Thursday, December 29, 2011

My final paper for my Adv. Haz. and Disasters class for my AMP.


Bryce Touchstone
GR8813 Advanced Hazards and Disasters
Mississippi State University; Fall 2011


Emergency Management Methods for Bushfires in Western Australia
            Outside of Antarctica, Australia is the driest continent on earth(BOM, 2011).  While it is comparable in size to the contiguous United States, it is geographically disadvantaged when it comes to rainfall in a couple of regards:  It lacks a major mountain range, and its continental poleward extent is well outside of the Antarctic, which provides little rainfall from orographic effects and quarantines the country from polar air outbreaks, as compared to the United States.  Australia relies heavily upon Tropical influences for rainfall in the North, and upon river systems to bring water down to the drier Southern regions. 
            Fire itself is controlled by the fire triangle of heat, oxygen, and fuel, while the fire environment is controlled by the fire behaviour triangle which consists of weather, topography, and fuels(COMET, 2009).  The elements of weather that affect fire behaviour are temperature, relative humidity, wind speed and direction, precipitation, and atmospheric stability(COMET, 2009).  Bushfires thrive under hot, dry, windy conditions, with natural ignitions of fuel coming often from lightning.  Under a regime of a stalled ridge with surface conditions hot and with relatively high pressure in place, particularly in summer months, bushfires can last for weeks.  In the Australian Outback region, oftentimes bushfires are beyond the capabilities of emergency services, and are extinguished only with the arrival of cooler temperatures and rainfall(Smith et al., 2009). Topography can act to both hamper and enhance the fire environment.  Dry inland salt lakes can create natural fire breaks, giving bushfires nowhere to spread to, given their lack of vegetation(O’Donnell, 2009).  Conversely, fire can spread as much as 2-3 times as fast upslope as it can downslope, so topography can play a very vital role in bushfire management, particularly in mountainous alpine areas(Hasson et al., 2008).  Fuels themselves are any form of ground vegetation capable of igniting or spreading a bushfire(DEC, 2011).  Some characteristics of fuels to be considered are fuel loading, the compactness of the fuels, fuel size, fuel shape, fuel (vegetation) type, and the horizontal and vertical extent of fuels(DEC, 2011).
            The occurrence of bushfires in Australia is mistakenly thought to be primarily in the southern regions.  However, research has shown that bushfires occur primarily in savannah landscapes of Tropical Northern Australia, which experiences monsoonal influences(Russell-Smith et al., 2007).  The study from Smith et al. utilized both Fire Hot Spot (FHS) and Fire Active Area (FAA) datasets, mapping daily fire activity with use of algorithms and 9-day burnt areas due to the orbital pass of the NOAA-AVHRR platform, respectively.  Smith et al. omitted nearly 90% of all individual fires acquired with the FAA method due to the level of error associated with the relatively small size of these fires, however in doing so, found that these fires accounted for less than 3% of the total burnt area.  Figure 1 shows the Seasonal (quarterly) distribution of FHS from 2002(Russell-Smith et al., 2007).  Figure 2 shoes the frequency of large fires derived from FAA mapping, from 1997-2004(RussellSmith et al., 2007).  The circled area represents the 2002-2003 southern Australian bushfires.  It should be noted that the FAA data was acquired from 1997-2004 for the entire country, and from 1990-2004 for Western Australia and Northern Territory.  For this particular study, only the years 1997-2004 were used.

Figure 1(Smith et al.)
Figure 2(Smith et al.)

