Summary – 27 May 2008

Our four visiting forecasters arrived ready to work, and the day promised a fair chance of Oklahoma-based operations. After a quick tour of the National Weather Center, the group convened in the NSSL Develoment Lab for orientation, followed by a map discussion. Participants were trained on the PAR and CASA data platforms before moving to the Hazardous Weather Testbed around 21 UTC. Software training for the WDSSII used real-time data of a supercell occurring near Altus, OK.

Kevin (WFO OUN) and Eric (WFO AFG) then jumped on at the PAR workstation to dissect the Altus supercell at long range. Brad (WFO SEA) and Mark (Environment Canada – Winnipeg) practiced WDSSII using KFDR data on the same supercell, and were on standby for possible CASA operations. By 23 UTC, though, it became clear that thunderstorms would propagate southward into northwest Texas…as stable air emanating from a second storm complex had overspread the CASA domain.

By 2330 UTC…real-time operations ended, and both groups of forecasters turned to archive events. The pace slowed down, allowing more time for discussion of data strengths and weaknesses. The PAR data, in particular, spurred some interesting ideas as to what forecasters would ideally like to receive from a radar system. The CASA participants expressed some difficulty operating in a small domain using multiple radars. They also noted that the KTLX 88D better sampled one occurrence of strong straight-line winds, simply owing to viewing angle. They were impressed, however, at the temporal and spatial resolution of the CASA data which captures many interesting storm and sub-storm scale features.

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Live Blog – 27 May 2008 (6:29pm)

Storms in western Oklahoma have either weakened or moved southward to very long range from central Oklahoma radars. Today’s severe potential is largely driven by the diurnal cycle, and there is little hope of additional activity; the MCS outflow from this morning simply proved too deep and widespread across central Oklahoma. The event did provide Eric and Kevin a chance to become familiar with PAR data, and they will continue that theme by working an archived event this evening.

Eric and Kevin Examine archived PAR data.

Meanwhile, Brad and Mark are viewing archived CASA data to increase their comfort level with the look and feel of that data. Between 2330 UTC and 0130 UTC they plan to run through another event in real-time playback to evaluate the utility of CASA data in making warning decisions.

Brad and Mark work with Jerry Brotzge viewing archive CASA data.

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Live Blog – 27 May 2008 (5:40pm)

PAR Temporal Resolution Discussion…

Eric & Kevin are working the Altus storm… and their first look at PAR and 88D side by side has sparked discussion of the differences in resolution and sampling techniques. Kevin would like to see enhanced azimuthal resolution (lower beam width) for PAR in the future. Kevin remarks that the 1-minute update has made it easier to pick up on new cell development along the storm’s rear outflow flank. The forecasters earlier observed a supercell split on the Elk City storm…and felt the rapid updates were beneficial to seeing this.

Eric has another interesting perspective. He thinks the 1-minute resolution might be “annoying” early in an event when you don’t yet have a particular severe weather threat or focus. It may be overwhelming to process so much data. Maybe we should apply the forecast funnel to this… and be able to choose when to switch from 5 or 10 minute resolution down to the 1-minute resolution as needed.

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Live Blog – 27 May 2008 (4:57pm)

PAR operations underway…

Kevin and Eric will begin Phased-Array operations centered on the Altus, OK, supercell. Mark and Brad will practice interrogating WSR-88D data using WDSSII while being on standby for either CASA operations or a CASA archive case later this evening.

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Live Blog – 27 May 2008 (4:41pm)

Western OK…IOP begins 5 PM

Forecasters completed PAR and CASA Training, and are now learning WDSSII using live data of a supercell near Altus, OK. There is a second severe storm near Elk City. Both storms are moving very slowly…seemingly balanced by southeasterly low level inflow and southwesterly mid level steering flow. They may also tend to propagate into the instability axis…which is unfortunately just west of the CASA network. With some luck, however, we could see storms reach the western parts of CASA later this evening. PAR operations will begin at 5 pm.

