Japanese


Estimation of rainfall rate with TRMM Microwave Imager TMI
(Comparison with Precipitation Radar PR)(Results of Mr. Ikai)

To study the global water cycle and mechanisms of the variation, continuous global observations of rainfall activities with satellites are important. Visible or IR observations, like observations with VIRS etc., can only surface temperature of the cloud top (that is, the height of clouds) and the characteristics of clouds and the rainfall rate is calibrated according to the relation of observed parameters and rainfall rate. However, TMI and PR can directly observe precipitation through clouds by microwaves. In this point, both of TMI and PR are of great advantege.
TMI detects microwaves radiated by the precipitation passively at 5 frequencies. PR sends out microwaves from an antenna actively and detects the backscattered radiowaves by the precipitation. 3 dimensional Rainfall rate can be estimated from their microwave measurements (power and time lag). Though TMI can observe more than three times larger area than that obverved with PR, TMI has large uncertainty over the land because of the large background emitted by the land. That is to say PR can observe the rainfall rate exactly over any surface conditions although it can observe only a narrow area.
Our objectives is to study when, where, how the TMI rainfall rate and PR rainfall rate are different and to contribute to the improvement of estimation of TMI rainfall rate by searching the origins of the differences.

It is well-known that TMI rainfall rate is 24% larger than PR rainfall rate in the zonal average over tropical region at the algorithm version 5 (Kummerow et al. 2000). We compared TMI and PR rainfall rates over the ocean, land and coast, in order to identify the origins of this difference. TMI rainfall rate is larger than PR rainfall rate over tropic or midlatitude summer ocean. On the contrary, PR rainfall rate is larger than PR over the midlatitude winter ocean. Over the midlatitude winter land, PR rainfall rate is twice larger than TMI. We investigated the vertical profile of TMI and PR rainfall rate, TMI freezing height, PR bright band height, PR storm height, TMI vertical and horizontal brightness temperature.
In this web page, we show the results over tha ocean written in a paper of Ikai & Nakamura (2003).
In this analysis, the calibrated brightness temperature of TMI (TMI-1B11), rainfall rate of TMI (TMI-2A12), rainfall rate of PR (PR-2A25), path integrated attenuation (PIA) of PR (PR-2A25) and gridded statistical three months averaged rainfall rate of PR (PR-3A25). Toolkit is version 5. We produced global data sets by averaging in 0.5 degrees (longitude) by 0.5 degrees (latitude) grid boxes. Three months from December 1998 to February 1999 (hereafter called DJF1999) and from June 1999 to August 1999 (hereafter called JJA1999) are used to see the seasonal change of the characteristics.
We found three plausible reasons for these differences. One is a problem in the freezing level assumption in the TMI algorithm for midlatitude region in the winter. That results in underestim ation of TMI-derived rain rates. Second is inadequate Z-R or k-R relationships f or convective and stratiform types in the PR algorithm. Third is wrong interpret ation of rain layer when freezing level is low and the rain type is convective. The strong bright band echo seems to be interpreted as rain and too strong rain attenuation correction is applied. This results in too strong rain rate by PR al gorithm.

Results

1. Comparison of TMI with PR

Global comparison of rain rates at surface level
we compared the three-month averaged TMI-rain with PR-rain on a global scale. Figure 1 shows global maps of the ratio of PR-rain to TMI-rain averaged for DJF1999 and JJA1999. In this figure, the ratios were plotted except for the grids where either the three-month averaged TMI-rain or PR-rain was below 0.05 mm/h. This is because TMI rain rate can easily become zero due to the TMI sensitivity while the minimum detectable rain rate of PR is about 0.5 mm/h. Though the very weak rain is generally negligible for total rain and ratios, elimination of very weak rain might have significant effect for weak rain regions. Some characteristics which could be noticed from Fig. 1 are as follows:
a) Generally TMI-rain is greater than PR-rain.
b) PR-rain is greater than TMI-rain in the north Atlantic and western part of the Pacific Ocean north of 30 deg N for DJF1999, and also PR-rain is also greater than TMI-rain in western part of Pacific Ocean south of 30 deg S for JJA1999.
c) TMI-rain is significantly greater than PR-rain in western part of the north Pacific Ocean for JJA1999, and south of 30 deg S for DJF1999 in the Pacific Ocean. TMI-rain is also significantly greater than PR-rain in tropical regions of central to the eastern Pacific Ocean for both season,.
d) PR-rain is greater than TMI-rain in mountainous regions over land, for example , Rocky, Andes, and Himalayan Mountain Ranges.

