Evaluation of a new X-band weather radar for operational use in south Sweden.

The performance of a new type of X-band weather radar (WR) for Sweden during a pilot run is studied. Compared to the conventional C-band WRs, the X-band WR covers a smaller area but with a higher spatiotemporal resolution, making it suitable for urban hydrological applications. Rainfall estimations from different elevation angles of the radar (levels) are compared at one-minute and single-event timescales with the observations of several rain gauges at different ranges using hyetographs. In general, the estimations aligned well with observations and the best match appeared for ranges as long as 5-10 km. Seemingly, radar estimations suffered from overshooting of lower lying showers by higher level scans in longer ranges (19-30 km) and from the reflectivity contamination due to moving objects in short ranges (<1 km). Also, the effective range of the radar dropped sharply for the moments when a cloudburst was located over the radar. Although various sources of error could affect the X-band WR rainfall estimates, higher resolution spatiotemporal rainfall monitoring for wider areas will benefit from an integration of data from a network of X-band WRs.


INTRODUCTION
Accurate rainfall data are undoubtedly a fundamental requirement to evaluate water availability and hazards for the environment and society across an area of interest such as an urban watershed. In addition, the impact of climate change with increased extreme rainfall events in many parts of the world calls for the development of more efficient hydrological modelling. Based on the characteristics of urban hydrology such as quick response time and runoff due to a higher percentage of impervious surfaces, it is evident that higher temporal and spatial resolution rainfall data are essential for input to hydrological models to simulate runoff accurately and eventually, for proper design of the drainage system. From previous studies, it is well known that the uncertainty in urban hydrological models is mainly due to the errors in rainfall data (Willems ; Thorndahl et al. ; Schellart et al. ).
Rainfall can either be directly measured fairly accurately at a point on the ground using an instrumented site with rain gauge or be indirectly estimated aloft by the recent technological advancements in the field of remote sensing techniques such as weather radar (WR). Rain gauges that traditionally provide required datasets for hydro-meteorological applications may not well reflect the distribution of areal rainfall depending on the density of the rain gauge network and the complexity of the train (Hiebl & Frei ). Remote sensing of hydrometeors using WR technique, provides a unique wealth of information on the short-term areal precipitation, of use for various hydro-meteorological applications. There are three frequency bands commonly used for rainfall estimation by WRs. Compared to the conventional C-and S-band WRs, which are widely used for weather surveillance, the X-band WR covers a smaller area but with a higher spatiotemporal resolution. As a result, recent studies suggest the use of observations at X-band frequency as an alternative or an addition to S-and C-bands data (Lengfeld et al. , ; Trabal et al. ) to fulfil the requirements of urban drainage system modelling, rainfall-runoff models of rural river systems, hydraulic simulations, detailed information on extreme events, etc.
More complex error characteristics and increase of higher intensity rain measurement uncertainty for radar data as compared to rain gauges traditionally limit the operational applications of radar data in urban hydrology (Einfalt et al. ). Due to the ongoing advancement in radar software, signal, and data processing as well as in data analysis methods and modelling, the number of urban hydrological studies relying on radar has increased immensely during the last decades (Thorndahl et al. ). Especially, dual-polarization radars are now an important tool for quantitative precipitation estimation (QPE) by providing more accurate physical information of hydrometeors as well as enabled methods for rain attenuation detection and rain drop size distribution (DSD) dynamics as compared to the single-polarization radar QPE (Cifelli & Chandrasekar ; Lim et al. ). Along this line, Kumjian () provides a descriptive review of the polarimetric radar variables, while Simpson & Fox () assesses the performance of QPE using single-and dual-polarization radar equations as a function of range for different rainfall regimes (summer and winter). Although, dual-polarization techniques and applications have been introduced to S-and C-band WRs for several decades, higher frequency polarimetric X-band WRs are now becoming popular for the sake of higher resolution QPE applications (Wang & Chandrasekar ; Lim et al. ; Li & Willems ). Given the existence of various error sources that affects radar estimates (e.g. signal attenuation, beam blockage, etc.), studies have employed different approaches to identify error sources (Van de Beek et al. ) and improve the QPEs using different combinations of X-band WR data with data from rain gauges (Wang et al. ) or radars with other frequencies (Lengfeld et al. ). Combining data from different sources requires remapping a so-called precise, mass-conserving methods as described by Sharif & Ogden (). Regardless of the methodological diversities, there is a consensus among the radar community that suitable precipitation data for urban hydrological applications are approximately a spatiotemporal resolution of about 1 km and 1-2 min (Einfalt et al. ; Ochoa-Rodriguez et al. ). A volumetric accuracy of less than three percent and 20 years, or more, of recording without missing data are as well required (Einfalt et al. ; Thorndahl et al. ).
