and Küchler et al. (2017) used liquid nitrogen – similar to the standard calibration method of microwave radiometers. Yet, the errors of the individual budget calibrations sum up, and there is a risk of overlooking error sources, e.g., due to an interaction between radar components. Therefore, it is advantageous to calibrate the full radar system end-to-end. Atlas (2002) provided an extensive overview of different end-to-end radar calibration techniques, most of them relying on observing objects with known radar cross sections. These reference targets included corner reflectors and various metallic or metallized spherical objects such as ping pong balls, ball projectiles from air guns, and Christmas ornaments. However, observations of reference targets require dedicated field operations and cannot be used to calibrate past data sets. Also, the observation of a reference target with radar can be challenging for a number of reasons. First, most reference targets do not move, and hence do not cause a Doppler shift; thus, the target's return cannot be distinguished from ground clutter unless the target is positioned far away from the surface. For lifting the target from the surface, past studies proposed using fiberglass poles (Kollias et al., 2016), tethered balloons (Atlas and Mossop, 1960), or unmanned aerial vehicles (Küchler et al., 2017). Second, the exact location of the target with respect to the radar needs to be known for calibration because reference targets are point targets. Instead, atmospheric hydrometeors are volume distributed targets. Third, the antenna properties are not well defined unless the target is in the antenna's far-field, i.e., at least a couple of hundred meters away from the radar. Lastly, receiver saturation must be avoided, which requires the use of an attenuator or a sufficient distance between the calibration target and the radar. Because of these reasons, calibration by reference targets is only feasible for scanning cloud radars but not for vertically pointing cloud radars, which are most commonly used.
Several studies have suggested calibrating radars by comparing their measurements of rainfall with integrated drop size distributions from ground-based disdrometers (Joss et al., 1968; Ulbrich and Lee, 1999; Frech et al., 2017). Tridon et al. (2017) proposed using self-consistency checks of retrievals from simultaneous radar observations at multiple frequencies to identify calibration problems. However, disdrometers and regular liquid precipitation are required for monitoring calibration continuously and the challenge of radome or antenna attenuation during precipitation events needs to be considered, particularly for vertically pointing systems.
If multiple radars are available, it is easier to achieve a relative calibration by cross-calibration. Cross-calibration also works when the radars have different frequencies, as long as the hydrometeors are small enough to assume Rayleigh scattering and differential attenuation is accounted for (Hogan et al., 2000; Kneifel et al., 2015; Ewald et al., 2019). If the radars are not collocated, the cross-calibration can also be done statistically by comparing long-term data sets. But such comparisons can be biased by different radar sensitivities and it is important to degrade both radars to the same sensitivity. Protat et al. (2011) compared observations statistically from the CloudSat satellite W-band radar with ground-based observations for relative calibration. Because CloudSat's calibration is well established (Tanelli et al., 2008), Protat et al. (2011) and Louf et al. (2019) proposed using CloudSat as a reference for absolute calibration of ground-based radars. However, long time series of at least several months are required (Kollias et al., 2019) and the method cannot be used to monitor radar calibration at higher temporal resolutions. Merker et al. (2015) proposed another method for absolute radar calibration of radars by intercomparisons, but their method requires a very specific setup with three small radars.
We can also avoid the problem of absolute radar calibration by using variables not affected by absolute calibration, such as the higher moments of the radar Doppler spectrum (Maahn et al., 2015), attenuation (Matrosov, 2005) and some polarimetric variables such as depolarization ratio (Matrosov et al., 2017), differential reflectivity, and differential phase shift (Oue et al., 2018). Yet, excluding variables reduces the information content of the observations significantly (Maahn and Löhnert, 2017) depending on the application.
In summary, no method for obtaining an absolute calibration is available that works in all situations. Either dedicated field campaigns or in situ observations of drop size distributions are required. Budget calibrations are not end-to-end, and relative calibrations require trusting the calibration of a reference radar. To close this gap, we investigate whether liquid cloud microphysical processes can be used for radar calibration. Luke and Kollias (2016) proposed using the unique relationship between the equivalent radar reflectivity factor (here referred to as reflectivity or Ze, in dBz, Smith, 2010) and the skewness of the radar Doppler spectrum (γ, unitless) during drizzle onset – commonly defined as drops exceeding the critical diameter for starting autoconversion (20 to 40 µm) – for calibration. Several studies have suggested that γ is helpful for studying drizzle formation (Kollias et al., 2011a, b; Luke and Kollias, 2013; Acquistapace et al., 2019). Further, Luke and Kollias (2016) suggested that the relationship between the liquid water path (LWP, in kg m−2) and the maximum reflectivity in the column max(Ze) contains information that can be used for radar calibration. LWP and max(Ze) are correlated because larger LWP values permit drops to grow larger by condensation and enhance the probability of drizzle formation leading to higher Ze values (see Fig. 1 of Acquistapace et al., 2019). In this study, we evaluate whether the Ze–γ and LWP–max(Ze) relationships can be used for calibrating vertically pointing cloud radars. In addition to these two relationships proposed by Luke and Kollias (2016), we also investigate the relationship between Ze and the mean vertical Doppler velocity (W, in m s−1) because W has been successfully used for drizzle detection (e.g., Shupe, 2007) due to the larger fall velocity of drizzle drops.
We run box model simulations of drizzle onset to develop the details of the method, characterize its uncertainties, and apply it to radar observations of the North Slope of Alaska (NSA) and Oliktok Point (OLI) ARM sites from 2016. The instruments, data sets, box model, and radar simulator used in this study are detailed in Sect. 2. The calibration methods used in this study are presented in Sect. 3. Besides the three new methods based on liquid cloud microphysical processes, we use a reference method to calibrate the two cloud radars relative to one another. For this, we modify the relative calibration method that Protat et al. (2011) proposed for calibrating ground-based cloud radars with CloudSat. In Sect. 4, we apply the various calibration methods to data from NSA and OLI and assess the temporal evolution of the calibration quality at both sites. Finally, concluding remarks are given in Sect. 5.
In this study, we use ground-based remote sensing observations from two observatories operated by the DOE ARM program located in northern Alaska: Utqiaġvik (ARM's North Slope of Alaska, NSA site, formerly known as Barrow, 71.323∘ N, 156.616∘ W) and Oliktok Point (OLI, 70.495∘ N, 149.886∘ W). While the former was established in 1996, the latter did not become fully operational until late 2015. Both sites are located on the coast of the Beaufort Sea and lie only 250 km apart. The synoptic-scale forcing is very similar, resulting in high correlations between both sites for sea level pressure and near-surface air temperature, humidity, and wind (Maahn et al., 2017).