An analysis of two separate bodies of researched focussed primarily on climate change implications on bushfire management in the twenty-first century discuss some of the weather-related reasons for Australia’s high degree of susceptibility to bushfires. Hennessy et al. conducted a study using historical weather data from 1974-2003 provided by the Australian Bureau of Meteorology (BOM) to generate climate change scenarios for 2020 and 2050, and to subsequently determine the likelihood of increased risk from bushfires in the twenty-first century.  The study concluded that the occurrence of very high and extreme fire weather days could increase from 4-25 percent by 2020 and from 15-70 per cent by 2050 across some regions of SE Australia.  It also suggested that elevated fire weather risks in spring, summer, and autumn could encourage more winter prescribed burning in future years, as well as to extend the annual bushfire season(Hennessy et al., 2006). 
Hasson et al. looked at potential high-impact fire days by modelling changes to temperature regimes in the twenty-first century under different emissions scenarios, coupled with “strong cold front” days, as research has shown that most high-impact fire weather events in the past 40 years in SE Australia, which experiences summer conditions similar to those found in Western Australia, have been associated with strong cold frontal passage(Hasson et al., 2008) under low- and high-impact scenarios for two twenty-year periods, 2050 and 2090.  The results of this research showed an increase in temperature during both twenty-year periods, and under both scenarios.  It was a recommendation from this body of work that these scenarios be taken into consideration for future fire management planning.
A very different body of research looked at the effects of topography, vegetation type, fuel age, and social factors as varying effects on the fire environment of South Western Australia(O’Donnell, 2009).  The study showed that fuel frequency decreased in wooded regions as compared to mallee and shrub land vegetation, with an increased probability of fire occurrence with increased fuel age.   There was also a relationship found between extensive fire activity (> 100,000Ha) and rainfall regimes; it was found these extensive fire activity periods were associated with below-average rainfall, and also that they were preceded by a year of above-average rainfall and low temperatures(O’Donnell 2009).  This indicates an occurrence of building and subsequent drying of large amounts of fuel, leading to greater fuel loads and environments more conducive to bushfires.
When dealing with the description of, management of, or discussion of a fire regime, it is necessary to distinguish an actual bushfire, or wildfire, from a planned and managed prescribed burn.  A bushfire is an unplanned fire, while a prescribed burn, as defined by the Department of Environment and Conservation under the government of Western Australia, is “the controlled application of fire under specified environmental conditions to a predetermined area…”(DEC, 2011).  With regards to emergency management for bushfires in Western Australia, the approach has seen changes in recent years, including this year.  There are multiple agencies with varied, and sometimes varied roles with regards to bushfire emergency management.  The state is divided into regions, and those regions into districts, each with a regional fire coordinator (RFC) and district fire coordinator (DFC), respectively, responsible for the fire management activities of their respective regions or districts (Figure 3).
Figure 3(Bryce Touchstone, Department of Environment and Conservation, Fire Management Services).
