DYNAMO/AMIE
S-PolKa Summary for 24 October 2011

Convective Outbreak Near S-PolKa

Prepared by
Robert A. Houze, Jr., Kristen Rasmussen, Stacy Brodzik, and Scott Powell

NOTE: This report may may be updated as new information becomes available,
and it may be accessed alternatively at:

http://www.atmos.washington.edu/~houze/DYNAMO-AMIE/

 

Yesterday was a major rain event at Gan and over the whole area scanned by the S-PolKa radar. The total rain area and rain amount over the radar area are shown in Figure 1 along with curves showing the breakdown into convective and stratiform components. Before 0400 UTC, the convective rain amount (upper panel) was greater than the stratiform. After that the rain was predominantly stratiform over the radar area. The rain area (lower panel) was mostly stratiform for the entire period. This rain event was associated with a giant ring of convection of the type we discussed in our 22 October summary. However, in that event S-PolKa observed convection on the edge of the ring at a late stage. In this event, S-PolKa observed convection in the outbreak that was the source of the ring that propagated outward. The METEOSAT imagery in Figure 2 provides an overview of the sequence. The first image (1400 UTC) was before the event started. At this time, significant convection was well east of Gan and over the Revelle (location NE). The Revelle radar was observing a mesoscale echo system with SW-NE and WSW-ENE oriented lines of convection and associated stratiform precipitation areas (left hand panel of Figure 3). The line west of the Revelle at this time was propagating toward the ship. However, this mesoscale convection was not ultimately associated with what occurred subsequently over the S-PolKa area. The 1830 UTC image in Figure 2 shows several small cells of high cloud tops appearing between the Revelle and Gan. These cells are the beginning of the outbreak observed by S-PolKa. In the next two panels, these cells were growing larger and moving into the S-PolKa area. By 0440 UTC (fifth panel of Figure 2 ) it was raining steadily at Gan. The radar sequence during this time will be discussed in some detail below. By about 0840 UTC, the ring of convection could be identified from the satellite infrared image. The cold cloud tops had moved SW of Gan, there was some clearing between Gan and the Revelle, and the Revelle radar was seeing mesoscale rain areas with embedded convective cells (right panel of Figure 3). The giant ring of convection continued to expand through 0030 UTC 25 October 2011 (last four panels of Figure 2 ). Figure 4 shows the echo pattern seen on the S-PolKa S-band radar at 0100 UTC. The area to the east of S-PolKa was convered by radar echo and WSW-ENE oriented lines of convection were located to the west. One line was extending nearly directly over Gan at this time and intersecting the stratiform region. Although a great deal of stratiform rain was to the east of the radar, the rightmost panel of Figure 4 shows that convective cells were embedded in the stratiform region. As will be shown by cross sections below, these cells were very deep and intense. Time-lapse viewing of the images shows that the cells in the lines to the west were moving eastward into the stratiform region, while the stratiform region was moving westward. Figure 5 shows the time  sequence of the radar echo pattern on the S-PolKa S-band radar for a little over five hours. Where the lines of convection to the west were intersecting the stratiform zone, very intense convective cells were seen, for example ENE of the radar at 0146 UTC and in the SE quadrant at 0246 and 0316 UTC. After that time (0446 and 0701 UTC in Figure 5), intense convection was still present but just out of radar range, as seen in the satellite image in the last panel of Figure 5.

At 0146 UTC, the S-PolKa S-band PPI shows one of the WSW-ENE bands west of Gan intersecting the radar site and Gan Island. The DOE Gan KAZR vertically pointing Ka-band radar obtained an interesting time section of this event (Figure 6). It shows downdraft at about 0117 UTc over ridden by updraft. The upper extension of the updraft slopes upward from ~0130-0145 UTC. The updraft speeds exceed 5 m/s.

The S-PolKa rain maps at 0200 (Figure 7) illustrate the intersection of the intense convective cells in the lines to the west with the large stratiform region to the east. The embedded cells in the stratiform zone appear to be extensions of the lines into the stratiform region, and much of the stratiform region contains embedded cells, some of which were very intense. Figure 8 shows the structure of an intense cell to the east. This cell was reaching over 17 km in height (lower left panel). The radial velocity data showed a gust front at about 105 km and a divergent signature near echo top. A convective-scale patch of enhanced outbound radial velocity is seen at the cell location in the PPI (upper left panel), indicative of downward transport of westerly momentum. The polarimetric particle identification pattern (upper and lower left panels) shows heavy rain at low levels with the cell lofting larger ice particles (light blue) to about 15 km height. Graupel signatures are seen both above and below the melting layer, both in the active cell and in the heavier stratiform zones surrounding the cells. The latter signatures are consistent with the stratiform precipitation being formed as convective cells collapse. The rain pattern over the S-PolKa region at 0300 UTC (Figure 9) look much the same as at 0200 UTC. Figure 10 shows another example of an intense cell embedded in the stratiform echo reaching about 17 km. This cell is so intense that it seems to have produced some upper-level clearing on either side of the cell, as if by upper level downdrafts responding to the buoyancy in the cell. The particle identification signatures (lower right) show a strong graupel signature right above the 0 deg C level and also some possible graupel mixed with the rain below. As in the other example, larger (more reflective) ice particles were being carried up to about 15 km. Figure 11 shows an example similar to the previous two examples in all respects. The radial velocity footprint of momentum transport is particularly strong in this case (upper right panel). Figure 12 shows an example of one of the embedded cells in the process of collapsing and turning into stratiform echo. Apparently, cells fed into the zone of widerspread echo from the west, grew into very intense cells, and collapsed into dense stratiform echo, which in turn was advected back westward.