2.2 Instruments and observations
Both sites are equipped with a 35 GHz Ka-band ARM Zenith Radar (KAZR). While the radar at NSA is a first-generation KAZR, the one at OLI is a second-generation KAZR2 with improved sensitivity (Table 1). The spectral resolution of the OLI KAZR2 was increased from 256 to 512 Doppler spectral bins on 16 June 2016. For the radar moments Ze, γ, and W, we use the radar product presented in Williams et al. (2018), which, unlike the standard ARM general mode (GE) moment products, includes advanced clutter removal and higher moments such as γ (Williams, 2018). Because turbulence can mask microphysical signals in γ, observations with high temporal resolution are usually required for minimizing broadening effects of the Doppler spectrum (Acquistapace et al., 2017). Instead, Williams et al. (2018) use a shift-then-average method to reduce the impact of turbulence on the radar moments, allowing the use of coarser temporal resolution (15 s). For temperature and humidity profiles, we use the standard ARM interpolated radiosonde product (ARM user facility, 1999) based on three (two) daily launches at NSA (OLI). Further, both sites are equipped with ceilometers for cloud base estimation (Vaisala CL31, ARM user facility, 1996) and microwave radiometers (MWRs) to retrieve LWP and integrated water vapor (IWV) using the MicroWave Radiometer RETrieval (MWRRET, Turner et al., 2007) and the Monochromatic Radiative Transfer Model (MonoRTM; Clough et al., 2005). To minimize MWR retrieval biases, we applied monthly offset corrections to the observed brightness temperatures using MonoRTM to forward model clear-sky radiosonde observations. At NSA, we estimate LWP from a combination of the 90 GHz channel of an RPG-150-90 radiometer (ARM user facility, 2006, the 150 GHZ channel was not operational in 2016) and the 23.8 and 31.4 GHz channels of a Radiometrics WVR-1100 radiometer (ARM user facility, 1993). At OLI we retrieve LWP from a three-channel (23.834, 30, and 89 GHz) Radiometrics PR2289 radiometer (ARM user facility, 2011). For identifying cloud phase, we use the phase classification by Shupe (2007), which depends on a combination of KAZR, MWR, radiosondes, and micropulse lidar (MPL, ARM user facility, 1990) measurements.
The site at OLI was also equipped with a Ka-band Scanning ARM Cloud Radar (KaSACR) from March 2016 to September 2017. However, the KaSACR was pointing vertically for only 10 min h−1. Combined with its reduced sensitivity, this leads to too few observations of liquid clouds, and thus we decided not to include KaSACR observations in this study.
Unless stated otherwise, Ze is corrected for gaseous attenuation (Rosenkranz, 1998) using the radiosonde profiles scaled by the MWR's IWV. Two-way integrated gaseous attenuation is typically less than 0.4 dB for the whole vertical column at the Ka-band. Attenuation by liquid water is neglected. W is adjusted to sea level air density following Zawadzki et al. (2005).
We analyze observations of the full year 2016 obtained at both sites. The time period was selected because the KAZR at OLI became fully operational only in fall 2015 and suffered from a malfunction of a phase-lock oscillator resulting in resonance peaks in the Doppler spectrum for most of 2017.
2.3 Box model
To simulate the transition from cloud droplets to drizzle drops in an idealized way, we use a zero-dimensional box model of the droplet collection process (Hoffmann et al., 2017). The box model results will allow us to determine the potential of using drizzle onset for radar calibration. The box model is based on the “superdroplet” approach, in which several hundred computational particles are simulated, each superdroplet representing an ensemble of real, identical droplets. We apply the so-called “all-or-nothing” approach to calculate collections among the superdroplets, which has been shown to accurately represent collision–coalescence in the superdroplet framework (Unterstrasser et al., 2017). The model is initialized using the so-called “singleSIP” method (Unterstrasser et al., 2017). In this method, the underlying droplet size distribution is divided into logarithmically spaced bins. Each bin is represented by one superdroplet, of which the diameter and weighting factor (the number of real droplets represented by that superdroplet) are determined by integrating the droplet size distribution across the bin. Here, we use 500 bins, i.e., 500 superdroplets, to represent the droplet size distribution.
While we also use measured droplet size distributions, we primarily use an idealized lognormal drop size distribution (Feingold and Levin, 1986) to evaluate the sensitivity of our calibration methods by varying the distribution's parameters systematically:
with D the droplet diameter, Ntot the total number of droplets, dg the geometric mean diameter, and σg the geometric standard deviation.
Collision–coalescence is steered by the collection kernel, in which the droplet velocity difference is calculated using terminal velocities by Beard (1976), the collision efficiencies are taken from Hall (1980), coalescence efficiency is assumed as unity, and turbulent enhancement is described as in Ayala et al. (2008) and Wang and Grabowski (2009). Turbulence enhancement of the collision process is controlled by a prescribed energy dissipation rate (see Riechelmann et al., 2012). The simulation time has been restricted to 3 h. Note that no other microphysical processes besides collision–coalescence are considered, and droplets are not allowed to sediment from the box; i.e., the liquid water content (LWC) remains constant (Hoffmann et al., 2017).
2.4 Radar simulator
To convert the drop size distributions (DSDs) of the box model into radar observables, we use the spectral radar simulator of the second-generation Passive and Active Microwave radiative TRAnsfer model (PAMTRA2; as in Maahn and Ori, 2019). Its physical basics are the same as for the first-generation PAMTRA (Maahn et al., 2015; Maahn and Löhnert, 2017), but it is designed in a more modular way. Because the drop size in the box model does not exceed 1∕10th of the radar wavelength (8.6 mm) for Ze<10 dBz, we can use the Rayleigh scattering assumption for estimating the radar backscattering cross section of the drops. From the backscattering cross section, the radar Doppler spectrum is estimated using the same fall-velocity–size relationship as in the box model (Beard, 1976). Unlike for Ze and W, broadening by the Doppler spectrum due to turbulence imposing random motion on the droplets needs to be accounted for when estimating γ. For this, we convolve a Gaussian velocity distribution with the idealized radar spectrum. The standard deviation of the Gaussian distribution depends mostly on the degree of turbulence and the contribution of the horizontal wind field to the radial velocity due to the finite radar beamwidth following Shupe et al. (2008). The former is estimated from the energy dissipation rate ϵ, which is varied as discussed below, and a constant horizontal wind of 10 m s−1 is assumed for the latter. Noise is added to the spectrum in correspondence with KAZR2 specifications after June 2016 (Table 1). From the simulated radar Doppler spectrum, we estimate its moments including radar reflectivity Ze, mean Doppler velocity W, and skewness γ following Maahn and Löhnert (2017).
3.1 Skewness and mean Doppler-velocity-based methods
We hypothesize that there are reference points during drizzle onset that have a typical Ze value, which can be constrained by γ or W. To determine these reference points we use and analyze the results of the box-model–radar simulator combination introduced above for simulating drizzle onset. Focusing on the formation of drizzle drops from cloud droplets – referred to as autoconversion – we assume that collision–coalescence is the dominating cloud process during drizzle onset and that other cloud processes can be neglected for this purpose. To assess the model's sensitivity to the microphysical properties of a given cloud, we first vary the initial DSDs (Sect. 3.1.1). Based on these results, we determine the best reference points for radar calibration (Sect. 3.1.2) and discuss how to apply these reference points to observations (Sect. 3.1.3).
