Articles | Volume 18, issue 11
https://doi.org/10.5194/amt-18-2481-2025
https://doi.org/10.5194/amt-18-2481-2025
Research article
 | Highlight paper
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12 Jun 2025
Research article | Highlight paper |  | 12 Jun 2025

The potential of observing atmospheric rivers with Global Navigation Satellite System (GNSS) radio occultation

Bahareh Rahimi and Ulrich Foelsche
Abstract

Atmospheric rivers (ARs) are comparatively narrow regions in the atmosphere that are responsible for most of the horizontal transport of water vapor in the extratropics, which are responsible for many extreme precipitation events and flooding at midlatitudes, including Europe and the US. The critical role of ARs in global moisture transport and precipitation dynamics necessitates accurate water vapor measurements for both understanding and forecasting these phenomena. While the integrated water vapor content (IWV) of ARs can be measured well with microwave and infrared sounders, the vertical structure is less well known. In this study, we analyzed whether specific humidity profiles and IWV values from Global Navigation Satellite System Radio Occultation (GNSS-RO) measurements provide additional information for the study of ARs, in particular regarding their vertical structure. The retrieval of water vapor from GNSS-RO data requires background information, which is usually incorporated by the one-dimensional variational method (1D-Var) that combines observations and background in an optimal manner. We compared data from the COSMIC Data Analysis and Archive Center (CDAAC), operated by the University Corporation for Atmospheric Research (UCAR) in Boulder, Colorado, with data from the Wegener Center for Climate and Global Change (WEGC) at the University of Graz, Austria. We found that retrievals from both centers agree very well in the altitude range, where the 1D-Var weights the observations strongly, even if the employed background profiles are very different. This demonstrates that GNSS-RO data indeed provide additional vertically resolved information, which was not already contained in the background or in operational analyses. IWV values from CDAAC and WEGC generally agree very well; however, both tend to underestimate the values obtained by Special Sensor Microwave Imager/Sounder (SSMI/S) data, since GNSS-RO profiles do not always reach the lowermost part of the atmosphere, leading to a systematic bias in the IWV data, which decreases with better penetration characteristics of the GNSS-RO data. The results suggest that it is promising to combine the GNSS-RO data – with very high vertical resolution with SSMI/S data – with high horizontal resolution to get a more compete view of the 3D structure of ARs.

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1 Introduction

The monitoring of global atmospheric water vapor is crucial for accurate weather prediction and understanding the dynamics of water vapor transport (WVT). Latent heat, released during condensation and absorbed when liquid water evaporates, is a primary driver of atmospheric processes. This underscores the essential role of water vapor in thermal energy transmission and the atmospheric hydrologic cycle (e.g., Businger et al., 1996; Emardson et al., 1998). Integrated water vapor (IWV), often expressed as precipitable water (PW), is crucial for environmental models.

Zhu and Newell (1998) proposed that the majority of water vapor transport across midlatitudes takes place through elongated features in the lower troposphere, known as atmospheric rivers (ARs). Generally, ARs are characterized by widths of approximately 1000 km, sometimes appearing narrower in specific scenarios. Their lengths usually extend to about 2000 km but can be longer under certain atmospheric conditions. Ralph et al. (2004) further refined the understanding of ARs, defining them as narrow corridors of water vapor that exceed 2000 km in length, are no wider than 1000 km, and have a PW of  20 mm (corresponding to IWV  20 kg m−2). This precise definition was later employed by Neiman et al. (2008b). Despite covering only about 10 % of the Earth's circumference at specific latitudes, ARs are responsible for more than 90 % of the meridional transport of sensible and latent heat from the (sub)tropics to midlatitudes (Zhu and Newell, 1998; Ralph et al., 2004).

ARs have been associated with extreme weather events, including flooding and heavy precipitation across various regions, causing significant damage (e.g., Ralph et al., 2003, 2006; Stohl et al., 2008). Given the challenge of analyzing and predicting ARs due to the scarcity of traditional meteorological observations over oceans, the optimal utilization of satellite data has been shown to enhance the accuracy of numerical weather prediction models (e.g., Ralph et al., 2004, 2006; Neiman et al., 2008b).

Since the 1990s, the number of observation techniques for measuring IWV has increased, with modern techniques providing high temporal resolution. Global Navigation Satellite System Radio Occultation (GNSS-RO), radiosonde, and microwave radiometer measurements of IWV have shown reasonable agreement (Bouma and Stoew, 2001; Güldner, 2001; Dai et al., 2002). PW derived from the Special Sensor Microwave Imager (SSM/I) is key for monitoring ARs over oceans (Ralph et al., 2004; Neiman et al., 2008b). The Special Sensor Microwave Imager/Sounder (SSMI/S) employed by the Defense Meteorological Satellite Program (DMSP) provides global coverage over the oceans for PW, with uniform sampling and mean errors under 0.5 mm (Xue et al., 2019). However, SSMI/S data are influenced by heavy rain and complicated by the large and highly variable emissions from land, limiting their application to oceanic areas (Elsaesser and Kummerow, 2008; Schluessel and Emery, 1990; Wentz and Spencer, 1998). The potential of GNSS-RO data for atmospheric moisture profiling builds on foundational work demonstrating the use of GPS techniques for retrieving water vapor. Bevis et al. (1992) pioneered the application of GPS for atmospheric studies, highlighting its capability to retrieve water vapor with high accuracy. This work laid the groundwork for subsequent developments in GNSS-RO, which has since evolved to provide vertically resolved profiles of atmospheric variables, making it an invaluable tool for understanding moisture distributions in phenomena such as ARs.

Significant progress has been made in the field of numerical weather prediction (NWP) over recent decades (Bauer et al., 2015; Alley et al., 2019). However, accurately predicting AR intensities and trajectories continues to pose significant challenges. For instance, the ensemble prediction system of the European Centre for Medium-Range Weather Forecasts (ECMWF) shows that, on average, only 75 % of its ensemble members can forecast the AR landfall location within a 250 km radius with a 2 d lead time, which decreases to below 25 % for forecasts extending to 5 d (DeFlorio et al., 2018). A crucial aspect of enhancing AR forecasts involves refining atmospheric state analyses. These analyses are pivotal as they provide the initial conditions for NWP models. Given the atmospheric system's inherent deterministic chaos, any initial inaccuracies can be amplified over time (Lorenz, 1969). This is especially true for global ocean regions, where direct observations are limited (e.g., Ota et al., 2013). The role of accurately observing atmospheric moisture becomes even more critical over these areas, as studies using adjoint models have demonstrated that the precision of short-term precipitation forecasts for ARs making landfall is highly dependent on the initial moisture estimates within and surrounding the ARs (Doyle et al., 2014; Stone et al., 2020; Demirdjian et al., 2020; Reynolds et al., 2019).

The GNSS-RO limb-sounding technique relies on GNSS radio signals that are refracted and delayed by the atmospheric refractivity field during their propagation to a receiver on a low Earth orbit (LEO) satellite. With the satellites' relative movements, the atmosphere is scanned vertically, providing excellent vertical resolution. Observations obtained from this technique are available in nearly all weather conditions, as signals in the L-band microwave range are unaffected by clouds, facilitating a seamless observation record without the need for intercalibration or temporal overlap between different missions (Foelsche et al., 2011a; Angerer et al., 2017).

The vertical resolution of GNSS-RO ranges from approximately 100 m in the lower troposphere to about 1 km in the stratosphere (Kursinski et al., 1997; Gorbunov et al., 2004), with variations identified by Zeng et al. (2019) based on the specific atmospheric layers and latitudes under observation. GNSS-RO thus captures high-vertical-resolution profiles of atmospheric bending angle and refractivity, which correlate directly with air density under dry atmospheric conditions.

For moist conditions in the troposphere, the retrieval requires a priori information. GNSS-RO data have therefore been primarily used for accurate monitoring of atmospheric temperature in the upper troposphere and lower stratosphere (e.g., Steiner et al., 2001; Foelsche et al., 2008).

However, the potential for observing water vapor in the (lower) troposphere is increasingly recognized (e.g., Kursinski et al., 1995; Bouma and Stoew, 2001; Rieckh et al., 2017), and GNSS-RO humidity data have even proven to be valuable under particularly dry conditions (Rieckh et al., 2018) and in the stratosphere – in the special situation after the Hunga Tonga eruption (Randel et al., 2023). GNSS-RO data have already been successfully used to observe ARs (e.g., Neiman at el., 2008a: Murphy and Haase, 2022).

High-vertical-resolution moisture retrievals have been shown to significantly enhance the forecasting of ARs by improving the representation of moisture profiles in NWP models. For instance, Ma et al. (2011) demonstrated that assimilating GNSS-RO data into weather models substantially improves AR landfall predictions. Similarly, Neiman et al. (2008a) and Xie et al. (2008) highlighted the value of GNSS-RO profiles in capturing vertical moisture structures critical for AR forecasting. These findings are further supported by Cucurull and Derber (2008) and Healy and Thépaut (2006), who reported improvements in moisture and temperature analyses through the inclusion of GNSS-RO data. These advancements underscore the potential of GNSS-RO observations to complement traditional horizontal measurements and address gaps in AR moisture structure analyses, particularly in regions with sparse observational data.

