Thursday, May 23, 2013

The Oklahoma and Tri-State Tornados


The catastrophic tornado that descended on Moore, Oklahoma on May 20th 2013 was one of the most intense yet observed. Now officially rated as an EF 5 system, the highest on the tornado rating scale, it is believed to have generated surface winds of around 340 km/hr (210 mph).


The tornado as it moved to the southwest of Moore - image from Wikipedia Commons (click to enlarge)

The funnel was estimated to have been more than 2 km (1.3 miles) across and during its 50-minute life span travelled some 27 km (17 miles), including a rampage across the highly populated Moore area.

The tragic death toll is, at the time of writing, 24 and more than 200 people were injured.  The damage bill will run into billions of dollars.

Comparisons with the infamous Tri State tornado of March 18 1925 have already been made. In this event a twister ripped through some twenty sizeable townships, including Gorham, Murphysboro, De Soto, West Frankfort and Parrish, all in southern Illinois, causing utter destruction right across the area.

Eventually the tornado crossed the border into Indiana, where it inflicted massive damage to the townships of Griffin and Princeton, before finally abating, after the longest continuous rampage of any known twister.

Contemporary newspaper article following the Tri State tornado of 1925 - image from Wikipedia Commons (click to enlarge)

Subsequent investigation of the damage trail revealed a monstrous gouge of destruction across the countryside, some 353 km (219 miles) long and about 1.2 km (three quarters of a mile) wide. From existing photographic evidence of the damage produced, experts have rated the Tri State as an F5 tornado.

In all, 695 people died - still the record by far for an American tornado. Over 2000 were injured and some 15,000 homes demolished.

It is difficult, if not impossible, to directly compare these tragedies, but one statistic does stand out – the massive difference in the death toll. During the Tri State event there was no organised tornado warning system, no radar imagery and no satellite photographs available. This twister struck virtually without warning.

For the Oklahoma event, effective short-term warnings were issued by the US National Weather Service and these, without doubt, saved many lives. The great strides in public education about tornados, as conducted by the Weather Service and other Government agencies have also been most effective. And this, together with publically available information on the Internet, plus the training and skill of the National Weather Service meteorologists, helped prevent another Tri State scale death toll.

The logo of the National Weather Service of the United States - image from Wikipedia Commons (click to enlarge)

Unfortunately tornados are part of the climatology of the southern parts of the United States but improved forecasting skill, together with technology and public education is making a real difference. Our hearts go out to the people on Moore in Oklahoma who have been devastated by this event.

For an Australian example of the increased effectiveness of weather forecasting see:

Sunday, February 17, 2013

Meteorite Rocks Russia


On Friday 15th February 2013, locals in the Russian city of Chelyabinsk were astonished to see a blinding light streak across the sky in the early morning glow, with a brightness rivaling that of the sun itself. Soon after, amid noises of rolling thunder, the ground shook, buildings swayed and windows shattered. It turned out later that some 1200 people had been injured, mostly by falling debris and flying glass from damaged buildings.

Reconstructing this extraordinary event, scientists concluded that the event was generated by a meteoroid exploding above the ground, producing a giant shock wave that blasted downwards and outwards and generating energy similar to that of a small nuclear explosion.

Planet Earth is enshrouded by a protective blanket - the atmosphere – that enables life as we know it, in all its forms, to exist. But of equal importance it provides an invisible shield that protects us from the fusillade of rocks called meteoroids that constantly bombard us from outer space.

When a meteoroid enters the atmosphere, travelling at speeds normally in excess of 50,000 km per hour, it begins to burn up because of friction with the atmospheric gasses. This produces a bright streak of light across the sky that is normally only visible at night. If you are to go outside on a clear night and observe the sky for a period of half an hour or more you will usually see one or more of these luminous, transient streaks that usually only last for less than a second. This streak of light is known as a meteor.

