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RESEARCH POSTER PRESENTATION DESIGN © 2015 www.PosterPresentations.com b) c) a) Introduction During the late morning of 16 December 2015 an EF2 tornado occurred 4 km southeast of Australia's busiest airport Sydney Airport. This tornado was notable in many ways: A relative abundance of observations was available, including the Kurnell C-band Doppler radar located less than 2 km from the tornado path The parent supercell tracked over water just off the east Australian coast during its life cycle, apart from when it briefly crossed the Kurnell peninsula when the tornado occurred. The tornado passed very close to an Automatic Weather Station (AWS) located on a jetty in Botany Bay at Kurnell which recorded a wind gust of 59.2 m s -1 (213 km/h, 115kts, 132mph) at 10:33 am local time. The wind gust measured by the Kurnell AWS is an Australian record outside of a tropical cyclone. There were several RFD pulses and strong gate to gate velocity couplets associated with the parent storm prior to the tornado Damage from the tornado was extensive with the Insurance Council of Australia reporting it to be the most costly disaster of the Australian 2015/2016 summer, costing insurance companies AU$206m. Kinematic assessment of Mesocyclone and Tornado Cyclone Thermodynamic Assessment of Pre-storm Environment Summary and Points for Discussion Doppler Radar and Storm Environment Observations of a Maritime Tornadic Supercell in Sydney, Australia Harald RICHTER 1 , Joshua SODERHOLM 2 , James TAYLOR 3 , Alain PROTAT 1 #155 1 Research and Development Branch Bureau of Meteorology, Melbourne, Australia 2 Climate Research Group University of Queensland, Brisbane, Australia 3 Extreme Weather Desk, Bureau National Operations Centre Bureau of Meteorology, Melbourne, Australia Dual Doppler winds were derived using Terry Hills S-band Doppler radar (~36km to the north of Kurnell) and the Kurnell radar (1.6km to the east of tornado track) The tornado parent cyclone appears as a zone of strong convergence / vorticity in the southwest corner of a ~7 km wide low-level mesocyclone refer figure 6 Just prior to tornado formation the storm ingested localised patches of enhanced 0.2-1 km storm-relative helicity (SRH) refer figure 7 The key contributor to the overall SRH values appears to be a 'vorticity sheet' within the storm inflow layer where the north-easterly inflow backs to north-westerly refer figure 8 AMDAR hodographs confirm very strong spatiotemporal variability in the SRH refer figure 9 Figure 7: 0.2-1 km AGL storm-relative helicity based on the dual-Doppler derived wind profile (shaded). Wind vectors are shown at 500 m AGL and also derived from dual Doppler. Storm motion (subjectively derived from Kurnell radar data around tornado time) used is 7.5 m s -1 towards 19 degrees. Bold contours show 35, 45, 55 and 65 dBZ outlines at 500 m AGL. Figure 1. Kurnell Doppler Radar imagery at 2319 UTC (10:19 am LT) at 0.24 o elevation; a) PPI reflectivity; b) PPI Doppler radial velocity. a) b) Figure 2. a) Approximate supercell storm track from 2130 UTC 15 December to 0030 UTC 16 December ; b) Tornado damage at Kurnell. c) Enhanced still frame from video showing tornado (Courtesy of Peter Grassmayr) Figure 3. One minute data from Kurnell AWS impacted by tornado. Black line indicates wind speed in knots (using left axis) and yellow line indicates wind direction (using right axis). Figure 10. a) 18 UTC 15 December 2015 ACCESS-R (red) model sounding and 19 UTC 15 December observed Sydney Airport sounding (black); b) Soundings based on a 6-hour forecast from the 18 UTC ACCESS-R run valid at 23 UTC (red), the 2256 UTC AMDAR (blue), the 2258 UTC AMDAR (green) and the 2311 UTC AMDAR (black); c) Hourly soundings at 18 UTC (black), 19 UTC (red), 20 UTC (blue) and 21 UTC (green) based on the 18 UTC run of ACCESS-R indicating the rapid removal of inversion prior to the Kurnell tornado. Figure 5 (right). Sydney airport AMDAR flight paths with height and time of data relay and 2306 UTC radar reflectivity overlay; Red 2256 UTC ascending; Orange 2258 UTC ascending; Yellow 2311 UTC descending. Figure 6. Dual Doppler winds at 2325 UTC at 1.5 km AGL(left) and 2331 UTC at 2.5 km AGL (right). Color fill is the corresponding reflectivity from the Kurnell radar. Winds shown as vectors with increased length corresponding to increased speed. 23:31 UTC 23:25 UTC 23:19 UTC 23:13 UTC Figure 8: Vertical profile of the streamwise vorticity taken at the locations of the 0.2-1 km SRH maxima (red dots southeast of Kurnell in Figure 7). 23:13 UTC 23:19 UTC Figure 11. 23 UTC ACCESS-R sounding (18 UTC run) with the hodograph winds derived from the 2313 UTC dual Doppler observations at the location of the SRH maximum (red dot) in Fig. 7a. a) b) c) Figure 4. Red dot indicates location of Kurnell Figure 9: Observed hodographs based on the 22:56 UTC (green), 22:58 UTC (blue) and 23:11 UTC (red) AMDARS shown in Fig. 5. (a) (b) (c) (d) An EF-2 tornado crossed a small Peninsula on 16 December 2015 just 4 km southeast of Sydney Airport A wind gust of 59 m s -1 was measured as the tornado moved offshore along the northern coastline of the Peninsula Small patches of large low-level storm-relative helicity are evident along the eastern coastline of Australia just ahead of the storm and prior to the Kurnell tornado In the vertical, these maxima in SRH are dominated by a sheet of large streamwise vorticity along the interface of north-easterly flow (below) and north-westerly flow (above) The processes for the cap removal (figure 10) are unclear, but candidates are high-based pre-existing light showers raining into a very dry capping layer and an inland push of easterly flow at 900 hPa, potentially associated with a mesoscale low. A firmly capped marine layer at 19 UTC experienced complete removal of the cap during the early morning hours (between 6 am and 10 am LT) refer figure 10

