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Showers and storms over WA's interior in unstable air. A cold front brings a few gusty showers to western Tas. A high over the southeast is causing stable weather over most areas while directing some showers over the east Qld & northeast NSW coasts.

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Drizzle ClearingSydneyNSW

16.7°C

14°C
22°C

Mostly SunnyMelbourneVIC

10.2°C

7°C
18°C

Mostly SunnyBrisbaneQLD

18.8°C

16°C
25°C

SunnyPerthWA

17.1°C

14°C
28°C

Mostly CloudyAdelaideSA

17.6°C

10°C
22°C

Fog Then SunnyCanberraACT

6.6°C

6°C
19°C

Late ShowerHobartTAS

11.6°C

11°C
18°C

Mostly SunnyDarwinNT

26.8°C

24°C
33°C

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Today, 6:44AM UTC

Wintry blast on the way

The mild autumnal weather that southeastern Australia has been basking in this week is about to come to an abrupt and chilly end, with snow possible down to 600 metres in Tas.  A strong cold front will cause the huge contrast in temperatures and is expected to sweep across southeastern Australia on Friday and into the weekend.  The cold front will drag a frigid airmass over the region late this week, dropping temperatures to 3-5°C below average and bringing subzero overnight temperatures to some areas. The wintry blast will reach Melbourne on Friday afternoon and Sydney later that night.  The image below shows forecast air temperatures around 1.5km above sea level on Friday, revealing how warm autumn-like air in the middle of the week will be replaced with a much colder wintry air mass by Friday.  Images: Forecast 850 hPa temperature at 10pm AEST on Friday, May 17, according to the ECMWF-HRES model.  The southeastern capital cities will see both maximum and minimum temperatures plummet from Friday, with the following temperatures forecast:  Hobart’s maximum will be 12-14°C on the weekend, which is 2-3°C below May’s average  Melbourne’s daytime temperature will struggle to reach 14°C on Saturday and the minimum temperature early on Sunday morning should drop to 7°C.  Adelaide’s overnight temperature Saturday into Sunday will drop to 5-6°C, which is around 4-5°C below the May average. The city should also see a run of 4 days from Saturday with the maximum reaching only 17-18 °C  Canberra will be freezing Sunday morning, with frost and a minimum of –1°C, the daytime temperature will reach only 13°C on Saturday  Sydney is also in for a cool weekend with daytime temperatures of 17-19°C, nighttime temperatures will drop to 7-9°C.  Brisbane’s minimum will drop to 11-12°C early Sunday and Monday mornings, which is 3-4°C degrees below May’s average.  These cool temperatures could feel up to 5°C cooler with strong southerly winds adding to the windchill.  These winds should increase wind power across the southeast over the weekend, after a lengthy period of lighter winds in recent months.   The wintry blast will also drop the snow level over the southern alpine regions, with the snow level expected to drop down to 600 metres in Tas.   Image: Snow on Mount Wellington, Tas on May,17 2022 Source: @jrikin   The Vic alps could also see snow down to 1400 metres, and while the NSW alps could see a dusting, it doesn't look like much will fall over the region at this stage.  

