Climate Driver Update
Climate influences in the Pacific, Indian and Southern oceans and the Tropics
For long-range forecasts of rainfall and temperature for Australia, please see our long-range forecast page. It provides the best guidance on likely conditions in the coming months, using the Bureau's climate model to take into account all influences from the oceans and atmosphere when generating its long-range forecasts.
The Climate Driver Update provides information on the broader hemispheric climate state, such as the El Niño Southern Oscillation and Indian Ocean Dipole. This information provides additional context to the rainfall and temperature forecasts.
Average of international model forecasts for NINO3.4
Average of international model forecasts for IOD
- See also: Links open in new window
- About Australian climate influences
- Climate model summary
- Long-range forecast
Sea surface temperature maps
Sea surface temperature maps are not available for forecasts before June 2021
Global sea surface temperature outlooks for the months and season ahead. Anomalies indicate the difference from normal.
SST outlooks for the next 3 months
Pacific Ocean
ENSO is the oscillation between El Niño and La Niña states in the Pacific region. El Niño typically produces drier seasons, and La Niña drives wetter years, but the influence of each event varies, particularly in conjunction with other climate influences.
International climate model forecasts
Graph details
The graphs are based on the ensemble mean for the most recent model run.
These graphs show the average forecast value of NINO3.4 for each international model surveyed for the selected calendar month. If the bars on the graph are approaching or exceeding the blue dashed line, there is an increased risk of La Niña. Similarly, if the bars on the graph are approaching or exceeding the red dashed line, there is an increased chance of El Niño.
- See also: Links open in new window
- ENSO Outlook status
- Climate model summary
- Long-range forecast
Weekly sea surface temperatures
Graphs of the table values
Monthly sea surface temperatures
Graphs of the table values
- See also: Links open in new window
- Animation of recent SST changes
- Weekly index graphs
- Sea surface temperature maps
- Map of NINO and IOD regions
5-day sub-surface temperatures
Monthly temperatures
Southern Oscillation Index
- See also: Links open in new window
- Monthly SOI graph
- 30-day SOI values
Trade winds
- Data Source: Links open in new window
- TAO/TRITON data
Cloudiness near the Date Line
About El Niño and La Niña (ENSO)
At a glance
ENSO is the oscillation between El Niño and La Niña conditions.
This climate influence is related to: El Niño La Niña The Australian Monsoon
What is it?
The term El Niño refers to the extensive warming of the central and eastern tropical Pacific Ocean which leads to a major shift in weather patterns across the Pacific. This occurs every three to eight years and is associated with a weaker Walker Circulation (see diagram below) and drier conditions in eastern Australia. El Niño Southern Oscillation(ENSO) is the term used to describe the oscillation between the El Niño phase and the La Niña, or opposite, phase.
In the eastern Pacific, the northward flowing Humbolt current brings cooler water from the Southern Ocean to the tropics. Furthermore, along the equator, strong east to southeasterly Trade winds cause the ocean currents in the eastern Pacific to draw water from the deeper ocean towards the surface, helping to keep the surface cool. However in the far western Pacific there is no cool current, and weaker Trades mean that this "upwelling" effect is reduced. Hence waters in the western equatorial Pacific are able to warm more effectively under the influence of the tropical sun. This means that under "normal" conditions the western tropical Pacific is 8 to 10°C warmer than the eastern tropical Pacific. While the ocean surface north and northeast of Australia is typically 28 to 30°C or warmer, near South America the Pacific Ocean is close to 20°C. This warmer area of ocean is a source for convection and is associated with cloudiness and rainfall.
However, during El Niño years, the trade winds weaken and the central and eastern tropical Pacific warms up. This change in ocean temperature sees a shift in cloudiness and rainfall from the western to the central tropical Pacific Ocean.
Neutral ENSO phase
Trade winds push warm surface water to the west and help draw up deeper, cooler water in the east. The warmest waters in the equatorial Pacific build up to the north of Australia and that area become the focus for cloudiness and rainfall.
La Niña
Trade winds strengthen, increasing the temperature of the warm water north of Australia. Cloudiness and rainfall north of Australia are enhanced, typically leading to above average winter–spring rainfall for eastern and central parts of the country, and a wetter start to the northern wet season.
