DYNAMO/AMIE S-PolKa Scientist Summaries - January 2012


OTHER MONTHS:
October, 2011
November, 2011
December, 2011

01 Jan 2011
Lines of Shallow Cumulus in Low Shear
02 Jan 2011
Dry Conditions Over Gan as Benilde Passes to the South
03 Jan 2011
Large Convective Line at Diego Garcia, Lines of Shallow Cumulus at Gan
04 Jan 2011
Lines of Shallow Cumulus at Gan, Eastward Propagating Deep Convection at Diego Garcia
05 Jan 2011
Dry Conditions Persist, S-PoKa Detects Precipitation Far to the North
06 Jan 2011
Deep Easterlies and Non-precipitating Shallow Cumulus Near Gan
07 Jan 2011
Clear Sky over Gan and Distant Cumulus
08 Jan 2011
Clear Skies Transitioning Into Lines of Shallow Clouds Overnight
09 Jan 2011
Boundary Layer Rolls and Upper-Level Moistening Over Gan
10 Jan 2011
Shallow Cumulus and High Clouds from the South
11 Jan 2011
Low-Level Moistening over Gan, the Approach of a Convective Band from the South, and the Formation of Cloud Lines
12 Jan 2011
Low-Level Moistening and Cumulus Rising Out of the Boundary Layer
13 Jan 2011
Convection Finally Returns to Gan
14 Jan 2011
Deep Convection All Around Gan


1 January 2012
fireworks1
hny
fireworks2
Lines of Shallow Cumulus in Low Shear

Prepared by
Deanna A. Hence, Casey Burleyson, and Zhujun Li


The positive velocity potential anomaly continues to spread eastward across the Indian Ocean, suggesting large-scale subsidence over the northern part of the basin (Figure 1). This large-scale subsidence likely contributed to the very low relative humidity conditions across the northern Indian Ocean, although convection continued to be active in the southern Bay of Bengal (Figure 2). A tropical disturbance is also festering SW of Diego Garcia. Tropical Cyclone Benilde became a Category 2 storm, and it continues to track southwestward away from Diego Garcia. Although the winds along the equator at 200 hPa remain predominately easterly from Sumatra westward to 80 E, at Gan the winds have turned southerly as they curve into the flow of a deep trough over India, creating a zone of diffluence west Gan (Figure 3). A mid-level cyclonic circulation is building off of the southern tip of India, with northwesterly winds over Gan. Gan is also in the exit region of a low-level westerly wind jet that is part of the circulation around Tropical Cylone Benilde.
 
Gan had ample amounts of precipitable water, but most of this moisture was confined to low-levels since the middle levels were extremely dry (Figure 4). The Revelle was in even drier conditions. Diego Garcia was on the edge of a midlevel moisture gradient, and was receiving a stream of water vapor from the NW (Figure 5). Towards the end of the day, the Diego Garcia sounding was very moist up until 800 hPa, but had several dry and stable layers above. The Revelle left station today as it returns to port (pink line, Figure 5). An 1800 UTC Revelle sounding shows the extermely dry air above 800 hPa.

Most of the precipitation over Gan was shallow and in the morning hours, although a stream of thick high cloud passed over about 1200 UTC (Figure 6). Mostly shallow cumuli were seen throughout the day, although the thicker upper-level cloud blanketed the sky near sunset (Figure 7). The day began with the layer below 650 hPa being very moist, but with very dry and stable air above that level (Figure 8). At 0000 UTC, the last pulse of the convective lines discussed yesterday went through the domain, with shallow convection that was mostly below the melting layer, relatively high wind speeds, and very little ice production (top panels, Figure 9). After the cluster of morning convective cells cleared out, the layer between 650-900 hPa began to dry out, creating a thick stable layer by 1200 UTC (Figure 8). Throughout the rest of the day, very shallow lines of cumulus clouds went through the radar domain, with some of the cells occasionally precipitating (lower panels, Figure 9). The 850-1000 hPa shear was ~5 m/s throughout the day (Figure 8).

One persistent radar artifact was third-trip echo from intense convection SE of the radar domain (Figure 10). This feature had low reflectivity and a strongly negative velocity signature in an otherwise positive velocity field. However, the linear depolarization ration (LDR), which generally becomes positive in second-trip echo, remained negative. This may be the reason why the particle identification algorithm misidentified this misplaced echo as cloud and drizzle hydrometeors.

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Figure 1. CPC 200 hPa velocity potential anomaly overlaid infrared imagery for 31 December.


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Figure 2. Visible satellite imagery overlaid with WWLN lightning data at 0700 UTC 1 January.


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Figure 3. IMD WRF-ARW 0000 UTC analyses for 0000 UTC 1 January at 200 hPa, 500 hPa, and 850 hPa.



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Figure 4. CIMSS MIMIC total precipitable water for 0400 UTC, and Meteo-France ARPEGE for 0000 UTC 1 January analyses at 500 and 850 hPa. *Note that there is no instrumentation in the SE corner of the depicted array at this time.


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Figure 5. Water vapor imagery and the Diego Garcia and soundings for 1800 UTC 1 January.


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Figure 6. ARM KAZR reflectivity data for 1 January.


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Figure 7. Photos looking SSE at 0400 UTC, ESE at 0700 UTC, and ESE at 1200 UTC 1 January.


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Figure 8. Gan soundings for 0000-1800 UTC 1 January.


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Figure 9. S-Polka reflectivity PPI and reflectivity, velocity, and PID RHI for 0000 UTC and 1716 UTC 1 January.


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Figure 10. Infrared satellite imagery at 0800 UTC and S-PolKa reflectivity (top), velocity, linear depolarization ration, and PID RHI (bottom) for 0816 UTC 1 January.

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2 January 2012

Dry Conditions Over Gan as Benilde Passes to the South

Prepared by
Casey D. Burleyson, Zhujun Li, and Deanna A. Hence


Flow over the central Indian ocean was very disorganized today as small localized features modified the wind fields at all three corners of the triangular DYNAMO array (Figure 1). Tropical Cyclone Benilde, with estimated maximum sustained winds of 75 knots at 0600 UTC, passed due south of Diego Garcia as it continued its southerly turn away from the equator. The Joint Typhoon Warning Center is forecasting the storm to weaken in the next 24 h. Low-level clockwise flow on the northwestern side of the storm merged with another cyclone positioned to the southwest of Diego Garcia. The low-level convergence at the centers of these two cyclones was associated with large distinct areas of deep convection in the satellite IR measurements (Figure 2). A small region of convective activity was also apparent east of Gan, in the former position of the Revelle. This feature was collocated with an area of 850 hPa velocity speed convergence in the 0600 UTC analysis from the French ARPEGE model (left panel, Figure 1). At 500 hPa a counterclockwise circulation enveloped the entire array with light and variable winds in the center (Figure 1, center), a feature that was reflected in the soundings from Gan which showed a noisy transition from low-level westerlies to upper-level easterlies between 625 hPa and 500 hPa (Figure 3).  Strong easterlies were present at 200 hPa over the northern portion of the array with weaker easterlies south over Diego Garcia (right panel, Figure 1). Most of the north-central Indian Ocean remained under a sizable region of positive 200 hPa velocity potential anomalies, implying upper-level subsidence (Figure 4).

The soundings from Gan showed the layer above 900 hPa to be extremely dry throughout the day, with sporadic moist layers aloft appearing only after sunset ( Figure 3). In contrast with yesterday, the surface mixed layer below 900 hPa was also relatively dry.  Only a small 900 hPa moist layer existed throughout the day. The time series of soundings over Gan shows that the layer below 700 hPa has lost the modest gains in moisture that we had seen in the previous few days (Figure 5). The integrated result of all this drying was a column integrated precipitable water estimate slightly above 40 mm (Figure 6). Dry conditions were manifested as very clear skies over Gan, with only scattered shallow cumulus clouds, presumably from the 900 hPa moist layer, early in the afternoon (top row of Figure 7). These clouds were mostly gone by 1200 UTC when the 900 hPa layer had dried out slightly compared to its morning values (bottom row, Figure 7). The ARM KAZR cloud radar was remarkably echo-free for the entire day (not shown). Winds in the lowest 4 km over Gan showed a persistent backing signature throughout the day (Figure 3). Speed shear in the lowest 2 km was less than 5 m/s.

S-PolKa observed no measurable precipitation today. The lines of non-precipitating clouds that were frequent over the past several days were no longer present. Despite the lack of weather echo there was a handful of interesting radar echoes. Strong moisture gradients near the surface resulted in some humidity rings generated by Bragg scattering (Figure 8). The cross-section through these rings shows the strongest scattering between 1-2 km. This layer is consistent with the small amount of moisture at 900 hPa that appeared in the soundings through the day (Figure 3). In addition to the humidity-gradient rings, overnight the SMART-R radar on Gan detected unusual ground clutter from the small atoll 100 km north of Gan (Figure 9). This was likely caused by anomalous propagation (AP) of the radar beam as it interacted with the strong low-level moisture gradients and possibly the nearly isothermal layer between 900 and 800 hPa. AP clutter was not observed in the S-PolKa data.

