p10.15 structure of mesoscale convective systems … · the polarimetric data of the c-pol radar is...

3
P10.15 STRUCTURE OF MESOSCALE CONVECTIVE SYSTEMS OBSERVED WITH POLARIMETRIC RADAR AND UHF WIND PROFILER DURING THE SOUTH CHINA SEA MONSOON EXPERIMENT (SCSMEX) Pay-Liam Lin*, Tai-Chi Chen Wang, , Tsu-Hsang Liu, Hsin-Hon Lin Department of Atmospheric Sciences National Central University, Chung-Li 320, Taiwan 1. Introduction The NCU ISS(Integrated Sounding System) and the BMRC dual-polarimeric doppler radar were deployed in Dongsha island during May 5 to June 25, 1998 for the SCSMEX. The primary goal of this deployment was to measure the mesoscale structure of convective weather system associated with the onset, maintenance and variability of the monsoon over the South China Sea area. The ISS observations provide a detail kinematic and thermodynamic structure change of the monsoon flow. The polarimetric data of the C-Pol radar is very helpful for the understanding of the stratiform and the convective characteristics, and the cloud physics and dynamics of the convective systems. The purpose of this paper is to present a brief overview of the mesoscale weather systems during SCSMEX and investigate the structure and evolution of mesoscale convective systems observed during the onset phase and post-onset phase of SCSMEX. 2. ISS observations The ISS deployed in Dong Sha Island consisted of a 915 MHz profiler, a Radio Acoustic temperature Sounding System (RASS), a GPS-based NAVAZD rawinsonde and a surface meteorological station. The 915 MHz profiler radar was used for measurement during non-precipitating period and for precipitating particles study and rainfall estimation during rainy period. The ISS operations revealed clearly the evolution of the mesoscale weather systems during SCSMEX(Fig.1), The low-level flow changed from a easterly to a south westerly during mid-May which is the onset phase of the South China Sea Monsoon(Lau, et al 2000). At the meantime, the Mei-Yu front established along the southern coast of China. The convergent flows associated with Mei-Yu front played a significant role in providing forcing of the weather observed over the northern part of the SCS. 3. Disturbed Period Mesoscale Structure A wide variety of convective systems were observed during the observational periods with a most active period occuring the onset of the monsoon. Two disturbed phases during SCSMEX were revealed by ISS observations. The first phase with subtropical origin appeared in May15-May20, the second phase with tropical origin occurred in June1-June9. Two major convective events occurred on May 18 and June 8 will be discussed.(Fig.2, Fig. 3, Fig. 4) For the mid-latitude influence case (May 18 th ), there were moderate shear at lower level and strong westerly at middle and upper level. It may explain that there were stratiform regions on both the front and rear sides of the convective region. For the tropical influence precipitating event(June 8 th ) the lower level shear was more stronger. The radar observations at ISS show strong squall line with pressure jump at meso high passing through and weak low following later. Temperature dropped 5 degree as cold pool arrived. 4. The C-Pol radar analysis The radar data collected by C-pol has been previewed. Several different types of precipitation systems has been observed. The polarimetric variables have been edited with thresholds method. The prelimary results of May 18 th and June 8 th were presented here. At 0300 GMT May 18 th , a squall line was approaching radar site from southeast direction with speed about 10m/sec. The leading edge convection reached 45 dBZ. By 0350 a stratiform anvil area developed in front of the leading convective area (the bright band located at 5km), the whole system weaken and lost its line shape(Fig. 6). The strong westerly observed by ISS profiler may explain the leading anvil. The condensate hydrometers were brought forward toward east and fell down to form the straitiform region. This stratiform region may cut off the warm and moist relative inflow from the east direction and weaken the whole system. The Zdr and Kdp fields were illustrated in Fig. 7 and 8. Compare the Zdr and Kdp patterns at 2km height, we found the attenuation in Zdr at the southwest direction. From the Kdp field the heavy rain area can be easily identified. In June 8 th case, an asymmetric squall line was observed, with much weaker south westerly above, only trailing anvil stratiform region was observed. As a contrast to the May 18 th case, the whole system maintained its intensity of the leading edge for more than two hours within the radar range. A weak mesocyclone was observed at the northern area. The Zdr and Kdp fields are consistent with the squall line feature. Integration with the other data will provide further insight of the microphysics and cloud dynamics. 5. Reference Lau K.M., Y. Ding, J.-T. Wang, R.Johnson, T. Keenan, R.Cifelli, J. Gerlach, O. Thiele, T. Rickenbach, S.-C. Tsay and P.-H. Lin, 2000: A Report of the field Operations and Early Results of the South China Sea Monsoon Experiment (SCSMEX). Bull. Am. Met. Soc _______________________________________________ * Corresponding author address : Dr. Pay-Liam Lin, Dept. of Atmos. Sci, Nat’l U., Chung-Li,320Taiwan, e-mail: [email protected]