3.1.1 Sensitivity study
Here, we show how Ze, γ, and W change with time during drizzle onset and how this is affected by the DSD and turbulence. For a reference run, we chose a set of parameters featuring a slow cloud-to-drizzle transition in agreement with observations of DSDs (Geoffroy et al., 2010) and turbulence (Shupe et al., 2012; Maahn et al., 2015): Ntot=108 m−3 as the initial drop number, σg=1.34 as the standard geometric deviation, m as the geometric mean diameter to describe the initial lognormal distribution (Eq. 1), and m2 s−3 as the turbulent energy dissipation rate. This DSD corresponds to 0.26 g m−3 LWC. The results of the reference run show (orange lines Fig. 1) that Ze increases monotonically with time and that γ reflects the typical competition of cloud droplets and drizzle drops in the radar Doppler spectrum (Kollias et al., 2011b). In the absence of drizzle, only backscattering by cloud droplets contributes to the radar Doppler spectrum. For this stage, the Doppler spectrum has a Gaussian shape (i.e., γ≈0), the variability of droplet fall velocities is small, and turbulence regulates the width of the Doppler spectrum. The critical droplet diameter required to start autoconversion varies between 14 and 80 m depending on the DSD (Liu et al., 2004). As soon as the first drizzle drops are created by autoconversion after 45 min, the γ values become positive (motion towards the radar is defined as positive in this study) because the drizzle drops extend the tail of the Doppler spectrum towards faster, more positive velocities. The maximum γ value of approximately 0.7 is reached at −20.2 dBz (referred to as in the following). When drizzle and cloud droplets contribute approximately equally to Ze, the shape of the spectrum is again more symmetric resulting in γ≈0. This stage is referred to as the cloud drizzle balance point in the following and is reached after another 45 min at −16.5 dBz (referred to as ). Finally, γ becomes negative when the spectrum is dominated by drizzle drops and the remaining cloud droplets extend the tail of the spectrum to the opposite, smaller-droplet side. However, simulated values significantly larger than have to be treated with care because drizzle removal from the cloud by sedimentation is not accounted for by the box model.
To assess the sensitivity of the Ze–γ relationship to microphysics, the initial parameters of the box model were perturbed. We chose the perturbations such that a realistic range is covered but made sure that drizzle is created neither instantly nor too slowly (i.e., no drizzle after 3 h runtime). To evaluate the sensitivity with respect to Ntot, we divided and multiplied Ntot by a factor of 2 (Fig. 1a). When cloud droplets dominate the radar signal, Ntot scales linearly with Ze in linear units and the offset between the model runs is close to 3 dB (corresponding to a factor of 2 as expected from the modification of Ntot). Consequently, the values are approximately 3 dB apart (−23.5, −20.2, and −17.6 dBz). However, autoconversion is more efficient for greater number concentrations (with constant droplet size), thus γ decreases faster as a function of both Ze and time than for the other runs. Due to these compensating effects, values are closer together (−16.5 and −15.4 dBz) than for the maximum of γ. Interestingly, this is not the case if we reduce Ntot by 50 %. Then, the Ze–γ line is shifted to the lower left and is −21.1 dBz and 4.7 dB smaller than for the reference run. For this run, autoconversion is so slow that after 2 h cloud droplets still dominate the spectrum and a reflectivity value of only −15 dBz is reached at the end of the 3 h simulation. For the run with doubled Ntot, the time required until the drizzle dominates the radar Doppler spectrum (i.e., γ<0) is less than 1 h.
For estimating the sensitivity to the width of the size distribution, we perturb σg by ±0.05 (Fig. 1b). If we perturbed the initial DSD width by larger values, the box model would create drizzle too slowly or too quickly for our purposes. While the values for both perturbations are about 2 dB apart, the difference between the values is 2.9 and 0.2 dB for the reduction and increase in σg, respectively. Similar to the doubled Ntot run, autoconversion is more efficient and faster when we increase σg. At the same time, a narrower distribution leads to a larger absolute γ value due to the reduced Doppler spectrum width of the cloud peak. Note that the reference run and the run with increased σg are almost identical for dBz, but the run with reduced σg remains different. This highlights that the presence of larger droplets in the initial spectrum (due to a larger standard deviation) is important for drizzle onset, but the effect saturates when drizzle drops become more numerous. This is similar for the runs where dg has been increased and reduced by ±1 µm (Fig. 1c). changes little when increasing dg (−16.3 dBz) but is reduced for a smaller dg (−19.4 dBz).
To assess the impact of turbulence on drizzle onset, ϵ is perturbed by an order of magnitude (Fig. 1d), in agreement with observations of Arctic clouds (Shupe et al., 2012). Enhanced turbulence leads to turbulent broadening, which reduces the γ magnitude by making the spectrum more symmetrical (Acquistapace et al., 2017). This is particularly visible for low reflectivities, which are dominated by cloud droplets. Turbulence only has a small impact on autoconversion, which can be seen by the slightly faster drizzle formation and the small change in of 0.2 dB. Similar results have been found in other simulations by Hoffmann et al. (2017), in which turbulence did not significantly change the timing of drizzle but rather the amount of cloud water transformed to drizzle.
In reality, a change in Ntot alone is not very realistic because when Ntot is increased, the available liquid is typically distributed on a larger number of smaller sized droplets. In other words, an increase in Ntot for fixed LWC, which would shift the Ze–γ relationship towards larger Ze values, is compensated for by a reduction of dg, which would shift the relationship to the opposite direction. To investigate this, we repeated the Ntot variation for fixed LWC by changing dg accordingly (Fig. 1e). Note that the required change in dg is larger (18.9 and 11.9 µm) than investigated above. As expected, autoconversion is more efficient in the low Ntot|LWC case, but there is apparently an upper threshold for , which increases only by 1 dB. For the high Ntot|LWC case, is reduced strongly from −16.5 to −22.9 dBz. Unlike for the other runs, drizzle formation is very slow and droplets still dominate after 2 h of model run time. Interestingly, the steeper slope of the Ze–γ relationship for the high Ntot|LWC case agrees with the results of Kollias et al. (2011a), who compared maritime and continental (implying higher Ntot values) data sets.
Collision–coalescence, including autoconversion, is a stochastic process so a random number generator is used in the box model for emulation. To make sure the runs are comparable, we previously seeded the random number generator with the same number for the sensitivity study. Here, we use five different seeds for the reference initial DSD to quantify the role of chance. Figure 1f shows that () varies significantly between −16.5 and −18.9 dBz (−20.0 and −21.6 dBz). We conclude from this that the stochastic nature of collision–coalescence reduces the impact of the clouds' initial DSD on the Ze–γ relationship. However, the impact of stochasticity is likely overestimated in the box model because of the limited number of simulated superdroplets (Dziekan and Pawlowska, 2017).
For comparison, we also evaluate the results of the sensitivity study with respect to the Ze–W relationship (Fig. 2). Generally, W increases with increasing drizzle concentration because the drop fall velocity depends strongly on size. On the one hand, W is more prone to biases than γ, e.g., due to inaccurate radar pointing or vertical air motion. While we assume that the latter cancels for longer time series, consistent lifting related to orography could bias W even for long-term data sets. On the other hand, W can be found in radar data sets more frequently than γ and observing W does not require a high temporal resolution (Acquistapace et al., 2017). The dependence on the initial DSD is similar to the Ze–γ relationship. The fact that drizzle develops more efficiently for DSDs with larger Ntot, σg, or dg can be seen from the slower W for the same Ze. This is because W (proportional to the first DSD moment for drizzle) increases more slowly with size than Ze (proportional to the sixth DSD moment). W does not depend on ϵ; therefore, the runs with different ϵ are practically identical. Unlike for , there are apparently no saturation effects limiting the variability of the Ze–W relationship.
3.1.2 Determining reference values
The sensitivity study evaluated only a single microphysical condition, which is not realistic for observations. Therefore, we investigate how stable the relations are for longer data sets with varying microphysical conditions and assess whether the Ze–γ and Ze–W relations have the potential to be used for radar calibration. For this, we used the box model and combined all perturbations of Ntot, σg, dg, and ϵ with each other to cover the parameter space of initial conditions better than for the sensitivity study. Every run was repeated five times with different assigned seeds (i.e., runs). To make sure the full cloud droplet to drizzle transition is included in the data set, only runs without drizzle at model initialization are considered. Also, runs without any drizzle production within 3 h are omitted, which leaves 340 runs.