El Niño
Trade winds weaken (or reverse) and warmer surface water builds up in the central Pacific. Cloudiness and rainfall north of Australia are supressed, typically leading to below average winter–spring rainfall for eastern parts of the country, and a drier start to the northern wet season.
The Southern Oscillation Index, or SOI, gives an indication of the development and intensity of El Niño or La Niña in the Pacific Ocean. The SOI is calculated using the pressure differences between Tahiti and Darwin. The following figure demonstrates the typical fluctuations in SOI over a period of 11 years. Positive SOI values are shown in blue, with negative in orange. Sustained positive values are indicative of La Niña conditions, and sustained negative values indicative of El Niño conditions.
How does it affect Australia?
Each phase of the ENSO has a very different effect on the Australian climate. El Niño and La Niña generally have an autumn to autumn pattern of evolution and decay. That is, they typically begin to develop during autumn, strengthen in winter/spring, then decay during summer and autumn of the following year. These effects are described in further detail on the following pages: El Niño and La Niña.
Further information and latest updates
Further information about the El Niño Southern Oscillation and its impact on the Australian Climate.
Timeline of monthly Southern Oscillation Index (SOI) values since 1876
Sustained negative values (bottom/yellow) of the SOI below −7 may indicate El Niño, while sustained positive values (top/blue) above +7 may indicate La Niña. La Niña and El Niño events since 1900 are indicated on the graph.
Drag graph slider to see full history and y-axis scale.
The Indian Ocean Dipole (IOD) is defined by the difference in sea surface temperatures between the eastern and western tropical Indian Ocean. A negative phase typically sees above average winter-spring rainfall in Australia, while a positive phase brings drier than average seasons.
International climate model forecasts
Graph details
The graphs are based on the ensemble mean for the most recent model run.
Thse graphs show the average forecast value of the IOD index for each international model surveyed for the selected calendar month. If the majority of models are approaching or exceeding the blue dashed line, then there is an increased risk of a negative IOD event. If the majority of models are approaching or exceeding the red dashed line, then there is an increased risk of a positive IOD event.
- See also: Links open in new window
- Climate model summary
- Long-range forecast
- See also: Links open in new window
- SST timeseries graphs
- Sea surface temperature maps
- Map of NINO and IOD regions
- 1960
- 1961
- 1963
- 1967
- 1972
- 1975
- 1990
- 1992
- 1994
- 1996
- 1997
- 1998
- 2006
- 2010
- 2015
- 2016
- 2019
- 2022
there have been 9 moderate to strong negative IOD events and 9 moderate to strong positive IOD events.
About the Indian Ocean Dipole (IOD)
Indian Ocean sea surface temperatures impact rainfall and temperature patterns over Australia. Warmer than average sea surface temperatures can provide more moisture for frontal systems and lows crossing Australia.
Indian Ocean Dipole
Sustained changes in the difference between sea surface temperatures of the tropical western and eastern Indian Ocean are known as the Indian Ocean Dipole or IOD. The IOD is one of the key drivers of Australia's climate and can have a significant impact on agriculture. This is because events generally coincide with the winter crop growing season. The IOD has three phases: neutral, positive and negative. Events usually start around May or June, peak between August and October and then rapidly decay when the monsoon arrives in the southern hemisphere around the end of spring.
Neutral IOD phase
Water from the Pacific flows between the islands of Indonesia, keeping seas to Australia's northwest warm. Air rises above this area and falls over the western half of the Indian Ocean basin, blowing westerly winds along the equator.
Temperatures are close to normal across the tropical Indian Ocean, and hence the neutral IOD results in little change to Australia's climate.
Positive IOD phase
Westerly winds weaken along the equator allowing warm water to shift towards Africa. Changes in the winds also allow cool water to rise up from the deep ocean in the east. This sets up a temperature difference across the tropical Indian Ocean with cooler than normal water in the east and warmer than normal water in the west.