2. Case Study

To investigate these characteristics, we selected five typical regions where either of two characteristics appears clearly. We additionally selected western part of tropical Pacific Ocean as a reference region where TMI-rain was generally greater than PR-rain, and these regions are shown in a lower panel of Fig. 1. We show results of events over ocean, east of Japan in Feb. 11th on 1999 (MWNP) and over ocean, east of Philippine in June 13th on 1999 (TWP). In those cases rainfall area extended horizontally over 40 km in along track direction, and a heavy convective rainfall area existed. Those case s were selected for the reason that the wide raining area existed in the narrow PR swath. Figure 2-1 shows scatterplots of TMI-rain versus PR-rain. In case of TWP, TMI-rain is greater than PR-rain by about 100%, and the slope is correspondingly 0.49. In contrast to case of winter MWNP, PR-rain is greater than TMI-rain by about 63%, and the slope is 1.64. This characteristic is similar to those in corresponding regions mentioned in the previous section on the global characteristics. We can also notice that the tendency of the overestimation of PR-rain is remarkable in grids where the convective rainfall defined by the PR-2A25 algorithm spreads widely, which are plotted by open circles in this figure. This indicates the problems are due to a relations between radar refrectivity factor and the rainfall rate, that is, Z-R and/or a relations between radar refrectivity factor and attenuation coefficient of rainfall, that is, k-Z, and/or a method for a correction of an attenuation for the precipitation, etc.
We compared the brightness temperature directly measured in TMI-10GHz vertical polarization channel (TMI-10GHzV-BT) with path integrated attenuation (PIA) derived from PR. The frequency of TMI-10GHzV is close to that of PR (13.8 GHz). The increase of TMI-10GHz-BT due to rain emission is nearly proportional to the path attenuation. The linearity also results in a small beam filling effect which is caused by the non-linear relationship between excess brightness temperature and rain rate. Because linear PIA (absolute value instead of value in dB) also relates nearly linearly to column total rain amount along the radar beam path, we converted PIA in dB to linear value for comparison. Figure 2-2 shows the scatterplots of TMI-10GHzV-BT versus linear PIA in the same cases in Fig. 2-1. In both cases, TMI-10GHzV-BT is strongly related with linear PIA in contrast to the rain rate case. This strongly suggests that generally TMI and PR both measure or estimate the path attenuation correctly regardless of regions and seasons. Though the surface condition affects the brightness temperature, we assumed that it is not crucial for case studies when we are interested only in excess temperatures. Investigating more details, the minimum of linear PIA of about 0.55 in the case of winter MWNP is smaller than in the case of TWP (about 0.65), although excess of TMI-10GHz-BT are almost the same. This indicates the differences of rainfall rates between TMI and PR is caused by their differences on the vertical profiles of the precipitation.