Today, 3:20AM UTC

Sun unleashes strongest flare of current solar cycle

The sunspot region that produced last week’s mesmerising aurora displays has just unleashed another strong solar flare, this one even more powerful than anything else seen during the current solar cycle. In case you missed it, large areas of the Northern and Southern Hemispheres were treated to vivid aurora displays late last week. Image: Aurora Australis seen from the Bendleby Ranges, SA on the weekend. Source: @bendlebyranges / Instagram These colourful night lights could be seen much further outside the polar regions than usual, including Florida and Queensland, thanks to a powerful geomagnetic storm created by multiple coronal mass ejections (CMEs) from the Sun. At its peak, last week’s geomagnetic storm reached the highest possible level on the G-scale (Extreme - G5), making this the first G5 storm since 2003. The CMEs that caused last week’s spectacular auroral displays originated from a cluster of sunspots designated Sunspot Region 3664, a region which also produced significant solar flares during the same period. At one point last week, this massive and complex sunspot cluster was about 17 times the diameter of Earth. FIND OUT MORE CORONAL MASS EJECTIONS AND SOLAR FLARES While the powerful geomagnetic storm that caused last week’s aurora displays has now calmed down, Sunspot Region 3664 has remained active. According to NOAA’s Space Weather Prediction Center, a solar flare with a magnitude of X8.7 was detected from Sunspot Region 3664 at 1651 UTC on May 14. X-Class flares are the strongest of four categories and this X8.7 flare is stronger than anything measured last week. In fact, it’s the strongest solar flare detected in the current solar cycle, which begun in 2019 and is expected to peak next year. WHAT IS THE SOLAR CYCLE? FIND OUT HERE Image: Predicted and observed sunspot numbers of the current solar cycle, which commenced in 2019. Source: NOAA / Space Weather Prediction Center. However, while the X8.7 solar flare that occurred on May 14 was stronger than last week’s flares, it was not oriented towards Earth when it occurred, and it is currently unclear whether a CME associated with this flare could glance Earth later this week. As of 0030 UTC on May 15, NOAA’s Space Weather Prediction Center said that the CME associated with this week's X8.7 flare "is currently being analyzed for any Earth-directed component.” Given the orientation of Sunspot Region 3664 at the time of the X8.7 flare, it is unlikely that we will see a repeat of the weekend’s wide-reaching aurora displays in the coming nights, even if we do see a glancing effect from this event. Image: The X8.7 solar flare – as seen in the bright flash on the right – on May 14, 2024. Credit: NASA/SDO The current solar cycle is expected to peak in 2025 before declining over the next 5 to 7 years. Sunspot activity will remain elevated around the solar cycle’s peak, maintaining an elevated likelihood of aurora displays on Earth.

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14 May 2024, 6:13AM UTC

Australia officially on La Niña alert

The BoM has officially placed Australia on a La Niña watch, less than a month after El Niño was officially declared over. "There are some early signs that a La Niña might form in the Pacific Ocean later in 2024," the BoM reported in its May 14 update. "As a result, the Bureau's ENSO [El Niño–Southern Oscillation] Outlook has shifted to La Niña Watch." What is La Niña? La Niña is a broad-scale circulation in the Pacific Ocean that is characterised by warmer-than-average sea surface temperatures to the northeast of Australia and abnormally cool water in the central and eastern equatorial Pacific Ocean. The warm oceans and humid atmosphere that are associated with La Niña typically cause increased convection over the western side of the tropical Pacific Ocean. This in turn drives above average rainfall and cloud cover across much of Australia. In its statement on Tuesday, the BoM said that when La Niña Watch criteria have been met in the past, a La Niña event has subsequently developed around half the time. The BoM said ENSO will likely remain neutral until at least July this year, however the early indications that a La Niña could eventuate in the second half of 2024 include: Sea surface temperatures (SSTs) in the central Pacific have been steadily cooling since December 2023. This surface cooling is supported by a significant amount of sub-surface cooling in the central and eastern Pacific. Australia's last La Niña ended in 2023. It came at the end of a triple La Niña in 2020/21, 2021/22 and 2022/23, just the third time in recorded history that the event has occurred three years in a row in Australia.

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14 May 2024, 3:01AM UTC

Can auroras affect aeroplanes?

Auroras lit up the skies on the weekend amid one of the strongest geomagnetic storms in years, but did this display impact aeroplanes and the aviation industry?  The spectacular exhibit was the aurora borealis/australis, or northern and southern lights seen in both hemispheres.      Images: Aurora Australis on Saturday, May 11 from Bendleby Ranges, SA (top), source: @bendlebyranges and Ricketts Point, Vic (bottom), source: @dayofthedreamer  These lights are typically only seen in the polar latitudes, but this weekend they were spotted in the Southern Hemisphere as far north as Mackay in Queensland. This was caused by the strongest solar flare and storm seen in over 20 years.  This auroral display was caused by a solar flare and multiple coronal mass ejections (CMEs) which erupted from the sun over a few days last week. Charged particles were then carried from the sun to earth by a solar wind.   When these particles reached earth, they interacted with our planet’s magnetic field and were driven towards the magnetic poles.   In the upper layer of the atmosphere called the ionosphere (90km above the surface) the solar wind collides with oxygen and nitrogen in this layer and produces a colorful display.  The southern lights typically occur between 50 and 800km above the surface, well above the layer of atmosphere that planes typically fly in.   So, do they impact aviation despite occurring well above the flight level?   Yes, space weather events like this can impact aviation communications, navigation and surveillance systems. They can also increase the radiation exposure of aircraft in the air.       Images: Aurora Australis from Virgin plane cockpit on Saturday, May 11. Source: @shelbytillett  The charged particles caused by CMEs can modify the upper layer of earth's atmosphere called the ionosphere, which can impact our technology systems.   High frequency radio communication depends on the ionosphere reflecting radio waves back down to earth.  Satellite communication, navigation and surveillance rely on the transmission of signals through the ionosphere.   According to the Bureau of Meteorology’s space weather department, >Space weather events that modify the density and/or structure of the ionosphere can therefore significantly impact the performance of HF COM, SATCOM and SATNAV systems". While communication and navigation can be impacted by the modification of the ionosphere, the electricity network can also be impacted. The storms can induce currents in power lines, overheating transformers, which can potentially cause power outages.   The strongest geomagnetic storm ever recorded occurred during September 1859, called the Carrington Event. This event caused multiple fires of telegraph systems across Europe and North America.  There have been no reports of negative major impacts of this solar storm, it was merely a spectacular display that captivated people across the world.   Unfortunately, auroras are notoriously difficult to forecast as they need multiple factors to line up for these beautiful lights to occur.  Looking ahead, the sun is nearing its solar maximum, which means we could see more sunspots on the sun's surface this year. This could increase our chance of seeing more spectacular displays in the coming months.