Generally this means there is less moisture than normal in the atmosphere to the northwest of Australia. This changes the path of weather systems coming from Australia's west, often resulting in less rainfall and higher than normal temperatures over parts of Australia during winter and spring.
Negative IOD phase
Westerly winds intensify along the equator, allowing warmer waters to concentrate near Australia. This sets up a temperature difference across the tropical Indian Ocean, with warmer than normal water in the east and cooler than normal water in the west.
A negative IOD typically results in above-average winter–spring rainfall over parts of southern Australia as the warmer waters off northwest Australia provide more available moisture to weather systems crossing the country.
Indian Ocean Dipole years
- 1960
- 1961
- 1963
- 1967
- 1972
- 1975
- 1990
- 1992
- 1994
- 1996
- 1997
- 1998
- 2006
- 2010
- 2015
- 2016
- 2019
- 2022
there have been 9 moderate to strong negative IOD events and 9 moderate to strong positive IOD events.
- See also: Links open in new window
- Indian Ocean Dipole outlook
- Indian Ocean outlook model summary
- Graph of latest IOD Index
The Southern Annular Mode, or SAM, refers to the north-south shift of rain-bearing westerly winds and weather systems in the Southern Ocean compared to the usual position.
Southern Annular Mode (SAM) history
About the Southern Annular Mode (SAM) forecast
At a glance
The Southern Annular Mode can result in enhanced rainfall in regions of southern Australia.
This climate influence is related to: ENSO Frontal Systems
What is it?
The Southern Annular Mode, or SAM, also known as the Antarctic Oscillation (AAO), is a mode of variability which can affect rainfall in southern Australia. The SAM refers to the north/south movement of the strong westerly winds that dominate the middle to higher latitudes of the Southern Hemisphere. The belt of strong westerly winds in the Southern Hemisphere is also associated with the storm systems and cold fronts that move from west to east.
During the summer and autumn months (December through to May) the SAM is showing an increasing tendency to remain in a positive phase, with westerly winds contracted towards the south pole.
The contribution that the SAM makes to the climate variability in Australia and the apparent positive trend in the SAM are relatively recent discoveries and as such are still active areas of research.
SAM summer negative phase
SAM summer positive phase
SAM winter negative phase
SAM winter positive phase
Where, when and for how long does it occur?
The diagram above shows the area affected by the Southern Annular Mode, when it occurs and how long it may last.
In terms of mean sea level pressure, the SAM affects the coastal regions of southern Australia throughout the year. Extreme negative phases of the SAM can cause increased rainfall and cold air outbreaks in southern Australia.
Each SAM event, both positive and negative, tends to last for around ten days to two weeks. The time frame between positive and negative events however is quite random, but is typically in the range of a week to a few months.
How does it affect Australia?
The impact that the SAM has on rainfall varies greatly depending on season and region. If Australia were a few degrees further south, then the impact of changes in SAM would be much more pronounced. The diagram below describes the average impact on rainfall during a "positive" (westerly winds further south) SAM event.
The SAM also has an impact on temperatures. In general, in areas where rainfall is increased, temperature is decreased whilst where rainfall is decreased, temperature is increased.
The diagram above shows the impact that a "positive" SAM event (decreased westerly winds) has on Australian rainfall. Shading indicates daily rainfall anomaly in mm/day for each of the seasons. (Source: Hendon et al. 2007)
An example
During July 2007, the SAM was in a strong negative phase. This was reflected in rainfall patterns across southern Australia.
The Madden–Julian Oscillation (MJO) is the major fluctuation in tropical weather on weekly to monthly timescales. It can be characterised as an eastward moving 'pulse' of cloud and rainfall near the equator that typically recurs every 30 to 60 days.
This tropical information is moving
Tropical outlooks are now available in Tropical monitoring. The Tropics section of the Climate Driver Update will be removed in October.
These charts are updated more frequently than Climate Driver Update editions, so may be more current than the MJO issue text (above).
Forecast MJO location and strength
The chart shows the strength and progression of the MJO through 8 different areas along the equator around the globe.
Area 3 is north west of Australia, 4 and 5 are to the north (the Maritime Continent), and 6 is to the north east.
