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Comparison of three retrievals of COSMIC GPS radio occultation results in the tropical upper troposphere and lower stratosphere
Earth, Planets and Space volume 69, Article number: 125 (2017)
Abstract
Combining geometrical optics (GO) and wave optics (WO), the COSMIC data analysis and archive center (CDAAC) retrieved two sets of dry atmosphere temperatures (T) from COSMIC GPS radio occultation (GPSRO), which are called atmPrf2010 and atmPrf2013. In atmPrf2010, the sewing height between WO and GO varies between 10 and 20 km, but is fixed at 20 km for atmPrf2013. The height resolution of the atmPrf2010 depends on the sewing height, while the T profiles by atmPrf2013 are smoothed over 500 m. We also derived T by applying WO throughout the troposphere and the stratosphere up to a 30km altitude, which is called rishfsi2013. The three retrievals have different characteristics in the height resolution around the tropopause. Therefore, we aim to examine a possible discrepancy in the statistical results of the coldpoint tropopause (CPT) and the lapse rate tropopause (LRT) among the three datasets, conducting their intercomparisons as well as the comparison between GPSRO and the simultaneous radiosonde dataset. We investigate the T variations in the upper troposphere and lower stratosphere (UTLS) over the tropics from October 1, 2011, to March 31, 2012, when radiosonde soundings were conducted as the CINDYDYNAMO 2011 campaign. The mean T profiles are consistent between atmPrf2010 and atmPrf2013, but rishfsi2013 results are colder (warmer) than the CDAAC retrievals below (above) the tropopause. The mean T difference between atmPrf2013 and atmPrf2010 is 0.17 K at the coldpoint tropopause (CPT) and −0.38 K at the lapse rate tropopause (LRT). On the other hand, rishfsi2013 shows a colder T at CPT by −0.77 and −0.59 K relative to atmPrf2013 and atmPrf2010, respectively, and the warmer T by 0.60 and 0.20 Kd at LRT. During CINDYDYNAMO, we found 134 radiosonde soundings that coincide with GPSRO within ±3 h and are collocated within 200 km from GPSRO. The mean T difference at CPT from the radiosondes is 0.32, 0.49 and −0.24 K for atmPrf2010, atmPrf2013 and rishfsi2013, respectively. Both atmPrf2013 and atmPrf2010 have a positive bias at CPT, while rishfsi2013 has a negative one. Similar comparisons at LRT are −0.45, −0.69 and −0.41 K, respectively, showing a negative bias for all GPSRO retrievals. The results show that rishfsi2013 is consistent with the retrievals at CDAAC and the radiosondes. Due to its good height resolution, rishfsi2013 is useful for studies on mesoscale T perturbations in the UTLS.
Introduction
The global positioning system radio occultation (GPSRO) technique is an active limb sounding of the Earth’s atmosphere and ionosphere using the characteristics of microwave propagation from GPS satellites at an orbit altitude of 20,200 km to the lowEarthorbit (LEO) satellites around 700 km (Ware et al. 1996). In April 2006, the University Corporation for Atmospheric Research (UCAR) and the National Space Organization (NSPO) of Taiwan jointly conducted a very successful GPSRO mission, called the Constellation Observing System for Meteorology, Ionosphere, and Climate (COSMIC), consisting of six LEO satellites (Anthes et al. 2008). The GPSRO has produced highly accurate atmospheric profiles, significantly improving the weather forecasting performance and providing longterm stable references for climate applications (e.g., Anthes 2011; Ladstädter et al. 2015). In addition, GPSRO temperature profiles with superior height resolutions provide a unique opportunity to study the mesoscale temperature fluctuations caused by atmospheric waves in the stratosphere (Alexander et al. 2008; Tsuda et al. 2011), and analysis of internal gravity wave parameters (Gubenko et al. 2011).
The fundamental retrieval techniques for the GPSRO data are geometric optics (GO) and wave optics (WO), assuming that the atmosphere has spherical symmetry (Melbourne 2004). The GO method constructs the L1 and L2 bending angles in the neutral atmosphere by the time derivative of the excess phase (Doppler) and the positions and velocities of the GPS and LEO satellites (Kuo et al. 2004). To reduce the influence of the ionosphere, optimal filtering is applied on the L2 bending angle. Then, the ionosphericfree bending angle is obtained by combining the L1 and L2 bending angles (Sokolovskiy et al. 2009; Schreiner et al. 2011). The vertical resolution of the GO profile is limited to about 1.4 km by the Fresnel zone (Kursinski et al. 1997).
In the lower atmosphere, where GO cannot solve the multipath problem caused by sharp vertical moisture gradients, the WO method is used by applying integral transforms to the entire raw phase and complex amplitude signals to derive the L1 bending angle. Typical WO methods are canonical transform (CT) (Gorbunov 2002; Gorbunov and Lauritsen 2004), full spectrum inversion (FSI) (Jensen et al. 2003) and phase matching (PM) (Jensen et al. 2004), which provide a good vertical resolution of about 0.1–0.3 km. The entire ionospherefree bending angle profile is, then, obtained by combining (sewing) the GO and WO profiles (Kuo et al. 2004; Schreiner et al. 2011).
The Abel inversion is applied to derive the refractive index profile from the ionospherefree bending angles. The dry atmospheric temperature (T) can be directly obtained by neglecting the effects of water vapor pressure on the refractive index and assuming a hydrostatic equilibrium and the ideal gas law. The T profiles significantly differ from the real temperature below about 6 and 10 km at high and low latitudes, respectively (ScherllinPirscher et al. 2011). Because the neutral atmospheric bending angle decreases exponentially with height, the retrieved profiles above about 40 km may contain measurement errors due to ionospheric noise.