In Sweden, the Swedish Meteorological and Hydrological Institute (SMHI) observes countrywide rainfall using a C-band WR network, with outputs generally at 15 min and 2 km resolution. A product based on these observations (at the same resolution), mainly designed for hydrological applications, is the HIPRAD data set obtained by adjusting QPEs to gridded observations from the national meteorological network (Berg et al. ). As for a potential augmentation for precipitation monitoring in urban hydrology applications, the southern Swedish water utility company, VA SYD, in collaboration with Lund University, has initiated a test of a new compact type dual polarimetric X-band WR for Sweden (South et al. ). The purpose of the test was, apart from expanding knowledge about how to measure and project precipitation data, to obtain an indepth understanding of how an X-band WR can be implemented as part of operation of a water utility. Some important advantages of such an X-band WR over the traditional C-band WR include smaller cost and size, lower power consumption, and higher spatiotemporal resolution.
Presenting an overall performance of the new WR using a pilot test in summer 2018, the paper aims at introducing the capabilities of the WR in QPE and discussing error sources that could affect it. Further, this study aims to investigate the potentials for improving high-resolution precipitation monitoring taking advantage of the polarimetric X-band WR. The study focuses on case study rainfall events with different intensity, rainfall distribution over time, and event duration to evaluate different potential error sources affecting the QPE as related to the rainfall pattern. In addition, rain gauge observations at several ranges (0-30 km) and radar data from the radar scanning in different elevation angles (2-8 ) are used to attribute the appeared errors to the range and elevation of the targeted sampling volume while the use of lowest radar level (0.5 ) is recommended to mitigate errors due to evaporation and wind drift (Simpson & Fox ). Finally, by looking into the short-term variability of local rain and applying a massconserving interpolation method, the study provides a ground to analyze the uncertainty of the radar-gauge comparisons.

Overview of the pilot test and radar characteristics
On 2018/07/03, a new WR device of the type Compact Dual Polarimetric X-band Doppler (FURUNO WR-2100) was installed at the geographic location of 55.67 N and 13.36 E in Dalby, southern Sweden. As a pilot survey, it was operated for 72 days (2018/07/03 14:14 to 2018/09/12 12:21 UTC). Accordingly, one binary data file with a fixed predefined format was automatically written for each scan of radar (i.e. 360 rotation round to azimuth) right into a server with scn file extension (hereinafter, scn file). Four of these files were every minute uploaded to the server each equivalent for a radar scan in a given elevation angle (level), which was 2, 4, 8, or 10 . Every scn file was about 15.2 MB, in total, and the size of stored data was approx. 6.48 TB for the whole operated time period. The temporal resolution for the radar was considered 1 min equal to the radar revisit time, while the spatial resolution was naturally variable by range. A sampling volume of the radar is specified by azimuthal and range/radial resolution; thus, it expands by range according to the radar beam width. For this pilot case, the radial resolution, which is practically governed by the storage and data transmission limitations, was fixed at 50 meter, and the number of range direction data for every scan-line (azimuth angle) was 1,002, thus the radar collected data in maximum 50.1 km (50 × 1,002) of range. As an example, the equivalent rectangle for a radar bin (a radar bin is the projection of a radar sampling volume on the Cartesian plane) in the range of 1 km was 50 × 47 m 2 (0.24 × 10 À2 km 2 ) while it increased to 50 × 471 m 2 (2.4 × 10 À2 km 2 ) in the range of 10 km for the beam width of 2.7 . The total number of sweeps (number of scan-lines) was 887 for a complete scan round to azimuth. Therefore, on average, the radar stored data for a scan-line were every 0.406 degree (¼360/887) of azimuthal change (sweep). In total, each scn file contained data from 888,774 (887 × 1,002) radar bins.