The primary method of bushfire mitigation is with an extensive, cross-regional prescribed burn plan, organized and overseen by the Department of Environment and Conservation (DEC), and carried out and reported on by the responsible RFC and DFC.  The Fire Management Services (FMS) branch of DEC delivers extensive GIS services, specifically mapping products, to field personnel with regards to fuel age, planned versus carried out prescribed burn, burn area, etc. to assist with each region’s seasonal prescribed burn plan.  The BOM issues seasonal climate outlooks, and specific bushfire outlooks, as well as daily bushfire conditions and warnings in the event of potential bushfire activity.  This information coupled with that provided by DEC is utilized on a daily basis by RFC’s, DFC’s, and field personnel to determine what, if any, prescribed burn activities will take place on that day.
            The Fire and Emergency Services Authority of Western Australia (FESA) is the primary agency within Western Australia that handles the preparation and response phases of bushfire emergency management state-wide.  FESA has published ‘Prepare. Act. Survive’, a comprehensive guide to ‘preparing for and surviving the bushfire season(FESA, 2011), which includes information on their three-step bushfire readiness scheme, prepare, act, and survive, and several, but equally important checklists including Important Contacts, Preparing Your Survival Kit, Preparing Your Property, Total Fire Bans Fact Sheet, Leaving For a Safer Place, Preparing to Actively Defend, and Planning to Actively Defend(FESA, 2011).
            The government has a policy of either evacuate or ‘Stay and Defend’ with regards to bushfires.  FESA and DEC both issue information regarding home preparation for ‘Stay and Defend’ scenarios, and FESA published a document on methods of preparing a home for ‘Stay and Defend’, among which are fire breaks around the perimeter of the residence, a vegetation-free buffer within the residence, and specific fire ember-resistant air conditioner units(FESA, 2011).  FESA is also the primary agency responsible for emergency response to cyclones, storms, floods, earthquakes, tsunamis, hazardous materials, and search and rescue incidents; as such, they have a number of warning and information dissemination systems, including the Standard Emergency Warning Signal (SEWS), a distinctive siren sound used to alert the target community of relevant safety information regarding a current disaster or emergency, and StateAlert, an automatic, web-driven service which delivers automatic emergency- and disaster-related information directly to landlines and registered mobile phones.
            The BOM issues a range of bushfire risk warnings within the framework of the Fire Danger Rating(FESA, 2011).  Bushfire danger ratings range from Low-Moderate, High, and Very High, to Severe, Extreme, and Catastrophic.  From this and other information, FESA issues a Bushfire Warning, which operates within a framework of Advice, Watch and Act, Emergency Warning, and All Clear(FESA, 2011).  It should be noted that ‘Stay and Defend’ is not advised for Fire Danger Ratings above Severe, as homes are not capable of being built to withstand bushfires in these conditions.  FESA is also primarily responsible for managing Total Fire Bans, as well as partnering with DEC in advising remote farmers and northern property owners of properties of substantial size on prescribed burn and winter burn activities.  Prescribed burn and winter burn is allowed to be carried out privately within certain restrictions, which include all private parties first consulting with their local council or shire and remaining vigilant of the fire environment and its capabilities during the week of the planned burn.
            Prior to February 2011, FESA was an independent agency, outside of government control.  In February 2011 a devastating bushfire in the Perth Hills of Western Australia, while claiming no lives, destroyed more than 70 homes.  As a result, on 23 February, WA Premier Colin Barnett ordered a review of the incident, and the inter-agency response, and a subsequent delivery of the report of findings and recommendations.  This task was assigned to former Federal Police Chief Mick Keelty.  The inquiry involved over 50 hearing with more than 100 witnesses over a period of 2 months, at local Kelmscott, Roleystone, and Armadale civic centers, among over venues.  The report, titled ‘A Shared Responsibility: The Report of the Perth Hills Bushfire February 2011 Review’, was submitted in August 2011, and noted multiple deficiencies on the part of FESA in working alongside DEC and volunteer fire fighters, and a lack of information sharing.  It also found that evidence provided by FESA was in many instances an attempt to hide FESA shortcomings.  Among the results of the report were 55 recommendations, among which were better inter-agency operations and communications, and that FESA’s board be disbanded and FESA itself be brought under government control.  FESA’s board was disbanded, its chief executive sacked, and FESA itself was later made into a government agency.