Both GNSS-RO and SSMI/S observations offer valuable insights, particularly over the ocean, and complement each other in various ways. The SSMI/S data can observe the IWV content, offering consistent horizontal information regarding the overall moisture content. However, they do not provide any details about the vertical distribution of moisture within the atmosphere. On the other hand, GNSS-RO measurements offer the ability to retrieve vertical profiles of atmospheric variables, such as moisture, with a high vertical resolution of approximately 200 m in the troposphere.

Despite their effectiveness in vertical profiling, GNSS-RO data have a limitation in their horizontal resolution. This limitation means that GNSS-RO data may not accurately capture small-scale horizontal variations in atmospheric moisture. Therefore, in applications where understanding both vertical and horizontal moisture distributions is essential, it might be beneficial to use GNSS-RO and SSMI/S data in tandem.

GNSS-RO data provide high vertical resolution for moisture profiling, offering unique insights into the moisture structure of ARs. This is particularly important for complementing mesoscale models like the Weather Research and Forecasting (WRF) model, which are widely used to simulate ARs, including their interactions with topography and precipitation processes. While mesoscale models provide detailed horizontal resolution, GNSS-RO adds vertically resolved information that is often missing in observational data or passive satellite sensors. This complementary role can enhance the representation of AR moisture distributions, especially in regions where models struggle with resolution or observational gaps.

In particular, GNSS-RO data are valuable for capturing sharp gradients in IWV at the edges of ARs, which are critical for understanding the transition between moist and dry regions. These gradients are often poorly resolved by traditional models and satellite observations, highlighting the unique contribution of GNSS-RO data. Integrating GNSS-RO observations with mesoscale models, especially through data assimilation, offers the potential to improve our understanding of AR dynamics and the processes leading to extreme precipitation and flooding.

In this study, we analyze whether GNSS-RO data provide additional water vapor information within and in the vicinity of ARs, given the fact that a priori information is needed to derive humidity profiles. Therefore, we focused on investigating the impact of background water vapor information on the GNSS-RO-derived humidity profiles. We aim to discern whether the variations in background water vapor datasets can introduce significant discrepancies in the final moisture profiles and, if so, to what extent, thereby shaping our understanding of atmospheric moisture profiles obtained through RO techniques.

This study is organized as follows: Sects. 2 and 3 provide an overview of the data and methodology used in this study. Section 4 discusses the results in detail, and Sect. 5 summarizes the key findings and suggests future research directions.

2 Data

2.1 GNSS-RO and 1D-Var methodology for atmospheric profiling

Since its operational inception in 2001, the GNSS-RO technique has significantly enhanced atmospheric profiling by providing high-resolution data on temperature, water vapor, and pressure. This advancement was built upon the foundational work of the 1995 GPS/MET mission, which pioneered the use of GNSS for atmospheric sounding, albeit with limitations in capturing detailed wet parameters at lower altitudes (Ware et al., 1996; Kursinski et al., 1997; Rocken et al., 1997; Steiner et al., 1999; 2001). Our study employs refined GNSS-RO data that overcome most of these historical limitations.

The GNSS-RO technique, which measures the phase delay of radio waves emitted by GNSS satellites, has become pivotal for capturing accurate vertical atmospheric profiles (e.g., Rieckh et al., 2018). Despite facing challenges in data accuracy at the lowermost altitudes and a resolution of approximately 200 km in the lower troposphere (Healy and Eyre, 2014; Scherllin-Pirscher et al., 2011), technological advancements in signal processing and data inversion have bolstered its reliability and precision, making the GNSS-RO technique a formidable tool in atmospheric research and analysis.

Occultation events, lasting 1–2 min, result in the bending and delay of signals due to atmospheric density gradients. The vertical refractivity profiles are derived using accumulated bending angles and observed phase data involving GNSS and LEO satellite orbits (Melbourne, 1994). The Abel transform allows retrieving atmospheric refractivity profiles from observed bending angles (Kursinski et al., 1997; Hajj et al., 2002). Once refractivity is obtained, atmospheric parameters like density, pressure, temperature, and water vapor pressure are derived using the Smith–Weintraub equation, the hydrostatic equilibrium principle, and the equation of state (Kursinski et al., 1995; Smith and Weintraub, 1953; Aparicio and Laroche, 2011).

In dry conditions, refractivity depends only on air density. “Dry temperature”, derived from GNSS-RO profiles by neglecting the water vapor contribution to refractivity, differs from physical temperature by less than 0.1 K above  15 km in the tropics and above 8 km in high-latitude winters (Foelsche et al., 2008; Danzer et al., 2014).

At lower altitudes, the presence of significant water vapor necessitates the use of additional background data to derive either physical temperature or specific humidity – or both (Kursinski et al., 1997). Two main methods exist for humidity derivation: direct retrieval and one-dimensional variational (1D-Var) retrieval. The direct method, once popular for moist air retrieval algorithms (Kursinski et al., 1995; Ware et al., 1996), uses climatological temperature information to retrieve atmospheric profiles but can introduce uncertainties from assumed background data. In the 1D-Var method, a cost function, J(x), is minimized:

(1) J x = 1 2 x - x b T B - 1 x - x b + 1 2 y 0 - H [ x ] T O - 1 ( y 0 - H [ x ] ) ,

where x is the state vector representing the atmospheric parameter being estimated (e.g., temperature or humidity). xb is the background state. B and O are error covariance matrices related to the background state and observation, respectively. y0 is the observation. H[x] is a forward operator mapping from state x to the observation space.

The use of this method results in an optimally estimated atmospheric state profile, providing a solid foundation for various meteorological applications by taking into account the uncertainties of the observations and of the background.

Different implementations of the 1D-Var method utilize RO observations along with prescribed background data. Specifically, the University Corporation for Atmospheric Research (UCAR) employs bending angle data, while the Wegener Center (WEGC) uses refractivity profiles as input for their retrieval process. These differences highlight the distinct methodologies utilized by each center to optimize their retrieval processes. The Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC) Data Analysis and Archive Center (CDAAC), operated by the University Corporation for Atmospheric Research (UCAR), employs the one-dimensional variational data assimilation (1D-Var) method for RO moist profiles. This 1D-Var method is utilized as there is significant humidity content. The presence of substantial moisture makes it impractical to directly use temperature measurements for retrieving wet parameters. Hence, the 1D-Var approach facilitates the extraction of these parameters in regions with high humidity. The Occultation Processing System (OPS) at WEGC has also implemented a simplified linearized 1D-Var method since 2013, with reliable results reported in several studies (e.g., Li et al., 2020). The accuracy and reliability of methods like those employed by CDAAC and WEGC hinge on the precise estimation of error correlations and the uncertainties in both the observational data and the background data, thereby shaping the quality of the retrieved moist atmospheric profiles (Li et al., 2020).

2.1.1 WEGC profiles

The WEGC provides RO level-2 profiles, which include both moist and dry atmospheric profiles from an altitude of 0.1 to 80 km with a vertical resolution of 0.1 km. For this study, we utilized level-2 moist profiles from WEGC to derive specific humidity profiles and calculate IWV values, specifically employing the latest version of WEGC data from the Occultation Processing System version 5.6 (OPSv5.6). WEGC utilizes spatially interpolated ECMWF forecast fields, 24 or 30 h in advance, as background data at the RO profile locations, referred to henceforth as ECMWF-b (Schwärz et al., 2016). Post-retrieval, a quality flag, using the ECMWF analysis data as a reference (ECMWF-r), is generated to evaluate the temperature and humidity profiles. These reference data do not alter the retrieved profiles but serves as a reference for quality assessment. Additionally, WEGC has developed a linearized version of the 1D-Var method to generate moist profiles (Kirchengast et al., 2010), relying mainly on the RO-retrieved dry temperature, with uncertainties modeled using an empirical error model (Scherllin-Pirscher et al., 2011).

GNSS-RO data provide altitudinal resolved information, but the profiles are not vertical and the tangent point (TP, the point of closest approach of the ray) travels significant horizontal distances during an occultation event (Foelsche et al., 2011b). Within the OPS retrieval framework, the TP is calculated assuming straight line propagation of the GNSS signals, and the mean TP (the “location of the profile”) is defined as the point where the straight line between the LEO and GNSS satellite would hit the Earth's surface, corresponding to an altitude of 10 to 15 km, depending on atmospheric density variations. This mean TP can be computed by just knowing the orbit parameters of the GNSS and LEO satellites, which allows predicting GNSS-RO event locations. It is well suited to describe the profile location for temperature information in the upper troposphere and lower stratosphere, but it does not represent the profile in the lower troposphere very well. This mean TP location is pivotal, since it is used to extract collocated profiles from other datasets, which provide essential background information for the retrieval process and for validating the profiles post-retrieval.

2.1.2 CDAAC profiles

Level-2 profiles from CDAAC can be found and downloaded at the CDAAC website (https://cdaac-www.cosmic.ucar.edu/, last access: 18 May 2025). The “wetPrf” file type encompasses the retrieved temperature, pressure, and water vapor partial pressure profiles, sampled every 0.1 km of altitude from 0.1 up to 40 km. Notably, data from GNSS-RO above 40 km are generally not applicable to compute wet profiles due to the upper atmosphere's extremely dry conditions, where water vapor is typically negligible or absent. For this study, the latest reprocessed version, 2013.2350, was utilized for its enhanced accuracy and data integrity.

