World Meteorological Organization Symposium on Nowcasting - WMO
World Meteorological Organization Symposium on Nowcasting - WMO
World Meteorological Organization Symposium on Nowcasting - WMO
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122<br />
P2.10<br />
Systematic variati<strong>on</strong> of Drop Size in c<strong>on</strong>vective of Beijing and Radar-rainfall Relati<strong>on</strong>s<br />
11:15 8.9 The GOES_R satellite proving ground: nowcasting applicati<strong>on</strong>s and<br />
results from the 2009 hazardous weather testbed experimental forecast<br />
and warning dem<strong>on</strong>strati<strong>on</strong><br />
Xian Xiao[1],Yu HaiYan[2]<br />
[1]Institute of Urban <str<strong>on</strong>g>Meteorological</str<strong>on</strong>g>, CMA No.55 Bei-Wa-Xi-Li Road, Hai-Dian District, Beijing,<br />
China ,100089 [2]Beijing Meteorology Bureau , No.44 ZI-Zu-Yuan-Lu Road, Hai-Dian<br />
District , Beijing , China ,10089 11:30 8.10<br />
Steven Goodman, James Gurka, Timothy Schmit, Mark DeMaria, Daniel<br />
Lindsey, Wayne Feltz, Scott Bachmeier, Kris Bedka, Steven Miller, Eric<br />
Bruning, Gary Jedlovec and Richard Blakeslee<br />
Detecti<strong>on</strong> and m<strong>on</strong>itoring of C<strong>on</strong>vective clouds by satellite<br />
Based <strong>on</strong> the raindrop size distributi<strong>on</strong> data of 50 c<strong>on</strong>vecti<strong>on</strong> precipitati<strong>on</strong> events measured<br />
Yann Guillou, F. Aut<strong>on</strong>es, Stéphane Sénési<br />
in Beijing during 2007 by a parsivel Disdrometer, which has 32 channels and measures the<br />
raindrop diameter from 0.62mm to 24.5 mm, microphysics parameters and its fluctuati<strong>on</strong><br />
features with the relati<strong>on</strong> between Z and R or coefficient a and exp<strong>on</strong>ent b , were analyzed. It<br />
found that the gamma functi<strong>on</strong> is more perfect agreement than Marshall-Palmer (M-P)<br />
exp<strong>on</strong>ential functi<strong>on</strong> between fits and observati<strong>on</strong>. The storms observed in Beijing could be<br />
divided into 3 phase: c<strong>on</strong>vective (C), transiti<strong>on</strong> (T), and stratiform (S). For different<br />
precipitating phase, the relati<strong>on</strong> between Z and R or coefficient a and exp<strong>on</strong>ent b, with<br />
raindrop size distributi<strong>on</strong> (DSD) parameters are quite different. The c<strong>on</strong>vective phase of a<br />
storm often accounts for a major share of the rain accumulati<strong>on</strong> despite its shorter durati<strong>on</strong>,<br />
which is always more than 76%. Six kinds of diameters are calculated, including the mean<br />
diameter D0, the mode diameter Dd, the mean volume diameter Dv, the predominant<br />
diameter Dp, the median volume diameter Dn and the median diameter Dnd , it found the<br />
mean diameter D0 has the same evolvement as the other except for the mode diameter Dd,<br />
which changes no systemically. For c<strong>on</strong>vective phase of each precipitati<strong>on</strong> , there were the<br />
biggest median diameter D0 and coefficient a; for transiti<strong>on</strong> phase of each precipitati<strong>on</strong>, there<br />
were the smallest median diameter D0 and coefficient a ; for stratiform phase , there were<br />
middle median diameter D0 and coefficient a. Especially ,when R , or N T , or Z gradually<br />
increases, coefficient a (or the exp<strong>on</strong>ent b) approaches to a c<strong>on</strong>stant value. Drop growth<br />
occurs predominantly below the 0°C level by collisi<strong>on</strong>, coalescence, and breakup in the<br />
c<strong>on</strong>vective phase. The light and role of cumulus merger process may influence DSD, which<br />
median volume diameter D0 grows as and so the DSD narrows; that is both â and Ð<br />
increase. Moreover, that there is a linear correlati<strong>on</strong> between R and Z , in other words ,<br />
exp<strong>on</strong>ent b is 1 , when Dm is a c<strong>on</strong>stant .However, when R<br />
11 :45 Closing Remarks<br />
P2.11<br />
The nowcasting feature analysis of heavy precipitati<strong>on</strong> supercell storm based Doppler<br />
weather radar observati<strong>on</strong><br />
ZHOU Xiaogang, LIU Shijun, LIU Hua<br />
Chinese <str<strong>on</strong>g>Meteorological</str<strong>on</strong>g> Administrati<strong>on</strong> Training Centre, Beijing 100081, China<br />
As China's new generati<strong>on</strong> of Doppler weather radar network, some cases <strong>on</strong> the supercell<br />
storm have been studied. The process of heavy precipitati<strong>on</strong> supercell storm has received<br />
relatively little research attenti<strong>on</strong> to date. The understanding <strong>on</strong> the supercell storm depends<br />
<strong>on</strong> careful analysis of the case. Here, an analysis is presented of a heavy precipitati<strong>on</strong><br />
supercell in Y<strong>on</strong>gzhou, Hunan province, in associati<strong>on</strong> with heavy hail and tornado <strong>on</strong> April 9,<br />
2006. Because of its generati<strong>on</strong>, development, maturity and demise were just moving<br />
Friday 4 September<br />
19