            It is worth noting one final update just prior to the writing of this paper.  On 23 November, 2011, dormant prescribed burns in the Margaret River jumped control lines under catastrophic fire weather conditions, creating a bushfire that destroyed over 30 homes.  Also across the southern region in the subsequent four days, 24-27 November, four other bushfires burned over 100,000Ha of land.  It was found that the government had only 9 of the 55 recommendations from the Keelty Report had been implemented prior to the 2011 summer bushfire season.  Having been part of the response to those incidents firsthand, as a member of DEC Fire Management Services, the relationship between DEC and FESA was, and will continue to be tested; this is a situation that will no doubt require effort on the part of all parties involved.
______________________________________________________
References
Bureau of Meteorology, cited 2011: Living with Drought.
[http://www.bom.gov.au/climate/drought/livedrought.shtml].
Department of Environment and Conservation, cited 2011: Prescribed burning.
[http://www.dec.wa.gov.au/content/category/49/865/2073/].
Department of Environment and Conservation, cited 2011: Wildfires.
[http://www.dec.wa.gov.au/content/category/49/866/2073/].
Fire and Emergency Services Authority of Western Australia, cited 2011: Your Guide to Preparing For and Surviving the Bushfire Season.
[http://www.fesa.wa.gov.au/safetyinformation/fire/bushfire/BushfireManualsandGuides/FESA_Bushfire-Prepare_Act_Survive_Booklet.pdf].
Fire and Emergency Services Authority of Western Australia, cited 2011: The Homeowner’s Bush Fire Survival Manual.
[http://www.fesa.wa.gov.au/safetyinformation/fire/bushfire/BushfireManualsandGuides/FESA_Bushfire-Homeowners_Survival_Manual.pdf].
Fire and Emergency Services Authority of Western Australia, cited 2011: Fire Danger Rating and What It Means To You.
[http://www.fesa.wa.gov.au/safetyinformation/fire/bushfire/BushfireFactsheets/FESA_Bushfire_Factsheet-Fire_danger_ratings.pdf].
Fire and Emergency Services Authority of Western Australia, cited 2011: Bushfire Warnings: What Should You Do?  Survive.
[http://www.fesa.wa.gov.au/safetyinformation/fire/bushfire/BushfireManualsandGuides/FESA_Bushfire-Prepare_Act_Survive_Booklet.pdf].
Hasson, A.E.A., Mills, G.A., Timbal, B., Walsh, K., 2008: Assessing the impact of climate change on extreme fire weather in southeast Australia. CAWCR Technical Report No. 007, 86 pp.
Hennessy, K., Lucas, C., Nicholls, N., Bathols, J., Suppiah, R., Ricketts, J., 2006: Climate change impacts on fire-weather in south-east Australia. CSIRO & BOM, Libraries Australia ID: 40171855, 91 pp.
Keelty, R., 2011: A Shared Responsibility: The Report of the Perth Hills Bushfire February 2011 Review. Special Inquiry pursuant to s24H(2) of Public Sector Management Act 1994, 211 pp.
MetEd Comet Module, cited 2009: S-290 Unit 1: The Fire Environment.
[http://www.meted.ucar.edu/fire/s290/unit1/navmenu.php?page=2.0.0].
O’Donnell, A., 2009: Historical Patterns of Bushfire in Southern Western Australia. Fire Note, Issue 48, 1-2.
Russell-Smith, J., Yates, C.P., Whitehead, P.J., Smith, R., Craig, R., Allan, G.E., Thackway, R., Frakes, I., Cridland, S., Meyer, M.C.P., Gill, A.M., 2007: Bushfires ‘down under’: patterns and implications of contemporary Australian landscape burning. Int’l. Jnl. of Wildland Fire, 16, 361-377.
Smith, K., Petley, D., 2009: Biophysical Hazards. Environmental Hazards Assessing risk and reducing disaster, Routledge, 221-230.