Radar algorithms for precipitation estimation QPE using WR is usually calculated based on reflectivity data, an important and basic parameter that is measured as an average value of the returned power of particles in a sampling volume by the radar. Reflectivity is an indirect measure of the raindrop size (diameter), number, and concentration, represented by the unit of mm 6 m À3 (the sixth power of raindrop diameters per volume of space). Although, the actual DSD and rain type (liquid, ice, or mixed) are unknown quantities to the radar, there are standard formula such as Z ¼ aR b used for determining the relationship between precipitation intensity (R) and the reflectivity factor (Z ) where a and b are parameters. The best known, and still one of the most used ones, is the Marshal-Palmer relationship where a ¼ 200 and b ¼ 8/5 ¼ 1.6. Since the atmosphere is a dynamic target, the reflectivity measurements are based on some assumptions (e.g. even distribution of many drops throughout the sampling volume), which are seldom met in reality. Therefore, in rainfall intensity measurement based on a fixed radar equation, there is a degree of uncertainty that could be variable by location and time according to the present type/status of rainfall. As a result, the QPE are practically presented by applying a bias correction procedure according to the rainfall observations through the terrestrial rain gauge or disdrometer networks. In this pilot test, however, we compared the QPE based on a fixed relationship (described in the following) assuming that a comparable ground was available for the chosen locations in the radar range during the rainfall events and the comparisons could be attributed to the radar performance.
The simplest precipitation estimation method available by the WR in Dalby is based on Equation (1), which is a rewritten form of the Marshal-Palmer equation where dBZ h ¼ 10 Log 10 Z h and subscript h for the reflectivity factor (Z ) indicates the horizontal polarization of the reflectivity. Accordingly, R zh (in mm h À1 ) is the rainfall intensity estimation based on the radar reflectivity data from the horizontal polarization.
No loss in signal intensity (attenuation) between the target and the radar is another assumption for applying the radar reflectivity data for QPE as described above. In reality, radar wavelengths, especially in X-band frequency, are subject to significant attenuation in the atmosphere, and this issue needs to be addressed. Attenuation correction methods established based on dual polarization radar variables can be helpful for this purpose. A polarimetric radar is capable of comparing the amplitude and phase of the received signals at both horizontal and vertical polarization, which could be different for oblate, non-spherical drops. For the Dalby WR, the rainfall attenuation was corrected by a general built-in method to the radar (described in the following) using the radar product K dp , the specific differential phase shift. K dp is defined as the range derivative of Ф dp , which is the differential phase (between two polarizations), along the wave propagation path. Ф dp is measured in radian (or degree) while K dp is in km À1 . The theory behind this attenuation correction method is that K dp is based on phase measurements, not signal intensity, and it is not affected by attenuation (Kumjian ). According to Bringi & Chandrasekar (), a linear relationship between the specific attenuation, A (in dB km À1 ) and K dp (in km À1 ) can present an excellent approximation at C-and X-band frequencies; in a complete form, A h (specific attenuation at horizontal) ¼ α K dp m and A dp (specific differential attenuation between horizontal and vertical) ¼ β K dp n where m and n are constants, typically close to one, and α and β are coefficients that generally increase by frequency. Since Dalby WR applies a 9.4 GHz frequency, the radar correction method uses default coefficients of 0.233 and 0.030. Therefore, the specific attenuations and corrected reflectivity values for every sampling volume i are calculated as: where Δr is the range increment (100 m by default), and Z h_cor and Z dr_cor are corrected reflectivity in the horizontal and corrected differential reflectivity (between horizontal and vertical polarizations), respectively, where dBZ dr ¼ 10 It is noteworthy that the coefficients' values for Equations (2) and (3) are recommended as a result of the temperature-averaged (0-30 C) fits based on scattering simulations using gamma DSDs over a wide frequency range (2.8-19.35 GHz) as presented by Jameson (). Although, A can vary by a factor of 1.5-2.0 in the 0-30 C temperature range, this dependency is weak for higher frequencies (bands >¼ 10 GHz) (Bringi & Chandrasekar ). However, applying accurate coefficients in Equations (2) and (3) still results in an approximate attenuation correction because K dp itself is noisy and insensitive at very small drops (<0.5 mm), while A is possible in accordance with the total content of water at any size in space (Bringi & Chandrasekar ). Non-meteorological echoes are also a cause of noisy K dp . The correlation between the horizontal and vertical polarization signal (ρ hv ) for favorable targets (e.g. rain) generally results in a high ρ hv (>0.95). So, for the polarimetric correlation less than a certain limit (i.e. 0.90) K dp is not calculated. ρ hv values for the Dalby WR are corrected using a built-in method for the signal-tonoise ratio as described in Shusse et al. ().