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Figure 1. 0000 UTC analysis from the French ARPEGE model at 850 hPa, 500 hPa, and 200 hPa.  (Note: The array drawn on these maps no longer reflects the true position of the Revelle or the Mirai as these ships have left station).


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Figure 2. Satellite IR measurements with lightning activity (purple hatches) at 1000 UTC.


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Figure 3. Soundings from Gan at ~0000 UTC (5 am), ~0600 UTC (11 am), ~1200 UTC (5 pm), and ~1800 UTC (11 pm).


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Figure 4. CPC 200 hPa velocity potential anomaly overlaid with infrared satellite imagery.


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Figure 5. Time series of the upper-air soundings from Gan from 12/25 through 1/2.


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Figure 6. CIMMS MIMIC Total Precipitable Water (TPW) product at 1000 UTC.


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Figure 7. Cloud photos looking N at 11 am (top left), SE at 11 am (top right), N at 5 pm (bottom left), and SE at 5 pm (bottom right).


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Figure 8. Humidity rings in the radar PPI scans (left) and in RHI scans (right).


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Figure 9. AP ground clutter observed overnight (~11 pm) by the SMART-R radar (left), but not S-PolKa (right).

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03 January 2012

Large Convective Line at Diego Garcia, Lines of Shallow Cumulus at Gan

Prepared by
Deanna A. Hence, Zhujun Li, and Casey Burleyson


Gan remains in a very dry region while a long band of convection arcs over Diego Garcia (Figure 1). Lightning remains active along portions of that convective band, within the dissipating remnants of Tropical Cyclone Benilde, and the persistent convective region to the east of Gan. The convective line over Diego Garcia lies in a region of weak easterly 200 hPa flow (Figure 2). The 500 hPa winds over Diego Garcia were very weak and variable. The northwesterly flow that is circulating around the deep 700 hPa trough brought ample amounts of moist air to Diego Garcia. The mid-level relative humidity was lower than on previous days (Figure 3).

The Diego Garcia soundings reflect the activity of the convective line (Figure 4). Throughout the day, the layer below 750 hPa remained very moist. At 0000 UTC, there was a dry layer between 350-750 hPa that was relatively stable, but the layer from 300-400 hPa was moist. By 0600 UTC, this upper moist layer dried substantially as convection over the island cleared. This upper layer began to moisten again by 1200 UTC as new convection began to initiate to the SE of Diego Garcia.

At Gan, the prevailing winds decelerated over the island at all of the levels shown (Figure 2). Gan continued to sit in a region of relatively low total precipitable water and low relative humidities at 500 hPa (Figure 3). At 850 hPa, Gan was on the dry side of the gradient of high humidities to the south. The skies over S-PolKa mostly contained shallow cumulus clouds throughout the day (Figure 5), most of which were in lines propagating southward but oriented NW-SE with the low-level winds (Figure 6). None of these clouds were deep enough to register on the KAZR radar, and no precipitation fell. Low-level shear was weak and mostly directional, and the upper-level layer of easterlies now extends down to 650 hPa (Figure 7). The rings of Bragg scatter in the humidity layers were particularly intense in the early morning hours, when numerous sharp humidity gradients were apparent in the sounding. By 1200 UTC, several of these Bragg scattering layers disappeared as the humidity gradients became less distinct.

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Figure 1. Visible satellite imagery overlaid with WWLN lightning data for 0700 2 January. (*Note that the Revelle is currently not on station at the NE point.)


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Figure 2. IMD WRF-ARW 0000 UTC analyses for 3 January at 200 hPa, 500 hPa, 700 hPa, and 850 hPa. The star indicates the approximate location of Gan.



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Figure 3. CIMSS MIMIC total precipitable water for 0000 UTC, and Meteo-France ARPEGE 0000 UTC analyses at 500 hPa and 850 hPa for 3 January. *Note that there is no instrumentation in the NE or SE corner of the depicted array at this time.


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Figure 4. Infrared satellite imagery (top row) and Diego Garcia soundings (bottom row) for 0000-1800 UTC 3 January.


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Figure 5. Photos looking NNE at 0400 UTC, ESE at 0700 UTC, and SE at 1200 UTC 3 January.


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Figure 6. S-PolKa reflectivity PPI overlaid visible satellite imagery for 1000 UTC 3 January.


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Figure 7. Gan sounding and S-PolKa reflectivity PPI and RHI for 0000 UTC and 1200 UTC 3 January.

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4 January 2012

Lines of Shallow Cumulus at Gan, Eastward Propagating Deep Convection at Diego Garcia

Prepared by
Zhujun Li, Casey D. Burleyson and Deanna A. Hence


Gan remained in a dry region with column integrated precipitable water less than 40 mm, RH less than 30% and 50% at 850 hPa and 500 hPa, respectively (Figure 1). The increase of convection and lightning activity over the southern Bay of Bengal was significant (Figure 2). At 850 hPa, Gan was in a region of northwesterlies where return flow over the north Indian Ocean was joined by the flow at the northern edge of cyclonic circulation driven by the Tropical Cyclone Benilde (left panel of Figure 3). Easterly to southeasterly winds prevailed near Gan at mid-levels (middle panel, Figure 3). At 200 hPa, the flow was southeasterly over Gan (right panel, Figure 3).

The Gan soundings showed surface northeasterlies, low-level northwesterlies, mid-level easterlies, and upper-level southeasterlies (Figure 4). The levels between these four layers where the wind direction switched roughly corresponded to three stable layers. The column of air from 450 to 600 hPa and from 800 to 850 hPa was slightly moistened through the day.

Nonprecipitating cumuli stretched in long NW-SE oriented lines across the radar domain and were both in the S-band reflectivity and in visible satellite imagery (upper row, Figure 5). These lines of non-precipitating shallow cumuli were all had tops lower than 4 km, consistent with the dryness between 600 to 900 hPa (lower row, Figure 5). Later in the day (~1700 and ~2300 UTC), shallow precipitating convective cells developed propagating southward on the west side of the radar (Figure 6). These cells were very small and short lived, but developed reflectivity up to 40 dBZ.

Soundings taken at Diego Garcia showed drying above 600 hPa and a change of wind direction from southwesterly to southeasterly at 500 hPa (Figure 7). An arcing band of convection was positioned over Diego Garcia for most of the day. The band was more intense in the early part of the day and became less active into the evening and overnight hours (Figure 2). Figure 8 shows a sequence of intensification of convection lying within this band from 55°E, 0°S to 80°E 15°S. The intensification started at about 57°E around 2100 UTC on 3 January, propagated to 70°E at 0500 UTC, and reached 75°E by 2100 UTC on 4 January. This westward propagating signal could have been associated with wave activity.

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Figure 1. CIMSS MIMIC total precipitable water for 0000 UTC, and Meteo-France ARPEGE 0000 UTC analyses at 850 and 500 hPa for 4 January. *Note that there is no instrumentation in the NE and SE corners of the depicted array at this time.


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Figure 2. Infrared satellite imagery overlaid with WWLN lightning data for 0000 UTC and 2300 UTC 4 January.


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Figure 3. IMD WRF-ARW 0000 UTC analyses for 4 January at 850 hPa, 500 hPa, and 200 hPa.


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Figure 4. Gan soundings for 0000-1800 UTC 4 January.


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Figure 5. Upper panels: S-PolKa PPI reflectivity over satellite visible imagery for 0407, 0607, and 1007 UTC. Bottom panels: photographs looking SE, SE and NE at 0400, 0600 and 1000 UTC 4 January.


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Figure 6. S-PolKa PPI reflectivity for 1722 and 2352 UTC 4 January.


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Figure 7. Diego Garcia at 0000, 1200, and 1800 UTC for 4 January.


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Figure 8. Satellite IR imagery for 2100 UTC 3 January, 0100, 0500, 0900, 1600, and 2100 UTC for 4 January.

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5 January 2012

Dry Conditions Persist, S-Pol Detects Precipitation Far to the North

Prepared by
Casey D. Burleyson, Zhujun Li, and Deanna A. Hence


The air over Gan remained abnormally dry today, with integrated total precipitable water values hovering around 40 mm throughout the day (Figure 1). A pocket of dry air straddled the equator across the entire Indian Ocean, sandwiched between a large area of contiguous moisture to the south and a more broken but equally moist region along 5ºN. The 850 hPa flow was westerly south of Gan and through the center of the DYNAMO array (left panel, Figure 2). Over the atoll and areas north the low-level flow was easterly with velocities increasing northward into the line of moisture along 5ºN. The transition from easterly to westerly winds west of Gan resulted in the a low-level boundary that stretched NW to SE from 0ºN,65ºE to 10ºS, 75ºE. The region south of this boundary had ample moisture that extended upward into the 500 hPa level, while the area on the northern side was comparatively dry. Convergence, confluence, or deformation along the boundary was associated with a long and persistent line of clouds and precipitation stretching NW to SE and eventually terminating at the western side of the DYNAMO array (Figure 3). In the afternoon, a lone precipitating cell within range of the radar formed along the line, giving S-PolKa its only view of precipitation for the day (Figure 4). Winds at 500 hPa were dominated by a large anticyclone centered over the Arabian Sea in the northern hemisphere, stretching from the Horn of Africa across India and into southeast Asia (center panel, Figure 2). In the southern hemisphere a smaller anticyclone was centered near 18ºS and 90ºE. At 200 hPa winds over the array were strong southeasterlies, which increased in speed over Gan (right panel, Figure 2).

