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By Edward J. Szoke, John Brown, and Brent Shaw |
Introduction
From 13 May to 25 June 2002, FSL scientists were
involved in the International H2O Project (IHOP), an
extensive field study covering the Southern Plains and
based in Oklahoma. More than 100 people participated
in the campaign to determine primarily how to improve
the characterization of the four-dimensional distribution
of water vapor and its application to better understand
and predict convection. The four main components of the
program included quantitative precipitation forecasts
(QPFs), convective initiation (CI), atmospheric boundary
layer processes, and instrumentation. FSL ran experimental
versions of local and national scale models during
IHOP to assist with nowcasting and short-range
forecasting and to determine whether such models could
provide useful forecast and nowcast guidance for
convective weather.
FSL's Rapid Update Cycle (RUC) model, a national
scale model, and the Local Analysis and Prediction
System (LAPS), a smaller scale model, were used during
IHOP. LAPS was designed to run onsite at a National
Weather Service Forecast Office (WFO), using local
analyses that take advantage of locally available data.
LAPS is currently running in AWIPS at WFOs on an
hourly cycle with a 10-km grid spacing. LAPS was run
at a 12- and 4-km horizontal grid resolution and used to
initialize some of the models that FSL ran during IHOP.
One goal of a short-range model is to provide better
prediction of precipitation without a spin-up period. To
aid in this goal a "Hot Start" scheme was developed using
the LAPS cloud analysis to prescribe a vertical velocity
profile where sufficiently deep clouds are present at
initialization time. The three-dimensional dynamical
relationship between mass and momentum is adjusted by
the LAPS balance algorithm to force consistency with
the diagnosed cloud vertical motions and allow for a
smooth model start. During IHOP, a 12-km horizontal
resolution MM5 hotstart initialized with LAPS was run,
with a nested 4-km version covering the IHOP
experimental domain (Figure 1). LAPS also was used to
initialize a similar 12-km setup for the Weather Research and Forecast (WRF) model. In addition to these models
initialized with LAPS, FSL ran a 10-km version of the
RUC model. The RUC model employs a three-dimensional
variational (3DVAR) analysis for the mass
fields, and initial RUC hydrometeor fields are adjusted to
correspond to base scan reflectivity patterns at the initial
time, but without any modification of the initial vertical
velocity field (in contrast to the hotstart method). The
models run by FSL for IHOP are summarized in Table
1. (These experimental model runs are archived by
UCAR at http://www.joss.ucar.edu/ihop.)
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Figure 1. The 12-km and inner 14-km IHOP domains
for LAPS MM5 and WRF runs (points every 12 km).
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Table 1. FSL Real-Time Models in IHOP (*except LAPS-WRF, available after IHOP) |
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Model |
Delta
x
km |
Number
Vertical
Levels |
Runs
Every
x Hour |
Forecast
Duration
(Hours) |
Convective Scheme |
Microphysics |
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MM5hot
MM5hot
LAPS-WRF*
RUC
RUC |
4
12
12
20
10 |
34
34
34
34
50 |
3
3
3
3
3 |
12
12
12
6-24
6-24 |
None
Kain-Fritsch
Kain-Fritsch
Grell-Devenyi
Grell-Devenyi
Ensemble-Closure |
Schultz
Schultz
NCEP-5
RUC/MM5 MixedPhase |
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Evaluation of Model Performance
One of our goals during IHOP was to compile a fairly
extensive subjective evaluation of the various models in
real time. Objective model evaluation was done within
FSL (see Brent Shaw's article WRF). In order to
perform subjective evaluation, an online evaluation form
was designed that allowed the forecaster/nowcaster to
document what the model was forecasting, the relationship
of various forcing features to the subsequent convection
forecast by the model, and the forecaster's confidence in the forecast. The forecasters also made many freeform
comments that give insight into how the models performed
with the various short-range forecast problems during
IHOP. A summary of these comments follows:
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The MM5 models using LAPS for the initial state did
an excellent job of initializing ongoing convection, but
often this convection was lost in the first hour of
simulation. Adjustments were made to the Hot Start
scheme for a set of post-IHOP reruns of both MM5
and the WRF model, and our preliminary evaluation of
some of these reruns indicates some improvement
with this problem. The most easily "lost" convection
involved elevated storms (nonsurface-based convection),
while very strong individual storms and lines
were much better retained from the initialization.
