Climate Driver Update
Climate drivers in the Pacific, Indian and Southern oceans and the Tropics


Average of international model forecasts for NINO3.4

Average of international model forecasts for IOD


Sea surface temperature maps

Sea surface temperature maps are not available for forecasts before Spring 2018

Global sea surface temperature forecasts for the months and season ahead. Anomalies indicate the difference from normal.

Sea surface temperature maps (select map for larger view)

SST forecasts 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.

NINO3.4 SST plumes from Bureau model forecasts, updated daily
Select to see full-size map of NINIO3.4 SST plumes from Bureau model forecasts, updated daily.

International climate model forecasts

Nino 3.4 2 month forecast
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.

Weekly sea surface temperatures

Graphs of the table values

Monthly sea surface temperatures

Graphs of the table values

5-day sub-surface temperatures

Monthly temperatures

Southern Oscillation Index

30-day SOI values for the past two years
Select to see full-size map of 30-day Southern Oscillation Index values for the past two years, updated daily.

Trade winds

5-day SST and wind anomaly from TAO/TRITON
Select to see full-size map of 5-day SST and wind anomaly from TAO/TRITON.

Cloudiness near the Date Line

About El Niño and La Niña (ENSO)

El Niño Southern Oscillation

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.

Map diagram of Neutral ENSO

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.

Map diagram of Negative ENSO

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.

Map diagram of Positive ENSO

The Southern Oscillation Index, or SOI, gives an indication of the development and intensity of El Niño or La Niña events 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.

 

graph of SOI

This graph shows the values of the SOI between 1991 and mid-2015. Monthly SOI data.

 

How does it affect Australia?

Each phase of the ENSO has a very different effect on the Australian climate. Events 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.

  • The Climate Driver Update provides the latest information on the state of ENSO and the likely effect this will have on Australia.

Timeline of monthly Southern Oscillation Index (SOI) values since 1876

Timeline graph of ENSO and SOI index

Sustained negative values (bottom/yellow) of the SOI below −7 may indicate El Niño, while sustained positive values 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.

IOD SST plumes from Bureau model forecasts, updated daily
Select to see full-size map of IOD SST plumes from Bureau model forecasts, updated daily.

International climate model forecasts

Latest IOD forecast
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.

  1. 1960
  2. 1961
  3. 1963
  4. 1964
  5. 1972
  6. 1974
  7. 1981
  8. 1982
  9. 1983
  10. 1989
  11. 1992
  12. 1994
  13. 1996
  14. 1997
  15. 1998
  16. 2006
  17. 2010
  18. 2012
  19. 2014
  20. 2015
  21. 2016
  22. 2019
  23. 2022
Since 1960, when reliable records of the IOD began, to 2016 there have been 12 negative IOD and 11 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.

Map diagram of Neutral IOD

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.

Map diagram of Positive IOD

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.

Map diagram of Negative IOD


Indian Ocean Dipole years

  1. 1960
  2. 1961
  3. 1963
  4. 1964
  5. 1972
  6. 1974
  7. 1981
  8. 1982
  9. 1983
  10. 1989
  11. 1992
  12. 1994
  13. 1996
  14. 1997
  15. 1998
  16. 2006
  17. 2010
  18. 2012
  19. 2014
  20. 2015
  21. 2016
  22. 2019
  23. 2022
Since 1960, when reliable records of the IOD began, to 2016 there have been 12 negative IOD and 11 positive IOD events.

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

Southern Annular Mode

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

Map diagram of Neutral sam

SAM summer positive phase

Map diagram SAM summer positive phase

SAM winter negative phase

Map diagram of SAM winter negative phase

SAM winter positive phase

Map diagram of SAM winter positive phase

Where, when and for how long does it occur?

 

Where, when and for how long does the Southern Annular Mode 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.

 

diagram showing the impact of the SAM

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

rainfall deciles thumbnail image

During July 2007, the SAM was in a strong negative phase. This was reflected in rainfall patterns across southern Australia.

Read more.

Further information and latest updates

 

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.

