10AM
Day 2 of the experiment brought another Moderate Risk region from the SPC, driven by a 30% CIG 2 Hail outlook. Thunderstorms were expected to form along an advancing dry line, with a diffuse temperature and moisture gradient in place from southern Oklahoma to northern Alabama as of 15Z. After our morning debrief, the Fort Worth-Dallas office (FWD) was a pretty easy pick for us to target today. After more discussion, we decided our second WFO should be further east ahead of some early morning convection in the Jackson, MS (JAN) office. Unfortunately the Lightning Stoplight product continued to face ingest issues and was unavailable today, and we hope to have it in AWIPS tomorrow. In the meantime forecasters viewed that data on the SPoRT Lightning Viewer and in GR2Analyst.
1 PM
Forecasters today were tasked with issuing simulated Severe Thunderstorm and Tornado warnings in WarnGen on AWIPS-II, along with providing decision support for mock-events that we created for each office. Today FWD was tasked with mock-DSS for a Red River BBQ Cookoff near Gainesville, TX, and JAN was tasked with mock-DSS for a hazmat spill near Waverly, MS. Shortly after operations began, CI occurred just west of the FWD CWA, and thunderstorms were maturing just west of the JAN CWA. This gave everyone plenty of storms to observe, and the forecasters with the chance to issue warnings and communicate hazards through decision support.
I spent part of the day in ops viewing the SZA imagery product on the west coast shortly after sunrise. When comparing SZA data in a modified Day Cloud Phase Distinction RGB against the traditional RGB, the differences are stark right at sunrise, and features stand out sooner. How much sooner is something we need to determine. There was a nice discussion in the morning about how SZA imagery may benefit WFOs in higher latitudes (main example: Alaska). I also compared the modified SZA RGB against CIRA’s GeoColor imagery, and found that more interesting than anything.
When zooming into the SZA imagery in north Texas, it appears the 0.69µm (channel 2) imagery has ‘gaps’ in highly reflective features. My first hypothesis is that the solar zenith adjustment is pushing reflectance factor values above 130% and creating plotting issues in AWIPS, but I feel like traditional ABI visible imagery saw similar artifacts in AWIPS after launch that had to be corrected.
Kevin