Upper-air soundings from Gan showed many of the same patterns that have characterized our persistent dry spell (Figure 5). Humidity was low through most of the column, with the exception of intermittent moistening of the layers centered around 900 hPa and between 600 and 700 hPa. By the evening any minor gains in low-level moisture had been wiped out by dry air within the 700-900 hPa layer (right panel, Figure 5). The layer between the surface and 800 hPa showed a noisy backing of the winds from northeasterlies to westerlies. Weak easterlies descended from 750 to 850 hPa between 0000 UTC on 5 January and 0000 UTC on 6 January. All of the soundings captured the strong southeasterly winds between 200 and 300 hPa.

Very shallow cumulus were scattered about during the day with a gradual clearing through the afternoon and into the evening (Figure 6). The dry air above the shallow cloud-bearing layer was readily apparent via its impact on the cloud field. Any individual cumulus with enough buoyancy (or bravery) to rise higher than the mean depth of the field was quickly stamped out by the entrainment of dryer air (Figure 7).

With the exception of the lone storm that cropped up off of the surface boundary to our west (Figure 4), S-PolKa observed no measurable precipitation within its maximum unambiguous range. Overnight, tall storms to our far north and northeast were observed by the radar in the form of multi-trip echo (Figure 8). The storms were far enough away that their radar returns were up to 3rd (between 300 and 450 km) and 4th (between 450 and 600 km) trip echos. These distances were reflected in the LDR values associated with these echos (right panel, Figure 9). Because S-Pol uses alternating H and V polarized waves, second trip echo will appear as anomalously high linear depolarization ratio (LDR) values--the radar algorithms indicate that almost all of the original outgoing wave has been depolarized into the other channel. The 3rd trip echo will have normal values well below 0. The LDR measured in these storms had areas of high values closer to the radar adjacent to lower values further away. This likely means the storm was on the border between the 2nd and 3rd trip returns, a location that is confirmed in the satellite imagery (top row, Figure 9).

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Figure 1. CIMMS MIMIC Total Precipitable Water (TPW) product for 0400 UTC on 5 January.


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Figure 2. 5 January 0600 UTC analysis from the French ARPEGE model at 850 hPa (left), 500 hPa (center), and 200 hPa (right). (Note: The array drawn on these maps no longer reflects the true position of the Revelle or the Mirai as these ships have left station).


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Figure 3. Visible satellite imagery at 0600 (left), 1000 (center), and 1300 (right) UTC on 5 January, with S-PolKa's 150 km range ring in the center.


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Figure 4. PPI of S-PolKa's reflectivity field at 1000 UTC (left) and a cross-section through the lone precipitating cell of the day (right).


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Figure 5. Upper-air soundings from Gan at 2335 UTC on 4 January (left), and 1135 & 2335 UTC on 5 January (center and right).


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Figure 6. Cloud photos looking west (top) and southeast (bottom) at 0400 UTC (left), 0800 UTC (center), and 1200 UTC (right) on 5 January.


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Figure 7. Photos taken 3 minutes apart of a relatively buoyant cumulus cloud rising into a layer of very dry air at 1030 UTC on 5 January.


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Figure 8. S-Pol radar reflectivity overlaid on IR imagery (left) and zoomed in to within the 150 km maximum unambiguous range (right).


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Figure 9. S-Pol radar reflectivity with IR imagery (top), reflectivity within 150 km (bottom left) and linear depolarization ratio (bottom right) at 1901 UTC.

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6 January 2012

Deep Easterlies and Non-precipitating Shallow Cumulus Near Gan

Prepared by
Zhujun Li, Deanna A. Hence, Casey D. Burleyson, and Robert A. Houze, Jr.


Gan remained under suppressed conditions with intense positive velocity potential at 200 hPa (Figure 1). The positive velocity potential over the northern and western Indian Ocean has stayed in this area since 31 December (not shown). The column integrated precipitable water indicated dryness along the equator from the the coast of Africa to the middle of the Indian Ocean (Figure 2). At 850 hPa, the region around Gan was in the center of a gyre that dominated the whole Indian Ocean basin, while Diego Garcia was in the region of strong westerlies on the southern boundary of the gyre (left panel, Figure 3). The 850 hPa winds over Gan varied through the in association with the circulation around the gyre (Figure 4). Strong easterlies prevailed over the northern Indian Ocean at 500 hPa, and over a large portion of the Indian Ocean at 200 hPa (middle and right panels, Figure 3). The winds over Gan had mostly easterly components at all levels by 1500 UTC (Figure 4). The entire column was persistently dry. At Diego Garcia, the layer between 850 hPa and 650 hPa stayed dry during the day, and the drying above 400 hPa was significant (Figure 5). Winds at 500 hPa changed from southwesterlies at the beginning of the day to southeasterlies by 1800 UTC.

Weekly sounding time series from Gan show a decrease of RH to less than 40% through the entire column, except in the boundary layer and several discrete upper layers (left panel, Figure 6). The wind speed below 500 hPa at Gan peaked on 2 January, and has gradually weakened since. At Gan the easterly wind components have been steadily descending; at the beginning of the period shown in the left panel Figure 6, the easterlies were only at levels higher than 300 hPa. At the present time the easterly layer extends all the way down to about 700 hPa. The upper-levels over Diego Garcia have moistened during the second half of the week (right panel, Figure 6), and the descent of easterlies did not occur there.

The band of convection along 5°N extended westward to 65°E by 0000 UTC 6 January, with extensive lightning activities (left panel, Figure 7). Part of this band (from 65° E to 80° E) dissipated by 1900 UTC (middle panel, Figure 7). To the south of Diego Garcia, convection continued to develop along 10°S from 50°E to 85°E (right panel, Figure 7).

There was no measurable precipitation near Gan today. Figure 8 shows zonally-oriented lines of non-precipitating shallow cumuli observed by S-PolKa in the late afternoon. The clouds were propagating southward. Photographs show cloud lines to the south and southeast of S-PolKa (upper middle and upper right panels, Figure 8). The RHI reflectivity observations indicate that the cloud tops were no higher than 3 km (bottom right panel, Figure 8). The RHI scan also shows distinct humidity-gradient layers at 2 and 3 km, corresponding to the stable layers at the same level in the Gan 1200 UTC sounding (upper right panel, Figure 4).

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am_ir_monthly_1.gif

Figure 1. CPC 200 hPa velocity potential anomaly overlaid infrared imagery for 5 January.



ops.CIMSS_MIMIC.201201060000.TPW.gif

Figure 2. CIMSS MIMIC total precipitable water for 0000 UTC 6 January.


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model.IMD_WRF_ARW_27km.201201060000.000_500mb_Height_Wind.gif
model.IMD_WRF_ARW_27km.201201060000.000_200mb_Height_Wind.gif

Figure 3. IMD WRF-ARW 0000 UTC analyses for 6 January at 850 hPa, 500 hPa, and 200 hPa.


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Figure 4. Gan soundings for 0000-2100 UTC 6 January.


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Figure 5. Diego Garcia soundings for 0000 UTC and 1800 UTC 6 January.


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Figure 6. Weekly sounding time series for Gan (left) and Diego Garcia (right) from 29 December to 5 January.


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20120106_19Z_lightningir.gif
20120106_23Z_lightningir.gif

Figure 7. Infrared satellite imagery overlaid with WWLN lightning data for 0700 UTC, 1900 UTC and 2300 UTC 6 January.


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20120106_1207_ppi_dbz.gif 20120106_1207_ppi_vel.gif 20120106_1207_rhi_dbz_120deg.gif

Figure 8. Upper panels: S-PolKa PPI reflectivity over satellite visible imagery for 1207 UTC, photographs looking SE and S for 1200 UTC 6 January. Bottom panels: S-PolKa PPI reflectivity, velocity, and RHI reflectivity for 1207 UTC 6 January.

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7 January 2012

Clear Sky over Gan and Distant Cumulus

Prepared by
Casey D. Burleyson, Deanna A. Hence, Zhujun Li, and Robert A. Houze, Jr.


