Download presentation
Presentation is loading. Please wait.
Published byHilary McCarthy Modified over 9 years ago
1
IHOP Science Meeting 24-26 March 2003 Multi-Platform Observations of a Bore Event on 4 June during IHOP Steven E. Koch Frederic Fabry, Bart Geerts, Tammy Weckwerth, James Wilson, Dave Parsons, and Wayne Feltz
2
Data used in Study of this Bore Event S-POL reflectivity, (radial velocity), refractivity Surface mesoanalysis plots Mesonet time series, incl.refractivity calculations AERI & CLASS thermodynamic structure evolution FM-CW, HARLIE, MAPR, (RAMAN lidar), (GLOW) UW King Air flight-level data High-resolution MM5 simulations (next talk)
3
Computation of Refractivity from Surface Data Refractivity Vapor Pressure
4
IHOP Science Meeting 24-26 March 2003 BORE A
5
S-POL: 0430 – 0730 UTC
6
Surface Analysis at 0500 UTC
7
FM-CW and HARLIE Displays of Bore A
8
FM-CW and MAPR Displays of Bore A
9
Bore A at Verles (0520 Z)
10
Bore A at Rusty Tank (0530 Z)
11
Bore A at Playhouse (0552 Z)
12
Bore A at Lincolns (0635 Z)
13
IHOP Science Meeting 24-26 March 2003 BORE B
14
S-POL: 1000 – 1200 UTC
15
Surface Analysis at 1000 UTC
16
FM-CW Display of Bore B UWKA Flight-level data
17
FM-CW and MAPR Displays of Bore B
18
temperature potential temperature vertical air velocitystatic pressure (u,v) theta-e mixing ratio SE NW Wave propagation UW King Air Data FL 1850 m AGL KA penetrated solitary waves at the top of the bore. The waves are ranked in amplitude (as in FM-CW). 3C cooling and 4 g/kg more moisture found at this level behind the bore (NW) – unlike the drying/warming seen in SPOL near-sfc refractivity. Vertical motions are in phase quadrature with theta and u/v, as in a typical gravity wave, but strangely out of phase with pressure fluctuations. Pressure variations are mainly a response of the aircraft to the vertical motion field. Mean 1.2 m/s updraft over 30 sec produces 35 m ascent or 3.5 mb hydrostatic pressure decrease.
19
Bore B at Verles (0942 Z)
20
Bore B at Rusty Tank (1020 Z)
21
Bore B at Playhouse (1022 Z)
22
Bore B at Lincolns (1100 Z)
23
AERI and ISS Detection of Bores A & B Potential Temperature Relative Humidity
24
Conclusions Two bores or solitons observed as fine lines in S-POL reflectivity and by FM-CW, MAPR, ISS, Mesonet, UWKA data systems: Bore A occurred along an outflow boundary that propagated eastward from the Oklahoma Panhandle Bore B occurred along a cold front enhanced by postfrontal convection in northwestern Kansas Solitary waves developed to the rear of each leading fine line atop a 700 – 1000 m deep surface stable layer. Depth of stable layer increased by 0.6 km with passage of leading wave in bores A and B. Solitary wave characteristics: periodicity = 15 – 30 min, horizontal wavelength = 10 – 20 km, phase speed = 11.4 – 12.6 m/s. Waves exhibited amplitude-ordering (leading wave always the largest one).
25
Conclusions Pronounced reduction in refractivity due to drying in surface layer occurred when the leading pressure jump was relatively strong. Cooling & moistening aloft occurring with passage of both bores a likely result of adiabatic lifting (seen in AERI data and UWKA data for Bore B). UWKA pressure data is confusing. Bore A appears to have been a soliton on a surface inversion layer. Bore B occurred at a higher elevation of 1.2 km as the inversion had lifted by that time, but problems remain with FM-CW data interpretation. It appears to have been a weakening soliton. Need to understand better why drying (reduction of refractivity) only occurs at certain times. Analysis of MAPR, GLOW, & SPOL wind data, additional mesonet data, and UWKA data will be needed.
Similar presentations
© 2024 SlidePlayer.com Inc.
All rights reserved.