Tropopause fluctuations, which play an important role in the exchange mechanism between the troposphere and the stratosphere, influence global climate variations (Fueglistaler et al. 2009; Gettelman et al. 2011). The longterm GPSRO data indicate climate change signals from warming in the upper troposphere and cooling in the lower stratosphere (Steiner et al. 2011). Many recent studies have utilized GPSRO data to investigate the variability in the upper troposphere and the lower stratosphere (UTLS) such as fluctuation details of the coldpoint tropopause (CPT) (Kim and Son 2012), and the occurrence of the multiple lapse rate tropopause (LRT) (Xu et al. 2014).
A multiple tropopause often appears in the equatorial region. Moreover, temperature variations near the tropical tropopause are more pronounced due to the effects of atmospheric waves. Thus, the detection of CPT and LRT may be affected by the height resolution of the T profile. Therefore, this issue needs to be considered when comparing CPT and LRT from the GPSRO retrievals and radiosonde data.
The COSMIC data analysis and archive center (CDAAC) of UCAR published the COSMIC GPSRO results in 2010 and 2013 using different retrieval algorithms. We also independently retrieved the COSMIC GPSRO data. In this paper, we conduct a statistical comparison of the T variations in the tropical UTLS region among these three GPSRO datasets. Additionally, we validate them by referring to simultaneous radiosonde data with an emphasis on the characteristics of the CPT and LRT.
“Data analysis” section outlines the three retrievals of the GPSRO data, while “Results and discussion” section compares the T profiles in terms of the CPT and LRT among the three GPSRO datasets. Finally, to validate the GPSRO results, they are compared to the radiosondes.
Data analysis
COSMIC GPSRO
CDAAC published Level 2 atmospheric dry profiles (atmPrf) in a height range up to 60 km from the ground. The first results were processed in 2006 and were reprocessed in 2009 (Sokolovskiy et al. 2009). Then in 2010, the atmPrf version 2010.2640 was published.
Wang et al. (2013) conducted a statistical test of the CDAAC atmospheric wet profiles (wetPrf) version 2010.2640. Compared to the global radiosonde data, a small bias of −0.09 K ± 1.72 K was observed in the height range from 925 to 10 hPa. On the other hand, Das and Pan (2014) reported that the temperature differences between CDAAC wetPrf (wet) and atmPrf (dry) version 2010.2640 are nearly zero from 200 to 10 hPa. Although the dry temperature retrieval deviates from the real temperature in a moist atmosphere (ScherllinPirscher et al. 2011), the atmPrf version 2010.2640 is not affected by water vapor above about 10 km. This bias estimated by Wang et al. (2013) can also be applied as an index for the dry atmosphere.
The most common dataset is the updated version of atmPrf products published by CDAAC, which is known as 2013.3520. This study employs both atmPrf 2010.2640 and atmPrf 2013.3520, which are hereafter referred to as atmPrf2010 and atmPrf2013, respectively. Table 1 shows their fundamental characteristics. The retrieval in atmPrf2013 and atmPrf2010 adopts the PM and FSI methods, respectively, in the lower atmosphere. However, at higher altitudes, both adopt the GO method.
For atmPrf2010, the FSI method was employed up to a specified altitude between 10 and 20 km, depending on the ionospheric noise (Sokolovskiy et al. 2010; Schreiner et al. 2011). The sewing altitude, which is where FSI switches to GO, is prescribed for each atmPrf2010 profile. Consequently, the height for the transition of the vertical resolution varies in the UTLS region for individual GPSRO events (Sokolovskiy et al. 2014).
For atmPrf2013, the sewing altitude from PM to GO is fixed at 20 km, producing a profile with the good height resolution up to 20 km. Height smoothing for altitudes between 10 and 20 km is applied to reduce the vertical resolution to 0.5 km, although the original height resolution of 0.1–0.3 km is kept below 10 km (Sokolovskiy et al. 2014).
Zeng et al. (2016) have suggested that in weather applications, the different dynamical extrapolation heights for each individual occultation profile, which is adopted in atmPrf2010, may be a better definition. However, for climate applications, it is better to fix the optimal transition height from GO to WO at constant altitude (20 km) as applied in atmPrf2013.
We used the version 3520 data of COSMIC GPSRO published by CDAAC, applying the same retrieval procedure and the background atmospheric model as in Tsuda et al. (2011). Hereafter, we call our results as rishfsi2013. The FSI software was coded at RISH with intensive support by CDAAC. We applied the FSI method up to 30 km with a vertical resolution of 0.1–0.2 km. Tsuda et al. (2011) reported that the FSI profile can be used to study mesoscale temperature perturbations such as atmospheric gravity waves with the upper limit about 28 km.
Figure 1 shows the total number of COSMIC GPSRO profiles in the 10°S–10°N latitude range from October 1, 2011, to March 31, 2012. This period was selected considering the availability of the radiosonde data for comparison, which is introduced in the next subsection. Two different versions of COSMIC GPSRO datasets by CDAAC as well as rishfsi2013 were processed. Compared to atmPrf2010 and rishfsi2013, atmPrf2013 has more atmospheric profiles; the totals are 12,760, 12,274 and 15,441, respectively. The difference in the number of retrieved profiles may be related to the truncation process of the L1 signal at the bottom of occultation (Schreiner et al. 2011). After selecting successfully retrieved GPSRO events in the three datasets, the total number of profiles available for comparison was 10,838.