A meteor in the night sky
(Image form Wikipedia Commons)

In most cases the chunk of rock will burn up or vaporize before reaching the ground, and it is this protective property of the atmosphere that has played a big part in the survival of life on the planet. Without it we would look like the Moon that has no such protection and is pockmarked with impacts from many thousands of meteoroids.

In some cases fragments will reach the surface of the Earth as a shower of rocks called meteorites and these are always interesting to scientists as they are ancient objects from the far flung reaches of outer space and often have a different structure and composition to rocks we find on Earth.

The surface of the Moon - scarred by countless meteoroid impacts.
(Image from Wikipedia Commons)

On rare occasions much larger meteoroids will enter the atmosphere, with a size big enough to prevent complete vaporization and these will reach the lower levels of the atmosphere partially intact and still travelling at tremendous speed. One of two things usually follows.

The first is what probably happened over Chelyabinsk – a massive mid air explosion that generates a blindingly bright flash, together with a shock wave and sound of rolling thunder. Smaller rock fragments will then shower across the area as meteorites. 

Russia was also the scene of another such event in 1908 when a monstrous air burst explosion over the Tunguska area produced a massive shock wave that flattened huge tracts of pine forest in the area, affecting a zone of around 2000 square kilometers. This was a much more powerful event that Chelyabinsk incident.

But what can also happen is when the rock remains largely intact all the way to the surface, eventually striking the ground with colossal force and producing a large impact crater. It has long been believed that an event such as this some 65 million years ago produced a cataclysmic explosion of such a scale that the atmosphere around the world was affected, with the extinction of the dinosaurs a consequence.

As a testament to this type of event, large impact craters can be found today, including “Meteor Crater” near Winslow, Arizona that was created about 50,000 years ago when a large meteorite slammed into the area. The crater is about 1.2 km across and 170 m deep.

Above: Meteor Crater, Arizona. (Image from Wikipedia Commons; Click to enlarge)

In Australia, Wolfe Creek is a large crater located in the desert of Western Australia about 150 km to the south of Halls Creek. It is estimated that this crater was produced by a meteorite that had a mass of some 50,000 tonnes striking the surface around 300,000 years ago. The crater is about 900 metres across and 60 metres deep.
Above: The Wolfe Creek Crater, Western Australia
(Image from Wikipedia Commons; click to enlarge)

What would happen if such an object were to stroke a modern city – such as Sydney or Melbourne? Well, the short answer is - disaster. The actual impact crater would take out a suburb, and the associated shock wave and impact vibrations would likely destroy much of the city. So should we be concerned?

Well the short answer to this is no. Events of such as Meteor Crater and Wolfe Creek probably only occur only about once every 50,000 years or so, and in the great majority of any future cases the actual impact point would be in non-urban area. You have more of a chance of being struck by lightning or kicked to death by a donkey that dying through meteorite impact.

Thursday, November 29, 2012

Swing Bowling


In most top class cricket teams today there is at least one swing bowler, one who can move or “swing” the ball from its initial line in the air, producing a difficult situation for the batsman, both from a scoring point of view and also just to survive at the crease.

One of the earliest exponents of swing bowling was the great Australian pace-man Frederick “The Demon” Spofforth (1853 – 1926), who began his spectacular Test career in 1877 at express pace, but later switched to variation in his bowling, including a mean in-swinger that produced plenty of wickets. 


Frederick Spofforth (1853 to 1926)
Test bowler for Australia - known as "The Demon"
(Image form Wikipedia Commons)

Known as “swerve” in the 19th century, it was further developed over the years and is now recognized as one of the main weapons in the arsenal of the fast medium bowler. The English quick James Anderson is recognized as one of the great swing bowlers of the present time.

Swing bowling is very much an art, and is produced through several different factors, including the way the ball is held on delivery, the nature of the shine on the ball, and perhaps a little more surprisingly, the weather.