RMM1 and RMM2 are mathematical methods that combine cloud amount and winds at upper and lower levels of the atmosphere to provide a measure of the strength and location of the MJO. When this index is within the centre circle the MJO is considered weak. Outside of this circle the index is stronger and will usually move in an anti-clockwise direction as the MJO moves from west to east.
Madden–Julian Oscillation (MJO) phase chart
Tropical atmospheric waves
About tropical waves
MJO
The Madden–Julian Oscillation (MJO) is the major fluctuation in tropical weather on weekly to monthly timescales. It can be characterised as an eastward moving pulse or wave of cloud and rainfall near the equator that typically recurs every 30 to 60 days.
Other tropical waves in the atmosphere
In addition to the MJO, other large-scale atmospheric waves also occur in the tropics. The main ones are the convectively-coupled Kelvin wave (KW), equatorial Rossby wave (ER), and mixed Rossby-Gravity wave (MRG). They can provide further insight into the current tropical weather, such as the location and development of tropical cyclones, and what may occur over the coming days to weeks. These waves occur year-round, but typically have a greater influence on tropical weather in the Australian region during the wet-season months of October to April.
Kelvin wave (KW)
Equatorial Kelvin waves are alternating low and high pressure centres along the equator that move from west to east. For consistency with the theoretical structure of Kelvin waves, convection (leading to cloudiness and rainfall) near the equator should be on the western side of the low pressure regions. In contrast, clear conditions should be found on the eastern side of the low pressure. Like other atmospheric tropical waves, alternating zones of cloudiness and clear weather can be seen on satellite imagery in association with an active Kelvin wave. The waves move in the same direction as the Madden–Julian Oscillation, from west to east, but typically 2 to 3 times faster.
Equatorial Rossby (ER) wave
In theory there are several different equatorial Rossby waves. The most commonly seen atmospheric ER wave, and the one we discuss here, has high and low pressure regions centred at latitudes about 10 degrees north and south of the equator. To be consistent with theory, the lows and highs should form a symmetric pattern about the equator. Due to the wind flow around these high and low pressure regions, some regions along the equatorial zone favour cloud and rain formation, while other regions favour stable, clear conditions. On satellite imagery equatorial Rossby waves can often be identified due to the presence of cloud systems at similar longitudes on both sides of the equator. These cloud systems, in conjunction with the off-equatorial low pressure, can be the precursors to tropical cyclones on either side of the equator. While equatorial Rossby waves move at a speed close to that of a typical Madden–Julian Oscillation pulse, they move in the opposite direction—from east to west.
Mixed Rossby-Gravity (MRG) wave
Like equatorial Rossby waves, mixed Rossby-Gravity waves also move towards the west, but MRG waves have their pressure centres arranged anti-symmetrically on either side of the equator. This means a low pressure centre on one side of the equator will be opposite a high pressure centre in the other hemisphere. Satellite analysis of mixed Rossby-Gravity waves shows favoured zones for deep convection, often with thunderstorm clusters, in an antisymmetric arrangement about the equator. Their speed of movement to the west is faster than that of an ER wave.
Images are from The COMET® Program, from Introduction to Tropical Meteorology.
The COMET® Website is at http://meted.ucar.edu/ of the University Corporation for Atmospheric Research (UCAR), sponsored in part through cooperative agreement(s) with the National Oceanic and Atmospheric Administration (NOAA), U.S. Department of Commerce (DOC). © 1997–2021 University Corporation for Atmospheric Research. All Rights Reserved.
MJO location and strength
These graphs show the strength and progression of the MJO through 8 different areas along the equator around the globe.
Area 3 is north west of Australia, 4 and 5 are to the north (the Maritime Continent), and 6 is to the north east.
RMM1 and RMM2 are mathematical methods that combine cloud amount and winds at upper and lower levels of the atmosphere to provide a measure of the strength and location of the MJO. When this index is within the centre circle the MJO is considered weak. Outside of this circle the index is stronger and will usually move in an anti-clockwise direction as the MJO moves from west to east.
Download data: RMM Data
*Note: There are missing satellite observations from 16/3/1978 to 31/12/1978.