Radiosondes
The Cooperative Indian Ocean experiment on intraseasonal variability in the year 2011 and the joint project of Dynamics of the Madden–Julian Oscillation (CINDYDYNAMO 2011) are part of an international collaborative campaign to collect in situ observations in the tropics (Yoneyama et al. 2013; Zhang et al. 2013). This project performed intensive radiosonde observations for about six months from October 1, 2011, to March 31, 2012, providing 7789 radiosonde profiles using Vaisala RS92SGPD and Meisei RS06G radiosondes from 19 ground stations spread over 35°E–140°E and 10°S–10°N (Fig. 2). In addition, radiosondes were launched every 3 h during the campaign from three research vessels (R/V): Baruna Jaya, Sagar Kanya and Mirai. The boxes in Fig. 2 denote their cruise tracks. The R/V campaigns varied from 3 weeks to 2 months. Moreover, a balloon was launched from Gan Island every 3 h from October 2011 to February 2012. Other ground stations with 12h routine soundings were located at Seychelles, East of Africa, Nairobi, Maldives, Sri Lanka, Singapore and 13 sites on the Indonesian maritime continents.
The original vertical resolution of the radiosonde data was about 10 m due to the twosecond recording intervals. To compare to the COSMIC GPSRO profiles, the radiosonde data were averaged every 100 m. We selected the COSMIC GPSRO profiles whose tangent points at a 10km altitude were within 200 km from the radiosonde sites, and their occultation time was within ±3 h from the balloon launch time. We chose the space and time separations for the comparison with radiosondes following the earlier studies (e.g., Kuo et al. 2005; Sun et al. 2010). For the comparison between COSMIC GPSRO and radiosondes, we found as many as 134 collocated profiles. Note that most of the radiosondes (128 out of 134) were launched during daytime. Hence, a potential difference between day and night launches was difficult to investigate in this study.
Figure 3 shows examples of the T profiles from the three GPSRO retrievals and a radiosonde. Two COSMIC GPSRO events on December 17, 2011, at 22:35:38 UTC (106.24°E, 5.23°S) and 20:18:51 UTC (106.23°E, 5.88°S) occurred nearby the single radiosonde in Cengkareng (Indonesia) at 23:31:00 UTC (106.68°E, 6.12°S). Both atmPrf2013 and atmPrf2010 show smooth data near the tropopause (left profiles), while rishfsi2013 shows detailed temperature variations consistent with the radiosonde result. On the other hand, atmPrf2010 agrees well with rishfsi2013 below 17 km (right profiles), indicating that the sewing height between the GO and WO methods is at 17 km. It is noteworthy that the height resolution of atmPrf2010 near the tropopause depends on the sewing altitude between GO and WO. In contrast, atmPrf2013 always shows a smooth profile up to 20 km. Because rishfsi2013 applies the FSI method up to 30 km, these data provide details of the T fluctuations in the entire height range.
We defined CPT as the coldest level in the 14 to 20km altitude. If more than two CPTs were identified, then the CPT height was determined by averaging all the corresponding altitudes. Following the WMO definition, we defined the LRT at the lowest level where the temperature lapse rate (−dT/dz) decreases to 2 K/km and the average of the lapse rate between this and higher levels within 2 km does not exceed 2 K/km. We applied the fivepoint center differential formula to derive dT/dz. The mean and standard deviation of CPT and LRT from all COSMIC profiles are 189.5 K ± 1.65 K at 17.2 km ± 0.3 km and 191.2 K ± 1.55 K at 16.4 km ± 0.3 km, respectively.
Results and discussion
We investigated the characteristics of the three retrievals of COSMIC GPSRO, concentrating on the temperature variations in the UTLS region in the tropics by comparing the three retrievals and subsequently validating them using simultaneous radiosonde data.
Comparison among the three retrievals
Figure 4 plots the mean and standard deviation of the difference of T (∆T) among rishfsi2013, atmPrf2013 and atmPrf2010 at 14 to 21km altitudes. We limited the lowest height at 14 km, because the dry temperature may become unrealistic due to the effects of the high humidity in the tropics. We also did not show the comparison above 20 km, because the focus of this study is the temperature variations in the UTLS region centered by the tropopause. Below 19 km, the mean ∆T between atmPrf2013 and atmPrf2010 is very small. Above 19 km, it is 0.1 K, at most. The interval of the standard deviation divided by the square root of the number of profiles, which is defined as the standard error of the mean from all ∆T, ranges between 3.7 × 10^{−3} and 9.8 × 10^{−3} K. Although the standard deviation below 16 km or above 19.5 km ranges 0.3–0.5 K, it is larger at 16–19 km around CPT.
The other two combinations (rishfsi2013–atmPrf2013 and rishfsi2013–atmPrf2010) show similar differences (Fig. 4). The mean ∆T at 14 km is −0.3 K, but gradually decreases with height; above 18.5 km, it becomes positive. We applied smoothing over 500 m to the rishfsi2013 profiles and calculated the mean and standard deviation of ∆T between the smoothed rishfsi2013 and atmPrf2013 (figure is not shown). The mean ∆T shows smaller values (about 0.1 K) than the mean ∆T for the rishfsi2013–atmPrf2013 comparison around the tropopause. The standard deviation around the tropopause is reduced from 1.2 to 0.8 K. Hence, the smoothing process to the rishfsi2013 may affect the mean ∆T around the tropopause only (~0.1 K), and it reduces the standard deviation.