Figure 13 shows that the S-PolKa rain pattern at 0400 UTC still contained substantial convection embedded in the broader stratiform echo pattern. At this time the S-PolKa site was under this echo region. Figure 14 shows the overcast and rain at 0419 UTC.  It is interesting that the cloud base was low. The stratiform cloud was not midlevel-based as might have been expected. At 0600, the precipitation on radar was nearly all stratiform (Figure 15). The Gan 0600 UTC sounding had a Zipser "onion" profile, of the type associated with stratiform anvil clouds (Figure 16); the warming and drying below 600 hPa gives the sounding an onion-like shape on the Skew-T diagram. The 0800 UTC rain pattern on S-PolKa was nearly all stratiform (Figure 17). However, the METEOSAT infrared satellite underlay in Figure 17, shows extremely cold cloud tops (~200 K) to the southwest, just beyond the maximum range of S-PolKa. The deep convection was evidently still active in this region, just out of radar range. The World Wide Lightning Location Network data show a lightning strike in the region (Figure 18), which is consistent with the large ice particles that we have seen being lifted to high levels (Figures 8, 10, and 11).

After the major event just described, a line of covection orinted SW-NE moved across the northwest quadrant (Figure19). It had a well defined gust front with (lower panel). The relationship of this line of convection to the other events of the day remains unclear.


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Figure 1. Rain area coverage and accumulation over the area covered by S-PolKa. Computed from polarimetric variables and the MISMO Z-R relation.



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Figure 2. METEOSAT Infrared images for 23-24 October 2011.

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Figure 3. Revelle C-band radar images from the 23 and 24 October 2011.




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Figure 4. From left to right, S-PolKa S-band reflectivity, polarimetrically derived rain rate, and convective (yellow) and stratiform (red) rain areas for 0100 UTC 24 October 2011.

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Figure 5. S-PolKa S-band reflectivity field for 24 October 2011, except last panel, which shows a METEOSAT infrared image with S-PolKa 150 km range ring highlighted.

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Figure 6. DOE KAZR vertically pointing Ka-band radar image for 0100-0200 UTC 24 October 2011.


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Figure 7. From left to right, S-PolKa S-band reflectivity, polarimetrically derived rain rate, and convective (yellow) and stratiform (red) rain areas for 0200 UTC 24 October 2011.




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Figure 8. S-PolKa S-band radial velocity and particle identification fields at 0.5 deg elevation at 0146 UTC 24 October 2011 (upper panels) and RHIs of reflectivity, radial velocity, and particle type along the yellow line in the (lower panels).




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Figure 9. From left to right, S-PolKa S-band reflectivity, polarimetrically derived rain rate, and convective (yellow) and stratiform (red) rain areas for 0300 UTC 24 October 2011.


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Figure 10. S-PolKa S-band reflectivity at at 0.5 deg elevation at 0252-0258 UTC 24 October 2011 (upper panel) and RHIs of reflectivity (lower-left panel) and polarimetric particle type (lower-right panel) along the yellow line in the upper panel.


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Figure 11. S-PolKa S-band reflectivity and radial velocity fields at 0.5 deg elevation at 0316-0328 UTC 24 October 2011 (upper panels) and RHIs of reflectivity (lower-left panel) and polarimetric particle type (lower-right panel) along the yellow line in the upper panels.




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Figure 12. S-PolKa S-band reflectivity and particle identification fields at 0.5 deg elevation at 0346-0357 UTC 24 October 2011 (upper panels) and RHIs of reflectivity (lower-left panel) and polarimetric particle type (lower-right panel) along the yellow line in the upper panels.


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Figure 13. From left to right, S-PolKa S-band reflectivity, polarimetrically derived rain rate, and convective (yellow) and stratiform (red) rain areas for 0400 UTC 24 October 2011.

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Figure 14. Photo looking east from S-PolKa at 0419 UTC 24 October 2011.



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Figure 15. From left to right, S-PolKa S-band reflectivity, polarimetrically derived rain rate, and convective (yellow) and stratiform (red) rain areas for 0600 UTC 24 October 2011.

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Figure 16. DOE Gan sounding for 0600 UTC 24 October 2011.



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Figure 17. From left to right, S-PolKa S-band reflectivity, polarimetrically derived rain rate, and convective (yellow) and stratiform (red) rain areas for 0800 UTC 24 October 2011.


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Figure 18. World Wide Lightning Location Network flash freqency for the 30 min preceding 1000 UTC 24 October 2011 superimposed on the METEOSAT infrared image. 

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Figure 19. S-Polka radar reflectivity (upper panel) and radial velocity (lower panel) fields at 0.5 deg elevation for 1216 and 1301 UTC 24 October 2011.