The Decay of Electric Field
in Anvils:
Observations and Comparison
with Model Calculations
J.E. Dye1, W.D. Hall1, J.C Willett2, S. Lewis1, E. Defer3, P. Willis4, D.M. Mach5,
M.G. Bateman5,
H.J. Christian5, C.A. Grainger6, J. Schild6,
and F.J. Merceret7
1 NCAR PO Box 3000, Boulder, CO 80307; 2 PO Box 41,Garrett Park MD; 3 National Observatory of Athens,
Athens, Greece; 4 NOAA/Hurricane Research Div., Miami FL; 5 NASA MSFC, Huntsville AL; 6 Univ. of No. Dakota, Grand
Forks ND, 7 NASA/KSC, Kennedy Space Center, Florida
ABSTRACT:
Airborne measurements of electric field and particle size distributions
made in anvils of active and decaying thunderstorms near Kennedy Space Center,
Florida coordinated with simultaneous radar observations are presented. The observations
in conjunction with a simple model are used to examine the decay of electric
field in anvils.
INTRODUCTION
Natural and triggered
lightning pose a threat to the launch of space vehicles and also personnel at
Kennedy Space Center and other launch sites. The Airborne Field Mill Project
(ABFM) was conducted during June 2000 and 2001 to examine the strength and
decay of electric fields in anvils, layer and debris clouds and how they are
related to microphysics and radar structure to better understand when hazard
from lightning might or might not exist. [Dye et al., 2002]. The
airborne observations were made from the Univ. of No. Dakota Citation II jet
aircraft and were coordinated with radar coverage from the Patrick Air Force
Base WSR74C 5 cm radar and the Melborne NEXRAD 10 cm radar. The vector electric
fields were measured using a set of 6 field mills as described in Mach and
Koshak, this conference.
EXAMPLE RESULTS FOR JUNE 13, 2000
Fig. 1 shows measurements
made on June 13, 2000 for a 7 minute period (~50 km of flight track). The
Citation investigated this anvil for over 3 hours, first with lightning present
and then for 2 hours after the last lightning. This pass at 11 km, –40 C, was
east to west across the anvil
|
Figure 1. Top Panel: Time history of
Particle concentrations measured by the following instruments: PMS FSSP (1 to 48 mm), light, solid line = total conc. on
right scale; PMS 2D-C (30 mm to ~3 mm), bold line = total conc.,
dashed line = conc. >1 mm on left scale; PMS 1D-C (15 to 960 mm), dotted line = total conc. on left
scale. Middle panel: Radar reflectivity curtain above and below
the aircraft from NEXRAD radar at Melborne FL, bold line = aircraft altitude. Bottom panel: Vertical component of the electric field, Ez, bold line on left on a linear scale, and the resultant vector field, Emag, light line on right on a log scale. |
while lightning was occurring in the storm core 25
to 40 km to the south. The maximum reflectivities encountered during this pass
were 15 – 20 dBZ from 2107 to 2108:30.
PARTICLE OBSERVATIONS
The microphysical
observations were made with five different instruments that spanned particle
sizes from a few microns to about five centimeters, thus from frozen cloud
droplets to very large aggregates. Measurements from an icing detector showed
no evidence of supercooled water in the example below or any other anvils
investigated. All particles discussed below are ice.
The measurements of Fig. 1 are representative of anvils studied at altitudes of 8 to 11 km (roughly -20 to –45 C). The concentrations in all size ranges increase as the aircraft moves into higher reflectivities, but usually larger increases occur for particles in the size range of 100 to ~500 mm than for particles >1 mm size. In regions with strong electric fields slightly downwind of storm cores there is a surprising degree of consistency in particle size distributions from storm to storm. The concentrations from 2108:00 to 2108:30 in Fig. 1 and Fig. 2 below are typical of those observed in other thick anvils near the storm core with electric fields >20 kV/m.