Tuesday, May 10, 2011

Discussion on the 27 April 2011 Tornado Outbreak

This is a discussion on the 27 April 2011 Tornado Outbreak.  For this review, Satellite Imagery, RaDAR Imagery, and mapping products will be used in conjunction with discussion.


Enhanced IR Image; .28.04.2011 @ 0645Z















The above image is an enhanced IR image from GOES East.  The Tx range has been adjusted to (150-330)K.  You can see the explosive convection ahead of the dry line over SE AL associated with synoptic-scale

Sunday, May 1, 2011

My RaDAR Paper for SatRad GR6753

A RaDAR Analysis of the 2007 Groundhog Day Tornado Outbreak, Central Florida

 
Introduction

          In the early morning hours of 2 February, 2007, ground temperatures were already rising to levels well above average; coupled with massive amounts of moisture and a powerful mid-level jet stream overhead, synoptic conditions were favourable for severe weather.  The instability and wind shear led to a system of squall lines and supercells across Central Florida which would produce multiple tornadoes, killing 21 people and causing over $200 million in damage.  One of the most dangerous aspects of these storms is that they began at night locally.

          Following is a description of multiple mesoscale events affecting Florida that day.  I describe these events using BR, CR, BV, SRV, VIL, and Tops products provided by NOAA’s HDSS Access System and displayed in GRLevel3.  When viewing these images, please note I use mostly 4-panel windows, with images designated in order from top right to top left, bottom left, and bottom right, the same as a mathematic Cartesian plane.  Also note, there are so many RaDAR signatures associated with this event, however only a few important aspects will be discussed.


RaDAR Analysis

          Below in ‘Img01’, an image of development in the proximity of KJAX Jacksonville, FL at 0224Z, which given the time of year and time difference makes it 2124L (Local).  The area of concern is the area approximately 60nm from the RaDAR unit, or halfway out, in the 3rd range ring.

Img01; BR0.5, BR1.5, BR2.5, CR; 0224Z
  





 
The majority of the reflectivity returns for the southern storm are in BR0.5 and 1.5 tilt angles, which at 60nm means they are at around 13,000 ft.  At a closer look in ‘Img02’, there is also a tight reflectivity gradient with what appears to be a BWER and inflow notch on the southern edge of this storm.  I would be watching for development within this storm.  This is shown by the reflectivity returns as well as relatively high inbound BV returns.  With the Mesocyclone algorithm marks shown for reference, the SRV0.5 product shows what appears to be cyclonic rotation on the WNW side of the storm, and also on the ESE side.  Oddly enough, just to the left of the mesocyclone marks, you can see decreased inbound velocities.  Also, in the reflectivity you see a WEC to the WNW of the main storm, which appears to be causing the entire system to rotate cyclonically.  So basically we have a rotating system with relative rotation within the system itself.  I would be very wary of this storm.

          ‘Img03’ shows what appears to be an MARC at 0319Z.  The BV and SRV both show high velocity differences over a relatively short distance, and given their tilt angles and proximity to the RaDAR unit,  puts this feature at approximately 10,000ft., which is consistent with MARC locations.  At this stage I would be issuing severe storm warnings for Saint Augustine and the surrounding areas due to the threat of powerful winds and downbursting winds at the surface, as well as the potential for hail, given the presence of an MARC signature.

Img02; BR0.5, BV0.5, SRV1.5, CR; 0224Z
  




Img03; BV0.5, BV0.5, SRV0.5, CR; 0319Z






 
Shifting now to KMLB in Melbourne, FL a few hours later, ‘Img04’ shows a WER coming in from the Gulf of Mexico onto the W coast of FL at 0725Z.  There is a tight leading edge reflectivity gradient and a vertical tilt as is evident by the BR1.5, VIL, and Tops products.  Upon seeing this come into viewing range, I would immediately issue a severe thunderstorm warning for Citrus and Sumter Counties, FL due to the potential for flash flooding, hail, downbursts and straight line winds, and possible future BWER development and tornadic formation.

Img04; BR0.5, BR1.5, VIL, Tops; 0725Z





Unfortunately, this storm does indeed intensify rapidly, as is shown by using the Lemon Technique in’Img05’ at 0803Z.  Looking at several levels of the BR product for the same storm you can see its layers vertically, which give a much clearer indication of the storm’s vertical structure, indicating such things as tilt, core location, and rotation.  It is now what appears to be a HP supercell.  You can see by the VIL  that the amount of precipitation aloft has increased dramatically.  There is also a slight vertical tilt, and an apparent hail core aloft.  This is shown by the BR2.5 product, and given its proximity to the RaDAR, approx.. 85nm, puts this hail core at between 25,000-30,000ft aloft.  At this stage, I would be issuing a severe thunderstorm warning for Sumter, Lake, and Marion Counties, FL, citing flash flooding, strong surface winds, and hail all as serious threats.  Additionally, due to the fact that the precipitation at the lowest tilt seems to be migrating slightly to the SW of the precipitation aloft, I would anticipate the imminent development of a BWER, subsequently erring on the side of caution and issuing a tornado watch for the same counties.