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Live Blog – 27 May 2008 (3:16pm)

Training Continues…3pm

The SPC has placed southwest Oklahoma, including most of the CASA domain, under a Severe Thunderstorm Watch until 03 UTC. The outflow boundary has zipped up with a pre-frontal trough from Shattuck to Mangum, OK. Scattered CBs have formed off and on in this zone…but none have quite taken hold, as convergence and lift remain quite shallow. Other thunderstorms have begun to sustain themselves farther south along the trough axis into Texas. Opportunity for more robust convective initiation should increase up into Oklahoma with additional heating/destabilization. Water vapor imagery also hints at the influence of a short wave ridge exiting western Oklahoma…with a more diffluent upper flow pattern approaching from eastern New Mexico/West Texas.

The forecaster/evaluators have switched places so that both sets of two will receive training on both the PAR and CASA experiments. The Oklahoma IOP will either begin at 4pm (WDSS training on the fly) or 5 pm (WDSS traning at 4pm).

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Outlook – 27 May 2008

Our four forecaster/evaluators (Eric Stevens, Brad Colman, Mark Melsness, and Kevin Brown) arrived at the NWC early this afternoon, and are ready to hit the ground running in this Holiday-shortened week. Today should be our best chance for a central Oklahoma IOP, so we have split the forecasters among PAR and CASA for training on those programs through 3 pm. After checking the weather… we may be able to swap and allow the groups to train on both programs. If weather dictates that operations begin prior to 5 pm, however, we will forego WDSSii Training. Kevin has WDDS experience, and other scientists are available to either drive WDSS or train the other forecaster “on the fly.”

The forecast is for thunderstorms to initiate near the intersection of a cold front and outflow boundary in northwest or west central Oklahoma. Other storms may initiate farther south along the outflow boundary toward southwest Oklahoma and western north Texas. Storms should then move east and southeast toward the PAR and CASA domains, although some southward propagation may occur within the instability axis. The northeastward extent of this activity toward central Oklahoma is somewhat in question…as that area was overturned by an MCS earlier today. At worst…we expect a few severe storms at long range but within the PAR domain. At best…we could have severe storms in both the PAR and CASA domain by early to mid evening. The Shear/CAPE combination is sufficient for rotating storms…and even a tornado threat just east of the outflow boundary…although weak mid level winds may lead to a quick transition toward high precipitation character.

Patrick Burke (EWP Weekly Coordinator, 27-30 May)

Tags: None

Week 4 Summary: 19-23 May 2008

This week, visiting participants included Steve Hodanish (WFO Pueblo, CO), Jonathon Howell (WFO Memphis, TN), Ryan Knutsvig (WFO Elko, NV), Steve Rogowski (WFO Sterling, VA), and Dave Patrick (Environment Canada, Winnipeg) as full-time participants. Other participants this week included Mike Magsig (WDTB), Paul Schlatter (WDTB), Don Rude (U. Virginia), Jerry Brotzge (OU) and an NSSL support team of Kevin Manross, Kiel Ortega, Kristin Kuhlman, Pam Heinselman, Dave Preignitz, Angelyn Kolodziej, and Greg Stumpf. Travis Smith (NSSL) was the Weekly Coordinator.

Monday, May 19:

There was very little threat of significant severe weather anywhere in the CONUS today, which made it an ideal training day for our visitors. The afternoon consisted of general orientation, map discussion, CASA & PAR orientation, and WDSSII training. In the evening, the forecasters participated in probabilistic warning guidance training on some real-time data SW of Brownsville, TX (issuing warning guidance for Mexico!)

Tuesday, May 20:

PAR and CASA playback cases in the afternoon, followed by a probabilistic warning IOP starting around 4pm CDT. The area of interest is the Carolinas and Georgia. A detailed summary of the post-event discussion for this case can be found in the blog entry “20 May 2008 – Summary”.

Wednesday, May 21:

Similar to yesterday – PAR and CASA playback cases in the afternoon, followed by an IOP around 6pm for NE Colorado. A detailed summary of the post-event discussion for this case can be found in the blog entry “21 May 2008 – Summary”.