Upon the calculation of corrected Z values using Equations (4) and (5), Dalby WR calculates precipitation intensity R as a function of both Z h_cor and Z dr_cor (in dB) through Equation (6).
Other possible combinations for precipitation estimation by the WR in Dalby are realized by direct use of K dp either with the corrected differential reflectivity as: R cor ¼ 26:0 × K 0:883 dp × 10 À0:0988×Z dr cor or as an individual variable in the form of: with default values of 19.6, 0.825, and 1.20 for c 1 , c 2 , and c 3 , respectively.
As discussed shortly before, K dp and, to some extent, Z dr are generally noisy for low reflectivity Z h . Therefore, in application of the above three algorithms, especially for Equation (8) when K dp and Z h are smaller than a threshold, rainfall is estimated only using the Z h . The threshold for the WR in Dalby is by default 0.3 km À1 and 30 dB. For such conditions, the attenuation correction parameter Kr in range r is calculated by the radar built-in process as function of R zh , from Equation (1), in-between the radar and targeted sampling volume as: and the corrected rainfall intensity can be presented as: Beam blockage (BB) due to ground clutter is another important source of error in QPE. A complete BB (CBB) in some azimuthal angles is sometimes inevitable at special locations such as rugged mountainous regions but it was not the case for the Dalby WR. More usual form of blockage is partial BB (PBB). False echoes due to PBB can be addressed by applying certain algorithms (e.g. Shakti & Maki ). There is not any procedure for clutter compensation builtin to the WR in Dalby. Therefore, no correction for the WR data was employed in this study. However, the radar data were investigated for the existence of BB during the pilot run.

Evaluation of QPE vs. rain gauge measurements
For a quantitative evaluation, the radar rainfall estimations at different levels were compared with the observations of rain gauges at different ranges at one-minute and single-event time scale. Data from rain gauges, mostly located in the municipalities of Malmö and Lund, were collected from the regional water utility company, VA SYD. Figure 1 shows a map of the spatial distribution of the rain gauges in the 50 km radius coverage of the radar. While the radar estimates instantaneous rainfall intensity (an intensity sample for a minute), the rain gauges accumulate and measure rainfall until the minimum amount of 0.2 mm is reached. Because of this intrinsic difference between the two data sets (gauge and radar), their hyetographs (i.e. graphs of rainfall intensity distribution over time) may not match each other even for an ideal estimation by the radar. Therefore, for visualizing the comparison between radar estimation and gauge observation, cumulative hyetographs are additionally presented. As the first 0.2 mm record of an event for the rain gauge could actually be accumulated from a few minutes before the time of record by the rain gauge, the equivalent radar data for a given event were selected from a few minutes before the first record of the event by the rain gauge. Thus, the beginning of the equivalent radar period was one minute after the first zero value in the time series of radar data in the period before the first 0.2 mm record of the event.