Upload: others

Post on 13-Feb-2020

0 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: P10.15 STRUCTURE OF MESOSCALE CONVECTIVE SYSTEMS … · The polarimetric data of the C-Pol radar is very helpful for the understanding of the stratiform and the convective characteristics,

P10.15 STRUCTURE OF MESOSCALE CONVECTIVE SYSTEMS OBSERVEDWITH POLARIMETRIC RADAR AND UHF WIND PROFILER DURING

THE SOUTH CHINA SEA MONSOON EXPERIMENT (SCSMEX)

Pay-Liam Lin*, Tai-Chi Chen Wang, , Tsu-Hsang Liu, Hsin-Hon LinDepartment of Atmospheric Sciences

National Central University, Chung-Li 320, Taiwan

1. Introduction The NCU ISS(Integrated Sounding System) andthe BMRC dual-polarimeric doppler radar were deployedin Dongsha island during May 5 to June 25, 1998 for theSCSMEX. The primary goal of this deployment was tomeasure the mesoscale structure of convective weathersystem associated with the onset, maintenance andvariability of the monsoon over the South China Sea area.The ISS observations provide a detail kinematic andthermodynamic structure change of the monsoon flow.The polarimetric data of the C-Pol radar is very helpfulfor the understanding of the stratiform and the convectivecharacteristics, and the cloud physics and dynamics of theconvective systems. The purpose of this paper is topresent a brief overview of the mesoscale weathersystems during SCSMEX and investigate the structureand evolution of mesoscale convective systems observedduring the onset phase and post-onset phase of SCSMEX.

2. ISS observations The ISS deployed in Dong Sha Island consisted ofa 915 MHz profiler, a Radio Acoustic temperatureSounding System (RASS), a GPS-based NAVAZDrawinsonde and a surface meteorological station. The 915MHz profiler radar was used for measurement duringnon-precipitating period and for precipitating particlesstudy and rainfall estimation during rainy period. The ISSoperations revealed clearly the evolution of the mesoscaleweather systems during SCSMEX(Fig.1), The low-levelflow changed from a easterly to a south westerly duringmid-May which is the onset phase of the South China SeaMonsoon(Lau, et al 2000). At the meantime, the Mei-Yufront established along the southern coast of China. Theconvergent flows associated with Mei-Yu front played asignificant role in providing forcing of the weatherobserved over the northern part of the SCS.

3. Disturbed Period Mesoscale Structure A wide variety of convective systems wereobserved during the observational periods with a mostactive period occuring the onset of the monsoon. Twodisturbed phases during SCSMEX were revealed by ISSobservations. The first phase with subtropical originappeared in May15-May20, the second phase withtropical origin occurred in June1-June9. Two major convective events occurred onMay 18 and June 8 will be discussed.(Fig.2, Fig. 3,Fig. 4) For the mid-latitude influence case (May

18th), there were moderate shear at lower level andstrong westerly at middle and upper level. It mayexplain that there were stratiform regions on boththe front and rear sides of the convective region. Forthe tropical influence precipitating event(June 8th)the lower level shear was more stronger. The radarobservations at ISS show strong squall line withpressure jump at meso high passing through andweak low following later. Temperature dropped 5degree as cold pool arrived.