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.

MJO phase diagram
MJO phase diagram

*Note: There are missing satellite observations from 16/3/1978 to 31/12/1978.

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

About the Madden–Julian Oscillation (MJO) forecast

Madden-Julian Oscillation

At a glance

The Madden-Julian Oscillation is associated with weekly to monthly periods of enhanced and suppressed rainfall over parts of Australia.

This climate influence is related to:   The Australian Monsoon   Tropical Cyclones   Tropical Depressions

What is it?

The Madden-Julian Oscillation (MJO) is a global-scale feature of the tropical atmosphere.

The MJO is the major fluctuation in tropical weather on weekly to monthly timescales. The MJO can be characterized as an eastward moving "pulse" of cloud and rainfall near the equator that typically recurs every 30 to 60 days. However, the signal of the MJO in the tropical atmosphere is not always present.

MJO effects are most evident over the Indian Ocean and western equatorial Pacific. It influences the timing, development and strength of the major global monsoon patterns, including the Indian and Australian monsoons.

Tropical cyclones are also more likely to develop in association with certain phases of a strong MJO event.

The MJO is associated with variations in wind, cloudiness, and rainfall. Most tropical rainfall comes from tall thunderstorms which have very cold tops. Thunderstorms that have cold tops emit only low levels of longwave radiation. Therefore, the MJO can be monitored by using satellite measurements of outgoing longwave radiation (OLR) to identify areas of cloudiness (low OLR) within the tropics.

Where, when and for how long does it occur?

 

where, when and for how long does it occur?

The diagram above shows the area most affected by the Madden-Julian Oscillation (MJO), the seasons during which the MJO's influence on Australia is greatest, and for how long each active phase of the MJO typically lasts.

 

How does it affect Australia?

The MJO has its greatest effect on the tropical areas of Australia during summer. It may have some effect on parts of southern Australia, however this impact appears small when compared to the effect on northern regions, and remains the subject of research.

The MJO can have an effect on the timing and intensity of "active" monsoon periods in northern Australia. This can lead to enhanced rainfall - in both the intensity of the rainfall and the duration of the rainfall.

An example

monthly rainfall deciles thumbnail image

During late January 2006, an active phase of the MJO coincided with an active monsoon period, resulting in enhanced rainfall over northern Australia.

Read more.

Further information and latest updates

The following links provide further information on the MJO.

  • The Tropical Climate Update provides information on the current phase of the MJO.
  • Technical information and maps relating to the Real-time Multivariate MJO Index, which is a way of monitoring the climate and weather variations caused by the MJO. Please note that this product is a research product, and as such is not always updated and may be under-going continual changes as it is developed.

 

SSTs for April 2023 were warmer than average over the eastern, southern and far west of the tropical Pacific Ocean. Warm anomalies up to 2 °C warmer than average were present over these regions, increasing to more than 4 °C warmer than average off parts of the South American coast.

Compared to March, large parts of the basin have warmed, especially in the east and south-west of the tropical Pacific.

Warm SST anomalies also continued in the southern Tasman Sea, between south-east Australia and New Zealand, as well as to the south-west of Western Australia. Warm anomalies off the west coast of Western Australia have eased to near-average values.

Globally, the April 2023 SSTs were the warmest on record. In the ERSSTv5 dataset, the global area-average SST was 0.71 °C above the 1961-1990 average, exceeding the previous April record of 0.67 °C in 2019.

For the week ending 21 May 2023, sea surface temperatures (SST) were warmer than average over the eastern equatorial Pacific Ocean, from around 140°W to the South American coastline. Compared to two weeks ago, these warm anomalies have remained similar in strength but increased marginally in spatial extent, reaching further westwards. Warm anomalies also exist across much of the Pacific south of 10°S.

Anomalously warm sea surface temperatures continue to persist in the western tropical Pacific Ocean increasing in spatial coverage in the last two weeks, meaning there is little temperature gradient along most of the equator barring near the South American coastline, and hence contributing to the limited opportunity for an atmospheric response to the eastern Pacific warming.