Evaluation of instantaneous complexity of local rain
In addition to the temporal issue discussed earlier, the idea behind the evaluation of the radar QPE based on the radargauge data comparison is that the rainfall at a point (i.e. rain gauge) is an ideal representation of the radar bin that contains it. This is true if the variability of the rainfall intensity within the radar bin is low, which is seldom possible especially for radar bins associated with large ranges. In order to evaluate this uncertainty, we compared the spatial variation of radar estimations from radar bins close to each other. Basically, since the azimuthal change for every sweep of the radar is a few times smaller than the radar beam width, there are obviously overlaps between the radar bins from consecutive scan-lines. Inspired by Sharif & Ogden (), we applied a geometrically precise interpolation method considering data from all radar sampling volumes (alternative bins) that contribute partially or totally within a given bin, by giving each a weight proportion to their spatial (areal, on the plane) contribution. Comparison of the interpolated values with the raw, single-bin data provided a basis to indicate instantaneous complexity of local rainfall.

RESULTS AND DISCUSSION
Evaluation of high intensity rainfall event Table 1 presents characteristics of a case study intense rainfall event observed by six rain gauges and different ranges of the radar (∼1-30 km) during the study period. For instance, the rain gauge at Södra Sandby, at a range of 5.6 km, recorded 24.6 mm rainfall during the 68-min event (from 00:47 to 01:54 UTC þ 2 on 2018/08/10), which is equivalent to a 0.36 mm min À1 average rainfall intensity. It is noted that the period of this event for each rain gauge (start and end time) was selected so that the time interval between two consecutive 0.2 mm recordings for a given rain gauge was not more than 10 min. Figure 2 illustrates the rainfall intensity variations (Figure 2(a)) as well as the cumulative hyetographs (Figure 2(b)) based on the rain gauge observations and the radar estimations for the event on 2018/08/10, described earlier in Table 1. According to both Figure 2   and 2(b), the radar estimations aligned generally well with the gauge observations, suggesting a potential for the radar bias correction against the observations. However, these figures also reveal an interruption of radar data collection, more obvious for the locations of the Arlöv, Turbinen, and Hammars Park rain gauges, from all radar levels between 00:20-01:00, although the rain gauges continued to record rainfall. As can be followed from the graphs in Figure 2(a), this interruption for each station started a few minutes after that the high intensity rainfall passed the rain gauge toward the location of the radar. As a result, the front of the rain (with a high intensity) positioned between the radar and the rain gauge. Thus, the radar signals were attenuated and caused an error in the rainfall estimation for this period. By investigating the areal rainfall maps from the radar, it was evident that the effective range of the radar dropped sharply when a cloudburst was located over the radar. This is a general flaw of the X-band WRs that is suggested to be resolved by a network of X-band radars, assuming that while one radar suffers an interruption, other ones may gather information at different angles. As discussed by South et al. (), the data from the C-band WR network of the SMHI showed to be less affected by the attenuation due to heavy rain, and as a result, could also provide information for the X-band WR monitoring. Figure 2(b) shows that the difference between the estimated rainfall at different levels increased by range. In addition, radar scans at higher levels (level 3 and, especially, level 4) could not properly detect the actual rainfall for ranges of 25 to 30 km where Turbinen and Hammars Park stations are located, respectively. This can be related to the overshooting of lower lying showers relative to the position of the radar sampling volume as it obviously rises by range in proportion to the radar elevation angle. However, it seems that the radar scans at Level 3 and Level 4 resulted in a better estimation of the rainfall as compared to observations at mid-ranges (∼5-10 km) where Södra Sandby and Lund Södra stations are located (Figure 2(b)).