Thursday, May 22:

HP Supercell event in Oklahoma, outside the PAR domain, but we worked it anyway to try to get the forecasters a real-time event.

Friday, May 23, Summary Discussion

CASA – no real-time operations this week.

  • Dave: really like the assimilated data display, saw it as advantageous to look at velocity data as vectors as opposed to the radial velocity display.
  • SteveH: 2D Wind display was a bonus.
  • Several forecasters like the idea of a 2D wind field presentation.
  • SteveH: would like to see data out to 60 km, or some way to see the big picture.
  • SteveR: not confident in the sectored scanning.
  • Dave: wants to make sure he can see low-level boundaries.
  • Need a visual cue for the cross-sections.
  • Dave: cross-section is overkill,
  • SteveH: can do the same thing better with rapid scan of sector
  • Dave: would like RHI capabilities.

PAR

  • SteveH: 100% wind/hail for HP supercell was a no-brainer, tornado was not so clear. Noisy, range-folded. Reflectivity was excellent, however, and FSI cross-sections were very useful. Thinks it will be a huge improvements once it gets the bugs out. Was most impressed by pulse storm playback case – can see core development aloft (rather than by luck with 88D).
  • Jonathan – good tool to update warnings as well. Can see more variation in intensity, see microbursts, etc.
  • No one uses detection algorithms in their offices, except for the gridded MESH. SteveH: can better interpret the raw data than algorithms. Need to be able to trust the algorithms (like MESH).
  • Dave: likes algorithms, if they are trustworthy.
  • Everyone liked the pulse storm case – “Pulse storms are a pain…!” – SteveH.
  • Jonathan: can see between volume scans.
  • This could help with longevity of warnings.
  • “The fire hose is coming, but that’s why they teach the fireman how to hold the hose!” – Steve H
  • Jonathan – not going to be a big change, things will look the same as the 88D (same conceptual models).
  • 3D will be valuable in the future – need to be integrated into operational system – lots of things need to be learned about it.
  • Scan strategies? SteveH: does it need to be adaptive? It already scans really quickly.
  • There are trade-offs with high-resolution temporal versus spatial sampling.
  • SteveR: higher resolution at lower tilts would be nice.
  • They would like to show some simulated cases to their staff. Could do in FSI. Have other training priorities, but could be worked in.

Probabilistic warning guidance:

  • Ryan: new way of thinking. More sophisticated users will love it.SteveH: thinks it is straightforward for forecasters.
  • Jonathan – protecting life is the primary objective; need to be clear on call to action (yes/no answer for most users)
  • SteveR: we could do both methods –
  • SteveH: need training to forecasters on what the probabilities mean. Need to train public is more important though – forecasters
  • SteveH doesn’t like the future trend prediction. Didn’t know what to do with it (forecasting the short-term intensity variations is very difficult)
  • Need organizational software

May 30 playback case:

  • Mark is very comfortable with a high level of automation, even for low-end warnings, so long as forcaster has final approval. Canadian way of doing things.
  • Eric thought the workload for the prob warn playback case was about right.

General final thoughts:

  • SteveR: exceeded expectations
  • SteveH: tour of SPC would be nice
  • All: Good pace – they were here to work, so no problems.
  • SteveH: more training on probabilistic warning tools. Had a good experience.
  • Dave: was action filled.
  • Jonathan: send out WDSSII to offices beforehand.
  • Jonathan: had a very good experience
  • They would come back next year.
  • SteveH: wants 30-minute training sessions.

Travis Smith (EWP Weekly Coordinator, 19-23 May)

Tags: None

Forecaster Thoughts – Jonathan Howell (2008 Week 4)

The Hazardous Weather Testbed (HWT) provided an excellent opportunity for forecasters to work side by side with researchers to evaluate radar technology and warning strategies developed for future use.  While participating in the experiment, I had the opportunity to evaluate the Phased Array Radar (PAR) and the Collaborative Adaptive Sensing of the Atmosphere (CASA) radars in both a real-time and archived environment.  Our group also tested the new experimental process which integrated short-term severe threat probabilities into operational severe thunderstorm and tornado warnings.  The outcomes of the experiments demonstrated potential significant advantages and challenges if implemented into an operational weather forecast office (WFO) setting.