Figure 2 illustrates the
changes in particle concentration and area size distributions for four 30 s
intervals during the anvil pass in Fig. 1. At the edge of the anvil the number
distribution is almost flat from 100 to 1000 mm, but as the aircraft moves
into the thicker part of the anvil the concentration of particles in the 100 to
~500 mm increase by a factor of ~50. During this
same period the concentration of >1 mm particles increases by a factor ~3.
Figure 2. Top panel:
Concentration size distributions (30 sec averages) for the indicated
initial times during the Citation pass shown in Figure 1. Bottom panel: Area size distribution for the same 30 sec
time periods. Light line on the left side of each plot -- FSSP (off scale for
area plots); Bold line – 2D-C; light line on right of each plot -- SPEC High
Volume Particle Spectrometer, HVPS, (~400 mm to ~5 cm range).
ELECTRIC FIELD OBSERVATIONS
Likewise electric fields are much weaker near the edges than in the central anvil or near the storm core. As in Fig. 1, the electric field is <3 kV/m for reflectivities <5 - 10 dBZ in edges of the anvil followed by a relatively abrupt increase in electric field as the aircraft flies into greater reflectivities in denser parts of the anvil or near the storm core. The electric field measurements show more variability and often increase much more abruptly than the increase in particle concentrations. The complex nature of the electric field structure and changes of polarity even when flying at constant altitude suggest that the charge distribution in these anvils is not a simple uniform layering of charge.
Strong electric fields (>10 kV/m) are associated with regions of reflectivity above the freezing level ³10 dBZ, but reflectivity >10 dBZ does not necessarily indicate strong fields. In strong electric fields particle concentrations are high in all size ranges and greater than in regions with weak (<3 kV/m) electric fields. Bateman et al., this conference, discuss the correspondence between electric field and reflectivity and investigate reflectivity parameters that might be used as possible indicators of the presence of strong electric fields.
PARTICLE SIZE DISTRIBUTIONS AND ELECTRIC FIELD DECAY
Willett and Dye (this
conference) use a simple model to calculate electric-field decay times based on
observed particle size distributions. The model assumes that a given size
distribution is uniform everywhere in the model anvil and that it remains
constant during the decay of electric field. This is not strictly correct, but
it provides an upper bound on what might be expected. A "high-field
limit" is identified, for ambient field intensities greater than about 1
kV/m, in which the model field decays linearly with time; and a decay time
scale, tE, is defined as the time
required for the cloud field to decay to zero from an arbitrary initial value
of 50 kV/m. tE is found to be proportional
to the particle effective electrical cross section (area), integrated over the
size distribution. See Willett and Dye for more details.
Figure 2 displays the area size distributions for this case. tE for the 4 time periods of Figure 2 is 340, 1256, 2656 and 5963 s, respectively. tE increases by a factor of almost 20 from the edge to the central part of the anvil.
In Fig. 2 the area distributions, which control tE, show a peak near 1 mm in the edge of the anvil, but as the aircraft moves into the central anvil, the area distribution becomes broad with a mode from 0.2 to 2 mm. In this case (and other cases we have examined to date) as the aircraft moves from the edge toward the central part of the anvil the largest increase in particle concentrations are of the 0.2 to 1 mm size particles. The results show this size range to be dominantly responsible for the increases in calculated electrical decay times.
COMPARISON OF CALCULATED AND OBSERVED DECAY TIMES
After lightning had ceased,
passes were made into the wind from the downwind tip of the anvil into higher
reflectivity in the remnants of the storm core. The southern most part of two
of these passes are depicted in Fig. 3. The maximum reflectivities from 2253 -
2258 were 14 to 17 dBZ and 12 to 15 dBZ for 2324 – 2330. The maximum electric
fields observed during the first pass were 39 kV/m at 2253:30. During the
second pass the electric fields had decreased to a maximum of 1.5 kV/m at
2253:30, a decay of 37.5 kV/m in 32 min (1920 s). By comparison the maximum in
the calculated E time scale, tE, for the decay from 50 kV/m was 1711 s for the
period 2253:30 to 2254:00. Using this time scale we calculate via equation 5)
of Willett and Dye, this conference, a time of 1275 s for the electric field
decay from 39 to 1.5 kV/m based on the 30 s average particle size spectra
observed at 2253.