Methodology: Until the end of 2013 we use the exact method of Wheeler and Hendon (2004, https://doi.org/10.1175/1520-0493(2004)132%3C1917:AARMMI%3E2.0.CO;2) and from 2014 we use the modified method of Gottschalck et al. (2010, https://doi.org/10.1175/2010BAMS2816.1).
Average weekly rainfall probabilities
These maps show average weekly rainfall probabilities for each of the 8 MJO phases. Green shades indicate higher than normal expected rainfall, while brown shades indicates lower than normal expected rainfall.
Select the 'Wind' checkbox to also show the expected 850 hPa (approximately 1.5 km above sea level) wind anomalies. The direction and length of the arrows indicate the direction and strength of the wind anomaly. The darker the arrow, the more reliable the information is.
The relationship of the MJO with global weather patterns changes with the season.
Read more: The Combined Influence of the Madden–Julian Oscillation and El Niño–Southern Oscillation on Australian Rainfall.
These maps show average minimum or maximum temperature anomalies for each of the 8 MJO phases. Red-yellow colours indicate higher than normal temperature, while blue colours indicate lower than normal temperature.
Select the 'Wind' checkbox to also show the expected 850 hPa (approximately 1.5 km above sea level) wind anomalies. The direction and length of the arrows indicate the direction and strength of the wind anomaly. The darker the arrow, the more reliable the information is.
The relationship of the MJO with global weather patterns changes with the season.
Outgoing longwave radiation (OLR) is often used as a way to identify tall, thick, convective rain clouds. These maps show the difference from expected cloudiness based on the position of the MJO. The violet and blue shading indicates higher than normal, active or enhanced tropical weather, while orange shading indicates lower than normal cloud or suppressed conditions.
Select the 'Wind' checkbox to also show the expected 850 hPa (approximately 1.5 km above sea level) wind anomalies. The direction and length of the arrows indicate the direction and strength of the wind anomaly. The darker the arrow, the more reliable the information is.
The relationship of the MJO with global weather patterns changes with the season
These maps show the atmospheric troughs and ridges (in blue and red, respectively) associated with the different phases of the MJO at the 500hPa level. The 500 hPa level is approximately 5500 m above sea level and is about the middle of the troposphere. Colour shading is only used where the geopotential height anomalies are determined to be statistically-significant at the 5% level.
Select the 'Wind' checkbox to also show the expected 850 hPa (approximately 1.5 km above sea level) wind anomalies. The direction and length of the arrows indicate the direction and strength of the wind anomaly. The darker the arrow, the more reliable the information is.
The relationship of the MJO with global weather patterns changes with the season
Global maps of outgoing longwave radiation (OLR)
Global maps of outgoing longwave radiation (OLR) highlight regions experiencing more or less cloudiness. The top panel is the total OLR in Watts per square metre (W/m²) and the bottom panel is the anomaly (current minus the 1979-1998 climate average), in W/m². In the bottom panel, negative values (blue shading) represent above normal cloudiness while positive values (brown shading) represent below normal cloudiness.
Regional timeseries charts of outgoing longwave radiation (OLR)
The charts linked from this map show the OLRs for the different regions within the Darwin RSMC area. The horizontal dashed line represents what is normal for that time of year (based on the 1979 to 1998 period). The coloured curve is the 3-day moving average OLR in W/m². Below normal OLR indicates cloudier than normal conditions in this particular area, and is shown in blue shading. Above normal OLR indicates less cloudy conditions and is shown in yellow shading.
Time longitude plots
Time longitude plots of daily averaged OLR anomalies (left) and 850 hPa (approximately 1.5 km above sea level) westerly wind anomalies (right) are useful for indicating the movement of the MJO.
How to read the Time longitude plots
The vertical axis represents time with the most distant past on the top and becoming more recent as you move down the chart. The Horizontal axis represents longitude.
Eastward movement of a strong MJO event would be seen as a diagonal line of violet (downward from left to right) in the OLR diagram, and a corresponding diagonal line of purple in the wind diagram. These diagonal lines would most likely fall between 60°E and 150°E and they would be repeated nearly every 1 to 2 months.