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Outflows tended to be easily produced from convection
in the MM5 model, especially so in the 4-km run,
whereas the RUC tended to be more conservative in
producing outflows but was able to do so.
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The most difficult storms to forecast were elevated
convection, which usually formed in the very early
morning (presunrise) hours and could persist for up to
6 hours after sunrise. Coincidentally, this type of
convection is also among the most challenging for
forecasters, as it can occur without any obvious
surface forcing feature present. Though seldom
producing severe storms (at least during IHOP),
elevated convective events were often of the "surprise" category. There were often indications in the model of
possible activity, for example in the form of midlevel
echo but without precipitation reaching the surface, so
an underforecasting of the convection. Convection associated with a warm front (on the cool side of the
warm front) also tended to be an area where the models
were deficient. This type of convection often was not
surface-based, sharing that characteristic with the
elevated storms noted above.
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Some of the forecasts of convective initiation along
drylines were quite good. For a few cases the model
beat the forecasters, particularly when temperatures
both at the surface and aloft were quite hot. In these
cases, forecasters overestimated the time it would take
to break the cap, while the model more correctly
forecast convective initiation earlier.
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Other good forecasts occurred with well-defined
surface-based forcing features, such as cold fronts.
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As noted earlier, there was some skill in the model's
ability to forecast storm type and evolution, with several
events during IHOP that featured upscale growth into
organized lines that often accelerated much faster than
indicated in the precipitation fields from conventional
models (for example, the Eta model).
Selected Case Studies From IHOP
Two cases are examined using both model runs during
IHOP and the reruns that occurred after IHOP. The
reruns provided a series of model runs from the WRF
model, which was actually run during IHOP but not able
to display in real time. As a result of the real-time
experiences during IHOP, we decided to apply
improvements to the hotstart method to the reruns. A
significant improvement involved removal of a warm
bias that existed in the LAPS initialization, and was likely responsible for overprediction of convective precipitation
during IHOP from the MM5.
2 June 2002: Dryline Case – On this day the western
half of the IHOP domain was dominated by very hot
temperatures, reaching the low 100s (oF) during the
afternoon. A well-defined dryline was not seen initially,
but was sharpened in the early afternoon, as shown by
the LAPS analysis of wind and dewpoint along with low-level
reflectivity in Figure 2. This sharpening first appeared
as a surge of westerly surface flow that emerged out of
eastern Colorado that then pushed into Kansas. On this
day, the IHOP forecasters predicted that a dryline would
become better defined during the afternoon (somewhat
later than what occurred) but they thought convective
initiation along it would occur fairly late in the afternoon
as they waited for the dryline to sharpen and temperatures
to break the significant cap that was in place. As it turned
out, the presence of the very hot surface temperatures
and a somewhat stronger and earlier dryline push than
expected allowed the cap to be broken and convective initiation to occur over 2 hours ahead of the IHOP
forecasters' prediction. It was noted in IHOP that the
MM5 model did a good job indicating this convection
earlier than expected, particularly the run initialized at
1500 UTC. Some of the runs from that day are examined
and the somewhat different forecasts are contrasted for
this relatively "tricky" case. With the expense of some of
the resources in IHOP, in particular the aircraft, timing
of convective initiation was a critical forecast issue. In
this case, even a forecast error of 2 hours for convective
initiation from a midmorning forecast was critical and
resulted in an aborted mission, since convection was well
underway before the aircraft (leaving Norman, Oklahoma)
could reach the dryline target.
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Figure 2. LAPS analysis of surface wind, dewpoint,
and low-level reflectivity at 2100 UTC 2 June. The
western portion of Kansas is in the center.
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We first examine some forecasts initialized at 1200 UTC
since reruns of both MM5 and WRF are available at this
time. A forecast from the MM5 run initialized at 1200
UTC and valid at 2100 UTC is shown in Figure 3. In this
and subsequent figures, when no contours are present,
the model is forecasting reflectivity aloft with no precipitation reaching the surface. For the most part, the
reflectivity values for the image in Figure 3 are 30 dBZ
or less. Some stronger cells are forecast for which these
surface reflectivity contours are depicted (e.g., in extreme
northeastern Nebraska and along the Iowa/Illinois border).