We extended the comparison among the three GPSRO datasets up to 30km altitude considering the top height of WO used in rishfsi2013 is 30 km (figure is not shown). The atmPrf2013 became gradually warmer than atmprf2010, and the difference became as large as 0.5 K at 30 km. The rishfsi2013 is warmer than both atmPrf2013 and atmPrf2010 by about 0.1–0.3 K and 0.2–0.5 K at 20–30 km, respectively. The difference above 20 km was in general larger for atmprf2010 than atmprf2013 by a factor of about 2. The standard deviation from all combinations of GPSRO datasets ranged 0.5–0.8 K at 20 km, and it increased to 1.0–1.5 K above 25 km. The difference between the rishfsi2013 and the two CDAAC versions may be related to the differences in the raw and smoothed atmospheric excess phase.
Considering the increase in the standard deviation of ∆T around the tropopause in Fig. 4, we investigated ∆T in more detail at both CPT and LRT. Figure 5a shows the daily mean time series of the difference of CPT temperature (∆T _{CPT}) and the difference of the corresponding altitude (∆H _{CPT}). Table 2 shows the mean, median and standard deviation of ∆T _{CPT} and ∆H _{CPT}. The mean ∆T _{CPT} is negative for rishfsi2013–atmPrf2013 and rishfsi2013–atmPrf2010, indicating that T _{CPT} of rishfsi2013 is generally colder than both atmPrf2013 and atmPrf2010. After January 2012, the daily mean ∆T _{CPT}’s of both rishfsi2013–atmPrf2013 and rishfsi2013–atmPrf2010 display similar variations. Consequently, ∆T _{CPT} for atmPrf2013–atmPrf2010 is close to zero. ∆H _{CPT}’s for the three pairs in Fig. 5b show short irregular variations. ∆H _{CPT} between the RISH and CDAAC datasets shows a small positive value. However, this result may be insignificant because the difference is within the standard deviation. Therefore, all three datasets are consistent when determining H _{CPT}.
Figure 6 and Table 3 describe the time series of the daily mean ∆T _{LRT} and ∆H _{LRT} as well as their statistical results. The magnitudes of the mean ∆T _{LRT} for all comparisons are less than 0.6 K, and the standard deviations do not exceed 0.3 K. The mean ∆H _{LRT} between rishfsi2013 and atmPrf2013 or atmPrf2010 shows a negative value, whereas the mean ∆H _{LRT} between atmPrf2013 and atmPrf2010 is slightly positive. The RISH and CDAAC data produce different behaviors between the temperature and the altitude of CPT and LRT. The mean T _{CPT} of rishfsi2013 is colder than the two CDAAC products. On the other hand, the mean T _{LRT} shows the opposite relation. Although the height differences of CPT and LRT are nearly zero, their signs are positive for CPT and negative for LRT.
We are interested in differences of the raw bending angles between the RISH and the CDAAC products. A comparison of the optimized bending angles among the three retrievals shows that rishfsi2013 has higher vertical resolution around the tropopause (figure is not shown). These variations seem to be attributed to the background atmospheric model used to optimize the bending angles or the difference in the vertical resolution due to sewing and smoothing. In the next subsection, we compare these GPSRO data with simultaneous radiosondes to ascertain which products are closer to the real atmosphere.
Comparison between three COSMIC GPSRO datasets and Radiosondes
Because radiosondes are considered as the standard measurement method of temperature, they are compared with the GPSRO profiles. Figure 7 shows the mean, the standard error of the mean and the standard deviation of ∆T between the three GPSRO retrievals and the collocated radiosonde profiles. In the entire height range, the average profiles of ∆T show similar variations, and the standard error of the mean ranges between 0.06 and 0.18 K. The rishfsi2013 agrees well with the radiosonde at altitudes of 14–16 km, except at 15 km. On the other hand, both atmPrf2013 and atmPrf2010 have positive biases of about 0.2 K. The three GPSRO results have negative biases of 0.3–0.8 K above LRT, which exists at 16.4 km.
The standard deviation is 1–1.5 K in the troposphere, but increases to about 2 K above the tropopause. The accuracy of temperature measurement with a radiosonde was conducted in the last decades (e.g., Kitchen 1989). Sofieva et al. (2008) showed that the standard deviation of temperature difference among radiosonde profiles obtained within 3 h and 200 km separation was 1 K at 15 to 20km altitudes. Our result is consistent with this evaluation. Larger deviations in the lower stratosphere are attributed to the effects of the spatial and the temporal variabilities caused by atmospheric waves (ScherllinPirscher et al. 2017; Suzuki et al. 2013).
We compared the atmPrf2013 with the radiosonde results after the 500 m smoothing (figure is not shown). The two comparisons, (atmPrf2013–radiosonde) and (atmPrf2013smoothed_radiosonde), are nearly overlapping, and the difference between the two mean ∆T profiles ranges from −0.1 to 0.1 K. The standard deviation becomes smaller as 0.2 K above the tropopause. Therefore, the smoothing process to the high vertical resolution T profiles seems to reduce only the standard deviation.
Figure 8 plots the time variations of ∆T _{CPT} and ∆H _{CPT}, while their statistical results are summarized in Table 4. The mean ∆T _{CPT} ranges within ±0.4 K, and its standard deviation is about 1.6 K. Although rishfsi2013 shows a colder temperature than the radiosonde, the CDAAC datasets are warmer. The mean of ∆H _{CPT} for all datasets is less than 0.1 km, and the standard deviation is about 0.5 km, which is consistent with the radiosondes.