Daily averaged OLR anomalies
Westerly wind anomalies
History
In the tropical Pacific Ocean, August sea surface temperatures (SSTs) were:
- up to 1.2 °C warmer than average across much of the western tropical Pacific Ocean, and reaching up to 3 °C warmer than average in the far east
- up to 2 °C cooler than average in patches of the equatorial Pacific, east of 130°W.
In Australian coastal waters, August SSTs were:
- up to 2 °C warmer than average in waters surrounding most of Australia, and up to 3 °C warmer than average to the south-west of the mainland and south-east of Tasmania.
Around the Maritime Continent, August SSTs were:
- up to 2 °C warmer than average to the north of the Maritime Continent, nearer to average for southern parts.
The Bureau's long-range forecast for October to December indicates SSTs are likely to be:
- between 0.8 to 2 °C warmer than average in northern and eastern Australian coastal waters
- up to 1.2 °C warmer than average in southern and western Australian coastal waters
- up to 2 °C warmer than average across parts of the Tasman Sea
- up to 2 °C cooler than average in the central equatorial Pacific, between 160°W and 100°W; and up to 1.2 °C warmer than average for most of the tropical Pacific west of 170°W and south-west Pacific.
Phenomena such as ENSO and the IOD are only broad indicators of the expected climate. The long-range forecast provides better guidance on local rainfall and temperature patterns.
For the week ending 29 September 2024, sea surface temperatures (SSTs) were:
- 0.8–2 °C warmer than the 1991–2020 average in the far western equatorial Pacific
- 0.8–2 °C cooler than average in the central equatorial Pacific
- mostly 0.4–0.8 °C warmer than average in the far eastern Pacific
- warmer than average across much of the north Pacific, with much of the region surrounding and to the east of Japan more than 2–4 °C warmer than average
- 0.8–2 °C warmer than average around much of Australia's coastline and across most of the Maritime Continent, with much of the area between north-west Australia and Indonesia 1.2–2 °C warmer than average.
The Niño indices for the week ending 29 September 2024 are: Niño3, −0.17 °C; Niño3.4, −0.43 °C; and Niño4, +0.13 °C. The Niño3.4 index has cooled in recent weeks, however its values reflect historically neutral ENSO conditions.
- The 30–, 60– and 90-day Southern Oscillation Index (SOI) for the period ending 29 September were +0.4, +3.0 and −0.4 respectively.
- The SOI values reflect ENSO-neutral conditions.
- Sustained positive values of the SOI above +7 typically indicate La Niña while sustained negative values below −7 typically indicate El Niño. Values between +7 and −7 generally indicate neutral conditions.
- Trade wind strength for the 5 days ending 28 September was close to average across the tropical Pacific.
- Monthly averaged trade winds have been stronger than average across the equatorial Pacific since July.
- During La Niña events, there is typically a sustained strengthening of trade winds across much of the tropical Pacific, while during El Niño there is a sustained weakening, or even reversal, of trade winds.
- A weak to moderate pulse of the Madden–Julian Oscillation (MJO) is currently in the Western Hemisphere and Africa (as of 29 September).
- Most models suggest the MJO pulse will move eastwards towards the Indian Ocean and weaken in the coming days. Some models suggest the MJO may re-emerge in mid-October over the Maritime Continent region.
Current state
- The Indian Ocean Dipole (IOD) is neutral. The IOD index for the week ending 29 September was −0.39 °C.
- Sea surface temperatures (SSTs) for the week ending 29 September 2024 were 0.8–2 °C warmer than the 1991–2020 average across much of the central and eastern Indian Ocean but close to average in parts of the western Indian Ocean.
- Some cooler than average waters have expanded near the Horn of Africa in the last fortnight over the western pole of the IOD.
- Closer to Australia, SSTs were up to 2 °C warmer than average for waters surrounding northern WA.
Forecast
- Most climate models indicate the IOD is likely to remain neutral, but weakly negative, for the rest of the year.
- One model indicates a negative IOD during October and November.
- IOD forecast skill has historically been low at this time of year for forecasts beyond two months ahead.
- Cloudiness near the equatorial International Date Line is currently below average as of 28 September.