Dry air continued to dominate the weather picture around Gan as the column-integrated total precipitable water estimate remained below 40 mm (Figure 1). Moisture in the western and central Indian Ocean was separated into two bands on either side of the equator, with the northern half of the DYNAMO array lying in the equatorial dry region, and the southern half in the moister area along the southern convective band. This pattern is contrasts with the larger amount of moisture that is evenly distributed from 15ºN to 15ºS over the entire maritime continent. The 0600 UTC model analysis from the French ARPEGE GCM shows the 50% RH contour extending vertically all the way into the 500 hPa level in both the northern and southern bands across the Indian Ocean (center panel, Figure 2). The low-level counterclockwise gyre mentioned over the past few days continued its slow westward propagation today, putting Gan in a region of weak low-level southerlies (left panel, Figure 2). Flow at 500 hPa was southeasterly through the center of the array. Winds transitioned to moderate easterlies west of Gan, such that weak mid-level divergence was apparently located over the atoll (center panel, Figure 2). Over the equator strong easterly winds at 200 hPa stretching across the entire basin (right panel, Figure 2) and flowing between anticyclonic centers on both sides of the equator. The western Indian Ocean remains under a sizable region of 200 hPa positive velocity potential anomalies, indicative of large scale subsidence aloft (Figure 3).

With the exception of transient moistening and drying at the top of the surface mixed layer, soundings from Gan showed very little variation through the day (Figure 4). A deep layer of easterly winds with maximum velocities just above 300 hPa dominated the profile between 650 and 200 hPa. Between 800 and 700 hPa winds veered smoothly from southerly to easterly, while in the boundary layer they were light and variable in all of the soundings. The descent of easterlies mentioned in yesterday's summary is still evident (Figure 5). Figure 4 shows that at least some easterly wind components were found intermittently through the whole troposphere throughout the day. Today marked the first day since Christmas in which the entire column of air was devoid of any persistent westerly winds.

The deep layer of moisture that characterized the last MJO event and dissipated quickly after Christmas has yet to recover (Figure 5). Consistent with the lack of moisture, the sky locally was nearly clear, and its color was a deep blue (Figure 6), indicative of no haze. Only a handful of scattered cumulus clouds appeared sporadically. Soundings from Diego Garcia were comparatively quite moist and had a deep layer of low-level westerlies that transitioned to upper-level easterlies around 500 hPa (Figure 7).

Precipitation in the central Indian Ocean was concentrated in two symmetric bands at 10ºN and 10ºS (Figure 8). Late in the day, two large regions of convective activity organized in both bands near 60ºE (right panel, Figure 8). Convective activity in the long line stretching from Sri Lanka to the windward shore of Sumatra decreased significantly during the day. S-PolKa was once again confined to observing only scattered non-precipitating shallow clouds and humidity gradient features. In contrast to the previous days, the long lines of cumulus oriented with the wind were noticeably absent (Figure 9). One possible explanation for this change is the lack of structure in the boundary layer winds, which would favor boundary layer rolls or other forms of linear cloud patterns. The time-lapse motion of the cumulus clouds observed by the radar showed a very slight counterclockwise rotation, consistent with the influence of the low-level gyre to our southwest.  

With the exception of a brief period at the end of 2011, no precipitation has been observed by S-PolKa for the better part of two weeks (Figure 10).

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ops.CIMSS_MIMIC.201201070600.TPW.gif

Figure 1. CIMMS MIMIC Total Precipitable Water (TPW) product for 0600 UTC on 7 January.


model.Meteo-France_ARPEGE.201201070600.000_850mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201070600.000_500mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201070600.000_200mb_Height_Wind.gif

Figure 2. 7 January 0600 UTC analysis from the French ARPEGE model at 850 hPa (left), 500 hPa (center), and 200 hPa (right). (Note: The array drawn on these maps no longer reflects the true position of the Revelle or the Mirai as these ships have left station.)


am_ir_monthly_1.gif

Figure 3. CPC 200 hPa velocity potential anomaly overlaid on infrared satellite imagery for 6 January.


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Figure 4. Upper-air soundings from Gan at 2336 UTC on 6 January (left), and 0835 UTC (center) and 1735 UTC (right) on 7 January.


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Figure 5. Vertical profile of moisture and winds over Gan from 8 December 2011 through 7 January 2012.


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Figure 6. Cloud photos looking E at 1100 UTC (left), 1200 UTC (center), and 1300 UTC (right) on 7 January.


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Figure 7. Upper-air soundings from Diego Garcia at 2317 UTC on 6 January (left), and 1114 UTC (center) and 2334 UTC (right) on 7 January.


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research.LTG_LARGE.201201071800.ltg_sat_IR.png

Figure 8. Satellite IR measurements and lightning activity indicators (purple hatches) at 1800 UTC on 6 January (left) and 1800 UTC on 7 January (right).


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Figure 9. PPI views of S-Pol radar reflectivity at 1000 UTC (left), 1100 UTC (center), and 1200 UTC (right) on 7 January.


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Figure 10. Daily rainfall accumulations recorded by S-PolKa from the beginning of the project through 7 January 2012.

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8 January 2012

Clear Skies Transitioning Into Lines of Shallow Clouds Overnight

Prepared by
Zhujun Li and Casey D. Burleyson


The large convection band in the northern Indian Ocean continued to propagate westward across the southern Arabian Sea with large amounts of lightning activity (Figure 1). The cyclone in the Mozambique Channel has been named Tropical Cyclone 05S, or Chanda, which moved southeastward during the day, and weakened after making landfall in western Madagascar (right panel, Figure 1). Meanwhile, the convection band positioned near Diego Garcia intensified during the day.

A large portion of Indian Ocean remained under suppressed conditions. There was a sharp gradient of 200 hPa velocity potential stretching NE-SW, from the Bay of Bengal to the south-central part of the basin (Figure 2). The dryness at the equator across the Indian Ocean remained, with precipitable water less than 40 mm near Gan (Figure 3). At 850 hPa, Gan was on the northeastern side of the gyre that dominated the western Indian Ocean, straddling the equator (left panel, Figure 4). The 850 hPa winds over Gan were mostly southwesterly, but varied substantially below this level through the day (Figure 5). Above 850 hPa, easterlies were dominant over Gan. Winds with significant southerly and northerly components were observed at 550 hPa and above 350 hPa respectively (Figure 5). From the African coast to the middle of Indian Ocean, strong easterlies were dominant at 500 hPa (center panel, Figure 4). At 200 hPa, three distinguishable rotational centers defined the wind field over the Indian Ocean (right panel, Figure 4). The flow from the gyre in the northern Indian Ocean to the one in the southern Indian Ocean contributed to the northerly component of the upper-level winds over Gan and Diego Garcia. Diego Garcia remained very moist below 700 hPa (Figure 6).

The S-PolKa PPI velocity field captured the change of wind direction from southeasterlies to northeasterlies at low-levels (bottom panels, Figure 7). The skies were mostly clear at S-PolKa during the daytime, with only very shallow clouds to the north (Figure 8). Lines of shallow clouds aligned with the low-level wind direction started to form overnight, propagating southwestward (Figure 7). The tops of these cloud lines reached up to about 3 km (top right panel, Figure 7). The orientation of the cloud lines was different from the zonally (east-west) oriented cloud lines observed over the past few days (6 January S-PolKa report).

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20120108_00Z_lightningir.gif
20120108_23Z_lightningir.gif
model.Meteo-France_ARPEGE.201201080000.000_850mb_RH_Wind.gif

Figure 1. Infrared satellite imagery overlaid with WWLN lightning data for 0000 UTC (left) and 2300 UTC (center) on 8 January. Meteo-France ARPEGE 0000 UTC 850 hPa analysis for 8 January (right). Note the location of the cyclone near Mozambique.


am_ir_monthly_1.gif

Figure 2.: CPC 200 hPa velocity potential anomaly overlaid infrared imagery for 7 January.


ops.CIMSS_MIMIC.201201080000.TPW.gif

Figure 3.: CIMSS MIMIC total precipitable water for 0000 UTC.


model.IMD_WRF_ARW_27km.201201080000.000_850mb_Height_Wind.gif
model.IMD_WRF_ARW_27km.201201080000.000_500mb_Height_Wind.gif
model.IMD_WRF_ARW_27km.201201080000.000_200mb_Height_Wind.gif

Figure 4. IMD WRF-ARW 0000 UTC analyses for 8 January at 850 hPa (left), 500 hPa (center), and 200 hPa (right).


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Figure 5. Gan soundings for 0000-1800 UTC on 8 January.


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Figure 6. Soundings from Diego Garcia at 0600 UTC (left) and 1800 UTC (right) on 8 January.


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20120108_0007_ppi_vel.gif 20120108_2052_ppi_vel.gif


Figure 7. S-PolKa PPI reflectivity (upper panels) and velocity (bottom panels) for 0007 UTC and 2052 UTC on 8 January.


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20120108_1100UTC_G.jpg 20120108_1100UTC_A.jpg 20120108_1100UTC_B.jpg 20120108_1100UTC_C.jpg 20120108_1100UTC_D.jpg 20120108_1100UTC_E.jpg

Figure 8. Panoramic view looking SW, W, NW, N, NE, E, SE (left to right) at S-PolKa at 1100 UTC on 8 January.