English fast bowler James Anderson - a noted swing bowler
(Image form Wikipedia Commons)

Bowling a swinger basically depends on the position of the seam on the ball through the delivery and this results in one side travelling through the air faster than the other. This is encouraged by polishing one side of the ball and assisted by the prevailing atmospheric conditions such as temperature, humidity, cloud cover, together with wind speed and direction.

The denser the air, the more swing is encouraged, so cooler air is a more fertile swing environment than warmer air. Up until quite recent times it was also believed that high humidity helped in encouraging swing, but new research has revealed the rather surprising fact that cloud cover may be far more important. In bright sunlight hot air rises from the surface of the pitch, creating a turbulent environment for the ball to pass through, which reduces swing. In overcast conditions there is less rising air, less turbulence and more swing.

All this means that cool, overcast weather is best for swing bowling and the swing can also be magnified if there is some component of the wind blowing across the wicket in the same direction in which the ball is swinging.

These conditions are met with far more often in England than Australia where hot and sunny weather is the norm during the summer months, but on occasion good swing bowling weather can emerge here as well. In the southern capital cities of Australia, such as Adelaide, Hobart, Melbourne and Sydney, this can happen in a southerly airflow following a cold front, when temperatures fall and cloud cover increases.

One of the greatest exhibitions of swing bowling ever seen was by the Australian Bob Massie in the Second Test at Lords in England during the 1972 Ashes tour.

In cool and cloudy conditions, Massie, coming alternately over and around the wicket, bent the ball through the air so prodigiously that many of his deliveries were virtually unplayable and the English batting was routed. His figures over the two innings were 8/84 and 8/53, representing match figures of 16/137, the third best test match figures of all time.

Massie’s display was a convincing demonstration of the tremendous potency of swing bowling, achieved when the bowler is on song and the atmosphere is just right for the purpose.

Great footage of Massie’s bowling during this Test can be seen at

Tuesday, November 13, 2012

在澳大利亚的中国


中国在澳大利亚的历史是一个有趣的。有几个中国人抵达澳大利亚在1800年初,但发现于1852年在澳大利亚农村地区的黄金生产的大量涌入,所有的金矿尝试自己的运气。

虽然很多最终还是回到了中国,中国移民搬离金矿和在悉尼附近开设小型企业,包括食品商店,并提供招待所。此外,中国市场花园窜出了在悉尼的郊区,蔬菜种植,后来在市场出售。中国人也开辟了家具制造工厂,在那里好,价格便宜的家具制造。

中国市场的园丁,悉尼,1893年

社区领袖,包括餐馆老板美梅光达在1890年的悉尼成为一个成功的受人尊敬的商人。男人像他那样多,逐步打破了当地对中国社会的偏见,它被越来越多地认识到,绝大多数的中国人的勤奋工作和良好的公民,澳大利亚。

一个皇家委员会在1891年举行“指称中国赌博和不道德”,并发现,中国的房子在悉尼整齐,很好的照顾和谁娶了中国男人的澳大利亚妇女发现他们良好的和有爱心的丈夫。




美梅光达

在中国和澳大利亚之间的关系是一个重要的转折点,当日本侵略中国南京在1937年,中国本土的社会团结。许多中国人参加了澳大利亚军队在第二次世界大战中抗击日本。

悉尼和墨尔本周围的大多数中国反对共产主义和不支持毛泽东政权在20世纪60年代,但在过去的三十年中,政治的情况已经淡化。在悉尼唐人街附近的语言反映了这一点 - 在60年代和70年代,这是几乎所有的粤语,但现在是压倒性的普通话。

在最近的时代,已成为澳洲的贸易联系越来越紧密,中国和这个行业现在是澳大利亚出口的最重要的因素之一。

悉尼的唐人街,一个众所周知的用餐区和旅游景点。

社会上也有显着增加之间的整合与异族通婚越来越受欢迎在过去的三十年,中国和澳大利亚的社区我个人熟悉这是我的女儿在法律上是中国的澳大利亚,当然是我的两个可爱的孙子。


澳大利亚著名的中国公民过去的150年:

美梅光达(1850年至1903年):在澳大利亚悉尼的中国商人和社区领袖。非常成功的商人

黄如彩(1925年至2009年):中国澳大利亚曾在澳大利亚军队在第二次世界大战的精英突击队的一员。被授予的杰出行为勋章,英勇的行动和后来的承澳大利亚勋章。

张任谦(1936年至1991年):中国的心脏外科医生和现代化的先驱,听到移植。获委任为伴侣澳洲的命令。拖马来西亚在1991年申办失败的勒索的罪犯被谋杀。






所以约翰(1946 - ):中国的澳大利亚商人,并两次当选市长的墨尔本市
















黄英贤(1968 - )澳大利亚参议员代表南澳大利亚州和一个联邦部长吉拉德政府

Sunday, August 12, 2012

In Flight Air Turbulence


One of the nagging worries with any aircraft flight is turbulence. It sometimes strikes without warning and can produce a frightening experience for even the most seasoned of fliers.

Mostly turbulence is only minor – a series of “bumps” that might last for a few seconds - but at the other end of the scale it can be far more serious. Major and abrupt vertical and horizontal changes in the position of the aircraft can throw loose objects and even people, around the cabin with injuries sometimes resulting. And at the extreme end of the spectrum turbulence can produce structural damage to the aircraft and in some very rare cases result in an aircraft accident.

Turbulence has four broad categories:

(1) Light: slight “bumpiness” but with little of no discomfort for passengers.

(2) Moderate: Passengers walking down the aisle will be moved off track; loose objects in the cabin will move about.

(3) Severe: Any standing passengers will be thrown off balance. Loose objects will pitch onto the floor.

(4) Extreme: Unsecured passengers thrown violently about – they may strike the roof or lateral areas of the cabin. Loose objects turn into interior missiles.

Cases three and four are quite rare but when they do occur can cause injury to passengers or cabin staff. In Australian airspace we see about between 2 and 3 reported significant turbulence encounters per month, or 24 to 36 per year. In terms of the number of flights and people carried during this time this represents only a very small percentage of flights.

In flight turbulence is caused by small scale currents or vortices in the air that produce “bumpiness” when the aircraft flies through it, similar in some ways to a car driving over a series of corrugations in the road. There are several ways turbulence is produced in the atmosphere.

Thermals: These are rising parcels of air generated by the atmosphere being in contact with a warm surface below (land or ocean). If there is sufficient moisture in the air, cloud will form over these thermals and form billowing cotton wool formations called cumulus cloud. An aircraft flying through this type of cloud will usually experience light to moderate turbulence.

Aircraft flying through cumulus clouds will normally experience turbulence because of the thermal activity. (Click to enlarge)

Thunderstorms: If rising air continues to be generated in a cumulus cloud it can grow to prodigious heights before it finally flattens out, typically at heights of 10 to 15 km above the ground. When the cloud grows to this height it contains regions of powerful “up and down” draughts in which there is a mixture of rain and hail, with lightning and thunder also added to the mix. This is a giant cumulus cloud, more properly called a cumulonimbus and is popularly known as a thunderstorm.

Pilots will avoid penetrating a cumulonimbus cloud because turbulence inside can be severe to even extreme. Fortunately these clouds are highly visible by day and also easily detectable on radar both day and night so are readily avoidable in a modern passenger aircraft.















Moderate to severe turbulence is often encountered within cumulonimbus clouds because of the violent mix of updrafts and downdrafts within. This diagram is not drawn to scale - in reality the aircraft would be less than the size of a pin head here. (Cloud image from Wikipedia Commons, click to enlarge)

An infamous case of thunderstorm penetration involving the loss of an aircraft occurred in November 1961 at Mascot airport in Sydney. See


Mechanical turbulence: As wind passes over the ground, air in contact with the surface is slowed by friction, while the air above continues at the unimpeded speed. This creates many thousands of rolling vortices, and depending on the wind speed and roughness of the terrain, these can extend upwards for a considerable height. Aircraft flying in these regions will encounter “bumpiness” called mechanical turbulence, that is usually only in the light to moderate range.