The insert shows a composite low-level reflectivity
image overlaid with a visible satellite image (white areas)
over a region centered on western Kansas. This indicates
that storms were really producing rain by 2100 UTC,
with maximum reflectivities exceeding 50 dBZ. Thus,
the MM5 12-km run was forecasting high-based
convection that would not produce precipitation, so it
correctly indicated that storms would be produced along
the dryline, but was underforecasting development. For
comparison, the post-IHOP rerun of the MM5 12-km
model for the same time is shown in Figure 4, and for the
WRF 12-km model in Figure 5. The MM5 rerun is very
similar to the original MM5 12-km run during IHOP, and
the WRF forecast from the 1200 UTC run valid at the
same time is also very similar. All the runs indicate
convective development with reasonable timing but only forecast virga-producing storms. The forecasts from
these same runs valid 3 hours later at 0000 UTC on 3
June (WRF is shown in Figure 6) were very similar to the
2100 UTC forecasts, in that there continued to be no
indication of storms that would produce precipitation. In
reality, the line of broken storms advanced slowly to the
east, and by 0000 UTC extended all the way from north-central
Kansas south-southwest to the far western
Texas Panhandle.
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Figure 3. MM5 12-km IHOP run of 9-hour forecast valid at 2100 ITC 2 June 2002. Image is a composite reflectivity, with contours indicating model surface reflectivity. Inset shows a composite low-level radar image at this time over western Kansas. |
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| Figrue 4. Same as Figure 3 except for a 9-hour forecast from the MM5 12-km rerun valid at 2100 UTC. |
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Figure 5. Same as Figure 3 except for a 9-hour forecast from the WRF 12-km rerun valid at 2100 UTC. |
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Figure 6. As in Figure 5 except a 12-hour forecast from WRF 12-km rerun valid 0000 UTC on 3 June. The insert depicts the actual radar reflectivity at this time. |
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The MM5 4-km run initialized at 1200 UTC produced
higher values of composite reflectivity, but still no surface
reflectivity (and therefore no precipitation reaching the
ground). On the other hand, the MM5 4-km run initialized
3 hours later at 1500 UTC did produce well-defined
surface storms, although slower than what actually
occurred and by 0000 UTC with a line of storms not far
enough east (Figure 7). The MM5 12-km run for this
same time made during IHOP (Figure 8) was not as
bodacious with storm development as the 4-km run, but
it did indicate a surface echo in the Oklahoma Panhandle, and another much farther north along the line. The actual
reflectivity at 0000 UTC is shown in Figure 9. Though the
forecasts (especially the 4-km runs) that were initialized at 1500
UTC were better than the 1200 UTC ones, for some reason this
improving trend did not continue with the 1800 UTC runs. The
6-hour forecasts from the various models (MM5 4-km, MM5
12-km IHOP run, MM5 12-km rerun, and WRF 12-km rerun)
are shown in Figure10 (a–d). The MM5 4-km run still correctly
produces a surface echo, but there is less an of echo than was
in the forecast from the 1500 UTC run, and the line of echoes
is even farther west. The MM5 12-km runs (Figures 10b and c)
are quite similar to each other, and neither predicts any surface
echo. Recall that the 1500 UTC 12-km IHOP run (Figure 8)
actually did predict an echo reaching the surface by 0000 UTC,
so the forecast initialized 3 hours later is not as good, similar to
the behavior of the 4-km run. Note that the WRF 12-km rerun
(Figure 10d) is actually a little drier than the MM5 12-km rerun
and similar to the WRF 12-km rerun from 1200 UTC.
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Figure 7. MM5 4-km 1500 UTC IHOP run 9-hour reflectivity forecast (as in Figure 3) valid 0000 UTC 3 June. |
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Figure 8. As in Figure 7 except for the MM5 12-km 1500 UTC IHOP run 9-hour reflectivity forecast valid 0000 UTC 3 June. |
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Figurre 9. Observed low-level radar reflectivity at 0000 UTC 3 June. |
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Figure 10. a, above left) MM5 4-km 1800 UTC IHOP run 6-hour reflectivity forecast (as in Figure 7) valid 0000 UTC 3 June. b, above right) As in 10a except for MM5 12-km run. c, below left) As in 10a except for MM5 12-km rerun. d, below right) As in 10a except for WRF 12-km rerun.