- Cloudiness has been below average for most of September.
- Prior to September, cloudiness has fluctuated around average levels for most of the year.
- Equatorial cloudiness near the International Date Line typically increases during El Niño (below average OLR) and decreases during La Niña (above average OLR).
The equatorial Pacific sub-surface temperature anomalies for the 30 days ending 25 September 2024 show:
- cooler than average waters in the eastern half of the equatorial Pacific down to about 200 m depth; waters are more than 4 °C cooler than average in a small area around 100 to 150 m depth
- warmer than average waters in the western half of the equatorial Pacific down to about 200 m depth, increasing to 300 m depth in the far west. Waters are 2 to 3 °C warmer than average in a couple of small pockets around 125 m depth.
For the 5 days ending 28 September 2024:
- the equatorial Pacific sub-surface temperature anomalies are within 2 °C of average for all areas, except in the shallow eastern sub-surface, where waters are more than 2 °C warmer than average.
- there are reduced observations in the eastern Pacific sub-surface in the latest 5-day analysis.
The El Niño–Southern Oscillation (ENSO) is neutral, with both sea surface temperatures (SSTs) in the central equatorial Pacific Ocean and atmospheric patterns at ENSO-neutral levels. While some atmospheric indicators such as pressure, cloud and trade wind patterns over the Pacific have been more La Niña-like over the past few weeks, there has yet to be a consistent/sustained signal.
The Bureau's model suggests SSTs are likely to remain within the ENSO-neutral range (−0.8 °C to +0.8 °C) throughout the forecast period to February 2025.
Of the 6 other climate models surveyed, 3 suggest SSTs in the tropical Pacific are likely to exceed the La Niña threshold (below −0.8 °C) from October, and another 3 models forecast SSTs to fall just short of the threshold from November. Should a La Niña develop in the coming months, it is forecast to be relatively weak (in terms of the strength of the SST anomaly) and short-lived, with all models indicating a return to neutral by February.
The Indian Ocean Dipole (IOD) is currently neutral, with the weekly IOD index of −0.39 °C (as of 29 September). Most models indicate that the IOD is likely to remain neutral, but weakly negative, for the rest of the year. An IOD event is unlikely.
Global SSTs remain at near-record levels, with temperatures since July falling just short of the record temperatures observed during 2023, yet well above all other years since observations began in 1854. The sustained nature of this significant global ocean heat suggests that climate patterns such as ENSO and IOD may not necessarily behave or evolve as they have in the past.
The Southern Annular Mode (SAM) is negative (as at 28 September). The SAM index is forecast to return to neutral levels during the coming week. A negative SAM typically decreases rainfall in eastern Australia during spring.
The Madden–Julian Oscillation (MJO) is currently located in the Western Hemisphere (as at 29 September). Most models suggest the MJO will move eastwards towards the Indian Ocean and weaken in the coming days and may reemerge in the Maritime Continent in mid-October.
ENSO, the IOD, the MJO and the SAM are broad indicators of the expected climate, and are just some of many factors in a complex system. The long-range forecast provides better guidance on local rainfall and temperature patterns.
- The Southern Annular Mode (SAM) is negative (as of 28 September) and has been hovering around the negative threshold for the past week and a half.
- The SAM index is forecast to return to neutral levels during the coming week.
- A negative SAM typically decreases rainfall in eastern Australia during spring.
- Predictability of the SAM beyond two weeks is typically low.
- ENSO is currently neutral.
- The Bureau's model suggests SSTs are likely to remain within the ENSO-neutral range (−0.8 °C to +0.8 °C) throughout the forecast period.
- Of the 6 other climate models surveyed, 3 suggest SSTs in the tropical Pacific are likely to exceed the La Niña threshold (below −0.8 °C) from October, while the other 3 models forecast SSTs to fall just short of the threshold.
- Should a La Niña develop in the coming months, it is forecast to be relatively weak (in terms of the magnitude of the SST anomaly) and short-lived, with all models indicating a return to neutral by February 2025.
- ENSO forecast skill is high at this time of year for up to 4 months ahead.
Product code: IDCKGEWW00
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