However in some cases, when strong winds blow over a mountain range, the air can organise itself into large organised waves that extend several kilometres downstream of the mountains. Very powerful rising and falling air currents are often present in these waves and organised bands of clouds sometimes form near the wave peaks. These waves are called lee waves or mountain waves and the clouds are called lenticular because of the characteristic “lens” shape they often adopt. Just as we see with waves on the ocean, mountain waves sometimes topple and break producing circulations called rotors.












Mountain waves (or lee waves) can produce severe turbulence. Clouds sometimes form at the peak of the waves. (Click to enlarge)

Turbulence produced by mountain waves can be moderate to severe, and in extreme cases, the actual destruction of an aircraft has been recorded. Perhaps the most infamous of these was the disintegration of a Boeing 707 jet, Flight 911 that was flying near Mt. Fuji in Japan on February 4th 1966. It is believed that the aircraft flew into an area of powerful mountain waves that produced extreme turbulence and failure of the air-frame. A detailed analysis of this incident can be found at


Wind shear:
Put simply, wind shear is the change of wind speed and direction with height or over a horizontal distance. There is always a degree of wind shear in the atmosphere, but when big changes take place over short distances, significant turbulence can result.

Wind shear turbulence can form when one layer of air slides across another, at a different speed or from a different direction, or both. This can generate wave like disturbances at the interface, called Kelvin Helmholtz waves, and if there is cloud present in this zone, the waves become visible.











Kelvin Helmholtz waves form when the winds above a certain layer (the dotted line here), are stronger than those below. (Image from Wikipedia Commons, click to enlarge)

But in many cases there is no cloud to alert the pilot that unusual atmospheric motion may be present and in these cases the phenomenon is referred to as “clear air turbulence” or CAT.

Jet streams, that are high-speed rivers of air that circulate the globe at approximately 10 to 15 km above the surface, are areas where CAT is often encountered. There are two main jet streams in each hemisphere, the polar jet and the subtropical jet and these meander and change direction as they circle the earth.

The main jet streams of the Earth. (Image from Wikipedia Commons)

Because jet streams are zones of high-speed winds running within the broad-scale atmospheric flow, there are surrounding regions where the wind speeds change quickly with both height and horizontal distance, and this can generate considerable wind shear and therefore turbulence. For more information on jet streams see


To get the issue of in flight turbulence into perspective it should be noted that even the most frequent fliers will never experience severe or extreme turbulence, and that the modern passenger jet is fantastically strong and well able to handle in flight turbulence in all its forms.

But for the passenger, by far the best protection against turbulence is to fasten your seatbelt. When not moving about the cabin keep the belt buckled up, and even if severe turbulence is encountered you will safely ride it out if properly secured. 

Wednesday, June 20, 2012

Darlinghurst Gaol


Any pedestrian visitor walking along Forbes Street, Darlinghurst will be immediately impressed by the tremendous stone walls stretching along the eastern side of the road, punctuated by a magnificent sandstone gateway – in fact the entrance to today’s National Art School.

But for much of the 19th Century this entrance was the gateway to death and damnation for many unfortunate Sydneysiders. For this was the entrance to the infamous Darlinghurst Gaol, a place of brutality, confinement and misery.

The original gaol in Sydney was located in George Street, but by the mid 1820’s was grossly overcrowded, and the conditions so barbarous, that the Government agreed that a new gaol was necessary. A wag noted at the time that at the George street lockup it was so overcrowded that whilst it was possible to hang six people at once, there was only room enough to hang two in comfort. This was classical “gallows humour” at its worst.

A site was chosen on the heights above Woolloomooloo and building commenced for a new gaol, using locally quarried sandstone cut and placed by convict labour to produce a rectangular space surrounded by four huge walls. This was known as the Woolloomooloo Stockade but it was not until 1841 that prison buildings within these walls were partially completed according to a plan prepared by the Colonial Architect, Mortimer Lewis. He based the design on the Eastern Penitentiary in Philadelphia, which featured a central building from which cellblocks radiated outwards, like the spokes of a wheel. 