Img05; BR0.5, BR1.5, BR2.5, VIL; 0803Z




 
In ‘Img06’, this storm has now become a well-defined supercell at 0811Z, exhibiting all of the signs, the tight reflectivity gradient on the inflow, or southern side of the storm, a BWER alongside the inflow notch, a hook echo, a slight velocity couplet shown in the SRV product, and even a v-notch formed from the shear striking the updraft and fanning out towards the NE.  You can also make out the FFD and RFD.  At this stage I am upgrading to a tornado warning for Sumter, Lake, Marion, and Volusia Counties, FL.  I would expect flash flooding, hail, powerful winds, and a tornado to either form or have already formed with this storm.

Img06; BR0.5, BR1.5, SRV0.5, CR; 0811Z






Img07; BR0.5, BV1.5, SRV1.5, CR; 0849Z
 





In ‘Img07’, you can now see it is very evident there is a tornado present due to the BWER, hooked and tightly-packed gradient nature to the reflectivities, and rotation couplets in both the BV and SRV products as shown by the localized area of inbound/outbound returns shown by the green and red returns, respectively.  I would have already issued an extended tornado warning for Volusia Co., FL, as well as Sanford Co, FL due to the risk of tornadic formation due to spinoff from the flanking line in the RFD of the supercell.
          Switching now to an event later that day, at around 1630Z, or 1130L.  ‘Img08’ shows a storm which appears to be a localized area of rotation, however it seems to have a lack of moisture.  If this were not Florida, I would go so far as to call this system a LP Supercell.  If you look closely, you can make out a slight BWER in the BR product.  You can also notice the slight relative rotation in the SRV product.  I would watch for future development with this storm, issuing a severe thunderstorm warning for Okeechobee Co., FL.


Img08; BR0.5, SRV1.5, BV0.5, CR; 1631Z





 
In ‘Img09’, you can now see a well-defined BWER on the S edge of the storm.  The rotation is more pronounced in the SRV and BV products as well.  The CR product shows that there is yet much more precipitation aloft.  I have also included an image, ‘Img09a’, of the BR product at 0.5, 1.5, and 2.5 tilt angles, as well as VIL to show the lack of substantial moisture in the vertical column above this storm as well as the SE tilt of this storm.  At this stage I would issue a severe thunderstorm warning and tornado watch for Okeechobee, Indian River, and St. Lucie Counties, FL.



Img09; BR0.5, SRV1.5, BV0.5, CR; 1700Z






In ‘Img10’, at 1738Z, you can see that the storm has hit the ocean, and gaining a water source, gained low-level moisture, caused further convection linearly along the N, and now has a well-defined area of inflow from the rear as shown in both SRV and BV products.  The storms died off soon after this, with the passage of a cold front.