The T profiles with the radiosondes and the FSI retrieval have good vertical resolutions, suggesting that they are sensitive to small vertical scale T fluctuations. Although the mean ∆T _{CPT} for rishfsi2013 is negative (Table 4), both atmprf2010 and atmprf2013 are positive, indicating that they are warmer than T_{CPT} by the radiosondes. It is reasonable that atmPrf2013 shows a positive ∆T _{CPT} because height smoothing reduces the sharp temperature fluctuations. Since atmPrf2010 is retrieved by either FSI or GO, depending on the signal condition, the mean ∆T _{CPT} becomes positive due to the mixing of the lowresolution GO results with the sewing altitude below CPT. It should be noted that the mean ∆T _{CPT} of atmPrf2010 is smaller than atmPrf2013, indicating that the former sometimes provides a sharp temperature around CPT (see Fig. 3).
Large T perturbations around the tropopause produce multiple minima in the T profile, which are defined as a multiple tropopause. The small difference of T at these minima can impact the determination of CPT and the corresponding altitude, H _{CPT}. The left profiles in Fig. 3 show a typical example; the CPT is defined at 16 km with the radiosonde, but is detected at 17.1 km with rishfsi2013, leading to a large ∆H _{CPT}, as shown in Fig. 8b. On the other hand, the example in the right profiles in Fig. 3 shows consistency in determining CPT by the three GPSRO retrievals and the radiosonde. Therefore, the large standard deviation of ∆H _{CPT} (0.5 km) may be due to the effects of a multiple tropopause when determining the coldest minimum.
The variation of ∆T _{LRT} is more complicated (Fig. 9). Table 5 describes the negative mean ∆T _{LRT} ranging from −0.41 to −0.69 K with a standard deviation of about 2.9 K. The ∆H _{LRT} is positive, indicating that the GPSRO determined the LRT at altitudes 0.1–0.2 km higher than the radiosonde.
We investigated the correlation between ∆T _{CPT} and ∆H _{CPT} in the scatter diagram in Fig. 10 (top panels). Both variables realize the zero mean and the median, but the distribution shows an uncorrelated pattern.
Figure 11 shows an example of the double tropopause near Surabaya, Indonesia, on October 4, 2011. The radiosonde was launched at 23:40:00 UTC (112.78°E, 7.37°S), and the GPSRO profiles were retrieved at 20:34:59 UTC (111.03°E, 7.11°S). Up to 18.5 km, rishfsi2013 and atmPrf2010 agree well, while atmPrf2013 displays a smooth profile. The temperature at 16–17.5 km shows a large difference, which seems to be attributed to the time and the spatial differences in the temperature field. In some cases in Fig. 10, ∆H _{CPT} becomes as large as ±2 km, but the corresponding ∆T _{CPT} is small. The left panel in Fig. 11 shows that the radiosonde identifies the colder T _{CPT} at a lower altitude than all the GPSRO datasets due to the small difference in the individual measurements of T _{CPT}. This example indicates that the determination of CPT as the coldest level from the profiles with different height resolutions may produce statistical differences when the multiple tropopause structures frequently appear.
The scatter diagram between ∆T _{LRT} and ∆H _{LRT} in Fig. 10 (bottom panels) shows a linear correlation. Because the LRT is mostly located below the CPT in the equatorial UTLS, the negative (positive) ∆T _{LRT} is associated with the positive (negative) ∆H _{LRT}, resulting in a negative linear tendency. For rishfsi2013 in the leftmost panel, both positive and negative ∆T _{LRT} are equally distributed. However, an asymmetric distribution is found for atmPrf2010 and atmPrf2013, which have smaller ranges of positive deviations of ∆T _{LRT}. The mean value of ∆H _{LRT} in Table 5 is nearly zero for rishfsi2013, but is as positive as 0.28 and 0.21 km for atmPrf2013 and atmPrf2010, respectively.
The right panel in Fig. 11 shows the Brunt–Väisälä frequency squared (N ^{2}). For the radiosonde profile, N ^{2} exceeds the threshold for LRT at 15.2 km, and the mean stability in the overlying 2km region satisfies the WMO definition. Consequently, LRT is identified at this altitude. The LRT with rishfsi2013 or atmPrf2010 is similarly determined at 15.6 km. The asymptotic structure of N ^{2} in Fig. 11 suggests that the actual LRT of these profiles is located around 16–16.5 km, but the enhanced stability at much lower altitudes affects the determination of LRT. On the other hand, atmPrf2013 shows a smooth N ^{2} profile without an N ^{2} enhancement at altitudes of 15–16 km. atmPrf2013 identifies the LRT at 16.2 km. We noticed that a profile with a higher vertical resolution is sensitive to a small perturbation of N ^{2}, which can influence the determination of the appropriate LRT. The smooth profile in atmPrf2013 captures a reliable LRT.
Discussion
In some cases, the T profiles show a bias in the UTLS region between atmPrf2010 and atmPrf2013. A typical example is shown in Fig. 12 where the GPSRO profiles were retrieved at 13:54:58 UTC (118.81ºE, 6.30ºS) and the radiosonde was launched in Makassar, Indonesia, at 11:30:00 UTC (119.53ºE, 5.06ºS) on October 19, 2011. The atmPrf2010 profile is warmer than the atmPrf2013 profile by about 2–3 K in the entire height range. CPT is located at 16.5–17.0 km for all the profiles (Fig. 12). Below CPT, the T profiles from both rishfsi2013 and atmPrf2013 agree well with the radiosonde. However, the radiosonde profile approaches the atmPrf2010 profile above CPT up to about 18.5 km.
The altitudes of CPT and LRT are nearly equal for the radiosonde and atmPrf2013. The LRT altitudes for atmPrf2010 and rishfsi2013 are found around 15.5 km, which is about 1.5 km lower than the other two profiles. The FSI retrieval was applied to both rishfsi2013 and atmPrf2010, where the sewing height was 19.5 km for atmPrf2010. Between these two retrievals, the dT/dz profile in the right panel of Fig. 12 agrees very well at 15 to 19.5km altitudes, suggesting that they capture the T perturbations identically. However, the T profiles show a constant bias between rishfsi2013 and atmPrf2010.