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b) c) a)

Introduction

During the late morning of 16 December 2015 an EF2

tornado occurred 4 km southeast of Australia's busiest

airport – Sydney Airport. This tornado was notable in many

ways:

• A relative abundance of observations was available,

including the Kurnell C-band Doppler radar located less

than 2 km from the tornado path

• The parent supercell tracked over water just off the east

Australian coast during its life cycle, apart from when it

briefly crossed the Kurnell peninsula when the tornado

occurred.

• The tornado passed very close to an Automatic

Weather Station (AWS) located on a jetty in Botany Bay

at Kurnell which recorded a wind gust of 59.2 m s-1 (213

km/h, 115kts, 132mph) at 10:33 am local time.

• The wind gust measured by the Kurnell AWS is an

Australian record outside of a tropical cyclone.

• There were several RFD pulses and strong gate to gate

velocity couplets associated with the parent storm prior

to the tornado

• Damage from the tornado was extensive with the

Insurance Council of Australia reporting it to be the

most costly disaster of the Australian 2015/2016

summer, costing insurance companies AU$206m.

Kinematic assessment of Mesocyclone and Tornado Cyclone Thermodynamic Assessment of Pre-storm Environment

Summary and Points for Discussion

Doppler Radar and Storm Environment Observations of a

Maritime Tornadic Supercell in Sydney, Australia

Harald RICHTER1, Joshua SODERHOLM2, James TAYLOR3, Alain PROTAT1

#155

1 Research and Development Branch Bureau of Meteorology, Melbourne, Australia

2 Climate Research Group

University of Queensland, Brisbane, Australia

3Extreme Weather Desk, Bureau National Operations Centre

Bureau of Meteorology, Melbourne, Australia

• Dual Doppler winds were derived using Terry Hills S-band Doppler radar (~36km to the north of Kurnell)

and the Kurnell radar (1.6km to the east of tornado track)