The wet profiles retrieved are collocated with various analytical datasets, including ERA-40 Interim reanalysis data (ERA), European Centre for Medium-Range Weather Forecasts (ECMWF) profiles, National Centers for Environmental Prediction (NCEP) operational analysis, and the Global Forecast System (GFS) data. These collocated profiles are accessible at CDAAC within the “eraPrf”, “echPrf”, and “gfsPrf” products. Predominantly, ERA data serve as background for CDAAC's 1D-Var retrieval process. The eraPrf type is matched with the RO profile and serves as the initial guess for moisture determination below 10 km and for comparison in post-processing. Should ECMWF profiles be utilized as the background for RO retrieval, it will be explicitly stated; however, the ERA-Interim dataset is typically the preferred source.

At CDAAC, the occultation point, i.e., the point on the Earth's surface to which the retrieved profiles are assigned, is estimated as the TP of the ray connecting GNSS and LEO for which the excess phase of the L1 signal is equal to 500 m. This, on average, corresponds to 3–4 km of altitude (https://cdaac-www.cosmic.ucar.edu/cdaac/doc/documents/roam05.doc, last access: 18 May 2025). This definition of the occultation point differs considerably from the one employed by WEGC (see Sect. 2.1.2), and it is better suited to represent the profile in the lower troposphere. As a consequence, the background (and reference) profiles at CDAAC and WEGC are extracted at quite different horizontal locations. This complicates a direct comparison of the results; however, it allows for a determination of the impact of the background – in particular in the case of strong horizontal variability, where the background profiles then represent very different atmospheric conditions (see Sect. 4).

2.2 SSMI/S data

SSMI/S observations are indispensable for continuous monitoring of atmospheric and oceanic phenomena such as integrated water vapor, temperature, and wind speed, offering comprehensive global coverage (NESDIS STAR, 2024). The instruments have a swath width of about 1400 km, allowing for extensive surveillance of Earth's surface. They simultaneously measure thermally emitted radiation across 24 channels, from 19 to 183 GHz, in a conical scanning mode. This multifaceted approach enables detailed observations of brightness temperatures at both microwave temperature and water vapor sounding channels, as well as imager channels, from a single scan angle, thus enhancing the analysis of atmospheric parameters including IWV. The observations are primarily performed over oceans where the retrieval algorithms for parameters like IWV are optimized for the marine environment. This focus is due in part to the more uniform and predictable emissivity of ocean surfaces compared to land, where varying emissivity can introduce retrieval challenges and reduce measurement accuracy. Hence, while SSMI/S data encompass the global surface, analyses and forecasts primarily leverage oceanic data for their reliability. For superior data quality, users can turn to the gridded DMSP SSM/I and SSMIS ocean data products from the Remote Sensing Systems (RSS). These products compile oceanic information across various timescales, providing an invaluable tool for those needing to analyze and visualize water vapor content. Enhanced data access is facilitated through Python plotting routines, as detailed in RSS data recipes, which assist in managing, plotting, and interpreting the stored values within these gridded, time-averaged oceanic datasets. This research incorporates data from the SSMI/S F16 and F17 satellites, launched on 18 October 2003 and 4 November 2006, respectively. The all-sky daily RSS ocean product for these satellites is accessible for download at the RSS website (https://www.remss.com/missions/ssmi/, last access: 8 June 2025). The horizontal resolution of SSMI/S data for IWV retrievals is generally between 25 and 50 km, while the vertical resolution is limited due to the nature of passive microwave radiometry, which yields integrated measurements of atmospheric parameters. Consequently, the SSMI/S IWV dataset represents the total water vapor content in the atmospheric column.

3 Methodology

3.1 Selected AR events

In this study, we screened dozens of AR events covered by GNSS-EO data, and we selected six different AR events to analyze and compare the retrieved moist profiles in detail. The selection of these events was based on several criteria. First, we captured the diversity of latitudinal regions in both hemispheres to reflect the influence of background water vapor on the retrieved profiles. Second, the AR events should fall into the period after 2007, when the COSMIC-1 constellation, consisting of six LEO satellites, started to provide dense observations (2007 to 2010) and cover other satellites such as Meteorological Operational (MetOp) satellites A, B, C; the Gravity Recovery and Climate Experiment (GRACE); TerraSAR-X (TSX); and the six satellites of the COSMIC-2 constellation. For each event we defined a rectangular latitude–longitude domain in order to also cover areas outside of the AR with a wide range of IWV values. The study domains of these six AR events are shown in Fig. 1, and detailed information on the study domains, period of events, and the available LEO satellites is shown in Table 1. The designations of the events refer to the area where the effects of the AR where most pronounced.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f01

Figure 1Study domain locations of the six selected AR events.

Table 1Detailed information on six selected AR events for comparison.

Download Print Version | Download XLSX

As an example, Fig. 2 illustrates the Iceland–UK AR event in 2009. During this event, four GNSS-RO satellites, namely COSMIC-1, MetOp-A, TSX, and GRACE, were operational and provided data for our analysis. The AR event spanned 5 d, starting on 10 October 2009 and ending on 14 October 2009. To capture the temporal evolution of the AR event, we created four separate plots, each corresponding to a specific day within the event period, excluding the first day (to save space). The figure showcases the spatial distribution of the IWV values (in kg m−2) obtained from the SSMI/S measurements, providing insights into the moisture content along the AR path. In addition, we have included all available GNSS-RO profiles within the study domain, where the colors of the circles represent different LEO satellites and constellations. While the figure showcases the horizontal moisture distribution derived from the SSMI/S observations, it juxtaposes this with the RO data points. From these RO data points, IWV can also be calculated for their corresponding locations. In Fig. 2, the white regions signify areas where no data are available, and these gaps originate from various sources. Instrument limitations contribute significantly to these data voids, as sensor sensitivity varies, especially under extreme environmental conditions, and resolution discrepancies might neglect small-scale features. Additionally, gaps in the satellite's swath coverage during its orbital pass can result in areas with missing data. Coastal zones are particularly challenging due to the abrupt land–water transition, which complicates the sensor's ability to distinguish signals accurately. The distinct reflection and refraction characteristics of varied surfaces along coastlines further complicate data retrieval processes in these regions. The data processing stage also plays a role, as it often involves rigorous quality control measures that might eliminate data points deemed unreliable or erroneous. Environmental factors, like areas with high IWV values and extreme meteorological conditions, may exceed the sensor's measurement capacity, leading to the absence of data in these sections. Moreover, there are also small spots with no data for reasons that might be transient and are not immediately identifiable, potentially arising from minor satellite function irregularities, data transmission glitches, or data processing errors.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f02

Figure 2Temporal evolution of the AR event over Iceland–UK from 11 to 14 October 2009, as observed by SSMI/S IWV measurements. The figure illustrates the spatial distribution of the IWV values and includes RO data points.

On 11 October 2009, the AR was observed in its initial formation stage, extending toward the western part of Ireland. The structure and alignment of the AR signalled a nascent phase, with moisture beginning to concentrate along its path. The following day, the AR exhibited a significant northward extension, reaching beyond 60° N latitudes. This expansion reflected an intensification of the AR, with moisture transport extending into higher latitudinal regions. On 13 October 2009, the AR made landfall, impacting the east and southeast coasts of Iceland and northern Scotland and Ireland. The moisture content within the AR had reached its peak. The AR's spatial distribution and moisture intensity on that day highlighted the event's maturity. On the last day, the AR had begun to weaken but maintained its position over the previously affected areas. The reduction in moisture content and intensity signalled the AR's dissipation stage, marking the beginning of the event's decline. A noteworthy aspect of this AR event was the transportation of high moisture content to latitudes beyond 60° N, a very uncommon phenomenon – in particular at this time of the year (Parracho et al., 2018). For example, SSMI/S IWV values had been observed to be as high as 38.7 kg m−2 at latitude 60.125° and longitude 12.875° or 36.0 kg m−2 at latitude 62.125° and longitude 12.125°, highlighting the significant moisture content transported during this event.

3.2 Calculation methodology for specific humidity and IWV using RO data

In this study, we evaluated specific humidity profiles and IWV values. Other parameters, such as relative humidity, mixing ratio, and precipitable water vapor, can be directly calculated using the moist air gas constant ratio parameter (Stull, 2017). As these other parameters' characteristics are similar to the two parameters, they are not discussed here.

For the WEGC data, specific humidity profiles are already calculated and available in the dataset. For the CDAAC data, the specific humidity q (g kg−1) needs to be calculated using the retrieved water vapor pressure e (hPa) and air pressure p (also hPa) profiles. Here, e represents the partial pressure exerted by the water vapor in the air. The specific humidity q is then calculated with the constant ε= 0.622, which is the ratio of the molecular mass of water (μwater vapor 18.015 g mol−1) to the molecular mass of dry air (μdry air 28.97 g mol−1) ε=μwatervaporμdryair. This ratio facilitates the conversion from water vapor pressure to specific humidity using the formula

(2) q = ε e p - 1 - ε e .

In this formula, q is the specific humidity, e is the water vapor pressure, and p is the total air pressure.

Second, to calculate the IWV value (kg m−2) of the GNSS-RO profile, the specific humidity of each height from the surface to the maximum retrieved height is integrated; ps is the surface air pressure, and g= 9.81 m s−2 is the mean acceleration of gravity at sea level at 45° latitude.

(3) IWV = - 1 g p s p q d p

By employing this methodology, we can quantitatively assess the specific humidity profiles and IWV values from the WEGC and CDAAC RO data during AR events.

3.3 The q-RAER metric: an overview and formula

The Retrieval to A-priori Error Ratio (RAER) profile is a critical tool employed to assess the reliability of retrieved data, offering insights into the relative influence of observed information and background (a priori) information. The RAER profile is expressed as a percentage and is calculated during the optimal estimation process.

