AIRBORNE FIELD MILL PROJECT
KENNEDY SPACE CENTER

SYNTHESIS FOR JUNE 18, 2001 - ABFM

Flight Summary (Non-Anvil Day)

Case 1 (Times: 2032 - 2203)
Type of case debris
Complexity moderate
Convection line of convection
Electric field
  kV/m
Min Em_m = 0.087
Max Em_m = 52.765
Mean Em_m = 10.769
Microphysics
  #/Liter
Max CON_FSSP = 48807.602
Mean CON_FSSP = 5320.459
Max Tot_con_1DC = 321.892
Mean Tot_con_1DC = 44.031
Max Tot_con_2DC = 412.961
Mean Tot_con_2DC = 55.730
Max 2DC_100_400 = 216.286
Mean 2DC_100_400 = 25.223
Max 2DC_400_1000 = 42.876
Mean 2DC_400_1000 = 7.438
Max 2DC_GT_1000 = 4.795
Mean 2DC_GT_1000 = 0.670
Location (x,y) ~ (0,-60)
Motion 0

Brief Description

There ws lightning in a cell to the west of the aircraft.



There was 45-50 dBZ reflectivity with lightning in the region the aircraft flew at 1844. There is really no storm motion so this is debris.







SYNTHESIS FOR JUNE 18, 2001 - ABFM

Investigator: Paul Willis
[presented on Apr 4, 2002]


 

ANALYSIS:

Beginning about 1900 (4km) , two major cells were developing, one just inland about 50 km S of Patrick, and the second about 140 km S of PAFB on the east shore of Lake Okeechobee. New cells formed between these two, and a more or less continuous line formed south from PAFB and along the east shore of the Lake by 2000 (4km) . By 2015 (4km) a new cell formed inland W of the Cape, and the cells down by the Lake appeared to dominate. The cells just N of the lake became dominant by 2045 (4km) , but a huge stratiform region developed south along the east side of the Lake, and a mostly stratiform line paralleled the coast to a point not far south of Patrick. The active cells continued to develop and move NW and W of the lake, while the anvil/stratiform areas remained in a line and propagated slowly to the east at levels from 7-10 km.

The citation started sampling about 2030 in nominally N-S tracks in these anvil/stratiform areas east and NE of the active convective cells until 2210.

A. Lightning

From 2030 the aircraft sampled just on the NE edge of the lightning, with most of the CG strokes to the SW 30 km, in the most active cells. From 2100 to 2130 only the southern parts of the flight legs touched on the lightning. From 2130 on the nearest lightning was well to the West of the flight tracks (50 km). From 2200 to 2210 the last flight legs, the nearest lightning was even further to the WSW (70km).

2030-2040 (lightning) 2040-2050 (lightning) 2050-2100 (lightning) the flight tracks are just inside the NW edge of the lightning

2100-2110 (lightning) 2110-2120 (lightning) 2120-2130 (lightning) lightning receding slightly to the S and W, but the south end of the flight tracks are still just in the lightning

2130-2140 (lightning) 2140-2150 (lightning) 2150-2200 (lightning) all lightning near flight tracks has dissipated and moved to W

2200-2210 (lightning) 2210-2220 (lightning) 2220-2230 (lightning) original lightning areas moved even further W, a new area to

the W and NW

B. Radar

The echo structure has been described above. The aircraft sampling was at 8 km altitude in the stratiform anvil line extending north parallel to the coast, and in the stratiform regions east of the active cells.

2045 (4km)
CAPPI 2042 strong convective cells N of Lake Okeechobee, a mostly stratiform line paralleling the coast N nearly to Patrick

2100 (4km)
CAPPI 2100 flight tracks roughly parallel the coast in the weak line and anvils from the cells N of Lake Okeechobee

2115 (4km)
CAPPI 2115 the N line of weak cells is pretty stationary, strong cells on the N side of Lake Okeechobee, developing and moving W, large stratiform area remaining to the E of Lake Okeechobee

2130 (4km)
CAPPI 2130 N extending line still intact and stationary, active cells are now well NW of Lake Okeechobee

CAPPI 2145 N line dissipating at 4km, large stratiform region is intact and now wraps around the E and N sides of Lake Okeechobee

The time history of this system, particularly where the charged hydrometeors were electrified, and transported from, is very complex. This detracts from a straightforward analysis. There seems to be two regimes in the advecting winds measured at the 8 km flight altitude - WNW and NE. One is probably the environmental flow, and the other the flow created by the mesoscale cloud system.

As mentioned last week, the radar scan strategy has shortcomings for producing 10 km CAPPI's., e.g. at 10 km. One scan intersects the cloud at a range, while the next one goes over the top. The overlap, and the voids must be considered when interpreting the data at anvil levels.

C. Electric Field Data

Electric Field

This case is characterized by very strong fields. Of particular interest are the fields after the lightning moves to the west, and some structure at the cloud edges. The fields (Ez) in the first half of the flight are predominantly + ( efield_2100-2115 ) , but in the second half there are interesting reversals. The period from 2150 ( efield_2145-2200) to the end of the flights are quite weak, ( efield_2200-2215) and this may be a good case to look at weakening, although perhaps we are too far east and did not stay long enough. A Lagrangian analysis will tell if this is a good weakening candidate.

D. MER plots (microphysics)

In general the strong fields are well correlated with high radar Z and high concentration of large particles, and total 2DC in this data set from 8km. There are some interesting fine scale exceptions in the details. The fields seem to decrease before the Z decreases, and before the cloud goes away at the cloud edges. At 2054-2059 ( mer_2058 ) there is a period of low Ez with moderate reflectivity factor Z. From 2133 and following ( mer_2130 ) ( mer_2137 ) , Ez goes, then Z goes, then the cloud edge is reached. From 2152-2203 ( mer_2153 ) ( mer_2203 ) Ez is gone, then radar going, and 2DC remains high to the cloud edge.

2034-2037 ( mer_2029 Extensive region of strong fields, EZ`40 kv/m, winds are complex changing from NW to NE in the high field region The fields are fairly well correlated with high Z, although the strongest fields are in 15-20 dBZ

2037-2040 ( mer_2037 There is a reversal at 2037-2038, the highest fields are close to the highest Z's, but the field seems to end, then the Z ends then the cloud ends

2048-2053 ( mer_2045) CAPPI 2050 This is a south to north pass, Ez -20 t0 -40, then +40 at 2050ff, the winds are NE in this region, very high Z and conc of > 1mm hydrometeors

2054 ( mer_2053 -30 Ez with strong Z to the surface below the aircraft, still moderately high hydrometeor concentrations

2055 long stretch of no fields, but mdt Z and still in cloud.

2100-2103 ( mer_2101) Ez -40 kV/m Ez, Z N cloud edge are all consistent

2106-2111 ( mer_2109 Ez, Z N all well correlated, first Ez goes to 0, then Z but N continues to 2114

2117-2124 ( mer_2117 complex anvil structure, but consistent winds from SW

2125-2132 ( mer_2125 at 2125 good high Z above the FL Ez of +35, 2128ff Ez of -40 for a long distance

2141-2148 ( mer_2141) Ez of +30 at 2146

SUMMARY

I don't think there is any occurrence of High E without nearby high Z

This is a potential case for decay of fields, but the sources of charge centers and the advecting flows may be too complex. It does have fairly extensive sampling in the same area. A Lagrangian analysis is probably needed.