Joint NWS SOO–NASA SPoRT Workshop Huntsville, Alabama 11-13 July 2006 Convective (and Lightning)...
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Transcript of Joint NWS SOO–NASA SPoRT Workshop Huntsville, Alabama 11-13 July 2006 Convective (and Lightning)...
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Convective (and Lightning) Nowcast Products: SATellite Convection AnalySis and Tracking (SATCAST) System
John R. Mecikalski1 (Assistant Professor)Kristopher M. Bedka2
Todd A. Berendes1
Simon J. Paech1
and Laci Gambill1
1Atmospheric Science DepartmentUniversity of Alabama in Huntsville
2Cooperative Institute for Meteorological Satellite StudiesUniversity of Wisconsin-Madison
Supported by:
NASA New Investigator Program (2002) NASA ASAP Initiative
The NASA SPoRT Initiative
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Outline
• Current capability: OverviewConvective initiation (CI)
• BackgroundError assessments in Daytime CI 0-1 h NowcastingConfidence analysisIncorporation of MODIS informationDiscriminant scoring for CI --> QPE
• Current & new initiatives: 2006Impacts of microwave data toward 0-2 hour QPE forecastingNighttime CI forecastingLightning (event) & Lightning Initiation forecastingCI/LI Climatology as f(location, time of year)GOES-R Risk Reduction (using MSG & MODIS)
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Methods: Convective Nowcasts/Diagnoses
How is this done?
Determine the necessary data to evaluate convective and lightning initiation from satellite
Is satellite data the best??
If so, how can it be used? Why might it be superior to radar?
A: Satellites “see” cumulus before they become thunderstorms!A: There are many available methods for diagnosing/monitoring cumulus motion/development in real-time (every 15-min). See the published research on satellite data usage !!!
So, once well-read, all the pieces are in place to move the (science) forward in the CI nowcasting arena, with satellite analysis as the centerpiece for 0-1 h CI nowcasting.
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Where are we now …
• Applying CI algorithm over U.S., Central America & Caribbean• Validation & Confidence analysis• Satellite CI climatologies/CI Index: 1-6 h• Work with new instruments• Data assimilation possibilities
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Convective Cloud Mask
• Foundation of the CI nowcast algorithm: Calculate IR fields only where cumulus are present (10-30% of a domain)
• Utilizes a multispectral and textural region clustering technique for classifying all scene types (land, water, stratus/fog, cumulus, cirrus) in a GOES image
• Identifies 5 types of convectively-induced clouds: low cumulus, mid-level cumulus, deep cumulus, thick cirrus ice cloud/cumulonimbus tops, thin cirrus anvil ice cloud
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
“Mesoscale” Atmospheric Motion Vector Algorithm
“Operational
Settings”
New Mesoscale
AMVs
(only 20% shown)
• We can combine mesoscale AMV’s with sequences of 10.7 m TB imagery to identify growing convective clouds, which represent a hazard to the aviation community
50% shown
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
CI Interest Field Critical Value
10.7 µm TB (1 score) < 0° C
10.7 µm TB Time Trend (2 scores)< -4° C/15 mins
∆TB/30 mins < ∆TB/15 mins
Timing of 10.7 µm TB drop below 0° C (1 score) Within prior 30 mins
6.5 - 10.7 µm difference (1 score) -35° C to -10° C
13.3 - 10.7 µm difference (1 score) -25° C to -5° C
6.5 - 10.7 µm Time Trend (1 score) > 3° C/15 mins
13.3 - 10.7 µm Time Trend (1 score) > 3° C/15 mins
CI Interest Fields for CI Nowcasting
from Roberts and Rutledge (2003)
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
2000 UTC
2030 UTC
2100 UTC
CI Nowcast Algorithm: 4 May 2003
• Satellite-based CI indicators provided 30-45 min advanced notice of CI in E. and N. Central Kansas.
• PODs ~45% at 1 km (FARs ~40%)
• NEW Linear Discriminant Analysis methods provide ~65% POD scores for 1-hour convective initiation.
CI Nowcast Pixels
These are 1 hour forecasted CI locations!