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9 January 2012

Boundary Layer Rolls and Upper-Level Moistening Over Gan

Prepared by
Casey D. Burleyson, Zhujun Li, and Wen-Chau Lee


Large-scale atmospheric conditions for precipitation continued to be unfavorable as the northern part of the DYNAMO array went another day without rain. A deep layer of dry air above the boundary layer combined with subsidence at 200 hPa to suppress any activity other than very shallow clouds (Figure 1). Water vapor in the western Indian Ocean remained concentrated in two bands straddling the equator, gradually merging into a more contiguous area east of 90ºE (Figure 2). At 200 hPa a northern shift in the easterly winds was centered due south from the tip of India (right panel, Figure 3). Moisture south of this feature filled in the eastern side of the old DYNAMO array (Figure 2). Moisture was displaced away from the equator on the northern side. These water vapor patterns were evident in the basin-wide distribution of cloudiness (Figure 4). Storm intensity, as measured by IR temperatures and lightning frequency, increased virtually everywhere through the course of the day. Diego Garcia was in the middle of the southern band of precipitation.

The upper-air soundings from Gan exhibited many of the patterns that have characterized the last week of dry weather, but also showed subtle changes (Figure 5). Dry air filled the column above the boundary layer, with easterly winds above 600 hPa. However, upper-level moisture slightly increased in the latter part of the day, particularly between 600 and 400 hPa (right panel, Figure 5). In the boundary layer, low-level northeasterlies in the morning eventually backed more than 100º counterclockwise, ending the day with a strong westerly component. The net result by 0000 UTC on 10 January was a 3 km deep layer of westerlies, with a peak velocity near 10 m/s around 800 hPa (right panel, Figure 5). These winds late in the day marked the first appearance of a westerly wind layer more than a few hundred meters deep in almost a week (Figure 6). The dominant signal in the soundings from Diego Garcia was the aforementioned southern band of moisture, with the layer of low-level westerlies also deepening from 4 to 5 km by the end of the day (Figure 7).

Despite no precipitating storms to observe, S-PolKa did have plenty of non-precipitating targets, especially before noon. A large field of low-level cumulus, aligned in long lines oriented with the prevailing wind, started to form after sunset on 8 January (S-PolKa Science Summary, 8 January). Overnight these lines filled much of theobservable area east of the radar. The lines were typically a few hundred meters wide, 1-2 km deep, anywhere from 25 to 75 km long, and spaced no more than 10 km apart (Figure 8). Clouds forming in the lines propagated from NE to SW through 0300 UTC on the 9th, at which point they began moving more from north to south. A photo of these clouds lines, taken between 0330 and 0400 UTC, is shown in Figure 9. Based purely on the appearance of the cloud lines it seems like they were forming in the upward branch of boundary layer rolls. A closer look at the soundings from Gan provided a lot of evidence that this was the case (Figure 10). Between 1800 and 2100 UTC on 8 January, when the lines first became clear, the soundings showed a strongly dry-adiabatic shallow boundary layer that is moist at the top and capped by shallow 1-2 K temperature inversion (first and second panel, Figure 10a & 10b). At 2100 UTC the winds in the boundary layer were purely northeasterly (they showed no directional shear) and had a maximum velocity of 5 m/s a few hundred meters beneath the inversion (second panel, Figure 10b). This pattern continued past 0000 UTC on the 9th as the lines become more clearly defined and started to appear in the area north of the radar (third panel, Figure 10c). The 0300 UTC sounding, approximately 2 hours after sunrise, showed a deeper boundary layer that was dryer at the top, as well the first appearance of directional wind shear, from NNE to NNW, just below the inversion (fourth panel, Figure 10d). These trends continued in the 0600 UTC sounding as the cloud lines became less distinct in the radar reflectivity (fifth panel, Figure 10e). By 0900 UTC only two lines of cloud remained to the southeast of the radar and they were completely gone by 1200 UTC (not shown). One could hypothesize that a combination of a deepening boundary layer and directional shear after sunrise made the boundary layer roll circulations harder to maintain, eventually leading to the breakup of the cloud lines. Cumulus clouds became more scattered in the early afternoon and the sky was clear by sunset (Figure 11).

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am_ir_monthly_1.gif

Figure 1. CPC 200 hPa velocity potential anomaly overlaid on infrared satellite imagery for 8 January.


ops.CIMSS_MIMIC.201201091200.TPW.gif

Figure 2. CIMMS MIMIC Total Precipitable Water (TPW) product for 1200 UTC on 9 January.


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model.Meteo-France_ARPEGE.201201090600.000_500mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201090600.000_200mb_Height_Wind.gif

Figure 3. 9 January 0600 UTC analysis from the French ARPEGE model at 850 hPa (left), 500 hPa (center), and 200 hPa (right). (Note: The array drawn on these maps no longer reflects the true position of the Revelle or the Mirai as these ships have left station.)


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research.LTG_LARGE.201201100000.ltg_sat_IR.png

Figure 4. Satellite IR measurements and lightning activity indicators (purple hatches) at 1200 UTC on 9 January (left) and 0000 UTC on 10 January (right).


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Figure 5. Upper-air soundings from Gan at 2335 UTC on 8 January (left), and 1135 UTC (center) and 2335 UTC (right) on 9 January.


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Figure 6. Vertical profile of moisture and winds over Gan from 2 January through 9 January 2012.


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Figure 7. Upper-air soundings from Diego Garcia at 2314 UTC on 8 January (left), and 1231 UTC (center) and 2318 UTC (right) on 9 January.


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Cloud_RHI_20120109_0000.gif

Figure 8. PPI and RHI of S-Pol radar reflectivity at 0000 UTC on 9 January.


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Figure 9. Cloud photos facing east (far left) through southwest (far right) sometime between 0330 and 0400 UTC. (Photo credit: Wen Chau Lee)

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Cloud_Line_SPol_Refl_PPI_20120108_2100.gif
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Figure 10. PPI view of S-PolKa reflectivity (top) and the upper-air sounding from Gan (bottom) from 1800 UTC on 8 January (far left) through 0600 UTC on 9 January (far right) in three hour intervals (a: 8 Jan/1800, b: 8 Jan/2100, c: 9 Jan/0000, d: 9 Jan/0300, e: 9 Jan/0600).


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Figure 11. Cloud photos facing east at 0600 UTC (1100 local time, left), 0900 UTC (1400 local time, center), and 1200 UTC (1700 local time, right).

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10 January 2012

Shallow Cumulus and High Clouds from the South

Prepared by
Zhujun Li and Casey D. Burleyson


Gan remained in the dry region covering the equatorial western and central Indian Ocean (Figure 1). The 200 hPa velocity potential anomalies showed continuing suppressed conditions over a large portion of the Indian Ocean (Figure 2). The divergence over the maritime continent at 200 hPa has intensified over the past several days, resulting in a strong upper-level east-west oriented velocity potential gradient.

At 850 hPa, both Gan and Diego Garcia were inside the region of westerlies which prevailed over the southern Indian Ocean (left panel, Figure 3). The northern Indian Ocean was mostly dominated by easterlies stretching all the way from the maritime continent to Africa. Winds over Gan at 500 hPa oscillated between easterly and southeasterly during the day (Figure 4). The occurrence of southeasterly winds at 500 hPa coincided with the change of winds from southeasterly to almost southerly above 300 hPa (upper right panel, Figure 4). At 500 hPa winds northeasterlies and southeasterlies merged into easterlies on the equator at about 75°E (middle panel, Figure 3).

Diego Garcia remained very moist from the boundary layer up to 200 hPa, except for the slightly drier layer in between 400 hPa and 500 hPa (Figure 5). Winds with an easterly component descended from 450 hPa to 650 hPa by 1200 UTC. The convective band positioned over Diego Garcia yesterday had weakened considerably by the end of the day, leaving only some high clouds drifting toward the northwest (Figure 6). During the later hours of the day, both KAZR and S-PolKa observed remnants of the storm to the south of Gan at about 9 km (Figure 7; bottom panels of Figure 8). After 1100 UTC, high clouds were spotted to the south of S-PolKa (right panel, Figure 9). These high clouds coincided with moistening above 300 hPa after 1500 UTC (bottom panel, Figure 4).

Through the day, the clouds around Gan were mostly extremely shallow (left panel, Figure 9). After 0800 UTC, stronger and more extensive echoes began to appear in the northeast sector of the S-PolKa PPI scan (upper panel, Figure 8). On average these echoes lasted over an hour, with their maximum height up to about 3 km (upper right panel, Figure 8). A line of shallow cumuli formed over S-PolKa near 0400 UTC (Figure 10). The cloud line stayed close to the coastline of the atoll until it finally dissipated by 1000 UTC. From 0400 UTC to 0800 UTC, it seemed the clouds moved back and forth in a direction perpendicular to the line itself, forming a wave like structure. This oscillation may be associated with land-sea interactions during the day.

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ops.CIMSS_MIMIC.201201100000.TPW.gif

Figure 1. CIMSS MIMIC total precipitable water for 0000 UTC 10 January.


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Figure 2. CPC 200 hPa velocity potential anomaly overlaid on infrared imagery for 9 January.