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In summary, for this case the models showed a dryline moving into western Kansas more or less as occurred. The main
message from the model runs is that convection would be initiated by the dryline, but the storms would be weak without
any surface rain, typical of high-based, mostly dry convection that might occur on such a hot day with marginal moisture. The 4-km MM5 runs
accurately indicated that more substantial
storms could occur that would produce surface
precipitation, and in particular the rerun initialized
at 1500 UTC was the closest to reality. In real time
during IHOP
forecasters saw
the 4-km run but doubted that such echoes could develop with the environment
that appeared to be in place, opting for a forecast of later
and weaker storm development than indicated by the model
(or than actually occurred). We are not certain at this stage
of our research why the runs initialized at 1800 UTC did not
perform as well as those initialized 3 hours earlier.
15 June 2002: Complex Case – All forms of convection
were evident in the 15 June 2002 IHOP case. This single
day began with early morning elevated storms, evolving
into a supercell storm that eventually produced a tornado,
moving to upscale growth of strong cells into an organized
line that bowed and accelerated southward out of the
domain. The actual focus of IHOP operations on this day
concerned where convective initiation would occur along
a dryline feature, which, like the rest of this case, was a
fairly complex feature with a double structure.
In examining the performance of the various models, we
will concentrate here on the convective types that occurred
rather than specifics of the dryline. Widespread
development of elevated convection over the Texas
Panhandle between 0800–0900 UTC was a forecast
issue for an early IHOP flight to investigate a low-level
jet. The storms eventually exceeded reflectivities of 50
dBZ at low levels, and persisted well into the daytime
hours (until around 1600 UTC). Fortunately, as forecast
by the Storm Prediction Center, the storms did dissipate,
allowing the rest of the day to become a very interesting
IHOP case. However, the development of the storms
was not anticipated by IHOP forecasters, and as is
typical in cases of elevated nighttime convection, was a
difficult forecast problem. A radar overview of the
storms is presented in Figure 11. The model simulations
from the 0600 UTC runs are depicted in Figure 12.
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Figure 11. Low-level reflectivity composites. Two strong surface-based storms are shown at the south end of the area (top left and right, 0900 UTC), as elevated convection develops to the north over the Texas Panhandle (bottom 1500 UTC).
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Figure 12. Model
simulations from the
0600 UTC 15 June
runs of the MM5 12-
km (top row), MM5
4-km (middle), and
WRF 12-km (bottom)
for the elevated convection
in the Texas
Panhandle. Reflectivity
is displayed as
before for the MM5
models, while the
WRF contours show
a composite and
image surface reflectivity. |
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At 0600 UTC (not shown) a couple of surface-based
storms formed at the southern end of the Texas Panhandle,
developing earlier in New Mexico and moving eastward.
These storms (shown in Figure 11) continue to move
southward with time. It is interesting that the Hot Start
method nicely initialized the LAPS runs (MM5 and
WRF) correctly with an echo at 0600 UTC, but the echo
was mostly lost within the first hour. Although loss of the
initial echo was a problem for other 0900 UTC cases
during IHOP and is the subject of ongoing work with the
Hot Start procedure, it appears particularly acute in
situations like this, where nighttime surface conditions
would not support surface-based storms. The area of
elevated storms developed north of the longer lived
echoes, and remained more or less in the same area,
peaking around 1200 UTC and diminishing rapidly after 1600 UTC. All three of the model simulations shown in Figure 12 that were initialized at 0600 UTC do develop some mid-level echo, but for the most part, it is not in the Texas Panhandle specifically, and is certainly slow to develop (for example, note the lack of any echoes at 0900 UTC). There are contrasting forecasts among the
three models, though, and apparent attempts at forecasting
the elevated storms. The MM5 12-km run shows some
significant surface echoes, though the southernmost
storm moved out of New Mexico apparently in the same
manner as the earlier strong storms. The more northern
cells develop in southeast Colorado and may well be the
models' forecast of elevated type storms. The MM5 4-
km run also shows these more northern storms extending
in a broken line from northwest to southeast. It is not certain what forced this line, but it could be more of a
development along a warm frontal type boundary that
was actually positioned somewhat farther east and
north. The WRF 12-km model appears to come closest
to positioning the mid-level echo correctly in the Texas
Panhandle, although it underpredicts the strength of the
storms with only limited surface reflectivity. (For the
WRF model the image shows surface reflectivity of 20
dBZ and above, with the white contours showing values
below 20 dBZ.)