The observed decay times are
longer than those calculated. However, the model assumes uniform microphysics
in the anvil and during the entire decay. The reflectivity below the aircraft
(Fig. 3) was 5 dBZ or more greater at 7 km than at 9 km, the aircraft altitude.
Clearly the largest particles were more numerous below the aircraft and quite
probably the intermediate sized particles as well. Measurements in this anvil
(Figs 1 and 2) and other anvils show that as reflectivity increases,
concentrations and area in all particle size ranges also increase, especially
from 0.2 to 1.0 mm. For the 30 s averages for 2105 and 2108 (Fig. 1) tE increased from 1256 to 5963
s, almost a 5 fold increase as a result of increased particle area at
intermediate sizes (See Fig. 2). The corresponding reflectivity increase was ~5
dBZ. It seems likely that if particle observations were available at 7 km for
this anvil, they would yield electric field decay times more than enough to
account for the difference between observed and calculated values discussed
above. None-the-less, this comparison of calculated and observed electric field
decay time shows that the decay times calculated in the model for this anvil
are roughly comparable to those observed.
A similar comparison for
June 14, 2000, a case where the aircraft flew in the greatest reflectivities in
the decaying anvil, shows the observed times for decay bracket those
calculated.
Figure 3: CAPPIS at 9 and 7 km for 2 periods with 9
min of aircraft track overlaid. Squares show track start. Lower Panels: Measured vert. field, Ez, (bold line, left
scale) and magnitude of total field, Emag, (thin line, logartithmic right
scale) for 2250 - 2300 and 2320 – 2330.
CONCLUDING REMARKS
Observations
of particle spectra and electric fields in anvils in regions with strong
electric fields show consistency of particle concentrations in all size ranges
from storm to storm. These observations in combination with model calculations
of electric field decay in a simplified anvil (Willett and Dye, this conference)
show that the particle size distribution controls the decay time of electric
field in these anvils. Particles of 0.2 – 1 mm size are predominantly
responsible for changes in decay times along and across the anvils. As air
containing ice particles moves out from the convective core into anvils and
downwind, the particle spectra change due to sedimentation, mixing and
evaporation and the time for decay of the electric field dramatically
decreases.
ACKNOWLEDGEMENTS;
We gratefully acknowledge support from the National Aeronautics and
Space Administration (Kennedy Space Center) and the National Reconnaissance
Office, the help and encouragement of John Madura and Phil Krider, and graphics
work of Kris Conrad.
REFERENCES
Bateman, M.G.,
D.M. Mach, S. Lewis, J.E. Dye, E. Defer, C.A. Grainger, P.T. Willis, H.J.
Christian, F.J. Merceret, 2003:
Comparison of in-situ Electric Field and Radar Derived Parameters for
Stratiform Clouds in Central Florida, This Conference.
Dye, J.E.,
W.D. Hall, S. Lewis, E. Defer, G. Dix, J.C. Willett, C.A. Grainger, P. Willis,
M. Bateman, D. Mach, H. Christian and F.J. Merceret, 2002: Microphysical Properties and the Decay of
Electric Fields in Florida Anvils, presented at AGU Fall Meeting, San
Fransisco, CA, Dec 2002. Abstract in EOS Trans. Amer. Geophys. Union.
Mach, D. M. and W. J. Koshak, 2003: General Matrix Inversion Technique For The Calibration Of Electric Field Sensor Arrays On Aircraft Platforms, This Conference.
Willett, J.C.
and J.E. Dye, 2003: A Simple Model to Estimate Electrical Decay Times in Anvil
Clouds, Proc. This Conference