It is calculated using the formula

(4) RAER = σ ret σ bg ,

where σret contains the square root of the diagonal elements of the retrieval error R, calculated as

(5) R = B - 1 + O - 1 - 1 ,

and σbg represents the standard deviation of the background error.

In the context of this study, the q-RAER profiles are provided within the WEGC dataset. Specifically, the q-RAER profile offers a critical evaluation metric for q retrievals, enabling researchers to discern the relative influence and dominance of observed versus background information at various atmospheric layers.

A RAER value of 100 % means that the RO observation uncertainty is extremely high and that the retrieved profile at this altitude is identical to the background profile. At altitudes with RAER > 70 % the retrieved profile is still background-dominated; this is usually the case above approximately 9 km at low latitudes and above 4 km at high latitudes during winter – but also in the lowest few hundred meters, where the RO refractivity profile can be biased due to super-refraction. At altitudes with RAER < 70 % the retrieved profile is observation-dominated and we can expect significant differences from the background profile.

4 Results and discussion

4.1 Overall comparison between the retrieved specific humidity profiles of CDAAC and WEGC with their background profiles

To assess the impact of background water vapor on the specific humidity profiles retrieved from RO data, a comparison is conducted using the complete dataset of occultations during AR events, along with their corresponding background and reference profiles. In this subsection, we have selected four examples to be discussed. These examples were chosen to represent a range of behaviors and patterns observed in the data, and they provide a concise yet comprehensive overview of the key findings. The selected profiles are those located inside or in the vicinity of the AR over the oceanic area. Among these, the first example serves as a general case, showcasing a common pattern observed across various profiles. The remaining three examples are selected to highlight instances where the background profile and the 1D-Var profile exhibit different and intriguing patterns. These examples are not exhaustive but provide insights into the diverse behaviors and characteristics observed in the dataset.

4.1.1 Iceland–UK 2009 AR event

Figure 3a and b illustrate the specific humidity profiles for the Iceland–UK 2009 AR event observed by a satellite of the COSMIC-1 constellation, including CDAAC 1D-Var, WEGC 1D-Var, ERA, GFS, ECMWF-r, and ECMWF-b, as well as the q-RAER profile for the WEGC-retrieved q profile. The distribution of IWV detected by the SSMI/S F17 satellite, along with the location of the RO event, is depicted in Fig. 3c. Figure 3d further displays the RO tangent point trajectories and reference points for both centers, with the lowest 14 km of each center's RO event indicated by a dashed black line and the highest altitude of the RO marked by a black triangle. The highest retrieved altitudes for WEGC and CDAAC were 80 and 40 km, respectively. This delineation of the RO event's lower-tropospheric region is essential because of the significant humidity gradient near the AR. In this example, the RO event is situated within the AR, where the SSMI/S IWV is approximately 30 kg m−2, as shown in Fig. 3c. All six specific humidity profiles generally exhibit similar patterns, despite variations in their IWV values. These IWV values, while slightly different, are in relative proximity to the SSMI/S IWV.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f03

Figure 3(a) Retrieved specific humidity profiles of CDAAC and WEGC with their reference and background profiles for a satellite of the COSMIC-1 constellation during the Iceland–UK AR event on 13 October 2009. All IWV values in panel (a) are in kg m−2. The WEGC specific humidity RAER profile is shown in panel (b). (c) Distribution of the IWV detected by the SSMI/S F17 satellite with the location of the RO events. (d) RO tangent point trajectory paths of WEGC and CDAAC.

The retrieved CDAAC profile displays more fluctuation compared to other profiles. Similar fluctuations in the CDAAC q profile are also observed in other examples. A possible explanation for this behavior could be a lower vertical correlation in the error covariance matrices. Note that the SSMI/S IWV map does not necessarily represent the exact IWV distribution at the time of the GNSS-RO event, since these maps are only available once per day.

4.1.2 UK 2020 AR event

Figure 4a illustrates specific humidity profiles for the 2020 AR event observed by MetOp-A. In this example, the RO event is located in the northern region of the UK 2020 AR event, near its edge.

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Figure 4(a) Retrieved specific humidity profiles of CDAAC and WEGC with their reference and background profiles for the MetOp-A satellite during the UK AR event on 24 February 2020. The WEGC specific humidity RAER profile is shown in panel (b). (c) Map of the IWV detected by the SSMI/S F17 satellite with the location of the RO events. (d) RO tangent point trajectory paths of WEGC and CDAAC.

While the results in Sect. 4.1.1 are typical for profiles in the core region of the AR, we chose this GNSS-RO profile since it nicely illustrates how the humidity retrievals operate when the background profiles are very different – because they have been extracted at different locations due to the different interpretation of the occultation location. Above 7 km, all specific humidity profiles still exhibit a similar pattern. For altitude above  9 km it is not surprising that the WEGC profiles closely follows the ECMWF-b profile, since the RAER values are close to 100 % and the retrieved profiles is therefore heavily background-dominated. However, below  7 km, where the RAER falls below 40 % and the observed data gain a high weight, there are large differences between retrieved and background profiles, in particular below  5 km, where the retrieved profile is way drier than the background profile. For the CDAAC retrieval the situation is different; here the background profile has been extracted in a very dry area (ECH stands for ECMWF profiles with high vertical resolution). For the CDAAC data, we do not have a value similar to RAER, but the large difference between the retrieval and background suggests that there is also a height weighting of the measurements in this altitude range. Interestingly, the WEGC and CDAAC retrievals agree quite well – even though the background data are so different. This increases confidence in the retrieved data and suggests that the GNSS-RO data indeed provide valuable humidity profile information – beyond the background.

Note that both retrieved profiles do not reach the lowest kilometer in this case (WEGC background and reference profiles are only stored in the altitude range, where there is also a retrieved profile), and the computed IWV values therefore underestimate the true values.

4.1.3 California 2019 AR event

Figure 5 illustrates an example of an AR event in California in 2019. The selected RO event in this case is located near the AR event, south of Hawaii (represented on the map as a gray triangle), as shown in Fig. 5c. Between 6 and 2 km, the ECMWF-b profile indicates higher humidity than the ERA5 and WEGC profiles. The WEGC q retrieval profile within this altitude range is significantly drier than its background profile. A moderate difference is observed between the CDAAC- and ERA5-retrieved q profiles in the layer from 4 to 2 km. The WEGC q profile stops at an altitude of 500 m, whereas the CDAAC profile extends to the lowest altitude. Although the CDAAC profile shows less humidity below 5.5 km, the calculated IWV value for CDAAC is slightly higher (WEGC IWV = 18.33 kg m−2 and CDAAC IWV = 20.75 kg m−2) because the WEGC q profile lacks humidity information in the lowest 500 m. Both background profiles have higher IWV differences of approximately 7.67 and 6.99 kg m−2 (ERA5 and ECMWF-b, respectively) compared with their respective retrieval q profiles, since the lowest part of the actual GNSS-RO profile extends into much drier areas than the vertical background profiles (note that the CDAAC algorithm better represents the actual TP trajectory).

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f05

Figure 5(a) Retrieved specific humidity profiles of CDAAC and WEGC with their reference and background profiles for the MetOp-A satellite during the California 2019 AR event. The WEGC specific humidity RAER profile is shown in panel (b). (c) Distribution of the IWV detected by the SSMI/S F17 satellite with the location of the RO events. (d) RO tangent point trajectory paths of WEGC and CDAAC.

The q-RAER profile also indicates that below 6 km, the observation data significantly influence the retrieved q profiles. The WEGC retrieval q profile is drier than its background profile between 5 and 2 km, whereas the CDAAC profile is wetter than its background profile. As in Sect. 4.1.2 it seems that both retrievals try to bring the retrieved profiles into close agreement, even though the background profiles are very different in this altitude range.

Despite methodological differences, there is a remarkable consistency in the final q profiles across the centers. This alignment, while exhibiting some variations, underscores the resilience and adaptability of the retrieval processes across different methodologies. Notably, these variations in the q profiles can be attributed to the differences in background water vapor information used in the 1D-Var methods, as exemplified in Fig. 6. This highlights the nuanced interplay between methodological choices in data retrieval and the influence of background atmospheric conditions.

4.1.4 Southern Africa 2009

Figure 6 depicts the southern Africa 2009 AR event by examining a profile from the COSMIC-1 constellation. The RO event is located on the southern edge of the AR and probes the atmosphere downward, moving toward the outside of the AR. In this example, the ECMWF-b profile (taken closer to the AR) displays significantly higher q values than WEGC between altitudes of 3.8 and 2 km, where the observation data are dominant (q-RAER profile). Moderate differences are also observed below 2 km and above 4.3 km, while between 3.8 and 4.3 km and up to 5.8 km the ECMWF-b profile is drier than the WEGC profile. Between 2 and 3.8 km, the CDAAC profile is also drier than its prior information.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f06

Figure 6(a) Retrieved specific humidity profiles of CDAAC and WEGC with their reference and background profiles for a COSMIC-1 satellite during the southern Africa AR event 2009. The WEGC specific humidity RAER profile is shown in panel (b). (c) Distribution of the IWV detected by the SSMI/S F17 satellite with the location of the RO event. (d) RO tangent point trajectory paths of WEGC and CDAAC.