A band of warm anomalies also stretches from the northern Maritime Continent, into the Coral Sea and to the north-east of New Zealand.

Warm SST anomalies persist in the southern Tasman Sea, from south-east Australia to around New Zealand, and near south-west Western Australia.

A cold SST anomaly off the NSW coast has increased in strength and spatial coverage over the last two weeks.

The latest values of the three NINO indices for the week ending 21 May 2023 were: NINO3 +1.0 °C, NINO3.4 +0.6 °C, and NINO4 +0.4 °C.

The 30-day Southern Oscillation Index (SOI) for the 30 days ending 21 May 2023 was −9.3, while the 90-day SOI value was -2.9. The 30-day SOI has maintained a negative value over the past fortnight, and both the 30-day and the 90-day SOI continue to demonstrate a gradual decreasing trend.

Sustained positive values of the SOI above +7 typically indicate La Niña, while sustained negative values below −7 typically indicate El Niño.

Trade winds for the 5 days ending 21 May 2023 were close to average over most of the tropical Pacific.

During La Niña there is 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 moderately strong Madden-Julian Oscillation (MJO) pulse is moving over the Western Pacific region and is forecast to move into the central Pacific region in the coming week. There is some variation amongst climate models, with some indicating marginal strengthening and continued eastwards progression across the tropical Pacific until the start of June, while others suggest the MJO pulse will rapidly weaken and become indiscernible. However, an MJO pulse over the western Pacific would likely weaken trade winds across the equatorial Pacific Ocean. This, in turn, would result in further warming of the equatorial Pacific Ocean and hence drive further development towards El Niño.

The Indian Ocean Dipole (IOD) is currently neutral. The IOD index value for the week ending 21 May 2023 was −0.15 °C, which is within neutral bounds (between −0.40 °C and +0.40 °C).

Weekly sea surface temperatures (SSTs) are above average across most of the tropical Indian Ocean, reaching up to 2 °C above average near the western Maritime Continent and in the far east. Warm anomalies also exist over much of the southern half of the basin, and off the southwest of Australia.

Small areas of cool anomalies exist in the central Indian Ocean and off the Pilbara and south-west coasts of Western Australia.

All international climate models surveyed by the Bureau suggest a positive IOD event may develop in the coming months. A positive IOD can supress winter and spring rainfall over much of central and southeast Australia, and if combined with El Niño, the drying effect is typically stronger and more widespread across Australia. However, model accuracy has historically been low at this time of year, and therefore outlooks for beyond June should be viewed with caution.

Cloudiness near the Date Line has recently been around average since late April 2023.

Equatorial cloudiness near the Date Line typically decreases during La Niña (positive OLR anomalies) and increases during El Niño (negative OLR anomalies).

The four-month sequence of equatorial Pacific sub-surface temperature anomalies (to 23 May 2023) shows warm anomalies across the basin, between 50 m and 250 m in the western Pacific, between 75 m and 175 m depth in the central Pacific and above 125 m depth in the eastern Pacific. Near the South American coastline, the depth of the anomaly increases again to about 200 m. Anomalies reached more than 2 °C warmer than average across much of this region.

Compared to previous months, cool anomalies have steadily decreased in extent, and are now absent. During April, warm anomalies expanded in extent to cover the whole basin, strengthening in the eastern Pacific during May.

For the five days ending 21 May 2023, sub-surface temperatures were warmer than average across the equatorial Pacific between about 50 m depth and 200 m depth in the western and central Pacific, and between the surface and 100 m depth in the eastern Pacific. Anomalies were more than 1 °C warmer than average across the basin, increasing to more than 3 °C in the west and 5 °C in the far east.

Compared to two weeks ago, warm anomalies have increased in strength over the far-east of the basin and also marginally in the west, whilst cooling slightly in the central Pacific.