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Figure 3. IMD WRF-ARW 0000 UTC analyses for 10 January at 850 hPa (left), 500 hPa (center), and 200 hPa (right).


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Figure 4. Gan soundings for 0000-2100 UTC on 10 January.


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Figure 5. Soundings from Diego Garcia at 0000 UTC (left) and 1200 UTC (right) on 10 January.


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Figure 6. Infrared satellite imagery overlaid with WWLN lightning data for 0000 UTC (left) and 2300 UTC (center) on 10 January.


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Figure 7. Vertically pointing ARM KAZR reflectivity data over Gan for 10 January.


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Figure 8. S-PolKa PPI (left panels) and RHI (right panels) reflectivity for 0813 UTC and 2228 UTC on 10 January.


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Figure 9. Photographs looking south at 0400 UTC and 1100 UTC on 10 January.


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Figure 10. Photographs looking SE at 0400 UTC, 0500 UTC, 0600 UTC, 0700 UTC, and 0800 UTC on 10 January.

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11 January 2012

Low-Level Moistening over Gan, the Approach of a Convective Band From the South, and the Formation of Cloud Lines Northeast

Prepared by
Zhujun Li and Casey D. Burleyson


The positive velocity potential anomaly over the DYNAMO array has weakened (Figure 1). The column integrated precipitable water estimates indicated that Gan remained in the east-west elongated region that was relatively drier than the surrounding area, but was more humid compared to yesterday (Figure 2). The 850 hPa analyses showed increased relative humidity over Gan during the day (Figure 3). The moistening below 600 hPa from 1200 UTC to 1800 UTC was notable in the Gan soundings, while the layer above 350 hPa became drier as the high clouds from the south dissipated overnight (Figure 4, Figure 5).

At 850 hPa, the wind field over northern Indian Ocean has lost its coherence. The easterly wind components from the maritime continent weakened before reaching the southern tip of India (Figure 3). The northeasterlies from the Arabian Sea contributed to the northwest side of the circulation that dominated the equatorial western Indian Ocean. The circulation at 500 hPa was quite similar to 10 January, except that the area of confluence by northeasterlies and southeasterlies on the equator has slightly moved to the west (left panel, Figure 6), causing the winds over Gan at this level to be more variable throughout the day compared to yesterday (Figure 4). At 200 hPa easterlies continued to prevail over the equatorial region across the Indian Ocean (right panel, Figure 6). The winds over Diego Garcia were mostly westerly at the low-levels and easterly above 500 hPa (Figure 7). Between 600 hPa and 700 hPa, the zonal component of the winds over Diego Garcia varied during the day. The convective band positioned over Diego Garcia that dissipated yesterday (10 January S-PolKa Science Summary) has reformed on the north side of its previous position, just to the south of Gan (Figure 8). This relocation corresponded to the northern extension of the 850 hPa westerly region through the day (Figure 3).

The sky over S-PolKa was mostly clear with remnants of the overnight high clouds until 0600 UTC (Figure 9). After 0900 UTC, the cumulus began to form lines that appeared on S-PolKa PPI scans as NW-SE oriented moderate echo lines (Figure 10). These cloud lines persisted and slowly propagated toward the southeast with the low-level wind until about 2000 UTC. Although the amount of clouds increased during the day, the cloud tops remained mostly below 2 km (Figure 9; Figure 10).

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am_ir_monthly_1.gif\

Figure 1. CPC 200 hPa velocity potential anomaly overlaid on infrared imagery for 10 January.


ops.CIMSS_MIMIC.201201110000.TPW.gif

Figure 2. CIMSS MIMIC total precipitable water for 0000 UTC 11 January.


model.Meteo-France_ARPEGE.201201110000.000_850mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201111800.000_850mb_RH_Wind.gif

Figure 3. Meteo-France ARPEGE 0000 UTC (left) and 1800 UTC (right) analyses at 850 hPa for 11 January. *Note that there is no instrumentation in the NE and SE corner of the depicted array at this time.


20120111_gan_00Z_sounding.gif
20120111_gan_06Z_sounding.gif
20120111_gan_12Z_sounding.gif
20120111_gan_18Z_sounding.gif

Figure 4. Gan soundings for 0000-1800 UTC on 11 January.


20120111_kazr_dbz.gif

Figure 5. Vertically pointing ARM KAZR reflectivity data over Gan for 11 January.


model.IMD_WRF_ARW_27km.201201110000.000_500mb_Height_Wind.gif model.IMD_WRF_ARW_27km.201201110000.000_200mb_Height_Wind.gif

Figure 6. IMD WRF-ARW 0000 UTC analyses for 11 January at 500 hPa (left) and 200 hPa (right).


20120111_diego_00Z_sounding.gif
20120111_diego_12Z_sounding.gif
20120111_diego_18Z_sounding.gif

Figure 7. Soundings from Diego Garcia at 0000 UTC (left), 1200 UTC (middle) and 1800 UTC (right) on 11 January.


20120111_00Z_lightning.gif
20120111_23Z_lightning.gif

Figure 8. Infrared satellite imagery overlaid with WWLN lightning data for 0000 UTC (left) and 2300 UTC (right) on 11 January.


20120111_0507_ppi_dbz.gif
20120111_0507_rhi_dbz.gif
20120111_0500UTC_B.jpg
20120111_0500UTC_E.jpg

Figure 9. S-PolKa PPI and RHI reflectivity (upper panels), photographs looking N and SE at 0500 UTC on 11 January.


20120111_0907_ppi_dbz.gif
20120111_0907_rhi_dbz.gif
20120111_0900UTC_B.jpg
20120111_0900UTC_E.jpg

Figure 10. S-PolKa PPI and RHI reflectivity (upper panels), photographs looking N and SE at 0900 UTC 11 January.

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12 January 2012

Low-Level Moistening and Cumulus Rising Out of the Boundary Layer

Prepared by
Casey D. Burleyson and Zhujun Li


The slow convergence of moisture from the north and south continued as Gan finished the day with a column-integrated precipitable water estimate slightly less than 50 mm (Figure 1). The two bands of moisture on either side of the equator, present for the past several days, finally merged in the western Indian Ocean. A slight separation was still apparent from 70ºE to 90ºE. Analysis from the Meteo-France ARPEGE GCM had the low-level moisture to the south of the equator being advected by strong westerlies stretching from 60ºE into the maritime continent (left panel, Figure 2). North of the equator, light northerly winds continued to bring moisture closer to the DYNAMO array. RH values at 500 hPa showed the southern line of moisture to be deeper than its northern counterpart (center panel, Figure 2). Westerly winds at 500 hPa formed a long line across the central and eastern Indian Ocean at 5ºS but were less coherent through the center of the array. Easterly winds along and north of the equator dominated at 200 hPa, including over the northern half of the DYNAMO array (right panel, Figure 2). Upper-level support for convection also became more favorable, as indicated by 200 hPa velocity potential anomalies being near neutral along the equator, with slightly positive (convergence) values to the north and slightly negative (divergence) values to the south (Figure 3).

Over Gan, the layer below 700 hPa moistened considerably during the day (Figure 4). At 800 hPa, RH values crossed the 60% threshold for the first time in a week (Figure 5). Late in the day cirrus clouds from the convection to the north and south of Gan were associated with sizable moistening above 300 hPa (right panel, Figure 4). The air between 700 and 300 hPa remained quite dry. Boundary layer winds backed from northwesterly in the morning to northerlies by 2100 UTC. Winds above the surface layer were predominately westerly up to 500 hPa and easterly above 375 hPa, with a relatively smooth transition in between. In contrast with the trend of deepening low-level westerlies over the past few days, the depth of the westerly winds remained relatively constant through the day. The column over Diego Garcia continued to be quite moist compared to Gan (Figure 6). Winds transitioned from low-level westerlies to upper-level easterlies at 700 hPa early in the day and at 600 hPa in the late afternoon.

Convective activity in the central Indian Ocean was concentrated in a band stretching across the basin between 5ºS and 10ºS, and in a less active line extending southwestward from the southern tip of India (left panel, Figure 7). The radar observed mostly scattered cumulus clouds that increased in number through the day (Figure 8; Figure 9). Thin cirrus generated in each of the cloud bands between 5ºS and 10ºS and in lines approached S-PolKa late in the afternoon (right panel, Figure 7; bottom right panel, Figure 10). With the exception of two lines that formed north and northeast of the radar, the clouds did not show any persistent organization (lower left panel, Figure 8). The aforementioned low-level moistening through the day coincided with cumulus eventually rising above the boundary layer to depths approaching 2.5-3 km late in the afternoon (bottom row, Figure 10). A large cluster of storms to the northwest of Gan led to sporadic multi-trip echo overnight (Figure 11). Negative measurements of the linear depolarization ratio (LDR) suggests these echoes were likely third trip, between 300 and 450 km away (right panel, Figure 11).