This discrepancy may be caused by the difference in the extrapolation height of the ionospheric correction or the difference in the bending angle optimization (Sokolovskiy: personal communication, 2017). We found similar cases in about 10% of the 134 collocated profiles. The differences between the two CDAAC products shown in Fig. 12 may be an unusual case because the statistical results in Fig. 7 show a very good agreement between atmPrf2010 and atmPrf2013.
The example in Fig. 11 indicates that the two versions of the CDAAC products have some discrepancies when determining the altitudes of CPT and LRT, resulting in inconsistencies of the corresponding CPT and LRT temperatures. Consequently, statistical analysis of the UTLS parameters should take such differences into account. The background model of climatology utilized in retrieving GPSRO profiles and the assumptions of the linear combination between L1 and L2 bending angles may control the apparent diversity between the three GPSRO profiles in Fig. 12 (Schreiner et al. 2011; Zeng et al. 2016).
We examined the T fluctuations retrieved by the three GPSRO datasets from individual comparisons (Fig. 12). The power spectral density of dT/dz (in K^{2}/km) is calculated as a function of the wavenumber (in cycle per kilometer) (Fig. 13). It should be noted that the first point in the spectra is affected by the Hanning window. At large wave numbers between 1.8 and 4.4 cycle/km, rishfsi2013, atmPrf2010 and the radiosonde show a large spectral density (i.e., 0.56–0.23 km in the corresponding wavelength) compared to the spectrum for atmPrf2013. This result confirms the smoothing of the atmPrf2013 profiles for wavelengths shorter than about 500 m, while atmPrf2010 and rishfsi2013 provide T profiles with the similar height resolutions as the radiosonde.
Conclusions
The dry atmospheric temperature (T) profiles were retrieved using both GO and WO at CDAAC, which are called atmPrf2010 and atmPrf2013, as well as another dataset at RISH named rishfsi2013. We investigated the T profiles collected from October 1, 2011, to March 31, 2012, when CINDYDYNAMO 2011 was conducted.
Firstly, we compared the three GPSRO retrievals, focusing on the T differences (∆T) in the tropical UTLS. The results of combining these three datasets, atmPrf2013–atmPrf2010, rishfsi2013–atmPrf2013 and rishfsi2013–atmPrf2010, are summarized below:

1.
The mean ∆T between atmPrf2013 and atmPrf2010 is nearly zero, while rishfsi2013 has a slightly negative (positive) bias below (above) the tropopause. All ∆T describe the large standard deviation around CPT.

2.
The mean values of ∆T _{CPT} and ∆T _{LRT} in all comparisons are less than 0.8 and 0.6 K, respectively, with a standard deviation <0.3 K. The rishfsi2013 results indicate a colder (higher) T _{CPT} (H _{CPT}) and warmer (lower) T _{LRT} (H _{LRT}).

3.
The discrepancies appear to be due to the difference in the background atmospheric models used for the ionospheric calibration or the difference in the vertical resolution due to sewing and smoothing.
Secondly, we further analyzed ∆T between the three GPSRO retrievals and 134 radiosonde profiles that are within 200 km and ±3 h.

4.
Below LRT, rishfsi2013 agrees with the radiosonde, while both atmPrf2013 and atmPrf2010 indicate a positive bias of 0.2 K. All GPSRO datasets have a negative bias of 1.0–1.5 K with a standard deviation of about 2 K in the lower stratosphere, which may be attributed to the spatial and temporal variations by the atmospheric waves.

5.
The mean values of ∆T _{CPT} and ∆H _{CPT} indicate that the three retrievals are consistent with the radiosondes. T _{CPT} of rishfsi2013 is colder, while that of the CDAAC profiles is warmer than the radiosonde within ±0.4 K. The different height resolutions in each retrieval influence the determination of CPT when a multiple tropopause appears.

6.
The scatter diagram between ∆T _{LRT} and ∆H _{LRT} indicates a negative linear tendency. The superior vertical resolution in the radiosonde, rishfsi2013 and atmPrf2010 when the sewing height is detected above the tropopause is sensitive to smallscale dT/dz perturbations. These fluctuations affect the determination of a reliable LRT; LRT is detected at a lower altitude and a warmer temperature. The smooth atmPrf2013 is more suitable to define LRT.

7.
The vertical wave number spectral density of dT/dz is consistent between the rishfsi2013 and the radiosonde in a vertical wave number range larger than 2 cycle/km (wavelength < 0.5 km). However, the spectral density for atmPrf2013 is much smaller due to smoothing.
The statistical results of CPT and LRT agreed relatively well among the three retrievals, although individual profiles sometimes showed considerable discrepancies in the CPT and LRT altitudes due to the multiple tropopause and the height structure of dT/dz. It is noteworthy that the atmPrf2010 dataset is a mixture of high and low vertical resolutions in the UTLS, depending on the sewing height for individual profiles. Therefore, one may need to pay attention when analyzing the details of tropopause structure related to the dT/dz, such as the tropopause sharpness (Kim and Son 2012). The T profiles of atmPrf2013 are useful for climatological analysis of UTLS, although they may not capture the fine structure of the tropopause because of the smoothing over 500 m.
Comparison of rishfsi2013 with the CDAAC products and radiosondes confirm its validity. The T profiles by rishfsi2013 provide a superior vertical resolution as good as 0.1 km throughout the UTLS region. Thus, rishfsi2013 is useful for studies on the T fluctuations around the tropopause as well as the behavior of the atmospheric gravity waves in the stratosphere. We encourage the international scientific communities to utilize rishfsi2013, which is now available via the IUGONET system (http://www.iugonet.org).