The CDAAC profile stops at 1 km, while the WEGC profile reaches the lowest 200 m of altitude. Consequently, the IWV value of CDAAC is lower than the others. The IWV value of ECMWF-b is closer to the observed SSMI/S IWV, which is about 17 kg m−2, and the WEGC IWV is 6.25 kg m−2 less than the SSMI/S observation. This pattern is also observed for the CDAAC IWV value, which is about 6.42 kg m−2 drier than its background ERA IWV. Again, we note that the SSMI/S IWV map does not necessarily represent the exact IWV distribution at the time of the GNSS-RO event.

It seems that the dry layer observed by both retrievals between  2 and  3 km may in fact have been even drier. It is better represented by CDAAC, where the background was already quite dry, whereas the WEGC retrieval could not reach such low values, since it was somewhat confined by the background profile, which was much too humid.

When analyzing specific humidity profiles retrieved from CDAAC and WEGC and comparing them to background profiles within AR events, noticeable variations and patterns emerge. The precise location of tangent point trajectories and reference points is crucial, especially when they are situated at the edges of AR events, where the humidity gradient is often significant, since background data are extracted at very different locations with different humidity regimes. This variance in the location of tangent point trajectories between CDAAC and WEGC adds another layer of complexity to interpreting the data. Understanding and accounting for these subtle differences in trajectory locations within a single RO event are essential for a more accurate analysis and interpretation of the humidity profiles during AR events, enhancing the reliability and precision of the findings derived from such data.

4.2 IWV comparison between CDAAC and WEGC

In this subsection, we compare the IWV data retrieved from the two centers, CDAAC and WEGC. RO data were collected from all active GNSS-RO satellites during the investigated AR events within the entire study domain (see Fig. 1 and Table 1), ensuring that we captured a wide range of IWV values retrieved by RO. To maintain consistency in our comparison, we included only data from satellites for which RO retrieval data were available in both the WEGC and CDAAC databases. From the six AR events studied, we have chosen three with the most interesting results for discussion in this paper. This focused approach allows for a clearer, more engaging analysis without overwhelming the reader with too much information.

We specifically calculate the IWV for profiles that reach altitudes of 1 km, 2 km, 500 m, and 200 m in both centers. In other words, we consider only RO profiles from both centers that extend to these specified altitudes for our IWV calculations.

We chose these specific altitudes for two primary reasons. First, lower altitudes tend to have higher concentrations of water vapor, and calculating the IWV at these levels provides a more representative assessment of the water vapor distribution within the atmosphere. Second, not all RO profiles are capable of reaching the lowest altitudes, so categorizing the data into these four different altitudes allowed us to capture a more comprehensive range of RO profiles, ensuring a more robust dataset for our analysis. Subsequently, the IWV values were integrated from these defined altitudes up to the highest retrieved RO profile altitude, facilitating a comprehensive comparison of IWV values across the selected altitudes.

4.2.1 UK 2020 AR event

Analysis of the UK 2020 AR event (see Sect. 4.1.2) reveals that the IWV measurements from the WEGC and CDAAC exhibit slight differences (Fig. 7), incorporating the following points.

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Figure 7Comparison of IWV (kg m−2) values derived from GNSS-RO profiles reaching specified minimum altitudes during the UK 2020 AR event. Each panel contrasts IWV values from WEGC with those from CDAAC. The four panels correspond to RO profiles reaching down to 2 km, 1 km, 500 m, and 200 m, respectively. RMSE and MBE units are in kg m−2 as well.

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A total of 163 GNSS-RO profiles reached at least 2 km altitude in both datasets, where CDAAC data show slightly smaller values than WEGC with a mean bias error (MBE) of 0.22 kg m−2 and a root mean square error (RMSE) of 1 kg m−2. The relationship is described by the regression line equation (y=0.97x-0.1), indicating a nearly one-to-one relationship with a minor offset.

As we descend to 1 km, the number of simultaneous observations decreases to 134, since fewer profiles reach down to this altitude. The MBE increased to 1.01 kg m−2 and the RMSE to 2.25 kg m−2. The correlation also deviated slightly, represented by the equation y=0.87x. On average, the CDAAC values are around 87 % of the WEGC values. A closer inspection, however, reveals that this systematic difference is largely due to data from the COSMIC-2 constellation.

Further down at 500 m, the observations decreased even more to 103. The MBE was 0.83 kg m−2 and the RMSE was slightly higher at 2.5 kg m−2, and CDAAC COSMIC-2 values are again systematically lower.

Lastly, only 39 profiles in both datasets reach down to the lowest altitude of 200 m, but the correlation is again very close to a one-to-one relationship (y=0.99x-0.3). The MBE is 0.38 kg m−2, and the RMSE is 1.84 kg m−2.

Predictably, as we descend in altitude, the IWV values generally increase due to the higher humidity levels commonly found at lower altitudes. This is, however, not necessarily and always the case, since that there is also a tendency for GNSS-RO profiles to reach further down in dry areas. A small ensemble of profiles reaching very low altitudes could therefore oversample particularly dry regions (see the example below in Sect. 4.2.2).

In conclusion, for the UK 2020 AR event, the IWV data from both CDAAC and WEGC are closely aligned, except for the COSMIC-2 profiles reaching down to 1 km and 500 m, respectively. The reason for this is currently unknown and justifies further analysis.

The differences in IWV between CDAAC and WEGC can be partially attributed to variations in the bending angle and refractivity retrieval methods. While both centers use the GNSS-RO raw data, their 1D-Var techniques and the associated background datasets differ significantly, which plays a larger role in shaping the retrieval results. Nevertheless, the observed IWV differences between the two centers remain relatively small, underscoring the robustness of the retrieval methodologies despite these variations.

4.2.2 Southern Africa 2009 AR event

The IWV measurements from the WEGC and CDAAC are compared in Fig. 8 for southern Africa 2009 (see Sect. 4.1.4) for different minimum altitudes.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f08

Figure 8Comparison of IWV values (in kg m−2) derived from GNSS-RO profiles reaching specified minimum altitudes during the southern Africa 2009 AR event. Each panel contrasts IWV values from WEGC with those from CDAAC. The four panels correspond to RO profiles reaching down to 2 km, 1 km, 500 m, and 200 m, respectively. RMSE and MBE are given in kg m−2.

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Based on 174 GNSS-RO profiles, which at least reached the highest altitude of 2 km, the IWV data from the two centers display a strong correlation (y=0.95x+0.3), with an MBE of just 0.01 kg m−2 and an RMSE of 0.8 kg m−2.

Descending to 1 km, the number of simultaneous observations is reduced to 139. The correlation remained strong, though the offset is higher (y=0.95x+1.0). The MBE increases slightly to 0.48 kg m−2 and the RMSE to 1.27 kg m−2.

Further down at 500 m, there is a nearly one-to-one correlation, but with an even more pronounced offset (y=0.97x+1.8), resulting in an increased MBE of 1.34 kg m−2 and an RMSE of 1.97 kg m−2.

At the minimum altitude of 200 m, observations dropped significantly to just 11. Over recent years, GNSS-RO profiles have reached lower and lower altitudes, but back in 2009 the lowest 200 m was still out of reach for most profiles.

Due to the limited ensemble size, these results may be less stable. Here, the correlation between the two datasets shows a greater deviation with a substantial positive offset (y=0.89x+4.6). The MBE is notably higher at 2.48 kg m−2, and the RMSE reaches 3.2 kg m−2.

In conclusion, for the southern Africa 2009 AR event, the IWV data from CDAAC and WEGC exhibit a strong correlation at higher altitudes, with some deviations becoming apparent as we descend. Overall, while the two datasets offer reliable insights across different altitudes, they also bring forth the importance of understanding the subtleties and potential discrepancies inherent in the data, especially at lower altitudes. Interestingly, while the maximum IWV recorded from an RO event at 500 m reached 37 kg m−2, it is worth noting that the maximum IWV for the RO profiles descending further to 200 m was 33 kg m−2 due to selective sampling of drier regions (see Sect. 4.2.1 above). This observation highlights the fact that not all RO profiles reaching the lowest altitudes include the highest IWV values.

4.2.3 California 2017 AR event

The IWV comparison for the California 2017 case highlights generally close agreement between the WEGC and CDAAC at all altitudes, with slight variations in the degree of offset (see Fig. 9).

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f09

Figure 9Comparison of IWV values derived from GNSS-RO profiles reaching specified minimum altitudes during the California 2017 AR event. Each panel contrasts IWV values from WEGC with those from CDAAC. The four panels correspond to RO profiles reaching down to 2 km, 1 km, 500 m, and 200 m. RMSE and MBE units are in kg m−2.

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For the RO profiles reaching to at least 2 km, with a sample size of 111 observations, the IWV data correlation is very strong (y=0.97x+0.1), having an MBE of only 0.09 kg m−2 and an RMSE of 0.68 kg m−2. Descending to 1 km, the number of observations moderately decreases to 95. The high correlation persists (y=0.98x+0.3) with a marginally increased positive offset, with an MBE of 0.15 kg m−2 and an RMSE of 1.09 kg m−2.

Descending to 500 m, based on 81 observations, the correlation between the two centers' IWV data remained extremely consistent (y=1.00x+0.5). The MBE increased to 0.45 kg m−2 and the RMSE to 1.41 kg m−2.

Lastly, further down at 200 m altitude, observations are based on 34 data points. The correlation remained surprisingly reliable with a one-to-one correlation and a minimal positive offset (y=1.00x+0.1), with an MBE of only 0.16 kg m−2 and an RMSE of 1.57 kg m−2.

