After a quiet first two days during our operation times, we had the chance to do real-time operations for the pseudo-GLM over the north Alabama domain Wednesday. The SPC outlook had a slight risk over the Memphis and Nashville, TN as well as Huntsville, AL county warning areas covering the northern half of our domain. Wind was the predominant threat, but severe hail was a possibility. Forecasters started in the Memphis county warning area to get a feel for the PGLM product in the far western part of the domain and then transferred to Nashville and Huntsville later in the evening. Overall, few warnings were issued, but this was a good event to introduce forecasters to the PGLM in real-time.
I will add a few general comments and then include two images from the event. Overall, like the 24 May 2008 archived case, the impression was that the PGLM served as a good situational awareness tool. I then asked about the resolution of the product. Again, the response is that forecasters always want better resolution. In this case, though, the PGLM was adequate for what it was being used to analyze. One comment was that the PGLM was useful to see the convective cores, particularly during initiation. The NLDN has been used in this role, but the PGLM can give a few extra minutes lead time on initiation since most storms initiate with intra-cloud lightning before cloud-to-ground strikes. Another interesting comment after the event was that the PGLM could be very useful for coastal WFOs where the offshore data is typically less reliable.
I will switch gears and go into some of the interesting things we saw yesterday. One item came from Huntsville's Hytop radar. The PGLM showed a jump in activity at 0016 UTC and then decreased. This was followed by a significant increase in the radar reflectivity at 0027 UTC at the -20 C isotherm level. This raised the question, "Why did was the lightning jump followed by an intensification in the radar signature?" This leads into the discussion of how lightning jumps precede severe weather. Typically, a jump will occur and then the lightning activity will decrease ahead of the severe weather event as the storm core descends. However, yesterday, we saw the echo tops increase after the lightning jump. This is likely a case of larger hail aloft developing, which results in weaker charging in the updraft. The result is less lightning, but stronger reflectivities.
Another fun example is in the image below.

This screen capture shows the PGLM flash extent density (as the 8 km blocks) along with the NLDN cloud-to-ground strike locations with the '-' and '+' symbols in yellow. Notice how the majority of storms have NLDN strikes co-located with PGLM flashes. The exception is the circled storm moving into the extreme western section of the Huntsville (HUN) county warning area. This storm was just developing and the PGLM began detecting lightning activity ahead of the NLDN strikes. The forecasters liked how this feature can be useful in detecting the initiation of convective cells and I pointed out the utility of the advanced lead time for the first cloud-to-ground strike for public products like airport weather warnings.
The second image, below, is an interesting combination of the PGLM with the IR satellite data that I have not seen used previously by forecasters.

I was interested in seeing this particular overlay and asked about its utility. The response was for monitoring the location of the convective cores. The IR shows the coldest cloud tops where convection is occurring, although cirrus can obscure what is happening below. By overlaying the PGLM over the IR imagery, the PGLM focuses the forecasters attention on the actual cores.
Overall, this was a good real-time event that generated good discussions throughout the evening.