Plan for the gaol, c 1840 signed by the Colonial Architect Mortimer Lewis. Mitchell Library, State Library of NSW, Call no: SSV1/Gao/Darh/1 - Click to enlarge)

On June 7th 1841 the prison, although incomplete, was ready for occupation and the residents of Sydney were treated to a remarkable procession when the prisoners from George Street were marched through the streets up to their new accommodation – Darlinghurst Gaol. The recollections of an old ex gaol warder, who saw the scene, recalled the events in the Sydney Morning Herald of 9th January 1914:

“On the morning of June 7, 1841, a strange procession passed through the streets of Sydney—119 men in convict garb, chained together, on their way from the old gaol to the new one. "The redoubtable Curran," remarked the "Sydney Gazette," of the period, "heavily ironed, took precedence of his brother culprits." Later in the day, the female prisoners, numbering about 50, passed through the streets”. (The Curran referred to was Paddy Curran – the bushranger who was to become the first man hanged at Berrima Gaol in 1842).

 And so began a period of 73 years when Darlinghurst gaol was the main detention centre for NSW, producing a long and brutal history involving floggings, hard labour, and on 77 occasions the “extreme penalty” of the law, which in those days was execution by hanging.

A "birds eye" view of the Gaol, the Illustrated Sydney News, November 1866. (Click to enlarge)

The Herald’s article of 1914 provided some further detail:

“The first execution at Darlinghurst Gaol took place on October 29, 1841, when George Stroud and Robert Hudson were hanged, the former for murdering his wife, the latter for the murder of a fellow-convict.
In those days, an execution was a public thing, and was witnessed by hundreds of people. It is stated that no fewer than 10,000 people assembled to see the execution of the notorious Knatchbull in 1844. Public executions were abolished in Sydney in 1853, and it was not till 15 years afterwards that they were abolished in England. In all, Darlinghurst has seen 76 executions”.

And by the way, if you think hanging was a humane method of execution, many existing records show otherwise. In several cases, the knot in the rope that is placed behind the ear slips out of position during the drop and instead of the neck being broken, slow strangulation results. In these cases the onset of death can take 15 to 20 minutes. This happened at Darlinghurst with the Mount Rennie executions and with the hanging of Digby Grand, the Auburn murderer.

After only 15 years of operation the gaol had become overcrowded, so an extra wedge of land was purchased at the northern end of the site and a “Y” shaped cellblock was built there. It was in the cleft of this “Y”, that a gallows was built, replacing the makeshift structure that had been used in front of the gaol in public executions, and later in the prison yard when these were abolished. A little later, the circular building at the centre of the complex was completed – with the ground floor a reception area and the upper floor the prison chapel.

Sentry towers were built on top of the walls at the corners and these were manned 24 hours a day. A senior warder described how the guards operated while on sentry duty when they had to call to the senior warder every half hour, even all through the night:

"Half-past 1 o'clock. . . All's well. . . Number one."
The sentry at the gate has spoken.
"Half-past 1 o'clock. . . All's well. . . .Number two."  
And sentry No. 2, revolver at side, proceeds on his rounds. All's well in wings A, B, and C.
"Half-past 1 o'clock. . . All's well. . . .Number three."  
All's quiet at the hospital. "Half-past 1 o'clock. . . All's well . . .Number four."
Nothing suspicious in the Burton-street wing—wing E.
Sentries No. 1, No. 2, No. 3, and No. 4 pass on. The senior warder, attentive and alert, has noted their reports. All's well at the gaol. All's silent”.

The neighbours near the gaol got used to the mournful calls of the sentries that floated over the rooftops of Darlinghurst night and day for 365 days of the year.