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ops.CIMSS_MIMIC.201201120000.TPW.gif
ops.CIMSS_MIMIC.201201130000.TPW.gif

Figure 1. CIMMS MIMIC Total Precipitable Water (TPW) product for 0000 UTC on 12 January (left) and 13 January (right).


model.Meteo-France_ARPEGE.201201120600.000_850mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201120600.000_500mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201120600.000_200mb_Height_Wind.gif

Figure 2. 12 January 0600 UTC analysis from the French ARPEGE model at 850 hPa (left), 500 hPa (center), and 200 hPa (right). (Note: The array drawn on these maps no longer reflects the true position of the Revelle or the Mirai as these ships have left station.)


am_ir_monthly_1.gif

Figure 3. CPC 200 hPa velocity potential anomaly overlaid on infrared satellite imagery for 11 January.


20120112_gan_03Z_sounding.gif
20120112_gan_12Z_sounding.gif
20120112_gan_21Z_sounding.gif

Figure 4. Upper-air soundings from Gan at 0235 UTC (left), 1135 UTC (center,) and 2035 UTC (right) on 12 January.


research.Weekly_Time_Series.201201130000.Gan.png

Figure 5. Weekly time series of the soundings from Gan from 5 January through 12 January.


20120112_diego_00Z_sounding.gif
20120112_diego_12Z_sounding.gif

Figure 6. Upper-air soundings from Diego Garcia at 2317 UTC on 11 January (left) and 1134 UTC on 12 January (right).


research.LTG_LARGE.201201120000.ltg_sat_IR.png
research.LTG_LARGE.201201121200.ltg_sat_IR.png

Figure 7. Satellite IR measurements and lightning activity indicators (purple hatches) at 0000 UTC (left) and 1200 UTC (right) on 12 January.


SPol_PPI_Refl_20120112_0300.png
SPol_PPI_Refl_20120112_0600.png
SPol_PPI_Refl_20120112_0900.png
SPol_PPI_Refl_20120112_1200.png
SPol_PPI_Refl_20120112_1500.png
SPol_PPI_Refl_20120112_1800.png

Figure 8. S-Pol radar reflectivity from 0300 UTC (upper left) to 1800 UTC (lower right) in three hour increments.


0400UTC-C_lowres.JPG
0800UTC-C_lowres.JPG
1200UTC-C_lowres.JPG

Figure 9. Photos looking east at 0400 UTC (0900 LT, right), 0800 UTC (1300 LT, center), and 1200 UTC (1700 LT, right).


SPol_RHI_PPI_Refl_20120112_0600.png
SPol_RHI_Refl_20120112_0600.png
SPol_RHI_PPI_Refl_20120112_1500A.png
SPol_RHI_Refl_20120112_1500A.png

Figure 10. S-Pol radar reflectivity in viewed in PPI (left column) and RHI (right column) format at 0600 UTC (top) and 1500 UTC (bottom) on 12 January.


MultiTrip_Sat_IR_20120112_1500.png
MultiTrip_SPolKa_Refl_20120112_1500.png
MultiTrip_SPolKa_LDR_20120112_1500.png

Figure 11. IR satellite measurements (left), S-Pol radar reflectivity (center), and S-Pol LDR (right) at 1500 UTC on 12 January.

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13 January 2012

Convection Finally Returns to Gan

Prepared by
Casey D. Burleyson and Zhujun Li


Conditions on Addu Atoll changed rapidly as convective lines from the north and south brought very moist air toward the equator. Total precipitable water values over Gan, which had been hovering around 40 mm for the past two weeks, climbed over 50 mm and were continuing to rise at 1800 UTC (Figure 1). The western Indian Ocean filled with very moist air from the equator to 10ºS. The buildup of moisture, particularly between 700 and 500 hPa, was captured in the upper-air soundings from Gan (left panel, Figure 2). High RH above 300 hPa was associated with a large amount of cirrus clouds streaming in from the convection to the north and south of S-PolKa. The layer between 500 and 300 hPa remained comparatively dry. Westerly winds continued to increase in depth, growing from 500 hPa to 400 hPa during the course of the day. This feature was seen clearer in the weekly time-series of RH and winds from Gan (Figure 3). Boundary-layer winds were generally out of the north, but ended the day northeasterly (right panel, Figure 2). Upper-level support for convection as indicated by the 200 hPa velocity potential field remained near neutral (Figure 4).

A long line of strong low-level westerly winds, stretching from the northern tip of Madagascar all the way into the maritime continent, accompanied the buildup of moisture along and south of the equator (left panel, Figure 5). This pattern was reflected to some degree in the 500 hPa wind analysis, with the exception that the winds in the far western Indian Ocean were less coherent (center panel, Figure 5). Winds at 850 hPa had a confluent signature over the northwest corner of the DYNAMO array where westerlies and northwesterlies merged. At Gan, surface westerlies gradually increased in velocity from a morning value less than 2 m/s to an evening peak of 4 m/s, then weakened into the night (Figure 6). At 200 hPa, winds along the equator were easterly in the western side of the basin and southeasterly in the eastern side (right panel, Figure 5). Winds in the northern hemisphere were much stronger than in the southern hemisphere.

The two approaching bands of deep convection had merged in the western Indian Ocean by the end of the day (top row, Figure 7). The convection intensified when the two lines joined, resulting in very cold cloud tops and increased frequency of lightning. A wide line of very intense storms stretched northwest to southeast through the DYNAMO array by 0000 UTC on 14 January (right column, Figure 7). Although deep convection moved closer to Gan than at any point this year, the deepest echoes stayed outside of S-PolKa's maximum unambiguous range (bottom row, Figure 7). The tall and intense storms nearby did occasionally fill the radar display with second-trip echo (Figure 8).

While most of the radar observations were non-precipitating clouds and multi-trip echo, S-PolKa did record measurable precipitation for the first time in more than 10 days. Rain came from scattered small cells that generally lasted for about an hour (left column, Figure 8). The most frequent 10 dBZ echo top height measured by S-PolKa was just under 5 km (slightly above the freezing level), with the deepest storms topping out between 8 and 10 km (left panel, Figure 9). Precipitation was generally light rain and drizzle (right panel, Figure 9). Moderate and heavy rain was observed, but far less frequent. The precipitating cells closest to the radar during the day conformed to these broad statistics very well (Figure 10). S-PolKa observed two clear cases of convection forming along a propagating outflow boundary. The first occurred near midday, with the boundary moving in from the north and shallow storms forming in a line oriented east to west (Figure 11). Convection in this event was completely gone by 1100 UTC. The second event began at about 1500 UTC as another line of clouds formed along an outflow boundary again moving toward the radar from the north (Figure 12). In this case the cells forming along the boundary never really strengthened--maximum reflectivity was <15 dBZ. Lesser surface instability at night and stronger directional wind shear between 1 and 2 km may have contributed to the differences in intensity between the two cases (left panel, Figure 2).

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ops.CIMSS_MIMIC.201201131800.TPW.gif

Figure 1. CIMMS MIMIC Total Precipitable Water (TPW) product for 1800 UTC on 13 January.


20120113_gan_03Z_sounding.gif
20120113_gan_09Z_sounding.gif
20120113_gan_15Z_sounding.gif
20120113_gan_21Z_sounding.gif

Figure 2. Upper-air soundings from Gan from 0235 UTC (far left) to 2035 UTC (far right) 13 January.


research.Weekly_Time_Series.201201140000.Gan.png

Figure 3. Weekly time series of the soundings from Gan from 6 January through 13 January.


am_ir_monthly_1.gif

Figure 4. CPC 200 hPa velocity potential anomaly overlaid on infrared satellite imagery for 12 January.


model.Meteo-France_ARPEGE.201201131800.000_850mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201131800.000_500mb_RH_Wind.gif
model.Meteo-France_ARPEGE.201201131800.000_200mb_Height_Wind.gif

Figure 5. 13 January 1800 UTC analysis from the French ARPEGE model at 850 hPa (left), 500 hPa (center), and 200 hPa (right). (Note: The array drawn on these maps no longer reflects the true position of the Revelle or the Mirai as these ships have left station).


research.ARM_Gan.201201132350.Met_meteogram.png

Figure 6. Daily time-series of wind speed (green line) and wind direction (blue line) from Gan on 13 January.


research.LTG_LARGE.201201130000.ltg_sat_IR.png
research.LTG_LARGE.201201131200.ltg_sat_IR.png
research.LTG_LARGE.201201140030.ltg_sat_IR.png
IR_Refl_20120113_0000.gif
IR_Refl_20120113_1200.gif
IR_Refl_20120114_0000.gif

Figure 7. Top Row: Satellite IR measurements and lightning activity indicators (purple hatches) at 0000 UTC (left) and 1200 UTC (center) on 13 January, and 0030 UTC (right) on 14 January. Bottom Row: Satellite IR Measurements with S-Pol radar reflectivity with a 150 km range ring at the same times.