3. Comparison of Vertical rain profiles (effects of TMI 0℃ height)

The fact that the relations between TMI-10GHzV-BT and PIA do not show significant differences suggests that the path-integrated liquid water content from TMI and path-integrated rain should generally be correct and that differences in rain retrieval algorithms in TMI and PR yield the disagreement of rain rates at the surface level. PR can observe directly the vertical rain profile and detect the bright band height (PR-BBH), which is an indicator of freezing height. However, TMI measures only the brightness temperature related with vertical integrated attenuation or water content. Therefore, in estimating the rain rate at surface from brightness temperatures of TMI, the vertical rain profile and freezing level are very important. TMI 2A12 algorithm estimates the freezing height (TMI-FH) by using a lookup table of the brightness temperatures of 19 GHz and 21 GHz and retrieves the vertical profiles of liquid water content etc. Figure 3 shows monthly averaged rain profiles from TMI (TMI-profile) and PR (PR- profile), and the profiles of ratio of TMI-profile to PR-profile (TMI/PR-profile) for the regions shown in Figure 1 except for TCP. These profiles were averaged for January 1999 and July 1999 including no-rain pixels. In these figures, the rain rate at the lowest layer (500 m) of PR-profile almost always corresponds to the near surface rain rate. In the regions of tropical and midlatitude summer except for MCNP where rain amount is very small, TMI-profiles have similar characteristics. There, each freezing level (TMI-FH) is expected between 4 km and 5 km in height and rain rate is decreasing downward slightly below the weak peak at 2 km, although the intensity of rain rate is different. In these regions, PR-profiles are almost uniform below the bright band height (PR-BBH). PR-BBH seems to be between about 4 km and 5 km in height, and is roughly the same as TMI-FH in each region. For these four regions, TMI- and PR-profiles are approximately uniform below PR-BBH, while the ratios are different. This indicates that the shapes of TMI-profiles are similar to those of PR-profiles. In the four midlatitude regions in winter (winter MNA, MWNP, MCNP, and MWSP), TMI -profiles increase rapidly downward from 4.5 km to 2 km and decrease towards surface below 2 km, while PR-profiles gradually increase downward from 4 km to 1.5 km or 2 km. Therefore, for these four regions very large overestimation of TMI (the ratio is at most about 4) between 3 km and 4 km appears. The ratio decreases towards surface rapidly, and represents only a weak overestimation of PR or TMI (the ratio is 0.8 to 1.5) at the surface. These characteristics mean that TMI-2A12 al gorithm distributes the vertically integrated water content into a tall column and the surface water content becomes less. In other words, it is suggested that TMI-2A12 algorithm uses an incorrect estimate of freezing level which is too high for midlatitude regions in winter, and it leads to the underestimation of TMI-rain .
We assessed the estimation of freezing level by TMI (TMI-FH) in comparison with the bright band height from PR by three-month averaged global data. We produced averaged TMI-FH from TMI-1B11 product, and compared TMI-FH with PR-BBH. TMI-FH is higher than PR-BBH by about 300 m to 500 m when TMI-FH or PR-BBH is high. The freezing height estimated from TMI is reasonable in tropical regions. However, when TMI-FH or PR-BBH is low, however, this three-month averaged TMI-FH is higher by about 1500 m to 2000 m than the three-month averaged PR-BBH. This difference is not reasonable. It suggests that TMI algorithm estimates the freezing level too high in the midlatitude winter hemisphere. This disagreement has also been shown in comparisons of freezing level derived from SSM/I. Figure 4 shows global maps of the ratio of TMI-FH to PR-BBH averaged for DJF1999 and JJA1999. The ratio is small (less than 1.2) in tropical and midlatitude summer regions, but it is great (over 1.2) in midlatitude winter regions. TMI-FH/PR-BBH has large values for the regions where PR-rain is greater than TMI-rain as shown in Fig. 1. Next, we compared the ratio of the three-month averaged PR-rain to TMI-rain (PR-rain/TMI-rain) with the ratio of the three-month averaged TMI-FH to PR-BBH (TMI-FH/PR-BBH) for DJF1999 and JJA1999. We show the average and standard deviation of PR-rain/TMI-rain against TMI-FH/PR-BBH of every 0.05 in Fig. 10. Though the standard deviation is large, these figures indicate that the larger TMI-FH/PR-BBH is, the larger PR-rain/TMI-rain is. For example, if TMI-FH is twice the PR-BBH, the surface TMI-rain is underestimated approximately by half compared with PR-rain (PR-rain/TMI-rain is about 0.7 to 1.5) by linear regression method. This suggests that the inadequate estimation of rain height for TMI causes the TMI-rain underestimate. In general, the TMI-rain is smaller than PR-rain in midlatitude regions in winter can be explained by the inadequate freezing level in TMI algorithm.
However, three-month averaged PR-rain is not always greater than TMI-rain in midlatitude winter regions. For example, in winter MCNP and over the midlatitude central south Pacific Ocean TMI-rain is greater than PR-rain. Also in summer MWNP and MWSP and TCP, the overestimation of TMI-rain was greater than other summer and tropical regions. To explain this zonal variation, we considered the Z-R relationship, rain type and attenuation correction in the following sections.

4.Effects of the rain types defined by PR algorithm
(Z-R and k-Z relationships)