The Pacific Ocean is currently ENSO-neutral (neither La Niña nor El Niño). Sea surface temperatures are warmer than average in the west and the east of the tropical Pacific. While all international climate models indicate it is very likely that tropical Pacific Ocean temperatures will reach El Niño thresholds during the southern hemisphere winter, an atmospheric response is also required for an El Niño to be declared. Thus far, little shift has been observed in atmospheric ENSO indicators with trade winds and cloudiness patterns in the Pacific remaining indicative of ENSO-neutral conditions. The 30-day SOI has dropped below the El Niño threshold, but sustained values are required for it to be considered a part of an El Niño response.

The ENSO Outlook remains at El Niño WATCH. This indicates there is an increased risk of an El Niño occurring this year, at least double the usual chance. History shows that when the ENSO Outlook has reached El Niño WATCH, El Niño has subsequently developed in about half of those years. El Niño typically suppresses rainfall in eastern Australia during the winter and spring months. The status of the ENSO Outlook does not change the Bureau's long-range forecast for drier and warmer conditions across much of Australia for winter. The Bureau's climate model takes into account all influences from the oceans and atmosphere when generating its long-range forecast.

The Indian Ocean Dipole (IOD) is currently neutral. All five models suggest that a positive IOD event could develop in winter. A positive IOD typically supresses winter and spring rainfall over much of Australia, and if it occurs with El Niño, it can exacerbate El Niño's drying effect.

A moderately strong Madden-Julian Oscillation (MJO) pulse is moving over the Western Pacific region and is forecast to move into the central Pacific region in the coming days. There is some variation amongst climate models, with some indicating marginal strengthening and continued eastwards progression across the tropical Pacific until the start of June, while others suggest the MJO pulse will rapidly weaken and become indiscernible. However, if the MJO pulse maintains its strength and continues to track over the western or central Pacific, it would likely weaken trade winds across the equatorial Pacific Ocean. This, in turn, would result in further warming of the equatorial Pacific Ocean and hence drive further development towards El Niño.

The Southern Annular Mode (SAM) index is currently positive and is expected to return to neutral towards the end of May. During autumn SAM typically has a weaker influence on Australian rainfall, but as we approach winter, positive SAM often has a drying influence for parts of south-west and south-east Australia.

Climate change continues to influence Australian and global climates. In April 2023, the global sea surface temperature (SST) was the highest on record for that month, while for the Coral Sea SSTs were the 2nd-highest on record. The Australian continent has warmed by around 1.47 °C over the period 1910–2021. There has also been a trend towards a greater proportion of rainfall from high intensity short duration rainfall events, especially across northern Australia. Southern Australia has seen a reduction of 10 to 20% in cool season (April–October) rainfall in recent decades.

The Southern Annular Mode (SAM) index is currently positive and is expected to return to neutral around the end of May.

During autumn SAM typically has a weaker influence on Australian rainfall, but as we approach winter, positive SAM often has a drying influence for parts of south-west and south-east Australia.

The El Niño–Southern Oscillation (ENSO) is currently neutral (neither La Niña nor El Niño).

The Bureau's ENSO Outlook is at El Niño WATCH. An El Niño WATCH is not a guarantee that El Niño will occur, rather it is an indication that some of the typical precursors of an event are currently in place. An El Niño WATCH indicates there is an increased risk of an El Niño occurring this year, at least double the usual chance.

Oceanic warming is continuing in the central and eastern tropical Pacific. However, the western Pacific also remains warmer than average. There are indications of some changes in the atmosphere but this needs to be sustained over several weeks or months.

While models are forecasting a very high likelihood that ocean temperatures in the central and eastern Pacific will reach El Niño thresholds in early spring, an accompanying shift in atmospheric circulation is necessary for an El Niño event to be declared. Due to the persistence of neutral atmospheric indicators over the tropical Pacific, our ENSO outlook remains at El Niño WATCH.

International climate models suggest further warming of the central and eastern tropical Pacific Ocean is likely. By July, all surveyed models indicate El Niño thresholds for sea surface temperatures will be met or exceeded. El Niño typically suppresses rainfall in eastern Australia during the winter and spring months.

Product code: IDCKGEWW00

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