Evaluation of lower intensity rainfall event
To further evaluate rainfall estimation obtained by the X-band WR, another rainfall event observed on 2018/08/13 was studied (Table 2). Compared to the event on the 10th of August (Table 1), the event on the 13 th was associated with a smaller amount of rainfall distributed over a longer period. Therefore, it is expected that the error caused by the signal attenuation due to the heavy rain was limited and radar estimations could be examined for other error sources. This low-intensity rainfall event, contained dry periods of about 30 min for all stations (Figure 3; between 00:50 and 08:00 UTC þ 2 on 2018/08/13). Figure 3 illustrates rainfall intensity variation (Figure 3(a)) and cumulative hyetographs (Figure 3(b)) for the six different locations presented in Table 2. According to Figure 3(b), at the farthest location to the radar (Hammars Park at range 30.1 km), the cumulative hyetographs of the estimated rainfall at level 1 and 2 and displayed more or less the same variation over the entire event, except for the appearance of a relatively high intensive period at about 04:00. The discrepancy for this period is even more obvious at the Turbinen location (Figure 3(b)) where radar estimation at none of the levels was successful. The inability of the radar during this abrupt change of rainfall intensity could be related to the discrete sampling feature associated to the time it takes for the radar beam to revisit a given point in space. According to the cumulative hyetographs for the two rain gauges located at Turbinen and Hammars Park (Figure 3(b)), the radar scanning at level 3 and 4 detected almost no rainfall. Therefore, it is expected that  the overshooting of the lower lying showers by the higher level scans of the radar at long ranges, which was previously discussed for the event on the 10th of August, was also the case for the event on the 13th. Overshooting might also be partially responsible for the underestimation that appeared at the lower levels of the radar (Figure 3(b)). By this assumption, the lower underestimation of rainfall for Hammars Park station compared to the Turbinen station, while it is at a longer range, could be explained by the fact that the observed rainfall at Hammars Park was lower than at Turbinen. If the event for Hammars Park had continued with the same intensity as for Turbinen, larger underestimation could have been present.
On the other hand, neither the overshooting nor the attenuation due to heavy rain could explain the difference between rainfall estimation at different radar levels for the shortest range (0.8 km) where Dalby station is located (Figure 3(b)). Actually, it is difficult to accept that the estimation at the different levels for the Dalby station in Figure 3(b) reflects actual vertical profiles of rainfall due to that the vertical distance between the levels at such a short range (<1 km) is quite small. Instead, this could be related to the reflectivity contamination caused by a moving object such as rotating blades of wind turbines (Mishra & Chandrasekar ), leaves of trees moving by wind, etc. Such an object may also cause a multi-path scattering of the signals before returning to the radar, which cannot be easily filtered out by usual clutter removing for most applications. As a result, more rainfall than is actually present is detected by the radar, especially at lower levels where the chance for visiting an object close to the ground is higher.
The rainfall intensities at the lowest level for the closest station to the radar, i.e. Dalby, are more jagged compared to the same event for the stations located at longer range (Figures 2(a) and 3(a)). This might be due to existence of moving objects. A more pronounced effect of this at the Dalby station is supported by the fact that the radar sampling volume is quite small at very short ranges and any misleading reflectivity from a moving object (e.g. a bird) with a certain size could contribute with higher weight to the rainfall estimation of that sampling volume. Anyway, the highest-level scan of the radar (level 4) provided an accurate estimation of rainfall for this location.
As shown by the cumulative hyetographs in Figure 3(b), the radar estimation at level 1 and 2 for a range of 5 and 10 km, where Södra Sandby and Lund Södra stations are located, adequately matched rain gauge observations. Good performance of the radar could also be observed for the rainfall event on the 10th of August (Figure 2(b)). Thus, quantitative rainfall estimation at mid-range (5-10 km) seems to be less affected by both signal attenuation due to heavy rain and by the false detection related to moving objects. However, the best estimation for the mid-range event on August 13 was presented by level 2 of the radar (Figure 3(b)), while the scan at higher level (3 and 4) presented the best estimation for the event on the 10th. This fact may suggest that the showers related to the event on the 13th were formed at lower elevations. This supports the assumption that the overshooting by even lower level scan of the radar was responsible for the considerably high underestimation appearing the range 19-30 km during this event (Figure 3(b)).

Integration of QPE results
As discussed above, there are several sources of errors influencing the rainfall estimations by the X-band WR. These errors can depend on time and location as well as the characteristics of the areal rainfall present in both time and space. Other important sources of error are related to the raindrop size distribution, ground clutter, false clutter filtering related to the near-zero Doppler velocities, and wetradome attenuation (Van de Beek et al. ). More reliable rainfall estimation can be provided by removing effects of as many of these errors as possible by incorporating a wider range of information from the Doppler data and the dual polarimetric variables in the combination of C-band and X-band weather radar data (Lengfeld et al. ). Moreover, the results show the importance of using an established combination of radar levels for any data adjustment procedure based on different range, intensity, etc. Such a procedure should be capable of a regular update after acquiring new records representing new facets of the variability in the involved processes, which obviously is not a straightforward task.