4. The C-Pol radar analysis The radar data collected by C-pol has beenpreviewed. Several different types of precipitationsystems has been observed. The polarimetric variableshave been edited with thresholds method. The prelimaryresults of May 18th and June 8th were presented here. At0300 GMT May 18th, a squall line was approaching radarsite from southeast direction with speed about 10m/sec.The leading edge convection reached 45 dBZ. By 0350a stratiform anvil area developed in front of the leadingconvective area (the bright band located at 5km), thewhole system weaken and lost its line shape(Fig. 6). Thestrong westerly observed by ISS profiler may explain theleading anvil. The condensate hydrometers were broughtforward toward east and fell down to form the straitiformregion. This stratiform region may cut off the warm andmoist relative inflow from the east direction and weakenthe whole system. The Zdr and Kdp fields were illustratedin Fig. 7 and 8. Compare the Zdr and Kdp patterns at 2kmheight, we found the attenuation in Zdr at the southwestdirection. From the Kdp field the heavy rain area can beeasily identified. In June 8th case, an asymmetric squallline was observed, with much weaker south westerlyabove, only trailing anvil stratiform region was observed.As a contrast to the May 18th case, the whole systemmaintained its intensity of the leading edge for more thantwo hours within the radar range. A weak mesocyclonewas observed at the northern area. The Zdr and Kdp fieldsare consistent with the squall line feature. Integration withthe other data will provide further insight of themicrophysics and cloud dynamics.

5. Reference

Lau K.M., Y. Ding, J.-T. Wang, R.Johnson, T. Keenan,R.Cifelli, J. Gerlach, O. Thiele, T. Rickenbach, S.-C. Tsayand P.-H. Lin, 2000: A Report of the field Operations andEarly Results of the South China Sea MonsoonExperiment (SCSMEX). Bull. Am. Met. Soc

_______________________________________________

* Corresponding author address : Dr. Pay-Liam Lin, Dept.of Atmos. Sci, Nat’l U., Chung-Li,320; Taiwan, e-mail:[email protected]

Page 2: P10.15 STRUCTURE OF MESOSCALE CONVECTIVE SYSTEMS … · The polarimetric data of the C-Pol radar is very helpful for the understanding of the stratiform and the convective characteristics,

Fig 1. Time series of surface meteorological elements during SCSMEX

Fig 2. Time series of the surface wind, temp,pressure, relative humidity and rainfall onMay 18, 1998

Fig 3. Time series of the surface wind, temp,pressure, relative humidity and rainfall onJune 8, 1998

Fig 4. Time series of reflectivity of UHF radar onMay 18, 1998

Fig 5. Time series of reflectivity of UHF radar onJune 8, 1998

Page 3: P10.15 STRUCTURE OF MESOSCALE CONVECTIVE SYSTEMS … · The polarimetric data of the C-Pol radar is very helpful for the understanding of the stratiform and the convective characteristics,

Fig. 7(a) The horizontal differential reflectivity field Zdr at 2km height. Contour interval is1 dB. (b) The vertical cross section of differential reflectivity Zdr. Contour interval is 0.2dB.

Fig. 8(a) The horizontal specific differential propagation phase shift field Kdp at 2km height. Contour interval is4deg/km.

(b) The vertical cross section of specific differential propagation phase shift Kdp. Contour interval is 2deg/km.

Fig. 6(a) The horizontal reflectivity at 2km height. Contour interval is 10dBZ. (b) The vertical cross section of reflectivity along the line shown in (a). Contour interval is 5 dBZ.

(b)

(b)

(b)

(a)

(a)

(a)