• The tornado parent cyclone appears as a zone of strong convergence / vorticity in the southwest corner

of a ~7 km wide low-level mesocyclone – refer figure 6

• Just prior to tornado formation the storm ingested localised patches of enhanced 0.2-1 km storm-relative

helicity (SRH) – refer figure 7

• The key contributor to the overall SRH values appears to be a 'vorticity sheet' within the storm inflow

layer where the north-easterly inflow backs to north-westerly – refer figure 8

• AMDAR hodographs confirm very strong spatiotemporal variability in the SRH – refer figure 9

Figure 7: 0.2-1 km AGL storm-relative helicity based on the

dual-Doppler derived wind profile (shaded). Wind vectors

are shown at 500 m AGL and also derived from dual

Doppler. Storm motion (subjectively derived from Kurnell

radar data around tornado time) used is 7.5 m s-1 towards

19 degrees. Bold contours show 35, 45, 55 and 65 dBZ

outlines at 500 m AGL.

Figure 1. Kurnell Doppler Radar imagery at

2319 UTC (10:19 am LT) at 0.24o elevation; a)

PPI reflectivity; b) PPI Doppler radial velocity.

a)

b)

Figure 2. a) Approximate supercell storm track from 2130 UTC 15 December to 0030 UTC 16 December ; b)

Tornado damage at Kurnell. c) Enhanced still frame from video showing tornado (Courtesy of Peter Grassmayr)

Figure 3. One minute data

from Kurnell AWS

impacted by tornado.

Black line indicates wind

speed in knots (using left

axis) and yellow line

indicates wind direction

(using right axis).

Figure 10. a) 18 UTC 15 December 2015 ACCESS-R (red) model sounding and 19 UTC 15 December

observed Sydney Airport sounding (black); b) Soundings based on a 6-hour forecast from the 18 UTC

ACCESS-R run valid at 23 UTC (red), the 2256 UTC AMDAR (blue), the 2258 UTC AMDAR (green) and the

2311 UTC AMDAR (black); c) Hourly soundings at 18 UTC (black), 19 UTC (red), 20 UTC (blue) and 21 UTC

(green) based on the 18 UTC run of ACCESS-R indicating the rapid removal of inversion prior to the Kurnell

tornado.

Figure 5 (right). Sydney airport AMDAR flight paths

with height and time of data relay and 2306 UTC radar

reflectivity overlay; Red 2256 UTC ascending; Orange

2258 UTC ascending; Yellow 2311 UTC descending.

Figure 6. Dual Doppler winds at 2325 UTC at 1.5 km AGL(left) and 2331 UTC at 2.5 km AGL (right). Color fill is

the corresponding reflectivity from the Kurnell radar. Winds shown as vectors with increased length

corresponding to increased speed.

23:31 UTC 23:25 UTC

23:19 UTC 23:13 UTC

Figure 8: Vertical profile of the streamwise vorticity taken

at the locations of the 0.2-1 km SRH maxima (red dots

southeast of Kurnell in Figure 7).

23:13 UTC 23:19 UTC

Figure 11. 23 UTC ACCESS-R sounding (18 UTC run) with the hodograph winds derived from the 2313

UTC dual Doppler observations at the location of the SRH maximum (red dot) in Fig. 7a.

a) b)

c)

Figure 4.

Red dot

indicates

location of

Kurnell

Figure 9: Observed hodographs based on the

22:56 UTC (green), 22:58 UTC (blue) and 23:11

UTC (red) AMDARS shown in Fig. 5.

(a) (b)

(c) (d)

• An EF-2 tornado crossed a small Peninsula on 16 December 2015 just 4 km southeast of Sydney Airport

• A wind gust of 59 m s-1 was measured as the tornado moved offshore along the northern coastline of the

Peninsula

• Small patches of large low-level storm-relative helicity are evident along the eastern coastline of Australia

just ahead of the storm and prior to the Kurnell tornado

• In the vertical, these maxima in SRH are dominated by a sheet of large streamwise vorticity along the

interface of north-easterly flow (below) and north-westerly flow (above)

• The processes for the cap removal (figure 10) are unclear, but candidates are high-based pre-existing

light showers raining into a very dry capping layer and an inland push of easterly flow at 900 hPa,

potentially associated with a mesoscale low.

• A firmly capped marine layer at 19 UTC experienced complete removal of the cap during the early

morning hours (between 6 am and 10 am LT) – refer figure 10