The next feature of interest is whether the models could
predict a long-lived echo that formed from a group of
small cells east of Denver (near Limon) at 1500 UTC
that gradually grew as they moved east, with more or less
one main storm by 1800 UTC that then turned to the right
as it moved into western Kansas (see the reflectivity
images in Figure 13). This storm became supercellular
but did not produce a tornado until 2100 UTC after it
intersected a pre-existing north-south dryline (the IHOP
focus) and then moved southward along it. Although the
resolution of the model runs at 12 km (and to a lesser
extent, 4 km) would appear to be too coarse to successfully
forecast an individual storm, some surprisingly excellent
forecasts have been made with a 10-km version of the
MM5, so we were interested to examine the models for
this event.
For this case the storm formed beyond the domain of the
MM5 4-km model, and shown in Figure 13 are forecasts
from the MM5 and WRF 12-km models rerun after
IHOP using some improvements to the hotstart method.
The runs are both initialized at 0600 UTC so the forecasts
shown begin 15 hours into the run. Both runs seem to develop storms by 1500 UTC in the correct location in
eastern Colorado, strengthening the storm and moving it
at about the right speed to near the Colorado/Kansas
border by 1800 UTC. The model then continues to
strengthen the echo and turns it to the right, in pretty good
agreement with the actual behavior. The MM5 rerun
tends to have a more concentrated and stronger surface
echo then the WRF, but both have fairly impressive
forecasts considering the one valid at 2100 UTC is a 21-hour forecast. The IHOP MM5 12-km run (which
extended to 12 hours) from 0600 UTC was not as
successful as the MM5 rerun, but had a weaker echo in
about the same location. For unknown reasons, the
forecasts from the IHOP runs initialized for 0900, 1200,
and 1500 UTC were not very good in forecasting this
long-lived system. Even the IHOP MM5 12-km 1800
UTC run, with the storm already in progress, did not have
a good forecast as it tended to lose the initialized storm
for the most part by 1 hour into the forecast.
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Figure 13. Comparison of the 12-km resolution MM5 and WRF model reruns initialized at 0600 UTC on 15 June with composite low-level reflectivity (top row). Model images and white contours are surface reflectivity (image is 20 dBZ and greater), with dimmer contours composite reflectivity. |
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In summary, results are mixed for this aspect of 15 June;
on one hand the 0600 UTC runs indicate some fairly
impressive predictability, but inability to repeat this
predictability for the IHOP runs closer to the event is
curious. We hope to compare MM5 and WRF reruns
from 1200 UTC to the 0600 UTC reruns to see if the
storm was still forecast for these later model runs.
The final portion of the 15 June 2002 case that is
examined involves the organization of three areas of
convection into a squall line by 0000 UTC on 16 June that
then accelerates southward out of the IHOP domain by
0600 UTC. A radar overview of this evolution is shown
in Figure 14. At 1800 UTC the organized storm discussed
earlier is just crossing into western Kansas, and at 2100
UTC is at the western end of the line segment located in
southwestern Kansas. By 0000 UTC a line extends from
northern Oklahoma west-southwest into the Texas
Panhandle, with the eastern portion developed from the
area of cells that moved south out of Nebraska. After
0000 UTC, the line organizes and accelerates as it bows
over western to south-central Oklahoma. The model
forecasts from the 0600 UTC reruns of the MM5 12-km
are shown in Figure 15 and the WRF 12-km forecasts are
shown in Figure 16. The MM5 organizes a group of cells in Kansas at 2100 UTC into a line segment close to
where it is actually found at 0000 UTC, then accelerates
the line southward. Although the actual line moves
faster than the forecast, the track is similar and the model
forecast includes a bowing line as observed. Considering
that the later period of this forecast is an 18–24 hour
forecast, it is fairly impressive, with the model doing a
very good job of forecasting the organization into an
accelerating, bowing line. This line forms in about the
right place even though the MM5 essentially misses all of
the storms that around 0900 UTC began to form in a
north-northwest to south-southeast line from central
Kansas to west-central Nebraska. These storms
continued to expand in about the same place, and appear
to have been, at least initially, somewhat elevated type storms that developed just ahead of a warm frontal
boundary. The earlier times of this MM5 forecast never
included anything but some mid-level reflectivity, and
even then it was west of where the line actually occurred.