The results show considerable spread for σ and W (Fig. 3) thus we were able to obtained a median relationship. For this, we bin the data by Ze (bin width 1 dB) and estimate the median values of γ and W for every bin. We smooth the resulting curve using the Savitzky–Golay filter (window length 7, polynomial order 2, Savitzky and Golay, 1964). That is particularly important when applying the method to observations (see below) because it makes the method more robust by increasing the number of observations contributing to a particular point on the curve. Typically, the smoothing changes by less than 1 dB. The resulting median relationships show the typical partly sinusoidally shaped Ze–γ relationship and an increase in W for dBz. We maintain that this median curve is much better suited for calibration because the mean reflectivity would be more sensitive to outliers. It is important to consider the whole Ze–γ relationship instead of determining a mean value for all Ze with γ=0. This is because a certain σ value is not unambiguous and, e.g., a value of γ=0 can also refer to a spectrum consisting only of cloud droplets.
To determine which point of the Ze–γ and Ze–W relations is most stable and best suited for calibration, we estimate the uncertainties of several Ze reference values for γ (maximum, ) and W ( m s−1) for comparison. The choice of the reference values is somewhat arbitrary, but the variability increases strongly outside the investigated range of reference values, which enclose the onset of drizzle. While the determination of max(γ) is straightforward, we estimate the other values by linear interpolation from the neighboring Ze bins. In case a reference point is crossed more than once by the median relationship (e.g., γ of cloud droplets is also close to zero), we choose the crossing associated with a larger Ze value. The use of the Savitzky–Golay filter ensures that adjacent Ze bins impact the reference values, which makes the method more stable. Unlike other Ze calibration studies (e.g., Protat et al., 2011), we do not need to account for radar sensitivity differences because the range of relevant Ze values is strictly limited and well above the sensitivity limit. To assess the stability of the reference values, we use a bootstrapping approach: we select 5 % of the 340 runs randomly 100 times and determine the resulting reference values for each subset. We estimate the final reference values and their uncertainties from the means and standard deviations, respectively (see uncertainty bars in Fig. 3). For γ, the comparison reveals that the variability of Ze is less for reference γ values 0 and −0.1 (± 0.7 and 0.8 dB, Table 2) than for the maximum of γ (±1.6). For W, the variability is generally larger (±0.8 to 1.9 dB).
Even though we chose the initial conditions to be representative of liquid stratiform clouds at high latitudes, it is possible that our choice of initial conditions is biased. Therefore, we repeated the box model experiment with initial conditions based on aircraft in situ observations from the same region as the cloud radars expecting that measured DSDs include all microphysical processes including advection and sedimentation (Fig. 4). For this, we use data of the 5th ARM Airborne Carbon Measurements (ACME-V) aircraft campaign. This campaign took place from June to September 2015 and included cloud probe observations near the North Slope of Alaska (ARM user facility, 2016). Here, we use liquid-only cloud observations in the vicinity of OLI and NSA. We use every 10th profile of the data shown in the Fig. 4a and b of Maahn et al. (2017). Except for the initial DSDs, the setup is identical to the idealized runs introduced above. ϵ was not measured during ACME-V and we apply the same ϵ values as for the sensitivity study to each measured profile (, 10−4, and 10−5 m2 s−3). Every run was repeated five times with different seeds; runs that did not produce drizzle or that included drizzle in the initial DSD were not considered. By doing so, we avoid the impact of potential sampling problems of large, rare drizzle drops by the in situ probes. This leaves 237 runs and the bootstrapping method is used to determine the uncertainties of the reference points. Even though the estimated Ze–γ and Ze–W relationships are more uneven, the general shape between −20 and −10 dBz is very similar to the runs using lognormal DSDs (Table 2).
Figures 3 and 4 contain only box model runs where drizzle eventually formed, but the minimum required Ze for drizzle formation is different for ACME-V data than for the idealized DSDs. While for the idealized DSDs drizzle is formed only when Ze of the initial DSD is at least −27 dBz, drizzle can form at less than −30 dBz for the ACME-V DSDs. We relate this to the non-idealized nature of the initial ACME-V DSDs and the fact that a single, larger cloud droplet can trigger drizzle formation if included in the observed DSD. As a side effect, the drizzle formation at lower Ze values leads to enhanced γ values below −20 dBz. This is most likely only a spin-up effect of the box model, which can be seen from the excellent agreement of the median curves for larger Ze. Note also that at −21 dBz γ is around zero due to competition between runs with higher and lower γ values. But this does not bias our calibration method because we only use the crossing with the largest Ze value.
For both initial DSDs, the variability determined from bootstrapping is minimal for γ=0.0 and W=0.25 m s−1, and we conclude that and are the best reference values for assessing radar calibration. Initializing the simulations with the lognormal and ACME-V DSDs, is and , respectively (Table 2). is estimated as and dBz, respectively. Combining both setups, we obtain and dBz. These values are very close to the value of −17 dBz proposed by Frisch et al. (1995) for distinguishing between drizzle-free and drizzle-containing clouds. Given the idealized setup, we likely underestimated the uncertainties of and and estimate the uncertainty to be at least 3 dB.
While it is true that we found a much larger variability of and for the sensitivity study (Sect. 3.1.1), we are confident that the reference values can still be determined with sufficient accuracy. We base this claim on the assumption that observations with reflectivities corresponding to drizzle onset (Ze −20 to −15 dBz) are likely dominated by clouds that produce drizzle slowly. Clouds with faster drizzle production reach larger reflectivities quickly, likely have a shorter lifetime, and do not contribute to the data set quantitatively. Clouds without or with extremely slow autoconversion rates will likely not reach Ze values larger than −20 dBz before the end of their lifetime. Together with the significant role of random effects, this indicates that the variability of the Ze–γ and Ze–W relationships for larger data sets is lower than estimated in the sensitivity study. By binning the box model results by Ze and determining the median γ and W values, we ensure that slow drizzle generating clouds also dominate our box model estimates because, similar to observations, clouds forming drizzle quickly in the box model also have quickly increasing Ze values. Therefore, these clouds contribute little to observations of reflectivities between −20 and −15 dBz.
This does not mean that and can be used to identify individual profiles with or without drizzle. As shown in the sensitivity study above and in Acquistapace et al. (2019), the variability from profile to profile can be substantial and Ze, γ, and W are not suited to identify the presence of drizzle for individual profiles.
3.1.3 Application to observations
In the following, we determine and from observations at NSA and OLI. Comparison with the theoretical values derived above will allow for evaluating the radars' calibration. We only use clouds identified by the Shupe (2007) method as purely liquid throughout the column. We expect that drizzle onset can be observed best in stratiform clouds due to their lower turbulence, and we limit our analysis to observations with a cloud base lower than 1000 m and cloud thickness less than 1000 m. Even though the Doppler spectrum peak identification algorithm provided by Williams et al. (2018) can identify atmospheric signals with a signal-to-noise ratio (SNR) as small as −15 dB, we only use data with SNR 5 dB because γ is a particularly noisy variable. We use the same method to estimate and from the observations as from the box model (see Appendix A for step-by-step instructions): the liquid cloud observations are binned by Ze (1 dB bin width), the median γ and W values are estimated for each bin, and the resulting curve is smoothed using the Savitzky–Golay filter. Bins with fewer than 100 observations are omitted from the analysis. To obtain and , the median relationships are interpolated linearly.