Abbreviations
 COSMIC:

Constellation Observing System for Meteorology, Ionosphere, and Climate
 CDAAC:

COSMIC data analysis and archive center
 IUGONET:

Interuniversity upper atmosphere global observation NETwork
 CPT:

coldpoint tropopause
 LRT:

lapse rate tropopause
References
Alexander SP, Tsuda T, Kawatani Y, Takahashi M (2008) Global distribution of atmospheric waves in the equatorial upper troposphere and lower stratosphere region: COSMIC observations of wave mean flow interactions. J Geophys Res 113:D24115. doi:10.1029/2008JD010039
Anthes RA (2011) Exploring earth’s atmosphere with radio occultation: contributions to weather, climate and space weather. Atmos Meas Tech 4:1077–1103. doi:10.5194/amt410772011
Anthes RA, Ector D, Hunt DC, Kuo YH, Rocken C, Schreiner WS, Sokolovskiy SV, Syndergaard S, Wee TK, Zeng Z, Bernhardt PA, Dymond KF, Chen Y, Liu H, Manning K, Randel WJ, Trenberth KE, Cucurull L, Healy SB, Ho SP, McCormick C, Meehan TK, Thompson DC, Yen NL (2008) The COSMIC/FORMOSAT3 mission: early results. B Am Meteorol Soc 89:313–333
Das U, Pan CJ (2014) Validation of FORMOSAT3/COSMIC level 2 “atmPrf” global temperature data in the stratosphere. Atmos Meas Tech 7:731–742. doi:10.5194/amt77312014
Fueglistaler SA, Dessler E, Dunkerton TJ, Folkins I, Fu Q, Mote PW (2009) The tropical tropopause layer. Rev Geophys 47:RG1004. doi:10.1029/2008RG000267
Gettelman A, Hoor P, Pan LL, Randel WJ, Hegglin MI, Birner T (2011) The extratropical upper troposphere and lower stratosphere. Rev Geophys 49:RG3003. doi:10.1029/2011RG0003555
Gorbunov ME (2002) Canonical transform method for processing radio occultation data in the lower troposphere. Radio Sci 37(5):1076. doi:10.1029/2000RS002592
Gorbunov ME, Lauritsen KB (2004) Analysis of wave fields by Fourier integral operators and their application for radio occultations. Radio Sci 39:RS4010. doi:10.1029/2003RS002971
Gubenko VN, Pavelyev AG, Salimzyanov RR, Pavelyev AA (2011) Reconstruction of internal gravity wave parameters from radio occultation retrievals of vertical temperature profiles in the earth’s atmosphere. Atmos Meas Tech 4:2153–2162. doi:10.5194/amt421532011
Jensen AS, Lohmann MS, Benzon H, Nielsen AS (2003) Full spectrum inversion of radio occultation signals. Radio Sci 38(3):1040. doi:10.1029/2002RS002763
Jensen AS, Lohmann MS, Nielsen AS, Benzon H (2004) Geometrical optics phase matching of radio occultation signals. Radio Sci 39:RS3009. doi:10.1029/2003RS002899
Kim J, Son SW (2012) Tropical coldpoint tropopause: climatology, seasonal cycle and intraseasonal variability derived from COSMIC GPS radio occultation measurements. J Clim 25:5343–5360. doi:10.1175/JCLID1100554.1
Kitchen M (1989) Representativeness errors for radiosonde observations. QJR Meteorol Soc 115:673–700
Kuo YH, Wee TK, Sokolovskiy S, Rocken C, Schreiner W, Hunt D, Anthes RA (2004) Inversion and error estimation of GPS radio occultation data. J Meteorol Soc Jpn 82:507–531
Kuo YH, Schreiner WS, Wang J, Rossiter DL, Zhang Y (2005) Comparison of GPS radio occultation soundings with radiosondes. Geophys Res Lett 32:L05817. doi:10.1029/2004GL021443
Kursinski ER, Hajj GA, Schofield JT, Linfield RP, Hardy KR (1997) Observing earth’s atmosphere with radio occultation measurements using the global positioning system. J Geophys Res 102:23429–23465. doi:10.1029/97JD01569
Ladstädter F, Steiner AK, Schwärz M, Kirchengast G (2015) Climate intercomparison of GPS radio occultation, RS 90/92 radiosondes and GRUAN from 2002 to 2013. Atmos Meas Tech 8:1819–1834. doi:10.5194/amt818192015
Melbourne WG (2004) Radio occultations using earth satellites. Wiley, New Jersey
ScherllinPirscher B, Kirchengast G, Steiner AK, Kuo YH, Foelsche U (2011) Quantifying uncertainty in climatological fields from GPS radio occultation: an empiricalanalytical error model. Atmos Meas Tech 4:2019–2034. doi:10.5194/amt420192011
ScherllinPirscher B, Randel WJ, Kim J (2017) Tropical temperature variability and Kelvinwave activity in the UTLS from GPSRO measurements. Atmos Chem Phys 17:793–806. doi:10.5194/acp177932017
Schreiner W, Sokolovskiy S, Hunt D, Rocken C, Kuo YH (2011) Analysis of GPS radio occultation data from the FORMOSAT3/COSMIC and Metop/GRAS missions at CDAAC. Atmos Meas Tech 4:2255–2272. doi:10.5194/amt422552011
Sofieva VF, Dalaudier FR, Kiwi R, Kyro E (2008) On the variability of temperature profiles in the stratosphere: implications for validation. Geophys Res Lett 35:L23808. doi:10.1029/2008GL035539
Sokolovskiy S, Schreiner W, Rocken C, Hunt D (2009) Optimal noise filtering for the ionospheric correction of GPS radio occultation signals. J Atmos Ocean Tech 26:1398–1403