Img09a; BR0.5, BR1.5, BR2.5, VIL; 1700Z








Img10; BR0.5, SRV1.5, BV0.5, CR; 1738Z








.BT

Friday, March 4, 2011

My Satellite Paper for Satellite & RaDAR Meteorology GR6753


The Use of Northern Hemisphere- and Southern Hemisphere-Associated IR Enhancements to Assess Southern Hemispheric Tropical Cyclone Intensity:  Tropical Cyclone Yasi
Bryce Touchstone
GR6753-501 Satellite and Radar Meteorology
Mississippi State University, Spring 2011
Introduction
In 1975, Vernon F. Dvorak created a technique, namely “The Dvorak Technique”, to assess current and future tropical cyclone intensity in the Atlantic Basin of the Northern Hemisphere.  The technique consisted primarily of satellite imagery analysis by a meteorologist based upon cloud patterns, to depict both the current intensity of the tropical cyclone, as well as its projected future state(Dvorak, 1975).  This method was based upon subjective methodology since the analysis was at the discretion of the human analyst.
Since the original Dvorak Technique relied on subjective analyst interpretation of both cloud patterns and empirical rules regarding cyclone intensity, and while this technique proved sufficient for operational meteorology, there were instances where discrepancies occurred between different analysis centres who were measuring the same tropical system.  A more objective method was necessary to compensate in these instances.  A computer-based algorithm was developed that analysed digital infrared imagery.  This algorithm, named “The Objective Dvorak Technique”(ODT), has been modified since its creation to include certain of the original Dvorak rules, more constraints, and a component of time-averaging.  This modified ODT is only applicable to tropical systems which have attained Tropical Storm or Hurricane strength(Velden, et. al., 1997).
While the algorithm component is beyond the scope of this project, there were IR Enhancement Curves associated with the ODT which I will use to analyse Tropical Cyclone Yasi during landfall of N Queensland, Australia, 2 February, 2011, with Category-5 Australian Tropical Cyclone Scale(ATCS)  (Category-4 SSHS) strength.  The use of the ODT has certain prerequisites, the afore-mentioned minimum strength category, and a well-defined eyewall; this is due to the fact that the ODT relies upon eyewall centre recognition to identify the centre of the storm.  Once this is identified, the temperature (typically land or ocean surface) is coupled with temperature of surrounding bands of convective cloud-top temperatures at 4-km intervals from 24 km to 132 km from the eyewall centre to produce a CI (Current Intensity) number, corresponding to a T-Number, depicting both the current and projected future states of the tropical cyclone’s intensity (Velden, et. al., 1997).  Since TC5- Yasi had a very well-defined eyewall, it has been decided to use IR Enhancements associated with the ODT to analyse the current intensity of TC5-Yasi.
After performing the IR Enhancements associated with the Northern Hemisphere method, an enhancement created by the Australian Bureau of Meteorology (BOM) will also be applied to compare the methods.
Climatological and Synoptic Setup
          The 2010/2011 Southern Hemisphere Summer was marked by unprecedented flooding in Australia as a result of a very powerful La Niña sector of the ENSO.  This La Niña peaked in early January, which was confirmed by Southern Oscillation Index (SOI) values, cloud patterns, and Pacific Ocean temperatures all showing a marked gradual return to ‘normal’ conditions subsequent mid-January, with further deterioration of La Niña expected to continue through the Southern Autumn (Australia BOM). 
TC2-Anthony, a weaker tropical system forming a week prior to Yasi, caused widespread rainfall and flooding in Vanuatu, Solomon Islands, and New Caledonia, and struck with Category-2 (ATCS) force around Townsville, forcing its way inland and dumping 100mm of rain in 6 hours 1300km inland in the Outback.  Yasi was identified by the Fiji Meteorological Service (FMS) as tropical disturbance “09F” 330km SW of Tuvalu on 26 January, 2011.  Warm sea surface temperatures and relatively low wind shear were ahead of its projected path, and 27 January saw an upgrade to tropical depression status, with little to no intensification on 28 January.  30 January saw rapid intensification and upgrade to tropical storm status by the Joint Typhoon Warning Centre (JTWC), and shortly thereafter upgrade to Tropical Cyclone Yasi by the FMS.  Tracking westward from 370km NE of Vanuatu, on 31 January, with ten minute sustained winds of at least 120km, Yasi attained Severe Tropical Cyclone Status(Wikipedia, BOM).  Below is Yasi’s track. 














Track of TC5-Yasi (Created by Keith Edkins and Iune using Wikipedia:WikiProject Tropical cyclones/Tracks. The background image is from NASA. Tracking data is from the  Joint Typhoon Warning Center.)