3.2 Liquid-water-path-based method
Here, we investigate the potential of the relation between LWP and Ze for calibration. While the relationships between γ or W and Ze are shaped by the drizzle onset process, the correlation between LWP and Ze is based on the fact that the likelihood of drizzle formation (i.e., increased Ze values) increases with increasing LWP. But there is also a correlation between LWP and Ze for non-drizzling clouds: cloud droplets can grow larger in deeper clouds with greater LWP values. Frisch et al. (1998) showed that for non-drizzling adiabatic clouds with constant Ntot, LWP is proportional to with for range gate i. While this relationship could be exploited for radar calibration assuming a fixed Ntot value, we were not able to apply the method to our data set successfully. This is likely due to challenges identifying a sufficient number of clouds fulfilling the conditions of the method (i.e., non-drizzling adiabatic clouds with constant Ntot). Instead, we decided to use the maximum Ze value in the column (max(Ze)) to combine the one-dimensional LWP with the two-dimensional, range-resolved Ze measurements. Not relying on the relationship found by Frisch et al. (1998) allows us to not distinguish between non-drizzling and drizzling clouds and use the very same data set as for the γ and W methods. Even though max(Ze) is likely noisier than, e.g., the mean of Ze in the column, max(Ze) has the major advantage that the maximum is less likely impacted by radar sensitivity than the mean because a truncation of a distribution's lower end does not impact its maximum.
3.2.1 Determining a reference relation
Similar to the Ze–γ and Ze–W relationships, and as shown for cloud-integrated reflectivity by Frisch et al. (1998), the LWP–max(Ze) relationship likely also depends on microphysical (e.g., initial Ntot) and dynamical (e.g., turbulence, entrainment and mixing) conditions. With respect to the LWP–max(Ze) relationship, we expect that higher Ntot values lead to reduced Ze values for the same LWP due to suppression of drizzle formation. But unlike the γ- and W-based methods, which focus on a very specific moment during drizzle onset, the LWP method is impacted by the full set of processes of droplet growth and drizzle formation, and is potentially impacted by multiple feedback processes between clouds and their environment. For example, the impact of Ntot on the LWP–max(Ze) relationship would be even larger assuming drizzle suppression due to enhanced Ntot leads to larger LWP values (Albrecht, 1989). However, the question of whether and how feedback processes compensate for a LWP increase is still debated (Stevens and Feingold, 2009). Focusing only on drizzle onset has allowed us to use a simple box model to determine the reference points for the Ze–γ and W relationships but addressing the question of how Ntot (and the related cloud condensation nuclei concentration) changes LWP cannot be answered with a box model and is beyond the scope of this study. Therefore, we decided not to use a model for determining a reference LWP–max(Ze) relationship. Instead, we will use the LWP–max(Ze) relationship of one site as a reference and determine the calibration offset of a second site from this. In other words, the LWP–max(Ze) relationship is used in a relative way unless we can trust the calibration of one of the radars, which would make it an absolute calibration similar to Protat et al. (2011). Similar to the γ- and W-based methods, this assumes that the LWP–max(Ze) relationship is sufficiently stable with respect to changes in microphysical and dynamical conditions. Because we have no box model to identify the LWP value with the lowest variability of max(Ze), we do not use a reference point but a reference relationship and minimize the mean weighted difference between reference and observed relationship.
3.2.2 Application to observations
To apply the LWP method to observations, we use the same liquid-only data set as for the γ- and W-based methods but restrict the observations to cases when the wind direction at cloud level is from the sea. In this way, we reduce the potential impact of local pollution at OLI (Maahn et al., 2017; Creamean et al., 2018), which could alter the LWP–max(Ze) relationship at OLI due to varying Ntot. To determine a LWP–max(Ze) relation for a certain period, we determine mean max(Ze) values for LWP intervals of 0.01 kg m−2 from 0.01 to 0.120 kg m−2 (see Appendix B for step-by-step instructions). For larger LWP values, the number of liquid-only cloud observations drops quickly for the Arctic data set used in this study. When using LWP for radar calibration, it is crucial that the MWR LWP retrievals are offset-corrected, as discussed in Sect. 2.2.
3.3 High-altitude clouds method
To evaluate the new methods independently, we apply the relative calibration method based on high-altitude clouds proposed by Protat et al. (2011). They estimated a relative calibration offset between CloudSat and ground-based cloud radars by comparing mean reflectivity values of high-altitude ice clouds. Here, we adapt this technique to the KAZR data set of NSA and OLI assuming that high-altitude ice cloud statistics are similar for both sites and have the same mean(Ze). This will only provide a relative calibration instead of an absolute one. Comparing mean(Ze) of two radars requires that both are limited to the same sensitivity level; therefore, we limit the OLI sensitivity to that for NSA. However, changing the relative calibration also changes the difference in sensitivity. To account for this, we implemented the iterative procedure proposed by Protat et al. (2011): after the calibration offset is estimated, the sensitivity limit of the radar at NSA is applied to the OLI radar and the relative calibration offset is estimated again. This procedure is repeated until the relative calibration offset converges.
For the comparison, we use all data with – according to radiosondes – an ambient temperature below 0 ∘C above a certain cutoff altitude. To avoid precipitation attenuation, profiles containing Ze values exceeding 10 dBz are discarded. Gaseous attenuation is not accounted for because both sites are expected to be, on average, equally affected. The cutoff altitude has to be high enough to avoid local impacts (e.g., due to pollution Maahn et al., 2017) and biases due to individual frontal systems but low enough to get a sufficient number of observations. For the latter, we have to consider the low height of the Arctic tropopause in winter. To identify the best cutoff height for every three month period, we apply different cutoff altitudes from 3000 to 7000 m to the data set and compare two quality control measures. First, we compare the vertical profiles of mean(Ze) for OLI and NSA before and after relative calibration. Second, we estimate cloud top altitude statistics, which depend strongly on radar sensitivity (Protat et al., 2011), using 500 m bins before and after calibration. We choose the cutoff height whose root-mean-square differences after calibration are best based on both methods.
In the following, we apply the three new calibration methods introduced above to the data sets of NSA (Sect. 4.1, Fig. 5) and OLI (Sect. 4.2, Fig. 6) in 2016. In Sect. 4.3, we will compare the new methods to the high-altitude reference method. We quantify the calibration quality using the calibration offset O defined as follows:
To investigate temporal trends, we group the data monthly and estimate the calibration offset for every month separately. We chose monthly intervals as a compromise between the ability to resolve rapid calibration changes and the need for a sufficient number of liquid cloud observations with varying microphysical properties. The only exception is June 2016 because the radar configuration was changed at OLI on 16 June 2016 (see Table 1), potentially affecting radar calibration. Therefore, the June data set contains only observations from the first half of June and the remaining observations are combined with the July observations. Due to instrument issues in the second half of June, this affects only a few observations.