A view of the gaol in 1874 from the October edition of the Illustrated Sydney News. (Click to enlarge)

As an interesting architectural feature, a tunnel was constructed that connected the holding cells beneath the adjoining Courthouse with the gaol. The prisoner would enter the tunnel on the gaol side and come up inside the Courthouse and then return by the same path.

As the years passed, construction proceeded, and by 1874, most of the main buildings had been completed. The main gate, opening out on to Forbes Street had been relocated from its original position a few metres up towards Burton Street and entirely remodelled in a rounded “buttress” style. This relocation was to prevent prisoners” rushing” towards the main gate from near the Governors residence.

Many famous and infamous prisoners passed through the gates of the gaol, including the bushrangers Frank Gardiner and George Scott (Captain Moonlite). Scott was executed for his crimes. Other bushrangers who were executed were the two Clarke brothers (hanged in 1867) and John Dunn, a member of Ben Hall’s gang (hanged in 1866).

Then there was Jimmy Governor who was executed in January 1901 for mass murder after a killing spree all across central NSW the previous year.

The infamous Mount Rennie rape case produced a dark climax when four youths, all under 20 years of age, (one only 17) were hanged at the gaol in January 1887, amid one of the great public controversies in Australia’s legal history.

Watercolour of the gaol by the inmate Henry Louis Bertrand, 1891. Bertrand was convicted of the murder of Henry Kinder in 1865 in one of Sydneys most notorious homicides of the time. He eventually served a 28 year sentence, one of the longest in Darlinghurst's history. Mitchell Library, State Library of NSW, Call no: SV1/Gao/Darh/2 - Click to enlarge)

The only woman to be hanged at the gaol was Louisa Collins who was executed in January 1889 for poisoning two of her husbands in order to receive life insurance payments.


Louisa Collins - executed at Darlinghurst Gaol in 1889.
(Photograph from the NSW State Records Office)

Our great Australian poet Henry Lawson also “did time” at Darlinghurst, for unpaid debts and non-payment of alimony. In his haunting poem “One Hundred and Three”, he describes the tough conditions at the prison, referring to it as “Starvinghurst Gaol”, because of the meagre rations given to the inmates.

The severe punishment of a flogging was liberally used at the gaol, right through into the last decade of the 19th century, and was always a brutal form of torture. The horror of a flogging was well caught in the article that appeared in a contemporary newspaper account on 13th February 1895:

RECEIVED HIS FLOGGING.
The young man, Robert Strong, for brutal assault upon a sailor, received his flogging of 20 lashes in Darlinghurst gaol on Saturday afternoon. From first to last stroke the man utterly broke down. He howled, wept, and prayed; his ejaculations, "Oh, God, have mercy," could be beard outside the gaol wails. When released he was able to walk with difficulty, and it was evident that he bad been effectually cowed, as there was the absence of that mock air of bravado visible as he marched to the whipping post.

Despite the heavy punitive nature of Darlinghurst, common to all 19th century Australian prisons, a real attempt at rehabilitation was also made, through trade training and education. In this respect the gaol was somewhat ahead of its time, particularly in comparison to other capital city gaols around Australia where punishment was placed well ahead of rehabilitation.

The gaol was an industrial prison, with a long line of workshops inside the wall on the eastern side. Diverse activities took place here, including broom and mat making, stonecutting, bookbinding and cobbling. During this work time strict procedures were in place and no conversation was permitted.

The gaol school room - from the Illustrated Sydney news of November 1866 (click to enlarge)

In what was very advanced thinking for the time some of the prisoners were also given instruction in a school room in order to achieve at least basic literacy before release. The Illustrated Sydney News reported in 1866 that the “Hours of labour were from 7 to 8, 9 to 12 and 1 to 4, in all 7 hours. A great many attend school; some one hour, others two hours, thereby reducing the hours of labour…”

There was a prison uniform that in its basic form consisted of a shirt with “Darlinghurst Gaol” surrounding a broad arrow on the back. There were variations of this uniform depending on the time of the year and the place of work of the prisoner.