SPolKa_Refl_PPI_20120113_0000.gif
IR_Refl_20120113_0000.gif
SPolKa_Refl_PPI_20120113_1800.gif
IR_Refl_20120113_1800.gif

Figure 8. S-Pol radar reflectivity alone (left) and overlaid on satellite IR measurements (right) at 0000 UTC (top) and 1800 UTC (bottom) on 13 January.


research.SPOL_Derived.201201130000.daily_echotops.gif
research.SPOL_PID.201201130000.PID_daily_by_altitude.gif

Figure 9. S-PolKa derived echotop heights for convective (top left) and stratiform (bottom left) precipitation. Particle type frequency at different altitudes (right) for 13 January.


Cell_Close_SPolKa_PPI_Refl_20120113_2145.gif
Cell_Close_SPolKa_RHI_Refl_20120113_2145.gif
Cell_Close_SPolKa_RHI_PID_20120113_2145.gif

Figure 10. PPI S-Pol radar reflectivity (left), and RHI cross-sections of reflectivity (center) and particle ID (right) near 2145 UTC on 13 January.


Case1_PPI_0800.gif
Case1_PPI_0830.gif
Case1_PPI_0900.gif
Case1_PPI_0930.gif
Case1_PPI_1000.gif
Case1_PPI_1000.gif
Case1_RHI_0800.gif
Case1_RHI_0830.gif
Case1_RHI_0900.gif
Case1_RHI_0930.gif
Case1_RHI_1000.gif
Case1_RHI_1030.gif

Figure 11. S-PolKa radar reflectivity observations of storms forming along an outflow boundary north of the radar, from 0800 (far left) to 1030 UTC (far right) 13 January in 30 minute increments.


OutflowLine_SPolKa_Refl_20120113_1500.gif
OutflowLine_SPolKa_Refl_20120113_1530.gif
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OutflowLine_SPolKa_Refl_20120113_1630.gif
OutflowLine_SPolKa_Refl_20120113_1700.gif

Figure 12. S-PolKa radar reflectivity observations of storms forming along an outflow boundary north of the radar, from 1500 (far left) to 1700 UTC (far right) 13 January in 30 minute increments.

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14 January 2012

Deep Convection All Around Gan

Prepared by
Casey D. Burleyson, Zhujun Li, and Robert A. Houze, Jr.


The northern part of the DYNAMO array transitioned from shallow to deep convection during the day. The convective band oriented west-east across the basin has moved closer to the equator as the 200 hPa velocity potential weakened and moistening occurred over the equatorial region of the Indian Ocean (Figure 1; Figure 2). Gan was near the confluence region at 850 hPa where northerly components on the western side of the cyclonic circulation merged with the westerly jet positioned just to the south of the equator (left panel, Figure 3). At 500 hPa, Gan was in the region of southwesterlies that extended from 70°E on the south of equator to the Bay of Bengal (middle panel, Figure 3). Further aloft, at 200 hPa, the northern Indian Ocean was dominated by divergence over the Bay of Bengal and convergence over the Arabian Sea (right panel, Figure 1). The 200 hPa winds over the central Indian Ocean changed from southwesterlies to southeasterlies across the equator (right panel, Figure 3).

Soundings from Gan showed upper-level moistening before 0900 UTC and winds changing from southerlies to southwesterlies (Figure 4). The air dried out slightly after 1500 UTC and had a reduced westerly wind component. Below 850 hPa, the winds over Gan were mostly northerlies and northeasterlies, with a maximum near-surface wind speed up to 10 m/s. Between 850 and 450 hPa there was a transition to westerlies and southwesterlies (Figure 4). The air between 500 hPa and 750 hPa was significantly moistened by 0900 UTC. The layer of easterlies from 450 to 300 hPa was collocated with very dry air. Diego Garcia continued to be quite moist (Figure 5). The winds through the entire column frequently changed direction.

The region between the equator and 10ºS in the western Indian Ocean was filled with intense deep convection (Figure 6). These storms spilled over into the DYNAMO array, finally bringing long-awaited precipitation to Addu Atoll. S-PolKa recorded an area-averaged rainfall total of 12.3 mm for the day, of which approximately 70% was classified as convective and the rest stratiform precipitation (Figure 7). Most of the rainfall came in the latter part of the day. In contrast with yesterday, large regions of heavy and moderate rain were observed (Figure 8). Almost all storms rose well above the 0 deg C level, generating lots of ice crystals both regularly and irregularly shaped. Echo-top heights of 10 dBZ reached up to 15 km for both convective and stratiform classified cells (Figure 9). Echo tops between 10 and 15 km were commonly observed.

Early morning precipitation moved in from the south and west of S-PolKa, while the area to the northeast was mostly covered by lines of non-precipitating clouds aligned NE-SW (Figure 10). These non-precipitating cloud lines were parallel to the low-level northeasterlies seen in the Gan soundings (Figure 4). Radial velocity estimates showed low-level winds with northerly components over most of the domain, but westerly winds on the far western edges of the domain (right panel, Figure 10). The radial velocities were thus consistent with model analysis for the day (left panel, Figure 3). A lull in the precipitation occurred around midday, followed by a gradual increase in isolated convection late in the afternoon (Figure 11). The deepest convection remained to our south during this time (bottom row, Figure 11). At 1800 UTC northerly winds continued to dominate most of the radar domain (left panel, Figure 12). A line of relatively shallow convection with a large trailing stratiform region approached S-PolKa from the north (Figure 12). Three hours later the winds were out of the northwest and the line from the north merged with a series of cells from the east to form a long line of intense convection stretching north-south across the entire radar domain (Figure 13). An RHI scan through a 14 km deep cell to our southeast showed a well-defined signature of leading convection and trailing stratiform (bottom left panel, Figure 13). The velocity cross-section was indicative of a descending rear-inflow jet with maximum velocity close to 20 m/s near the surface (bottom center panel, Figure 13). The stratiform region contained smaller ice up to heights of nearly 16 km, dry aggregates intermittently up to about 10 km, and a layer of wet aggregates dominating the melting layer (bottom right, Figure 13). Small amounts of graupel were evident in the upper and lower parts of the bright band, as we have seen previously in episodes of deep convection and stratiform precipitation.

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am_ir_monthly_1.gif

Figure 1. CPC 200 hPa velocity potential anomaly overlaid on infrared imagery for 13 January.


ops.CIMSS_MIMIC.201201142000.TPW.gif

Figure 2. CIMSS MIMIC total precipitable water for 2000 UTC 14 January.


model.IMD_WRF_ARW_27km.201201140000.000_850mb_Height_Wind.gif
model.IMD_WRF_ARW_27km.201201140000.000_500mb_Height_Wind.gif
model.IMD_WRF_ARW_27km.201201140000.000_200mb_Height_Wind.gif

Figure 3. IMD WRF-ARW 0000 UTC analyses for 14 January at 850 hPa (left), 500 hPa (center), and 200 hPa (right).


20120114_gan_03Z_sounding.gif
20120114_gan_09Z_sounding.gif
20120114_gan_15Z_sounding.gif
20120114_gan_21Z_sounding.gif

Figure 4. Gan soundings for 0300-2100 UTC on 14 January.


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20120114_diego_18Z_sounding.gif

Figure 5. Soundings from Diego Garcia at 0000 UTC (left) and 1800 UTC (right) on 14 January.


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Figure 6. Infrared satellite imagery overlaid with WWLN lightning data for 2200 UTC on 14 January.


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Figure 7. Hourly rainfall estimates from S-Pol for 14 January.


research.SPOL_PID.201201140000.PID_daily_by_altitude.gif

Figure 8. Particle ID statistics from S-Pol for 14 January.


research.SPOL_Derived.201201140000.daily_echotops.gif

Figure 9. Echotop height frequencies for different intensities of convective (top) and stratiform (bottom) precipitation on 14 January.


IR_Refl_20120114_0600.gif
SPol_Refl_PPI_20120114_0545.gif SPol_Vel_PPI_20120114_0545.gif

Figure 10. S-Pol radar reflectivity over laid on satellite IR imagery (left), radar reflectivity (center), and radial velocity (right) near 0600 UTC (1100 LT) on 14 January.


SPol_Refl_PPI_20120114_0900.gif
SPol_Refl_PPI_20120114_1200.gif
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IR_Refl_20120114_1500.gif

Figure 11. S-Pol radar reflectivity at 0900 UTC (1400 LT, top left), 1200 UTC (1700 LT, top center), and 1500 UTC (2000 LT, top right). S-Pol reflectivity over laid on satellite IR imagery for the same times (bottom).


SPol_Vel_PPI_20120114_1800.gif
SPol_Refl_PPI_B_20120114_1800.gif
SPol_Refl_RHI_B_20120114_1800.gif

Figure 12. PPI views of radial velocity (left) and radar reflectivity (center), and an RHI of reflectivity (right) at 1800 UTC on 14 January.


20120114_2322_ppi_dbz.gif
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20120114_2322_rhi_vel_136.gif
20120114_2322_rhi_pid_136.gif

Figure 13. S-PolKa PPI reflectivity (top left) and velocity (top center), satellite infrared imagery overlaid with S-PolKa PPI reflectivity (top right). RHI reflectivity, velocity and particle ID (bottom row) for 2322 UTC on 14 January.

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