4.1 Calibration of North Slope of Alaska (NSA) data
For NSA, the monthly Ze–γ relationships follow a sinusoidal-type curve similar to the box model (Fig. 5a), indicating that the phase classification is correctly identifying liquid clouds. This is also supported by the fact that all but one month (April 2016) feature W<0.2 m s−1 for dBz, as expected for liquid clouds without ice (Fig. 5e). Also, most monthly LWP–max(Ze) relationships (Fig. 5i) have a similar shape and align within a couple of dB. For the Ze–γ relationship, most monthly relationships have values between −20 to −17 dBz, but there are a couple of outliers. The monthly Ze–γ relationships that are shifted towards smaller (e.g., December 2016) or larger values (e.g., July 2016) show a similar shift for the Ze–W relationship, indicating that both methods are consistent. The shift in the corresponding LWP–max(Ze) relationships is smaller, but the December and July relationships are still below and above the mean relationship, respectively (Fig. 5i). As discussed above, this could be related not only to a change in radar calibration but also to a change in the dominating microphysical conditions. We estimate the calibration offsets Oγ=0 and OW=0.25 from and , respectively, following the definition in Eq. (2) (Fig. 7a, Table 3). Over the course of the year, Oγ=0 varies between −2.8 and 7.2 dB with a mean of 1.8±2.5 dB. OW=0.25 is between −2.8 and 3.7 dB and has a mean of 0.1±2.0 dB. Even though there are a couple of outliers enhancing the variability, the standard deviations of 2.5 and 2.0 dB of Oγ=0 and OW=0.25, respectively, are consistent with the assumed uncertainty of the methods of at least 3 dB. Comparing Oγ=0 and OW=0.25 reveals that the differences are smallest in summer when the number of observations is largest (corresponding to the number of reflectivity observations in the two bins adjacent to and , Fig. 7c). Because the methods require a sufficient number of drizzling liquid clouds, we expect that the accuracy of the calibration estimate is reduced in winter. The sensitivity study (Sect. 3.1.1) revealed that higher Ntot concentrations for fixed LWC could lead to higher and values. Assuming that Arctic haze – pollution transported to the Arctic from midlatitudes – peaks in spring (Shaw, 1995) and leads to enhanced Ntot values, the increased Oγ=0 and OW=0.25 could be related to a change in Ntot values. Besides this potentially seasonal impact, we cannot identify any trends for NSA. The yearly mean values of 1.8 and 0.1 dB for Oγ=0 and OW=0.25, respectively, indicate a slight positive calibration offset for NSA. Given the uncertainties, this agrees with Kollias et al. (2019), who estimated KAZR's O to be around 3 dB at NSA by using CloudSat observations.
We did not estimate a reference LWP–max(Ze) relationship from a model, but given that the KAZR's calibration at NSA is – according to the γ and W methods – stable and accurate within 2 dB, we can use the LWP–max(Ze) relationship at NSA as a reference. We obtain the reference by taking the mean of the monthly LWP–max(Ze) relationships weighted by the number of observations. Based on the average of the yearly mean Oγ=0 and OW=0.25 values (1.8 and 0.1 dB, respectively), we apply an O value of 1 dB (see Table 4). This allows us to estimate monthly OLWP values from the mean difference between the reference and the corresponding monthly relationship (Fig. 7a, Table 3). We decided to weight the mean difference by the number of observations in each LWP bin because the seasonality of the LWP distribution is high and there are only few observations for higher LWP values in winter. Bins with fewer than 100 observations are skipped. Obviously, this is of limited use for determining an absolute calibration at NSA, but it allows us to compare the variability of OLWP with Oγ=0 and OW=0.25. OLWP varies between −1.6 and 1.9 dB with a standard deviation of 1.1 dB, which is a ∼50 % reduction in comparison to Oγ=0 (2.5 dB) and OW=0.25 (2.0 dB). Because it is highly unlikely that a variation in the real O would compensate for the variability of OLWP but not the variability of Oγ=0 and OW=0.25, we conclude that the LWP–max(Ze) method is the most stable method. The uncertainty of the LWP method is probably half of the two drizzle onset methods (i.e., 1.5 dB).
Another way to compare the accuracy is to compare the Ze-based relationships after correcting using the various calibration methods. Of course, the variability of is zero when applying Oγ=0 (Fig. 5b) and the same applies to W (Fig. 5g) and LWP (Fig. 5l). Also, OW=0.25 leads to a reduction of the variability of relationship and vice versa (Fig. 5c, f). This shows the consistency of both methods but is also related to the fact that the and reference values are close, thus both methods use similar sub-data sets. When applying, e.g., OLWP to the Ze–γ relationship (Fig. 5d), the variability of is not reduced; the inverse operation (applying to LWP–max(Ze) relation) even enhances the variability (Fig. 5j). This indicates that the variability of Oγ=0, OW=0.25 and OLWP is dominated by their intrinsic variability and not by real changes in O. This is another indication that O at NSA was very stable in 2016.
4.2 Calibration of Oliktok Point (OLI) data
For OLI, the relationships align less well than for NSA. Even though most Ze–γ relationships show a quasi-sinusoidal shape, varies between approximately −28 and −12 dBz (Fig. 6a). This is confirmed by the spread of (Fig. 6e) and the LWP–max(Ze) relationships (Fig. 6i), which vary consistently with the Ze–γ relationships. The corresponding Oγ=0, OW=0.25 and OLWP (with the latter estimated using NSA as a reference, Table 4) values vary between −6.9 and 11.0 dB (dotted lines Fig. 7b). There is no reason why the intrinsic variability of the relationships at OLI should be that much higher than at NSA. We conclude that the KAZR at OLI was not properly calibrated, with O likely strongly changing with time. We note that some monthly relationships look different even after applying Oγ=0, OW=0.25 and OLWP (estimated using NSA as a reference, Table 4). Even after applying a calibration correction (Fig. 6b, g, l), the spread of the relationships is larger than for NSA. Some months have a drastically reduced amplitude of the Ze–γ relationship. Further, many months feature W>0.25 m s−1 also for dBz. Lastly, the LWP–max(Ze) relationship is much more curved than the reference relationship in some months. This indicates that the phase classification was not working properly and the data set also contains nonliquid clouds. The phase classification by Shupe (2007) depends on absolute Ze values, e.g., by assuming that – under certain conditions – clouds are mixed-phase for dBz. Consequently, a large positive calibration offset O might result in mixed-phase and ice clouds being falsely classified as liquid clouds because their Ze value is underestimated. Mixed-phase and ice clouds, however, have different and probably more variable Ze–γ, Ze–W, and LWP–max(Ze) relationships. A simple solution would be to constrain the data set to cases with a temperature larger than 0 ∘C, but this is not feasible for Arctic sites because few observations would remain. Instead, we run the classification by Shupe (2007) assuming different calibration offsets Ophaseclass from −6 to +10 dBz (with 2 dB steps) and estimate the relationships for every assumed offset. Note that Ophaseclass impacts only which data points are selected based on the phase classification, and we do not modify the Ze values themselves for obtaining , and the reference LWP–max(Ze) relationship. To obtain a phase classification consistent with the calibration offset, we choose the run with the smallest difference between Ophaseclass and Oγ=0 (or OW=0.25, OLWP). Typically, the smallest difference is less than the 2 dB step size of Ophaseclass. After accounting for Ophaseclass, the magnitudes of the Ze–γ relationships are more similar (Fig. 8b), the W for small Ze values is reduced (Fig. 8g), and the LWP–max(Ze) relationships are less curved (Fig. 8l). With respect to the used number of observations (Fig. 7d), application of Ophaseclass reduces the number of observations by approximately half and makes them more similar to NSA. This indicates that nonliquid clouds have been successfully removed from the data set by accounting for Ophaseclass. Interestingly, the differences between O with and without accounting for Ophaseclass are often smaller than 2 dB (Fig. 7b). This suggests that the methods are more robust than expected and can provide meaningful calibration estimates even if the liquid cloud data sets are contaminated by nonliquid clouds.