In the California 2017 AR event, the IWV data from WEGC and CDAAC show very close agreement at all altitudes, with only slight variations noted. The analysis, conducted at various altitudes and based on different numbers of observations, consistently yields strong correlations between the two datasets.

In examining the IWV data from the UK 2020, southern Africa 2009, and California 2017 AR events, the correlation between CDAAC and WEGC is generally strong. In summary, across all three events and various altitudes, the data demonstrate a consistently strong correlation, with MBEs ranging from approximately 1.01 to 2.48 kg m−2 and RMSEs from 0.68 to 3.2 kg m−2.

4.3 GNSS-RO and SSMI/S IWV comparison

This section focuses on a comparative analysis of IWV values derived from two distinct observational sources. The first set of IWV values is obtained from RO profiles reaching down to an altitude of 200 m and is sourced from CDAAC and WEGC. This calculation of IWV from the lowest 200 m to the uppermost altitude of the RO profiles is designed to capture all possible humidity content, given that not all RO profiles can reach the Earth's surface. The second set of IWV values comes from observations made by SSMI/S.

The comparison is structured to assess how well these two data sources align or differ in terms of IWV measurements. In this analysis, a critical aspect to consider is the spatial resolution of the SSMI/S measurements, which is approximately 0.25° × 0.25° in latitude and longitude, translating to a spatial coverage of about 27 km for each grid square at the Equator. Furthermore, the obliquity of the RO profiles is an important factor in this methodological consideration. It is essential to understand that RO profiles are not perfectly vertical (see Sect. 2.1.1), which influences the representation of the atmospheric column in comparison to the SSMI/S observations.

For the purpose of comparison with the SSMI/S IWV values, it is crucial to accurately determine the most representative latitude and longitude coordinates. Given the spatial resolution of the SSMI/S data, the most representative coordinates for this comparison are identified based on the lowest 2 km segment of the RO profiles. This decision is informed by the fact that each SSMI/S grid, covering approximately 27 km, can encompass the lowest 2 km of the RO data. In most cases, the lowest 2 km of the RO data is contained within one of the SSMI/S grids. By selecting the latitude and longitude from this part of the RO profile, the study ensures a more accurate and meaningful comparison of the IWV values between the two observational methods

4.3.1 Iceland–UK 2009 AR event

In Fig. 10a, based on 111 observations, the correlation yields an MBE of 3.35 kg m−2 and RMSE of 6.41 kg m−2. This relationship between the CDAAC and SSMI/S datasets is encapsulated by the equation y=0.79x+1.7. This suggests that the CDAAC values approximate to about 79 % of the SSMI/S values, accompanied by a noticeable offset.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f10

Figure 10Comparison of IWV values (in kg m−2) derived from GNSS-RO profiles from CDAAC (a), WEGC (b), and SSMI/S observations during the Iceland–UK 2009 AR event. The IWV values from each GNSS-RO profile are computed from 200 m altitude up to the uppermost limit of each profile. The SSMI/S IWV values are extracted at the latitude and longitude that correspond to the 2 km altitude of the GNSS-RO profiles. MBE and RMSE values are given in kg m−2.

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On the other hand, Fig. 10b contrasts the WEGC IWV against the SSMI/S IWV with 96 observations. The correlation here exhibits an MBE of 3.20 kg m−2 and an RMSE of 5.92 kg m−2. The relationship can be characterized by y=0.80x+0.7, implying that WEGC values are closely aligned, being around 80 % of the SSMI/S values, and with a slightly diminished offset compared to the CDAAC data. Both CDAAC and WEGC IWV datasets, as illustrated in Fig. 10, exhibit a reasonably close alignment with the SSMI/S IWV values, but both underestimate the SSMI/S IWV values in a similar way.

Notably, in Fig. 10b, the WEGC dataset is slightly smaller, with 15 fewer events, than the CDAAC dataset in this case study. Additionally, the number of RO profiles by the GRACE satellite is six in Fig. 10a and only one in Fig. 10b. Furthermore, the number of COSMIC-1 observations is considerably larger in Fig. 10b, while MetOp-A observations are more prominent in Fig. 10a.

Since the water vapor content in the lowest 200 m is missing in the GNSS-RO-derived IWV values we have to expect a (slight) underestimation, but the results are somewhat lower than anticipated.

As RO profiles often do not reach the surface, we observe a systematic underrepresentation of the “true” IWV content in these cases. The missing lowest 200 m is not a specific threshold but rather a practical limit chosen to balance ensemble size and penetration depth. While some profiles penetrate further down, they are insufficient to create statistically meaningful results. This limitation likely leads to an underestimation of IWV, particularly in regions with high moisture concentrations near the surface. Further investigations could address how much this underrepresentation impacts the total IWV retrievals and explore ways to account for this bias.

4.3.2 Southern Africa 2009 AR event

The second comparison focuses on the southern Africa AR event in 2009 as visualized in Fig. 11. Delving into Fig. 11a, based on 39 observations, a correlation emerges with a marked negative offset of the CDAAC data (y=0.92x-3.7), leading to an MBE of 6.04 kg m−2 and an RMSE of 7.2 kg m−2. As a result, almost all CDAAC values are lower than the corresponding SSMI/S values.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f11

Figure 11Comparison of IWV values (in kg m−2) derived from GNSS-RO profiles from CDAAC (a), WEGC (b), and SSMI/S observations during the southern Africa 2009 AR event. The IWV values from each GNSS-RO profile are computed from 200 m altitude up to the uppermost limit of each profile. The SSMI/S IWV values are extracted at the latitude and longitude that correspond to the 2 km altitude of the GNSS-RO profiles. MBE and RMSE values are given in kg m−2.

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Transitioning to Fig. 11b, which contrasts WEGC IWV against SSMI/S IWV, the dataset is drawn from 67 observations. The correlation manifests an MBE of 4.78 kg m−2 and an RMSE of 6.71 kg m−2. This relationship can be expressed by the equation y=0.71x+1.6, indicating that WEGC values around 10 kg m−2 are quite well represented, while higher values are underrepresented.

In this AR event, the CDAAC dataset includes 39 events, whereas WEGC includes 67 events, and in most other cases there are more CDAAC than WEGC events reaching down to 200 m altitude. Notably, there are no TSX and GRACE RO events observed to reach the lowest 200 m of altitude in Fig. 11a and b.

4.3.3 California 2017 AR event

The final analysis focused on the California 2017 AR event. The outcomes of this assessment are visualized in Fig. 12.

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Figure 12Comparison of IWV values (in kg m−2) derived from GNSS-RO profiles from CDAAC (a), WEGC (b), and SSMI/S observations during the California 2017 AR event. The IWV values from each GNSS-RO profile are computed from 200 m altitude up to the uppermost limit of each profile. The SSMI/S IWV values are extracted at the latitude and longitude that correspond to the 2 km altitude of the GNSS-RO profiles. MBE and RMSE values are given in kg m−2.

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Starting with Fig. 12a, from a sample of 126 observations, the correlation yielded an MBE of 2.28 kg m−2 and an RMSE of 4.92 kg m−2. The relationship between the CDAAC and SSMI/S datasets can be expressed by the equation y=0.82x-1.1.

Proceeding to Fig. 12b, the dataset comprises only 40 observations reaching down to 200 m. Here, the correlation shows an MBE of 1.06 kg m−2 and an RMSE of 4.47 kg m−2. This relationship is characterized by the equation y=0.83x+1.3, signifying that the WEGC values are close to 83 % of the SSMI/S values, but with a contrasting positive offset.

Especially during this event, the numbers of ensemble members in both datasets are strikingly different, which is remarkable since both datasets are based on the same low-level data.

The cut-off heights for RO profiles differ between UCAR and WEGC due to variations in retrieval methods and the application of different quality control measures. These differences in cut-off heights result in distinct numbers of events recorded by each center. In this specific case, the variations in cut-off heights play a significant role in the differences observed between CDAAC and WEGC event counts.

4.4 Comparison of CDAAC and WEGC IWV values with background profiles

In this subsection, we examine the IWV values obtained from CDAAC and WEGC centers in relation to their corresponding background profiles. The comparison has been conducted for profiles which reach altitudes of at least 2 km, 1 km, 500 m, and 200 m. By considering the background profiles, we aimed to assess the differences between the background and retrieved IWV values of the two centers. Through this investigation, we seek to identify any discrepancies or biases between the IWV values and the corresponding background profiles.

4.4.1 Iceland–UK 2009 AR event

For the Iceland–UK 2009 AR event, this resulted in a set of eight plots, with four comparing CDAAC IWV against ERA IWV shown in Fig. 13a–d and another four contrasting WEGC IWV against ECMWF-b as seen in Fig. 13e–h.

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Figure 13Comparison of IWV values (kg m−2) retrieved from CDAAC and WEGC centers against their respective background profiles during the Iceland–UK 2009 AR event. Eight panels are distributed over two columns, examining four distinct altitudes: 2 km, 1 km, 500 m, and 200 m. In the left column, panels (a)(d) display the relationship between IWV values from ERA background profiles and IWV values from CDAAC, noting that the TSX satellite uses ECH as the background information. Conversely, in the right column, panels (e)(h) present comparisons between IWV values from ECMWF-b background profiles and IWV values from WEGC. RMSE and MBE units are in kg m−2.