The difficulty in handling convection that may not have
been surface-based or forced by a distinct low-level
boundary is similar to the problems that all of the models
had with the elevated convection in the Texas Panhandle
discussed earlier.
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Figure 14. Series of
composite low-level
reflectivity images
showing the organization
of cells into a
fast-moving squall line
on 15 June 2002.
Images are every 3 h
beginning at 1800
UTC, with the
reflectivity scale as in
Fig. 9. |
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Figure 15a |
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Figure 15b |
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Figure 15c |
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Figure 15d |
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Figure 15e |
(Figure 15a, top; 15b, second from top; 15c, middle, 15d, second from bottom; 15e, bottom. Times correspond to the radar images.)
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A similar set of forecasts from the WRF 12-km rerun is
shown in Figure 16. The WRF forecasts have a little
more surface reflectivity than the MM5 forecasts, but
like the MM5 run also misses the warm frontal convection
discussed earlier. By 0000 UTC (compare Figures 15c and 16c), the forecast for the developing line segment is
similar to the MM5 and about in the same location,
though the WRF continues to produce far more echo
presence (and hence precipitation), with a large diffuse surface echo extending to the east-northeast of the line.
This is a better forecast than the MM5 for the extent of
echo if one compares it to the observed echo at 0000
UTC that shows an extensive area of moderate-strength
surface echo in about the same position as the WRF
forecast. After 0000 UTC the forecast is not quite as
good as the MM5 run with a smaller line that is located
a bit too far east. However, like the MM5 rerun, it is
impressive that the WRF model was able to predict the
upscale growth to a bowing line in about the right place
and about when it occurred. |
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Figure 16 a–e. As in
Figure 15 but for the
WRF 12-km rerun
initialized at 0600
UTC on 15 June.
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The MM5 runs during IHOP extended out only to 12
hours, compared to 24 hours for the reruns, so for
comparison, runs beginning at 1500 UTC for the 12-km
MM5 and at 1800 UTC for the 4-km MM5 will be shown.
The 1500 UTC MM5 12-km IHOP run is shown in
Figure 17. Note how the initialization from LAPS nicely
captures the ongoing convection at 1500 UTC (Figure
17a), although the storms are quickly lost, mostly in the
first hour. This occurred at times with MM5 during
IHOP, as noted earlier, and for this case may have been
exaggerated somewhat because much of this convection
near an apparent warm front may not have been surface-based.
Unfortunately there is such a loss of echo that by
the 3-hour forecast (valid at 1800 UTC), a composite
echo is forecast but none is predicted to reach the
surface. Right after 1800 UTC, however, the mid-level
echo shown entering northwest Kansas in the 1800 UTC
forecast strengthens rapidly, then expands to form the
line segment shown in the forecast valid at 2100 UTC.
This line segment then moves southward and strengthens
and expands, bowing somewhat at 0000 UTC but then
becoming more of a straight line by 0200 UTC. The line
in this forecast does not accelerate as fast as in the 0600
UTC forecasts from the WRF and MM5 reruns shown
earlier. |
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Figure 17 a–e.
As in Figure 15
except for the
MM5 12-km
forecast made
during IHOP
and initialized
at 1500 UTC.
Note that the
12-hour forecast
was not
available, so
the 11-hour
forecast valid
at 0200 UTC is
in Figure 17e.