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
An Example over the Tropics: CI
An example of the CI nowcasting method over
Central America:
• Real-time
• Every 30 min during the day (nighttime coming soon)
• GOES (MODIS soon)
• RED/GREEN pixels have highest CI probability
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
“Interest Field” Importance: POD/FARCI Interest Field Critical Value
10.7 µm TB (1 score) < 0° C
10.7 µm TB Time Trend (2 scores)< -4° C/15 mins
∆TB/30 mins < ∆TB/15 mins
Timing of 10.7 µm TB drop below 0° C (1 score) Within prior 30 mins
6.5 - 10.7 µm difference (1 score) -35° C to -10° C
13.3 - 10.7 µm difference (1 score) -25° C to -5° C
6.5 - 10.7 µm Time Trend (1 score) > 3° C/15 mins
13.3 - 10.7 µm Time Trend (1 score) > 3° C/15 mins
• Instantaneous 13.3–10.7 um: Highest POD (84%)• Time-trend 13.3–10.7 um: Lowest FAR (as low as 38%)• Important for CI & Lightning Initiation
8.5-10.7 m (MODIS)
> 0° C
> 0° C
3.7-10.7 m (MODIS)
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Use of MODIS in Convective Initiation Forecasts
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
• The lower right shows the supercooled water in green.
• Proof of concept for determining the difference between supercooled water and glaciated towering cumulus clouds.
Super-cooled tops:Lightning indicator as a function of convective
environment
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
New: CI/LI Linear Discriminant Analysis (LDA)
Some correlation between aconfidence in CI [f(LDA score)] and30-min dBZ (increase): QPE nowcast
• Improved POD of ~65and FAR of ~34%
• A virtual-radar from satellite
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
New: CI/LI Linear Discriminant Analysis (LDA)
Number of Interest Fields
Radar dBZ t=t+30 min
LD
A S
core
LD
A S
core
Low correlationHigh correlation
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Outline
• Current capability: OverviewConvective initiation (CI)
• BackgroundError assessments in Daytime CI 0-1 h NowcastingConfidence analysisIncorporation of MODIS informationDiscriminant scoring for CI --> QPE
• Current & new initiatives: 2006Impacts of microwave data toward 0-2 hour QPE forecastingNighttime CI forecastingLightning (event) & Lightning Initiation forecastingCI/LI Climatology as f(location, time of year)GOES-R Risk Reduction (using MSG & MODIS)
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Detecting Convective Initiation at Night
Detection of convective initiation at night must address severalunique issues:
a) Restricted to 4 km data (unless MODIS is relied upon)b) Visible data cannot be used to formulate cumulus maskc) Highly-dense, GOES visible winds are unavailable for trackingd) Forcing for convection often elevated and difficult to detect
(e.g., low-level jets, bores, elevated boundaries)
However, the advantages are:a) Ability to use ~3.9 m channel (near-infrared) data (!!!)b) More “interest fields” become available for assessing cumulus cloud
development
Therefore, new work is toward expanding CI detection fornocturnal conditions, and/or where lower resolution may bepreferred (i.e. over large oceanic regions).
Wayne Mackenzie, MS student
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Detecting Convective Initiation at Night
Nighttime CI: SoutheastOklahoma
Enhanced 10.7 m
SHV: 3:44 UTC
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Detecting Convective Initiation at Night
Use of 3.9 µm channel:
10.7-3.9 m channel difference (Ellrod “fog” product)13.3-3.9 m6.5-3.9 m
Evaluation is being done in light of the forcing for the convection (e.g., low-level jets, QG).
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006 kkoooooooookkkkkkkkkkk
Satellite-Lightning Relationships• Current Work: Develop relationships between IR TB/TB trends and lightning source counts/flash densities toward nowcasting (0-2 hr) future lightning occurrence•Supported by the NASA New Investigator Program Award #:NAG5-12536
• Incorporate in NWS Lightning Hazard/Prediction Tool
2047 UTC
2147 UTC
Northern Alabama LMA Lightning Source Counts
2040-2050 UTC
2140-2150 UTC
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006kkkkkkkkkkkkkkk
2040-2050 UTC
2140-2150 UTC
Northern Alabama LMA Lightning Source Counts
Lightning InitiationPotential
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
GOES CI Interest Fields: 21 July 2005 (afternoon)
CI Climatology Research
Details:-topography-main updrafts
…for LI1 km Resolution
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
Hyperspectral: GOES-R & GLM
LEFT8.508-10.98 m Band
Difference: Red (’s >0)
= Ice
Comparison between the 10.98
m (right) and 11.00 m (far right) bands:
22 UTC 6.12.2002
Small wavenumber changeresults in significant changesin view: Low-level water vapor Surface temperature Subtle cloud growth& microphysical changes
Joint NWS SOO–NASA SPoRT Workshop
Huntsville, Alabama 11-13 July 2006
For the NWS … Real-time use & evaluation
In addition
A web-basedevaluationis beingperformedin a post-shift formatduringJuly andAugust 2006.
Smoothing...