Sokolovskiy S, Rocken C, Schreiner W, Hunt D (2010) On the uncertainty of radio occultation inversions in the lower troposphere. J Geophys Res 115:D22111. doi:10.1029/2010JD014058
Sokolovskiy SV, Schreiner WS, Zeng Z, Hunt DC, Kuo YH, Meehan TK, Stecheson TW, Mannucci AJ, Ao CO (2014) Use of the L2C signal for inversions of GPS radio occultation data in the neutral atmosphere. GPS Solut 18:405–416. doi:10.1007/s102910130340x
Steiner AK, Lackner BC, Ladstädter F, ScherllinPirscher B, Foelsche U, Kirchengast G (2011) GPS radio occultation for climate monitoring and change detection. Radio Sci 46:RS0D24. doi:10.1029/2010RS004614
Sun B, Reale A, Seidel DJ, Hunt DC (2010) Comparing radiosonde and COSMIC atmospheric profile data to quantify differences among radiosonde types and the effects of imperfect collocation on comparison statistics. J Geophys Res 115:D23104. doi:10.1029/2010JG014457
Suzuki J, Fujiwara M, Nishizawa T, Shirooka R, Yoneyama K, Katsumata M, Matsui I, Sugimoto N (2013) Theoccurrence of cirrus clouds associated with eastward propagating equatorial n = 0 inertiogravity and Kelvin waves in November 2011 during the CINDY2011/DYNAMO campaign. J Geophys Res 118:12941–12947. doi:10.1002/2013JD019960
Tsuda T, Lin X, Hayashi H, Noersomadi N (2011) Analysis of vertical wave number spectrum of atmospheric gravity waves in the stratosphere using COSMIC GPS radio occultation data. Atmos Meas Tech 4:1627–1636. doi:10.5194/amt416272011
Wang BR, Liu XY, Wang JK (2013) Assessment of COSMIC radio occultation retrieval product using global radiosonde data. Atmos Meas Tech 6:1073–1083. doi:10.5194/amt610732013
Ware R, Exner M, Feng D, Gorbunov M, Hardy K, Herman B, Kuo Y, Meehan T, Melbourne W, Rocken C, Schreiner W, Sokolovskiy S, Solheim F, Zou AR, Businger S, Trenbeth K (1996) GPS sounding of the atmosphere from low Earth orbit—preliminary results. Bull Am Meteorol Soc 77:19–40
Xu X, Gao P, Zhang X (2014) Global multiple tropopause features derived from COSMIC radio occultation data during 2007 to 2012. J Geophys Res Atmos 119:8515–8534. doi:10.1002/2014JD021620
Yoneyama K, Zhang C, Long CN (2013) Tracking pulses of the Madden–Julian oscillation. Bull Am Meteorol Soc. doi:10.1175/bamsd1200157.1
Zeng Z, Sokolovskiy S, Schreiner W, Hunt D, Lin J, Kuo YH (2016) Ionospheric correction of GPS radio occultation data in the troposphere. Atmos Meas Tech 9:335–346. doi:10.5194/amt93352016
Zhang C, Gottschalck J, Maloney ED, Moncrieff MW, Vitart F, Waliser DE, Wang B, Wheeler MC (2013) Cracking the MJO nut. Geophys Res Lett 40:1223–1230. doi:10.1002/grl.50244
Authors’ contributions
The author N analyzed the data, created the figures and wrote the paper. TT contributed to the manuscript in general. Both authors read and approved the final manuscript.
Acknowledgements
We acknowledge CDAAC for the use of the COSMIC GPSRO datasets. We are grateful to Dr. S. Sokolovskiy and Dr. Z. Zeng for their valuable suggestions. We also thank Dr. Atsuki Shinbori for registering the RISH COSMIC GPSRO dataset in the IUGONET system. This work was partially supported by JSPS KAKENHI Grant Number JP15H03724. One of the authors (N) received a scholarship for his Ph.D. from the Program of Research and Innovation in Science and Technology (RISETPro), Ministry of Research, Technology and Higher Education (RISTEKDIKTI) of Indonesia.
Competing interests
The authors declare that they have no competing interests.
Availability of data and materials
The atmPrf version 2010.2640 (atmPrf2010) and 2013.3520 (atmPrf2013) are available at the CDAAC (http://www.cosmic.ucar.edu). The rishfsi2013 dataset can be found via http://search.iugonet.org/list.jsp (IUGONET), which is formatted in the NetCDF file named as RISHANA_YYYY.DDD.nc, where YYYY and DDD are the year and Julian day, respectively. The radiosonde data from the CINDYDYNAMO 2011 are provided by the Japan Agency for MarineEarth Science and Technology (JAMSTEC) (http://www.jamstec.go.jp/iorgc/cindy/) and Earth Observing Laboratory (EOL) of UCAR (https://www.eol.ucar.edu/field_projects/dynamo).
Funding
This work was partially supported by JSPS KAKENHI Grant Number JP15H03724 and the RISH Kyoto University (Mission 53).
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Noersomadi, Tsuda, T. Comparison of three retrievals of COSMIC GPS radio occultation results in the tropical upper troposphere and lower stratosphere. Earth Planets Space 69, 125 (2017). https://doi.org/10.1186/s4062301707107
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DOI: https://doi.org/10.1186/s4062301707107