When analyzing O values for OLI, the decrease from June to July 2016 stands out. Even though the decrease magnitude varies between −5.6 and −12.5 dB, all methods show this decrease (Fig. 7b, Table 3), and a similar change was reported by Kollias et al. (2019). Based on discussions with the DOE ARM program, the decrease coincides with a change in the KAZR radar configuration (including the calibration constant) on 16 June 2016, though the details of the change are unclear. To find out more about this decrease, we also analyze collocated KaSACR measurements. Even though the KaSACR data set size was not sufficient to apply the new calibration methods, we can compare KaSACR and KAZR Ze measurements directly for the two weeks before and after the step on 16 June 2016. This comparison shows a decrease in the difference between both radars of 7.5 dB (not shown). Because we have no indication for a simultaneous change in the KaSACR's configuration or calibration, we attribute this change to the KAZR confirming the step identified by the liquid cloud methods. The fact that the relative difference between KAZR and KaSACR was almost zero after 16 June 2016 indicates that the change of the KAZR's configuration was made on purpose to make the measurements of both radars match. After June, all liquid cloud methods show a gradual increase in O with time. Except for December 2016, where fewer than 1000 observations are available, the agreement of the various methods is high, which indicates that the gradual trend is likely related to the radar and not to the intrinsic variability of the liquid cloud methods. The gradual trend could indicate hardware problems or a dependence of O on the ambient temperature. The latter could also explain the gradual decrease in O before June 2016. Even though all methods agree about the sign of the trend in spring, O is higher for the γ- and W-based methods than for the LWP method, which is similar to our results for NSA. Therefore, the higher Oγ=0 and OW=0.25 values could be related to Arctic haze, which apparently has a larger impact on and than the LWP–max(Ze) relationship. Based on this and on the reduced variability for NSA, we conclude that OLWP is likely best suited for performing an absolute calibration at Arctic sites.
The median difference between Oγ=0 and OW=0.25 is very similar for OLI and NSA (1.6 and 1.7 dB, respectively), which could indicate a systematic bias between our box-model-based estimations of and . The fact that the mean Oγ=0 value of 1.8 dB for NSA for 2016 is closest to the 3 dB estimate of Kollias et al. (2019) might suggest that is closer to reality than .
4.3 Relative calibration of North Slope of Alaska (NSA) and Oliktok Point (OLI) data
The high-altitude calibration method only allows a relative calibration, which we analyze in Fig. 9 for NSA and OLI. We found that individual events can bias the statistics when applying the high-altitude calibration method to monthly periods; therefore, we applied the methods to intervals of three months with the bin threshold of 1 July 2016 shifted to 16 June 2016. The standard deviation between the different cutoff heights varies between 0.9 and 2.3 dB, which is probably a good estimate for the uncertainty of the high-altitude calibration method. Assuming that the NSA calibration was stable, the relative comparison reveals the decrease in O at OLI on 16 June 2016. When using the best cutoff altitudes, the decrease is estimated to be −5.9 dB, which is – given the different time intervals used for estimating O – in good agreement with the estimate based on the KaSACR–KAZR comparison (−7.5 dB) and the LWP-based method (−5.6 dB).
A comparison of relative calibration with the high-altitude cloud method and the new methods (Sects. 3.1, 3.2) is presented in Fig. 10. This requires deriving a relative calibration from Oγ=0, OW=0.25, and OLWP by subtracting OLI from NSA and averaging the monthly O estimates to 3-monthly values. While the combination of both calibrations generally combines the uncertainties of both estimates, some potential error sources cancel out. This is particularly true for any constant or seasonal biases of estimating , , or the reference LWP–max(Ze) relationship. Given the uncertainties, there is excellent agreement (difference <3 dB) between the high-altitude and liquid cloud methods for April to December 2016 showing the general feasibility of the liquid cloud methods. For the winter period (January–March), the agreement is worse, which is likely related to the less robust statistics due to the reduced number of liquid clouds. Moreover, the data sets used for the high-altitude method and the liquid cloud method are not necessarily obtained at the same time even though they are averaged to the same intervals. This would require the high-altitude ice clouds and the liquid clouds to always occur at the same time, which is not the case. In particular, when O is shifting quickly, such a temporal mismatch can contribute to the observed differences between the methods. Even though the difference between the LWP-based method and the high-altitude clouds method can be up to 2.7 dB in late 2016, the mean difference is lower (0.9 dB) than for the γ-based (2.0 dB) and W-based (1.6 dB) methods. This confirms our previous conclusion that the LWP-based method has the smallest intrinsic variability and likely works best for estimating O in the Arctic.
In this study, we investigate the potential for using the imprint of liquid cloud processes on DSDs for radar calibration. Specifically, we investigate the relationships of radar reflectively Ze to the skewness of the radar Doppler spectrum γ and to the mean Doppler velocity W. Moreover, we use the relationship between the maximum Ze value in the column (max(Ze)) and the liquid water path LWP measured by a microwave radiometer (MWR). These methods close an important gap in our ability to monitor and assess radar calibration.
The fact that we focus only on drizzle onset for the Ze–γ and Ze–W relationships allows us to use a box model (Hoffmann et al., 2017) coupled to the PAMTRA2 radar simulator (Maahn et al., 2015) to determine the dependency of the relationship on the initial DSD and random effects. Depending on initial cloud microphysical conditions and, to a lesser extent, random effects, we determine typical relationships for γ and W as a function of Ze. We find that compensation and saturation effects reduce the variability of the Ze–γ and Ze–W relations, which allows us to identify reference values of γ and W with minimal variability during drizzle onset. For γ, we find that Ze variability is smallest for dBz when cloud droplets and drizzle contribute to reflectivity equally, i.e., γ=0. For W, we identify the smallest variability for W=0.25 m s−1 and dBz. Because we cannot quantify feedback effects of clouds and their environment on the LWP–max(Ze) relationship with a box model, we do not use a model to obtain a reference relationship. Instead, we use the approach for relative calibration between two radars.
Applying the methods to radar observations of low-level Arctic liquid clouds at the ARM North Slope of Alaska (NSA) and Oliktok Point (OLI) sites, we identify median Ze–γ, Ze–W, and LWP–max(Ze) relationships. We applied the methods to monthly intervals to identify rapid changes but obtain a sufficient number of liquid cloud observations (at least 1000 data points for a 15 s temporal resolution). For NSA, the observed relationships are in general agreement with the box model simulations and we successfully identify the reference Ze values for γ=0 (3 dBz) and W=0.25 (3 dBz). We use the difference between measured and modeled Ze reference values for assessing the calibration offset O on a monthly basis. Considering the 3 dB uncertainties of and , the calibration at NSA is relatively stable and O is on average around 1 dB (Fig. 7a). The good calibration of the NSA KAZR motivated us to use the LWP–max(Ze) relationship at NSA as a reference for absolute calibration. The variability of the estimated OLWP is smaller than for Oγ=0 and OW=0.25, indicating that the LWP-based method has an uncertainty of about 1.5 dB and is less impacted by microphysical and dynamical conditions. The difference between the methods is largest for the winter months (Fig. 7a), indicating that the lower number of liquid clouds might limit the quality of the O estimation. Also, the phase classification algorithm employed might struggle in winter to remove all mixed-phase clouds from the data set as required.