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For the CDAAC IWV versus ERA IWV comparison, a general trend can be observed. As altitude decreases from 2 km to 200 m (Fig. 13a–d), the MBE grows more negative, indicating a progressively larger underestimation of the CDAAC IWV values compared to the ERA background. Concurrently, the RMSE also increased, suggesting increasing variability in the comparison. The regression equations showed a steady decrease in the slope, implying a less direct correlation between the datasets as altitude decreased. The most pronounced deviation was noticed at 200 m altitude, where the equation is y=0.66x+2.4, denoting a significant positive offset and reduced slope.

On the other hand, the WEGC versus ECMWF-b comparison shows a different picture. Throughout the altitudinal range of 2 km to 200 m (Fig. 13e–h), the MBE values remain less than 2 kg m−2, suggesting a closer alignment of WEGC values with the ECMWF-b background. The RMSE values, while increasing as altitude decreases, are generally lower than their CDAAC counterparts. The regression equations exhibit a consistent and high correlation between the datasets across all altitudes, with slopes nearing unity at higher altitudes and a minimal offset.

In the in-depth analysis of the IWV values against their corresponding background profiles, an important distinction emerges regarding the CDAAC background data sources. While most satellites employ ERA as their background data, TSX uniquely utilizes ECH profiles. This distinction becomes particularly evident when observing Fig. 13a–d.

From Fig. 13a–d, a notable pattern arises: the TSX data points predominantly align with the 1 : 1 line, indicating a direct correlation with the background data. In stark contrast, data from other satellites consistently tend to underestimate the IWV values. This implies that, among the satellites examined, TSX exhibits a closer alignment and is more correlated with the background data than other satellites.

The presence of TSX data along the 1 : 1 line reinforces its accuracy and alignment with the ECH profiles it uses as a background. This emphasizes that while the retrieved IWV values are not highly sensitive to the choice of background profile, the background profile can influence the bias relative to the true IWV. For example, ERA background profiles tend to exhibit a wet bias, which is corrected in CDAAC retrievals, resulting in drier values closer to the true IWV. Similarly, ECH profiles without this wet bias result in CDAAC retrievals that align more closely with them. It is noteworthy that while background profiles generally exhibit higher IWV values in Fig. 13a–d, the retrieved IWV values in CDAAC tend to be drier, with the exception of TSX data.

Close agreement between retrieved and background-derived IWV is not necessarily good or bad, even more since we know from Sect. 4.3.1 that there is close agreement of the IWV values derived from CDAAC and WEGC data, respectively. A quite possible explanation is that the ERA-derived IWV values are indeed too high, whereas the CDAAC retrieval brings the profiles into closer agreement with the “truth” and (in this case) with the WEGC data.

4.4.2 UK 2020 AR event

In the second study case centered on the UK 2020 event, an analysis was undertaken to evaluate the IWV values from the CDAAC and WEGC centers against their respective background profiles across four distinct altitudes: 2 km, 1 km, 500 m, and 200 m. These results are visually represented in Fig. 14a–h.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f14

Figure 14Comparison of IWV values retrieved from CDAAC and WEGC centers against their respective background profiles during the UK 2020 AR event. Eight panels are distributed over two columns, examining four distinct altitudes: 2 km, 1 km, 500 m, and 200 m. In the left column, panels (a)(d) display the relationship between IWV values from ECH background profiles and IWV values from CDAAC. Conversely, in the right column, panels (e)(h) present comparisons between IWV values from ECMWF-b background profiles and IWV values from WEGC. RMSE and MBE units are in kg m−2.

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For the CDAAC IWV, which uses ECH profiles as its background data, the correlation with the background is observed across Fig. 14a–d. At 2 km, the correlation exhibits a slight underestimation with an MBE of 0.4 kg m−2 and an RMSE of 1.1 kg m−2. As altitude decreases, this underestimation becomes more pronounced, reaching an MBE of 0.78 kg m−2 at both 500 and 200 m. The regression slopes for these altitudes indicate that the CDAAC values are generally around 85 % to 91 % of the background values, with a slight positive offset.

Figure 14e–h showcase the comparison for WEGC IWV data. At 2 km altitude, the data almost mirror the background with an MBE of 0.01 kg m−2. However, as we descend in altitude, there is a gradual shift towards underestimation, reaching an MBE of 1.12 kg m−2 at 500 m. The regression slopes remain relatively close to unity, especially at higher altitudes, suggesting a strong alignment with the background data.

Comparing these findings with the previous study case for the UK–Iceland 2009 event, some distinctions emerge. In the 2009 event, while the retrievals for most satellites at CDAAC used ERA as the background, the exception of TSX utilizing ECH profiles stood out due to its close alignment along the 1 : 1 line. In the 2020 event, the utilization of ECH profiles as the background for CDAAC IWV seems to offer a more consistent and aligned IWV estimation across altitudes compared to when ERA was predominantly used as the background in the 2009 event.

The choice of ECH profiles for CDAAC IWV in the 2020 event appears to enhance its correlation, echoing the superior alignment observed with TSX in the 2009 event, which also used ECH profiles. This emphasizes the important role of background data in shaping the accuracy and reliability of satellite-derived IWV values, with ECH profiles emerging as a potentially more aligned choice in these study cases.

Interestingly, COSMIC-2 data provide additional insights into these differences. As shown in Fig. 7, CDAAC COSMIC-2 data appear noticeably drier than WEGC data, suggesting that the ECMWF-b profiles used by CDAAC may inherently exhibit a drier bias compared to the ECH profiles used by WEGC. However, in Fig. 14, no significant bias is observed relative to the background for either center. This discrepancy may arise from differences in retrieval methodologies, quality control measures, or the atmospheric conditions during these events. The COSMIC-2 results highlight the importance of evaluating biases across different altitudes and conditions to better understand the impact of background profiles on retrieval outcomes.

4.5 Comparative analysis of WEGC specific humidity profiles with ECMWF background data across events

In this subsection, we compare the specific humidity profiles retrieved by WEGC with their corresponding ECMWF background data across different events. The goal of this analysis is to understand the extent and nature of discrepancies, if they exist, between the retrieved and background data and analyze the effect of background water vapor on the retrieved q.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f15

Figure 15Comparison of specific humidity profiles retrieved by WEGC against ECMWF background data for each event. (a) Difference in specific humidity (qwegcqECMWF-b) plotted against altitude. (b) Mean specific humidity represented by a solid line, with the standard deviation (SD) denoted by a dashed line.

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Initially, the differences between the specific humidity values retrieved by WEGC (qwegc) and those from ECMWF (qECMWF-b) were computed for profiles reaching a minimum altitude of 500 m. These differences are visualized in a plot against altitude (Fig. 15), offering a clear representation of how deviations vary with height. To ensure a substantial data sample while maintaining the ability to analyze specific altitudes like 2 and 1 km, only profiles reaching down to the lowest 500 m are incorporated in this comparison. A decision to narrow down to 200 m would have resulted in a restricted sample size, potentially skewing the insights. Subsequent to this, for the plotted differences, the mean specific humidity and its standard deviation (SD) are computed for each satellite individually.

Furthermore, the relative specific humidity difference (RSHD) was calculated and visualized for each event, providing a quantitative measure of the accuracy of the retrieved data in relation to the background, which is defined as

(6) RSHD = q retrival - q reference σ reference ,

where qretrieval is the specific humidity retrieved from GNSS-RO data, and qreference is the specific humidity from the reference dataset. This metric provides a percentage-based comparison of differences, allowing for direct evaluation of retrieval accuracy.

Lastly, to assess the variability and dispersion of the relative humidity differences, the interquartile range (IQR) and standard deviation for the relative specific humidity differences are plotted. This comprehensive approach ensures a holistic understanding of the alignment between the WEGC-retrieved data and the ECMWF background across different altitudes and satellites.

https://amt.copernicus.org/articles/18/2481/2025/amt-18-2481-2025-f16

Figure 16Detailed assessment of specific humidity relative differences across different events. Each of the six plots represents an individual event, containing three distinct visualizations for every satellite present: (i) relative specific humidity difference (RSHD) in percentage, showcasing the discrepancies between retrieved and background values; (ii) standard deviation (SD) of RSHD, highlighted to capture the variability in differences; and (iii) interquartile range (IQR) of RSHD, emphasizing the middle 50 % spread of the differences.

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Upon reviewing Fig. 16, which, in combination, covers six distinct events, several patterns emerge. The plots showcase specific humidity relative differences when comparing WEGC retrievals against ECMWF background data. This difference representation, spread across different altitudes, grants a layered perspective on the retrievals for each event.

It is evident that the differences are generally minimal at higher altitudes. This is inferred from the concentration of data around the zero-difference mark in these regions, signifying that the humidity values are small to begin with and that the WEGC retrievals closely mirror the ECMWF background data. However, as one moves to lower altitudes, the spread of differences broadens, indicating an increase in discrepancies between the retrievals and the background. This is not a bad thing, since it just means that retrievals differ from their respective backgrounds, which is – in general – related to an increase in information content.

Figures 15 and 16 illustrate the potential biases in GNSS-RO retrievals in the lower troposphere, where super-refraction and other effects can influence the retrieved values. These biases, which are more pronounced in the CDAAC TSX data, underscore the importance of considering lower-troposphere uncertainties when interpreting IWV retrievals.

Another striking observation is the variability between different datasets or satellites within each event. While some datasets exhibit a tight clustering of differences around the zero mark, others display a broader spread.