In the broom factory, showing the broad arrow motif on the back of the prisoners shirts - from the Illustrated Sydney News November 1874 (click to enlarge)

In common with many 19th century prisons, tobacco was the currency within the walls. Friends of the prisoners would walk up Burton Street and throw tobacco packages over the walls where they would be eagerly seized by the inmates. Tobacco was used as trade in all sorts of transactions within the walls, swapping it for food, drink and perhaps for privileges from a corrupt guard.

After many years of increasing difficulty associated with an ever-rising inmate population and nowhere to expand, the inevitable happened and the Government looked for another site for a gaol.

Finally, in 1914, after 73 years of operation, Darlinghurst Gaol was closed and the existing prisoners taken by special tram out to the new accommodation at Long Bay. During the First World War Darlinghurst was used as an internment camp for Irish and German nationals, and then in a remarkably enlightened move it was transferred to the NSW Department of Education.

















Above: The interior of the Darlinghurst gaol chapel c 1880. The stained glass windows were removed and taken out to the new chapel at Long Bay in about 1913. They were then returned to their original location in Darlinghurst in 1981. Mitchell Library, State Library of NSW, Call no: SPF/168 - Click to enlarge)

After extensive renovation it was born again in 1921 as East Sydney Technical College, and since 1995, the National Art School. Today the buildings remain externally intact and form a unique example of a complete 19th century Australian prison complex. 


 The gates to the National Art School today - once the entrance to the dreaded Darlinghurst Gaol.
Image from Wikipedia Commons (click to enlarge)

Left: The shirt design motif worn by prisoners c 1880. 


References: Hope in Hell - Deborah Beck, Allen and Unwin, 2005

























For a great series of contemporary images see

http://www.flickr.com/photos/9028007@N05/sets/72157622607281922/

Sunday, June 10, 2012

Heat in Cars

Heat in Cars

During the warmer months it's a good time to remind ourselves about the dangers of locking children or pets in cars parked outside, particularly in bright sunlight.

It’s often tempting to do this, perhaps to pop into a shop for just a few minutes, without all the hassle of buckling and unbuckling seatbelts and arranging prams and strollers.

However even a short time can be extremely dangerous, particularly during the summer months. Tests have shown that on a 30C (86F) day, as measured in the shade, a car parked in the sun can heat up from 20C (68F) to 44C (111F) in only ten minutes. After 20 minutes, temperatures inside the same car can hit 60C (140F).

Temperatures can ramp up to 60C (140F) inside a car parked in the sun in less than half an hour.

The shape of the car, its colour, interior type and the amount of window and windscreen glass also affect the way the vehicle heats up, as do other variables such as cloud cover, wind and the angle of the sun. But the effects of these are usually quite minor and any vehicle parked outside on a hot day will heat up quickly. And contrary to popular opinion, leaving the windows partially down does not solve the problem – it may just slow the heating process slightly. There is no safe way to do it.

Even hi-tech modern vehicles, such as this Honda Civic, can heat up to dangerous interior temperatures when parked outside during bright sunlight conditions. (Image from Wikipedia Commons - click to enlarge)

But perhaps of even greater significance is that controlled tests have also revealed that we don’t need very hot weather to produce dangerous temperatures inside cars; even in mild conditions of around 22C (72F), interior temperatures can rapidly ramp up to 40C (104F) plus in less than an hour in bright sunlight conditions.

Small children confined in these sauna-like temperatures can dehydrate rapidly, and suffer an onset of hyperthermia, where the core temperature of the body rises to dangerous levels, above 40C (104F) on occasion. This can create a serious and sudden medical emergency with hospitalisation required, and in extreme circumstances fatalities have occurred.

In the United States, where these figures are readily available, more than thirty children die each year of heatstroke, after having been locked in cars parked outside. There are probably numerous examples of pets dying under similar circumstances.

So the summer message is clear – don’t expose your children or pets to these risks, even for a short period of time.