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07 May 2024, 11:23PM UTC

How severe thunderstorms impact energy infrastructure

Earlier this year destructive thunderstorms and winds equivalent to a category two cyclone lashed Victoria, bending towers and toppling trees and poles.  So, how can thunderstorms damage energy infrastructure, and are these events getting worse?   This event occurred during mid-February 2024, when a strong cold front generated severe thunderstorms and localised wind gusts of 130km/h after a prolonged period of extreme heat. The image below shows a squall line around 1,500km long causing lightning across four states in February.  Image: Himawari-9 satellite image, lightning and radar on Tuesday, February 13 at 3pm AEDT.  The destructive winds were caused by microbursts, which bent towers and toppled trees and poles in Vic, leaving thousands without power.   Image: Damaged transmission towers at Anakie, Source: AAP  Microbursts are a localised column of sinking air (downdraft) within a thunderstorm and is usually less than 4km wide. The cold, heavy air within this downdraft descends rapidly to the surface and then spreads out in all directions as it hits the ground. The image below shows how wind gusts are produced in thunderstorms.    Microbursts can be destructive and cause wind gusts above 100 km/h, which can be a risk for power infrastructure. The force applied to the structure is roughly proportional to the speed squared.  Fierce wind gusts from thunderstorms can:  Knock down trees, which can fall onto power lines  Topple poles  Knock out transmission towers.  Microbursts typically occur during the warmer months of the year and, unfortunately, they can develop rapidly and last for only a short period of time, making them difficult to predict and warn communities about.   Have these thunderstorm events become more severe in Victoria?   The severe thunderstorm season across southern Australia occurs during the warmer months of the year, between November and April.   While thunderstorms are more common across northern Australia, Qld, and NSW, they do occur frequently in the summer months. The map below shows the annual average lightning density in Vic between July 2014 and June 2023, with the most lightning occurring in the northeast high country each year.      Image: Weatherzone’s Total Lightning Network Annual lightning density mean between July 2014 and June 2023.  You can see in the map above that lightning is common to the north of Ballarat near Learmonth and Miners Rest, with the region seeing 37.7 pulses per year. The high country near Benalla and Whitfield recorded an average of 28.1 pulses, Thorpdale in Gippsland saw 24.5 pulses, and Melbourne only 8.2 pulses per year.    Research has shown that the warming climate is increasing the risk of heatwaves and bushfires, which can impact energy infrastructure. Unfortunately, it is unknown how global warming will affect thunderstorms and their associated destructive winds. To research climate change's impact on thunderstorms, we would need quality data that dates back well into history. Unfortunately, detecting lightning is a fairly new phenomena, so a solid climate base to compare data to is not currently existent.   According to the University of Melbourne researchers and Watt Clarity, ‘The evidence we do have suggests continued climate change may potentially increase the risk of extreme winds from thunderstorms. This is partly due to more moist and unstable air, which are essential for thunderstorms to form. We think these conditions could occur more often with climate change, in part because warmer air can hold more moisture.’   Indeed, much of Australia had an unusually stormy summer 2023/24, with Melbourne, Canberra and Brisbane all seeing 5 to 6 extra storm days a season. The map below shows that an unusually high number of thunder days were seen over most of Qld, NSW, SA, Vic, the ACT and Tas during the summer of 2023/24 compared to the average of the most recent nine years.  Image: Thunder day anomalies for summer 2023-24 versus the average thunder days for the nation’s nine most recent summers (2014/15 to 2022/23). 

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