 
Enhancement Process
 Figure 1 – Mollweide IR Composite, 0900Z, .02.02.2011. (Greyscale)










Figure 2 – Mollweide IR Composite, 0900Z, .02.02.2011. (Inverse Greyscale)
 
Figures 1 and 2 are the unenhanced IR images of Tropical Cyclone Yasi (henceforth TC5-Yasi) during landfall on 2 Feb., ’11, S of Cairns, displayed in Greyscale and Inverse Greyscale, respectively.  Inverse Greyscale will be retained for the subsequent enhancements.  The first enhancement to be performed will be a simple ZA Enhancement to better show temperature contrast across the temperature spectrum of our interest.  To obtain the temperature range necessary, I have applied contrasting colours at 10K-intervals beginning at 217K per ZA Enhancement table, Lecture 6, Slide 5 of my GR6753 lecture notes to identify the coldest cloud-top temperatures within the cyclone, and the resulting image and breakpoints with corresponding colours are shown in Figures 3 and 4, respectively.  Note the well-defined eye in this image.


















Figure 3 – Resulting image showing rough temperature estimates






Figure 4 – Breakpoints inserted at 10K-intervals and corresponding colours
( (167-177]K = Purple; (177-187]K = Blue; (187-197]K = Green; (197-207]K = Yellow; (207-217]K = Red)
















Figure 5 - Temperature Histogram, 0900Z, .02.02.2011.

The temperature range can be seen in the Temperature Histogram for this particular image in Figure 5.  This histogram is a rough diagram, but cannot be relied upon for absolute values as there may be ‘outliers’ which may not be visible to the eye as a result of the large y-axis scale, thus the systematic approach is necessary.  As a result, the lowest (coldest) temperature interval is [197-187)K, thus a new range of 170K-315K will be selected, 315K because temperatures above 42C are not of interest to this project.  The resultant image from this ZA Enhancement is shown in Figure 6.






















Figure 6 – Image after ZA Enhancement applied.

The next step is the application of a BD Curve for Tropical Cyclone Intensity which is used in the ODT(Cooperative Institute for Meteorological Satellite Studies, University of Wisconsin-Madison), Figure 7.  An attempt to recreate this Enhancement Curve is displayed with breakpoint values along the colour table in Figure 8.  The resultant image of the application of this BD Curve is shown in Figure 9.  As you can see, given the poor resolution of the image, the application of this BD Curve is a disaster.  Comparing our image to that of the CIMSS shows that higher resolution will produce much more useful data.  While synoptic scale features are vaguely identifiable, the relatively narrower convective cloud band surrounding the eyewall cannot be discerned or evaluated using the BD Curve at this resolution.





















Figure 7 – BD Curve, CIMSS







Figure 8 – Breakpoints inserted per BD Curve intervals






















Figure 9 – BD Enhancement Curve

One other IR Enhancement to attempt is the Tropical Cyclone IR Enhancement Curve from the Australian Bureau of Meteorology.  Below is a sample image of this curve and its corresponding colour/temperature values in Figures 10 and 11, respectively.

















Figure 10 – Two Tropical Cyclones off of NT and WA, Australia.
"Satellite image processed by the Bureau of Meteorology from data received from the geostationary meteorological satellite MTSAT-1r operated by the Japan Meteorological Agency".















Figure 11 – BOM TC Key 
The breakpoint/colour table and resultant image after the application of this IR Enhancement are shown in Figures 12 and 13, respectively.



Figure 12 – Breakpoint/Colour Table














Figure 13 – Satellite image after application of BOM TC IR Enhancement

It is obvious that the BOM TC IR Enhancement is much more successful at this resolution.  The intense convective cloudbands to the E, N, and W can be seen much more clearly here.  In the future, it would be much more useful to have higher resolution IR data.  Perhaps with the launch of the new GOES-R, this will be available in the future.

References
-Australian Bureau of Meteorology (http://www.bom.gov.au)
-Cooperative Institute for Meteorological Satellite Studies, University of Wisconsin-Madison (http://cimss.ssec.wisc.edu/tropic2/misc/other/faq/faq_enhance.html)
-“Tropical Cyclone Intensity Analysis and Forecasting from Satellite Imagery”, Vernon F. Dorak, 1975
-“Development of an Objective Scheme to Estimate Tropical Cyclone Intensity from Digital Geostationary Satellite Infrared Imagery”, Christopher S. Velden, Timothy L. Olander, Raymond M. Zehr

.BT