The sensitivity of GNSS-RO retrievals to vapor a priori differs between specific humidity profiles and IWV values. As shown in Figs. 4a and 6a, the altitude-dependent sensitivity is related to RAER values, with lower RAER indicating stronger observational influence. IWV retrievals, however, may not consistently align with background IWV due to their integration over the vertical profile, which can amplify or mask biases in the lower troposphere. This is particularly evident in CDAAC TSX data (Fig. 6a) and the comparisons presented in Figs. 15 and 16, where systematic biases in the lower troposphere contribute to differences in IWV values.

Conclusively, these figures offer a deep dive into the nuances of specific humidity retrieval differences when juxtaposed against a consistent background dataset. They underscore the variability introduced by different datasets or satellite sources. The consistent patterns across events also hint at systematic challenges or characteristics inherent to the regions or times of the events studied.

5 Conclusions and outlook

The critical role of atmospheric rivers (ARs) in global moisture transport and precipitation dynamics necessitates accurate water vapor measurements for both understanding and forecasting these phenomena. While the integrated water vapor content (IWV) of ARs can be measured well with microwave and infrared sounders, the vertical structure is less well known. In this study, we analyzed whether specific humidity profiles and IWV values from Global Navigation Satellite System Radio Occultation (GNSS-RO) measurements provide additional information for the study of ARs, in particular regarding their vertical structure. The retrieval of water vapor from GNSS-RO data requires background information, which is usually incorporated by the one-dimensional variational method (1D-Var) that combines observations and background in an optimal manner. We compared data from the COSMIC Data Analysis and Archive Center (CDAAC), operated by the University Corporation for Atmospheric Research (UCAR) in Boulder, Colorado, with data from the Wegener Center for Climate and Global Change (WEGC) at the University of Graz, Austria.

A significant part of our study addresses the performance of the 1D-Var systems at CDAAC and WEGC, particularly when there are large differences between the RO observations and the background data. The different computations of tangent point trajectories and reference points, especially when they are situated at the edges of AR events with a pronounced humidity gradient, can lead to the extraction of background profiles at very different locations with different humidity regimes. When comparing data from different centers it is important be aware of this in order to better understand potential differences.

Despite these differences, the 1D-Var method at both centers yields remarkably similar retrieved profiles, in particular in the altitude range where the 1D-Var scheme allows for a strong weighting of the observations. This consistency across different centers highlights the 1D-Var system's robustness and adaptability in handling diverse atmospheric conditions, demonstrating its capacity to produce reliable profiles despite varied and contrasting background data. However, it is clear that background water vapor significantly shapes the retrieved profiles, especially where weighting of the observations is weak.

GNSS-RO data provide accurate specific humidity profiles; however, challenges in reaching the lowermost troposphere lead to systematic underrepresentation of the IWV values. The altitude-specific assessments shed light on the variability of IWV data and the performance of RO profiles across different atmospheric layers. Additionally, the integration of Special Sensor Microwave Imager/Sounder (SSMI/S) IWV values offered a broader perspective, revealing gaps in RO profiles and suggesting the potential for augmenting RO IWV measurements with SSMI/S observations.

Comparing forecast data from the European Centre for Medium-Range Weather Forecasts (ECMWF) profiles with ECMWF analysis data at the GNSS-RO profile locations generally shows very small changes – even though the GNSS-RO profiles have been assimilated into the analyses. This indicates that GNSS-RO humidity information still has a limited impact on analyses – even though they have a demonstrated information content. It therefore seems useful to employ GNSS-RO (and other) data for direct observations of ARs.

The good agreement between RO-derived IWV values from CDAAC and WEGC and between WEGC and ECMWF together with a marked discrepancy between CDAAC and ERA5 suggests that the ERA5 reanalyses might indeed have a wet bias.

As a next step, we recommend combining RO profiles with SSMI/S IWV observations to compensate for the missing lower parts of the RO profiles. While SSMI/S provides integrated water vapor data with horizontal resolution, it lacks vertical detail, making it a complementary dataset to RO profiles, especially near the edges of ARs where humidity gradients are most pronounced. Future research should focus on integrating complementary datasets, such as GNSS-RO and SSMI/S, within advanced data assimilation systems. This integration can enhance the resolution of the three-dimensional moisture structure of ARs, particularly in the lower troposphere where GNSS-RO data have known limitations. Furthermore, combining the vertical resolution of GNSS-RO data with the horizontal coverage of SSMI/S in real-time operational forecasting systems could improve AR predictions and provide insights into extreme precipitation events.

Another important aspect of future work is the global availability of GNSS-RO data, which allows for studying ARs in regions that lack routine measurement campaigns or mesoscale modeling studies. For instance, GNSS-RO data have proven invaluable in a current study analyzing ARs over Africa, a region that remains understudied in this context. Expanding such analyses to other underrepresented regions could significantly advance our understanding of ARs and their impacts worldwide.

In conclusion, our research offers a comprehensive exploration of humidity profiles and IWV values within AR events. It illuminates the complex interplay between retrieval methodologies, tangent point trajectories, and background data, as well as their collective impact on the retrievals. Our findings not only advance the understanding of atmospheric moisture profiling but also set a direction for future research. Emphasizing the synergy of different observational tools and datasets, this study advocates for an integrated approach to achieve a more accurate and comprehensive understanding of atmospheric conditions, particularly focusing on the dynamic nature of atmospheric rivers.

Code availability

The analysis in this study was conducted using Python scripts developed by the authors. These scripts were specifically tailored for the different assessments presented in the paper and are not part of a standardized or reusable software package. Due to its length, case-specific nature, and the current lack of documentation suitable for public release, the code has not been deposited in a public repository. However, the authors are happy to provide the scripts upon reasonable request for academic and research purposes. Interested researchers can contact the corresponding author at bahareh.rahimi@uni-graz.at.

The analysis was conducted using Python 3.11 (https://www.python.org/, Python Software Foundation, 2022) along with several open-source libraries, including NumPy (https://numpy.org/; Harris et al., 2020), pandas (https://pandas.pydata.org/; McKinney, 2010), xarray (https://docs.xarray.dev/en/stable/; Hoyer and Hamman, 2017), Matplotlib (https://matplotlib.org/; Hunter, 2007), and netCDF4 (https://github.com/Unidata/netcdf4-python, Pierce, 2022).

Data availability

The GNSS-RO data from the UCAR CDAAC system are publicly available at https://doi.org/10.5065/ZD80-KD74 (UCAR COSMIC Program, 2022). The SSMIS F16 and F17 v7 data used in this study were obtained from the NASA Global Hydrology Resource Center DAAC and are available at https://www.remss.com/missions/ssmi (Wentz et al., 2012). The GNSS-RO data processed by the Wegener Center for Climate and Global Change (WEGC) are not publicly available due to institutional access restrictions. However, they are available upon reasonable request from the WEGC at the University of Graz (https://wegcenter.uni-graz.at/en/, last access: 18 May 2025).

Author contributions

This article was jointly conceptualized by both authors. UF provided guidance, engaged in critical discussions, and oversaw the research process. The first author, BR, performed the computational and analytical work and was responsible for writing the manuscript draft, which was then revised by UF. UF's mentorship and expertise contributed to shaping the research direction and methodology. Both authors contributed to the interpretation of the results.

Competing interests

The contact author has declared that neither of the authors has any competing interests.

Disclaimer

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.

Special issue statement

This article is part of the special issue “Observing atmosphere and climate with occultation techniques – results from the OPAC-IROWG 2022 workshop”. It is a result of the International Workshop on Occultations for Probing Atmosphere and Climate, Leibnitz, Austria, 8–14 September 2022.

Acknowledgements

The authors thank Mark Schwärz and Andrea K. Steiner (Wegener Center for Climate and Global Change, University of Graz, Austria) for invaluable discussions.

This research was funded in whole, or in part, by the Austrian Science Fund (FWF) under the research grant DOI https://doi.org/10.55776/W1256 (Austrian Science Fund (FWF), 2023; doctoral program “Climate Change: Uncertainties, Thresholds and Coping Strategies”) and by the University of Graz. For the purpose of open access, the authors have applied a CC BY public copyright license to any author-accepted manuscript version arising from this submission.

Financial support

This research has been supported by the Austrian Science Fund (grant no. W1256).

Review statement

This paper was edited by Anthony Mannucci and reviewed by two anonymous referees.

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Executive editor
Atmospheric rivers (ARs) are recognized as significant contributors to extreme precipitation at mid-latitudes and may increase in frequency and intensity due to climate change. This timely study is the first the show the potential value of GNSS radio occultation (GNSS RO) remote sensing to the study of ARs and in particular how the high vertical resolution of GNSS RO provides information that is complementary to other techniques. The combination of GNSS-RO data with mesoscale models, particularly through assimilation, could further improve our understanding of AR dynamics and the processes leading to extreme precipitation and flooding. This is an important direction for future studies.
Short summary
The study investigates using Global Navigation Satellite System Radio Occultation (GNSS-RO) to analyze the vertical structure of humidity in atmospheric rivers (ARs). Specific humidity and integrated water vapor from the COSMIC Data Analysis and Archive Center (CDAAC) and the Wegener Center (WEGC) are compared with the Special Sensor Microwave Imager/Sounder (SSMIS), showing that GNSS-RO adds vertically resolved data. Despite a slight low bias, combining GNSS-RO and SSMIS improves AR analysis.
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