Uncertainty of estimations
It should be noted that the generally lower accuracy of the radar estimation for larger ranges could be related to the fact that the radar sampling volume expands as the range increases and the assumption of a uniform rainfall for a certain radar bin is less valid. As a result, radar calibration based on rain gauge observations can be biased if the spatial variability of rainfall is so high that a point measurement obtained from a rain gauge is not a good representative of a radar bin containing it.
Comparing the interpolated values with the raw, singlebin radar data were used to indicate instantaneous complexity of local rainfall. Since the average sweep change for the radar was almost 0.4 , while the beam width is 2.7 , six pre and six post scan-lines can contribute to a given bin. Figures 4 and 5 show differences between the interpolated and raw radar data for radar bins positioned at 19 and 30 km ranges. As a result, a difference is present for both ranges, but more significant deviation can be observed in Figure 5, which is related to the longer range as compared to Figure 4. This may be due to that a 0.4 sweep is equivalent to 147 m distance in the 19 km range while it is 209 m in the 30 km range.
The WR in Dalby several times displayed sporadic lowintensity echoes in some specific bins close to the radar location and within a 10 km range during clear sky, without any rain or cloud. These echoes are most likely produced by PBB from tall buildings close to the radar or signal contamination due to moving objects, e.g. moving wind turbine blades or flying birds. However, these error sources seem to be less important in distorting QPEs as compared to other error sources, such as attenuation during heavy rain and overshooting. Figures 2(b) and 3(b) showed the best match between the radar and rain gauge data for the 5-10 km range while radar bins in this range interval included the highest false, non-rainfall echoes. This may be related to the fact that the radar is sensitive to clear-sky conditions. Another reason can be that the intensity of false echoes is generally lower than echoes from areal rainfall filling. Even if the effect of these errors is negligible for individual rainfall events, failure to remove them may result in uncertainty when using correction methods such as mean field bias. As a result, the clutter removing should be applied to the radar QPEs (Shakti & Maki ).

CONCLUSIONS
Various hydro-meteorological applications including rural and urban flood management require accurate short-term areal precipitation data. As a pilot test, a compact new type of ground-based X-band WR was installed for the first time in Sweden and was operated for 72 days. The X-band WR is suitable for urban hydrology applications by providing higher spatiotemporal resolution estimations of rainfall, but for smaller areal coverage, compared to the conventional S-band and C-band WRs.
To evaluate rainfall estimation from the X-band WR, two case study rainfall events (a high-intensive and a lowintensive summer rainfall event) for six rain gauge stations located at different range from the radar were studied. It was shown that the estimation of high-intensity rainfall was subject to attenuation due to heavy rain so that gathering of data was practically interrupted, especially at ranges  longer than 20 km. For the two investigated rainfall events, overshooting of the lower-lying showers by the higher-level scans of radar (i.e. elevation angles 8 and 10 ) caused huge underestimation at ranges as long as 19-30 km. On the other hand, rainfall estimation at short ranges (<1 km), especially by lower-level scans (i.e. elevation angles 2 and 4 ), was found to suffer from reflectivity contamination due to moving objects in the radar vicinity, resulting in overestimation. The results of this study showed that the rainfall estimation by the X-band radar in mid-range (∼5-10 km) was the most accurate as it was less affected by reflectivity contamination, overshooting, and attenuation due to heavy rain.
In conclusion, higher resolution spatiotemporal rainfall monitoring for wider applications will benefit from the integration of data by network of X-band WRs, assuming that deficiencies of individual radars can be overcome by a system of radars. Due to the various sources of error affecting rainfall estimation, however, radar data cleaning is not a straightforward process. It will require detailed studies discriminating between the affecting sources, according to the characteristics of the areal rainfall in time and space. Therefore, more investigations are needed that can combine data of different sources to improve estimation methods. An interesting prospect mentioned above (section 3.3) is to use local X-band data to improve the quality of the national WR-based products, that way producing an added value also outside the X-band domain.