My experiences with the PAR radar equipment were very positive.  This technology will likely exceed the capabilities of the current WSR-88D radar network.  The primary advantage to using the PAR radar technology is the rapid update of base radar data.  During the experiment, I was able to rapidly identify important convective structural features that led to quicker warning decisions and longer warning lead times.  Another important advantage of the rapidly updating PAR data was the ability to identify important storm features in the 1 minute PAR data that would not have been sampled by the 5 minute WSR-88D scans.  In addition, the 1 minute update PAR data better portrayed storm evolution.  This was particularly advantageous during an archived unorganized pulse severe thunderstorm event which we used the PAR radar to conduct warning operations.  As a warning decision maker, I was able to observe the initiation of collapsing cores aloft and issue warnings with enhanced lead time.  The current scan limitations of the WSR-88D likely would have further delayed my decision to warn during this event.

Advantages of the PAR radar exceed any limitations that I experienced.  The only minor limitation to the PAR radar will be the ability of the radar operator to adjust to the much faster influx of additional radar data.  I think this will primarily be an initial challenge which will be overcome quickly by warning forecasters.  In fact, I felt comfortable with the increased radar data flow after a few days of use.  Overall, my experiences using the PAR radar were very positive and I hope that this technology will eventually be implemented into the NWS field offices.

Another radar system which we experimented with was the CASA radar network.  The CASA radars also proved to be a robust network that provided advantages to warning forecasters during experimental warning operations.  As is the case in most NWS County Warning Areas (CWA) and in the Memphis CWA, sampling low-level storm characteristics using the current WSR-88D radar network at extended distances from the radar is very difficult or impossible due to radar spacing issues and curvature of the earth.  This greatly limits warning forecaster’s ability to observe important low level storm at large distances from the radar.  The greatest advantage that I see to implementing the CASA radar network is the ability to limit gaps in low-level radar coverage.  This will provide warning forecasters with improved radar information necessary for longer lead time and improved warnings.  In addition, enhanced low level radar information allows warning forecasters to better define geographically where the greatest storm threats exist.  While participating in the HWT, I experienced these benefits firsthand.  The CASA network would likely be best implemented as a compliment to the PAR radar network.  By locating CASA radars in between the traditional PAR (current WSR-88D sites) radars, the system would become very robust and most beneficial to the NWS warning process.

The HWT also tested the capabilities and practicality of probabilistic warnings.  Probabilistic warnings appear to present the greatest challenge of all the new techniques tested.  Researchers envision probabilistic warnings eventually replacing current NWS warning practices.  As a forecaster using the new probabilistic warning technique, I found the process difficult to employ and likely confusing to the public.  The primary limiting factors of probabilistic warnings in my opinion include, (1) quantifying specific threats and expressing those threats in a proper manner to the public, (2) warning forecaster work load issues, and (3) public response problems associated with different threat percentages.  The NWS mission statement clearly reflects the important role that severe weather warnings play in protecting life and property.  The primary reason that the NWS issues severe weather warnings is to encourage the public to take actions required to protect themselves from dangerous weather.  I believe that eliciting public response to probabilistic warnings will be a significant challenge since every person’s threat threshold is different.  Probabilistic warnings may create confusion and limit public response to warnings and should primarily be available only to very high end users (if they can understand the process and find it beneficial).

Overall the HWT was a great opportunity for me to evaluate potential NWS technology of the future.  Collaboration between researchers and operational forecasters is a great way to share ideas, provide feedback, and get useful technology into NWS field offices.  The HWT and similar collaborative experiments hopefully will continue into the future.  I look forward to the eventual release of new and improved technology into the field.  Finally, I would like to thank those involved for giving me the opportunity to participate in this experiment and hope to again be involved in similar projects in the future.

Jonathan Howell (NWS Memphis TN – Week 4 Participant)

Tags: None