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A comparison of the MM5 IHOP 12-km and 4-km runs initialized at 1800 UTC is shown in Figure 18. The two runs did capture the evolution to a line that accelerated and bowed with time. Organization into a stronger system with more bowing happens in the 4-km run ahead of the 12 km run, with the 4 km likely able to capture storm outflows better with its higher resolution. The 4-km run by 0500 UTC is still slower than reality with the position of the
line, but not by much. A similar
set of model runs for the 2100
UTC initialization, when the
convection was beginning to
organize more, is shown in Figure
19. Although there is some loss
of the system in the first hour of
the forecast after a good job of
initialization (Figures 19a and
19e), more is retained than in
some of the other runs because
of the presence of a stronger
echo at 2100 UTC. The MM5
12-km run is similar to the run
initialized at 1800 UTC, although
it develops a line sooner (by 0000
UTC) and ends up with a line
position by 0600 UTC closer to
reality and similar to the 0600
UTC MM5 rerun shown earlier
(Figure 15e). Interestingly, the
MM5 4-km run from 2100 UTC
does not organize the convection
into a line as fast as it did with the
1800 UTC run, and even at 0300
UTC has more of a broken line
(not as good a forecast). By 0600
UTC it organizes the line more
and accelerates it south of the 4-
km domain, similar to the movement
that was observed. |
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a)
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f) |
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b) |
g) |
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c) |
h) |
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d) |
i) |
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e) |
j)
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Figure 18 a–j,
right. Comparison
of MM5 4-km (left
column) and MM5
12-km (right) forecasts
from the 1800
UTC runs. Reflectivity
is shown, as
in previous figures.
Note that the
11-hour forecast,
not the 12-hour, is
shown in 18e and
18j.
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a) |
e) |
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b) |
f) |
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c) |
g) |
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d) |
h) |
Figure 19 a–h (from top left to
bottom right). As in Figure 18
except for the runs initialized at
2100 UTC 15 June 2002.
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It is apparent that all the models were able to predict the
upscale growth and organization of the convection into a
line with good location and timing for the most part.
There was good agreement between the different models
and usually between the different initialization times. A
consensus forecast from an ensemble viewpoint of the
various runs would have been a good one. The dprog/dt
method did not necessarily verify as well, however,
especially for the MM5 4-km runs, with the 2100 UTC
run not as good a forecast as earlier runs.
Summary and Future Work
The model forecasts examined here from two IHOP
days encompass a variety of forecast problems typically
encountered especially east of the Rocky Mountains,
including convective initiation along a dryline, prediction
of supercells, upscale growth and organization of storms
into a squall line, and the very tricky forecast of overnight
elevated convection. The forecasts presented well
represent the behavior of the models used during the
IHOP period, and indicate that there is potential for such
models to offer forecast guidance that can be valuable to
forecasters trying to predict convection. The model was
most successful when the convective initiation was
forced by a well-defined surface boundary, as in the 2
June 2002 case, and had the most difficult time with
storms forced by more subtle boundaries (like the warm
front on 15 June) or by no apparent surface boundary,
like the elevated storms in the Texas Panhandle on 15
June. Some of the forecasts of supercell formation and
movement, as well as upscale growth that occurred on 15
June were impressive, and there was even skill shown
for such developments beyond the typical 6–12-hour
limit that one might suspect for convective forecasts.
During IHOP, the RUC and MM5 special model runs by
FSL were extensively used to help make short-range
forecasts, with the models displayed on the FSL FX-Net
workstation. Partial examination of an extensive real-time
questionnaire completed by the forecasters for as
many model runs as possible during IHOP has yielded
constructive insight into various model issues that
occurred, as well as how much the forecasters trusted
some of the predictions.
Often these predictions carried far more detail as well as
forecast precipitation (convection) than would be indicated
by the operational models (Eta or GFS), and in some
cases, some forecasters needed a spin-up time to
understand whether the forecasts could be believed and
how best to use them. For this study, we will continue
completion of the analysis and questionnaires. We also
want to examine model performance over a broader
spectrum of IHOP days, not in the detail as was done for
15 June but more by phenomenon, such as the different
convective types discussed for this same case.
Editor's Note: A complete list of references and more
information on this and related topics are available
at the main FSL Website www.fsl.noaa.gov, by clicking
on "Publications" and "Research Articles."
(Edward Szoke is a meteorologist in the Forecast
Research Division headed by Dr. John McGinley.
He can be reached at Edward.J. Szoke@noaa.gov,
or at 303-497-7395.) |
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