For OLI, we identify serious problems with maintaining an accurate radar calibration. Most remarkably, we find that O decreased 5 to 7 dB in June 2016 (Fig. 7b), which was likely related to a change in radar configuration even though the details cannot be reconstructed. Further, we identify a slowly decreasing and increasing trend of O in spring and fall, respectively, of 2016. Similar to NSA, the agreement between the liquid-cloud-based methods is reduced during winter, indicating that a sufficient number of liquid cloud samples is required for the method to work properly. Despite this, the Ze–γ, Ze–W, and LWP–max(Ze) relationships for OLI are consistent after application of a calibration correction (Fig. 6b, g, l). This indicates the ability of the methods to correct also for larger O values as long as the calibration offset is considered during the phase classification (Shupe, 2007) for identifying liquid clouds. The LWP-based method matches the high-altitude cloud reference method best. Considering the error margins, our results are in excellent agreement with Kollias et al. (2019). By applying the CloudSat method by Protat et al. (2011), they found a similar drop for OLI and a 3 dB offset for NSA.
In summary, we find that liquid cloud microphysical processes can be used for radar calibration in the Arctic. The Ze–γ, Ze–W, and LWP–max(Ze) relationships contain valuable information that can be used to determine the cloud radar calibration offset O. Due to the effect of turbulence on radar observations, the γ-based method likely works best for stratiform clouds, which are typically not that turbulent. In comparison to other calibration methods for cloud radars, the new methods have several advantages. Most importantly, no dedicated field campaigns are required and the methods can be easily applied to past data sets. In comparison to the method by Protat et al. (2011), the liquid cloud microphysical processes methods can be applied to shorter time intervals, which better enables the detection of sudden changes. Also, our methods do not depend on CloudSat, which is likely close to the end of its lifetime. Further, the method can be – with limited accuracy in winter – applied to year-round observations even at high latitudes because liquid clouds occur throughout the year. The γ- and W-based methods require supporting instrumentation (microwave radiometer, lidar, radiosonde observations) only for the identification of liquid clouds. If the presence of ice and mixed-phase clouds can be ruled out by other means (e.g., at subtropical or tropical sites), application of the method is possible without any additional instrumentation. The LWP-based method requires a collocated MWR that has to be calibrated carefully using an offset correction during clear-sky periods. While we found the LWP-based method to work best, the question of whether or is the second-best method for calibration is still open. The box model indicates a larger stability for , but the variability of observed is lower at NSA. Assuming the NSA KAZR calibration was stable, this would indicate that is slightly better suited. Yet, is more easily affected by biases, e.g., due to persistent vertical air motions related to orography. These biases could be an explanation for the small 1.6 to 1.7 dB offset between the - and -based calibration estimates. Instead, γ is less affected by biases, but the observations are noisier, require a high temporal resolution, and most standard radar products do not include γ. Likely, it is best to apply all three methods and use the agreement between the methods as an indicator for the quality of the calibration offset estimate. With respect to the calibration offset O for OLI and NSA in 2016, we recommend using the results of the LWP–max(Ze) method for OLI (Fig. 7b, Table 3) and using an offset of +1 dB for NSA.
Further research is needed to reduce the uncertainty of the methods and to assess the dependence of the reference Ze values on climatological and environmental conditions like the availability of cloud condensation nuclei. The reference Ze values and relationships need to be carefully reevaluated when applying the method to radar observations from other regions. This also applies to the LWP–max(Ze) relationship where we used the relationship obtained at NSA as a reference. However, it is not clear whether this relationship is applicable to other sites or whether it is valid only at the North Slope of Alaska. Sites with a radar with stable calibration offsets could be used to assess the seasonality of the used reference relationships over multiple years. Further, an extension of the method to mixed-phase and ice clouds would be desirable, but the greater variability of ice particles shapes, fall velocities, and radar backscattering cross sections makes this even more challenging than for liquid clouds. Even though the method has been developed for Ka-band cloud radars, it should be generally applicable to zenith pointing radars using other frequencies. For W-band radars, we expect that the Rayleigh approximation is also mostly valid because – according to the box model – drizzle drops are small enough to assume Rayleigh scattering for Ze values smaller than −13 dBz. However, one has to correct for attenuation by atmospheric gases and liquid water, which are stronger at W-band.
All ARM data products used in the current study are available at the ARM archive: https://doi.org/10.5439/1027736 (ARM user facility, 1990), https://doi.org/10.5439/1046211 (ARM user facility, 1993), https://doi.org/10.5439/1181954 (ARM user facility, 1996), https://doi.org/10.5439/1095316 (ARM user facility, 1999), https://doi.org/10.5439/1025250 (ARM user facility, 2006), https://doi.org/10.5439/1025248 (ARM user facility, 2011), and https://doi.org/10.5439/1346549 (ARM user facility, 2016). Please refer to the references for the data stream names and DOIs. The PAMTRA2 model is available at https://doi.org/10.5281/zenodo.2552448 (Maahn and Ori, 2019).
To apply the γ and W methods (Sect. 3.1) to a different data set, apply the following steps:
Prepare monthly data sets of radar, ceilometer, and MWR observations.
Correct Ze for gaseous attenuation and adjust W to sea level air density.
Remove data points with SNR dB, below cloud base, and corresponding to clouds with cloud base >1000 m or cloud thickness >1000 m.
Bin γ and W data using Ze (1 dB spacing) and determine median γ and W values for each Ze bin.
Interpolate reference values and by interpolating relations from adjacent Ze bins. Make sure adjacent bins include at least 1000 observations.
Determine Oγ=0 and OW=0.25 from difference of and to reference values and ,dBz, respectively1.
Limit data to marine winds using radiosondes (Only for this study).
Estimate max(Ze) for each vertical profile.
Make sure monthly data sets include at least 1000 observations.
Bin max(Ze) using LWP (0.01 kg m−2 spacing) and determine mean max(Ze) for each bin with at least 100 data points.
Minimize the difference of the LWP–max(Ze) relation with the reference relation (In this study, Table 4) to estimate OLWP.
MM developed the methodology, ran the model, analyzed the data, and drafted the manuscript. FH developed and adapted the model. MS provided the phase classification. All authors contributed to the methodology, the interpretation of the results, and the editing of the paper.
The authors declare that they have no conflict of interest.
We thank the technicians of the ARM program for operating the instruments in Alaska, Davide Ori (University of Cologne) for supporting us with the PAMTRA2 development, and Dave Turner (NOAA) for providing MWRRET. We acknowledge valuable discussions with Tim Lyons (CU Boulder) and Joseph C. Hardin (PNNL) and thank Graham Feingold (NOAA) for reviewing the manuscript prior to submission. This work was supported by the US Department of Energy (DOE) Atmospheric Systems Research (ASR) program (DE-SC0013306, DE-SC00112704) and the NOAA Physical Sciences Division (PSD). This research was performed while Fabian Hoffmann held a visiting fellowship of the Cooperative Institute for Research in Environmental Sciences (CIRES) at the University of Colorado Boulder and the NOAA Earth System Research Laboratory. We thank the two anonymous referees for their reviews.
This research has been supported by the U.S. Department of Energy, Biological and Environmental Research (grant nos. DE-SC0013306 and DE-SC00112704), the NOAA Physical Sciences Division (PSD), and the Cooperative Institute for Research in Environmental Sciences (CIRES) at the University of Colorado Boulder (visiting fellowship grant).
This paper was edited by Mark Kulie and reviewed by two anonymous referees.
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For radars with large calibration offsets (>4 dB), the phase classification needs to be estimated for several calibration offsets Ophaseclass (2 dB spacing). The Ophaseclass is chosen that matches the derived Oγ=0 and OW=0.25 best.