PR-rain is derived by the Z-R relationship after attenuation correction depending on the k-Z relationship, while TMI-rain is translated from water content of each layer (R-W relation). The Z-R, k-Z and R-W relationships depend on the drop size distribution (DSD) and terminal velocity of rainfall drops. In PR-2A25 algorithm Z-R and k-Z relationships are changed according to the rain types (convective, stratiform, and others) defined by the vertical and horizontal rainfall structure. Convective type rain has a greater rainrate than stratiform rain by about 1.3 when both have the same radar reflectivity. Furthermore, the difference of rain rate at surface level between the convective and stratiform rain types may be emphasized through attenuation correction using the different k-Z relationship according to rain types. In addition to this, PR-2A25 algorithm uses different profiles of the Z-R relationships according to rain types. The fitting of the k-Z profile and real microphysical one are very important to calculate at tenuation. Therefore, we investigated the relationship between rain type and the PR-rain/TMI-rain. Figure 5-1 and figure 5-2 are the scatterplots showing ratio of convective rainfall amount of PR to total (PR-Ratio-conv) versus PR-rain/TMI-rain in oceanic regions between 5°N and 10°N for DJF1999 and JJA1999 and for the regions between 30°N and 35°N for DJF1999, and between 30°S and 35°S for JJA1999, respectively. We used only grids where both TMI-rain and PR-rain were over 0.1 mm/h. Figure 5-3 and figure 5-4 show the mean and standard deviations of Figs. 5-1 and 5-2, respectively. In the midlatitude winter, the bright band height has a lot of variation and it seems that the characteristics are different for high and low bright band cases. Thus, in midlatitude regions we separated the cases in which bright band height is below 2400 m or above 2400 m. Assuming that the temperature decreases at 6 K/km, the criterion corresponds the sea surface of 15 degrees Celsius. If the Z-R relationship has no difference between convective and stratiform rain, PR algorithm which uses different Z-R relationships for rain types would give biased rain rates. In Figs. 5-1 and 5-2, the solid lines show regression lines. In Figs. 5-3 and 5-4, the solid lines have inclinations of 1.3. if Z-R relationships are not different for convective and stratiform rain types. The these regions in Figs. 5-1, 5-2, 5-3 and 5-4 show that the greater the three-month averaged PR-Ratio-conv is, the larger the three-month averaged PR-rain estimates in comparison with the TMI-rain. In zonal regions of 30°N-35°N and 30°S-35°S when PR-BBH is high, the regression line and the solid line nearly coincide. This coincide may suggest that effect of the difference between convective and stratiform rain type in the PR-2A25 algorithm yield s this disagreement. In the zonal region of 30°N-35°N and 30°S-35°S with high PR-BBHs, and 5°N-10°N, the small difference of slope between regression line and a line with inclination of 1.3 may be due to the effect of attenuation correction of only k-Z relationship. But we can not conclude whether the disagreement is originated by PR or TMI. On the other hand, in the zonal region of 30°N-35°N and 30°S-35°S when PR-BBH is low, the difference of slope between regression line and a line with inclination of 1.3 is more significant. This difference seems not to be explained from the effect of the k-Z relationships on rain types. This difference may be caused by inaccuracy of attenuation correction when PR-BBH is low.

Conclusions

Over the ocean, the general overestimation of TMI-rain was confirmed. PR-rain is greater than TMI-rain in part of the midlatitude winter regions. The discrepancy between TMI-rain and PR-rain also showed regional variation.
The systematic differences in the three-month averaged PR-rain and TMI-rain seem to appear as a combination of the following causes: (1) overestimation of TMI-FH, (2) inadequate Z-R and k-Z relationships for convective and stratiform rain types, (3) inadequate estimation of hydrometeor profiles for convective rain cases. The regions where PR-rain is systematically greater than TMI-rain are over the midlatitude north Atlantic Ocean, the midlatitude western north Pacific Ocean, and the midlatitude western south Pacific Ocean in midlatitude winter. In these regions, both TMI-FH/PR-BBH and PR-Ratio-conv were high and PR-BBH was low. The regions over the midlatitude central north Pacific Ocean and the central south Pacific Ocean had the characteristics of the overestimation of TMI-rain, even though they were located in midlatitude winter hemisphere. Above two regions certainly have the tendency of high TMI-FH/PR-BBH and low PR-Ratio-conv. This fact suggests that the effect of overestimation of TMI-FH was compensated by the effect of small PR-Ratio-conv. Therefore, those two regions have only small TMI-rain overestimation. For the tropical region and midlatitude region in summer hemisphere, the regions where TMI-rain is much greater than PR-rain located in summer midlatitude western north Pacific and central south Pacific Ocean and the tropical central Pacific Ocean. In these three regions, TMI-FH/PR-BBH did not differ much from TMI-FH/PR-BBH, but PR-Ratio-conv was much smaller than other tropical regions and summer regions. This can be understood by the effect of PR-Ratio-conv. We studied the general characteristics of rain rate derived from TMI-2A12 and PR- 2A25 algorithms. This kind of comparison is very valuable for the development of algorithms for microwave instruments, precipitation radar, and combination of the both onboard future satellites. For example, the microwave imager and the precipitation radar could be the principle sensors in the future Global Precipitation Measuring (GPM) mission. In this study we restricted to oceanic region. Now, this kind of exercise has been performed over land where microwave radiometers do not detect radiation from liquid water directly.
This page is cited from one part of Ikai & Nakamura (2003). Please read this paper if you want to know in detail. Please see Masunaga et al. (2002), Furuzawa(Akimoto) & Nakamura (2005) etc. as the similar paper as this Ikai & Nakamura (2003),


References
Ikai, J. and K. Nakamura, J. Atmos. Oceanic Technol., 20(12), 1709-1726, 2003.
Masunaga, H. et al., J. Applied Meteorology, 41, 849-862, 2002.
Kummerow, C. et al., J. Applied Meteorology, 39, 1965-1982, 2000.
Furuzawa, Akimoto F. and K. Nakamura J. Appl. Meteor., 44(3), 367-383, 2005.