A monthly summary of the status of El Niño, La Niña, and the Southern Oscillation, or ENSO,
based on the NINO3.4 index (120-170W, 5S-5N)
As of mid-March 2026, the equatorial Pacific is transitioning from declining La Niña conditions toward ENSO-neutral. The latest CCSR/IRI ENSO plume forecast favors ENSO-neutral conditions at approximately 90% for March–May 2026, with a slim 9% chance of El Niño development. ENSO-neutral remains the dominant category during Apr-Jun (53%), but with El Niño probabilities increasing rapidly (47%). Starting in May-July, El Niño probabilities become higher than ENSO-neutral and remain in the range of 72% to 80%, with ENSO-neutral the second most likely outcome.
Figures 1 ((the official CPC ENSO probability forecast) and 3 (the objective model-based IRI ENSO
probability forecast) are often quite similar. However, occasionally they may differ noticeably.
There can be several possible reasons for differences. One is the human forecasters, using their
experience and judgment, may disagree to some degree with the models, which may have known biases.
Another reason is the models are not run at the same time that the forecasters make their assessment,
so that the starting ENSO conditions may be slightly different between the two times. The charts
on this Quick Look page are updated at two different times of the month, typically about a week apart,
with the IRI forecast run later. Also note that the CPC forecast starts on the previous season
while the IRI forecast starts on the current season.
Click on the for more information on each figure.
El Niño and La Niña events tend to develop during the period Apr-Jun and they
Tend to reach their maximum strength during October - February
Typically persist for 9-12 months, though occasionally persisting for up to 2 years
Typically recur every 2 to 7 years
IRI ENSO Forecast
IRI Technical ENSO Update and Model-Based Probabilistic ENSO Forecast
Published: March 19, 2026
Note: The SST anomalies cited below refer to the OISSTv2 SST data set, and not ERSSTv5. OISSTv2 is often used for real-time analysis and model initialization, while ERSSTv5 is used for retrospective official ENSO diagnosis because it is more homogeneous over time, allowing for more accurate comparisons among ENSO events that are years apart. These two products may differ, particularly during ENSO events. The difference between the two datasets may be as much as 0.5 °C. Additionally in some years, the ERSSTv5 may tend to be cooler than OISSTv2 in the context of warming trends, because ERSSTv5 is expressed relative to a base period that is updated every 5 years, while the base period of OISSTv2 is updated every 10 years. In February 2021, both datasets were updated to reflect the 1991-2020 climatology period.
Recent and Current Conditions
The observed SST anomaly in the NINO3.4 region during the Dec–Feb 2026 season was -0.45 °C, and for February 2026, it was -0.20 °C. The most recent weekly average (week centered on March 11, 2026) of the NINO3.4 index was -0.0 °C. These values indicate that Pacific sea-surface temperature anomalies have weakened to ENSO-neutral levels. The CCSR/IRI’s definition of El Niño, requires that the monthly SST anomaly in the NINO3.4 region (5°S-5°N; 170°W-120°W) exceed +0.5 °C. Similarly, for La Niña, the anomaly must be -0.5 °C or colder.
By mid-March 2026, the already weak La Niña had continued to decline in oceanic aspects (e.g., equatorial SSTs approaching neutral levels), while atmospheric features persisted in showing La Niña characteristics. In February 2026, the Southern Oscillation Index (SOI) was +11.0, while the equatorial SOI was +1.2, indicating a strengthening of the pressure gradient between the two regions. The most recent (week centered on March 16, 2026) low-level (850-hPa) winds were near average across the eastern equatorial Pacific, with slightly stronger than normal easterlies in the central-eastern Pacific region. Enhanced convection over Indonesia (below-average OLR) and suppressed near the Date Line (above-average OLR) persisted in a La Niña pattern, albeit weak/muted, reflecting the shift to ENSO-neutral. However, above-average subsurface temperatures have amplified and expanded across the Pacific Ocean, extending to the far eastern Pacific. Warmer subsurface waters now dominate much of the basin, and due to this subsurface warming and its eastward progression, the Niño 1+2 index has gradually increased over the past four weeks to +1.5 (week centered on 11 March 2026), with the Niño 3 index at +0.4. Taken together, these conditions signal the fading of La Niña conditions in the central-eastern equatorial Pacific toward ENSO-neutral, with increased chance of El Niño development.
It is worth noting that the Relative Oceanic Niño Index (RONI), which measures sea surface temperature anomalies in the eastern equatorial Pacific relative to the rest of the equatorial band, has consistently exceeded the −0.5 La Niña threshold for the past several overlapping seasons. For Jul–Sep, Aug–Oct, Sep–Nov, Oct-Dec 2025, Nov-Jan 2026, and Dec-Feb 2026 the RONI was -0.63, -0.77, -0.87, -0.93, -0.97, -0.90 °C respectively.
Expected Conditions
Note – Only models that produce a new ENSO prediction every month are considered in this statement.
The El Niño/Southern Oscillation (ENSO) Diagnostic Discussion, released on 12 March 2026 by the Climate Prediction Center (CPC)/NCEP/NWS, issued both “La Niña Advisory”, and “El Niño Watch” with a transition from La Niña to ENSO-neutral is expected in the next month, with ENSO-neutral favored through May-July 2026 (55% chance). In June-August 2026, El Niño is likely to emerge (62% chance) and persist through at least the end of 2026.
The latest set of ENSO prediction models from mid-March 2026 is now available in the CCSR/ IRI ENSO prediction plume. These are used to assess the probabilities of the three ENSO categories by using the average value of the NINO3.4 SST anomaly predictions from all models in the plume, equally weighted. A standard Gaussian error is imposed over that averaged forecast, with its width determined by an estimate of overall expected model skill for the season of the year and the lead time. Higher skill results in a relatively narrower error distribution, while low skill results in an error distribution with width approaching that of the historical observed distribution.
According to the March 2026 CCSR/IRI ENSO plume forecast, ENSO-neutral conditions are favored for March–May (MAM) 2026 with a 91% probability, while El Niño has only a slim 9% chance during this period. ENSO-neutral conditions are favored to remain dominant through April–June 2026 (around 53% probability), with El Niño chances increasing to about 47%. Going further forward, El Niño is expected to emerge and persist through the end of the forecast period (Nov-Jan 2026/27), with probabilities up to 72–80%. ENSO-neutral probabilities drop into the 20s, while La Niña redevelopment chances stay low (under 5%).
Caution is advised when interpreting these longer-lead ENSO forecasts, as they extend through the boreal spring predictability barrier; accordingly, long-range outlooks should be viewed with appropriate uncertainty, even if they suggest a possible emerging outcome. A plot of the probabilitiessummarizes theforecast evolution. The climatological probabilities for La Niña, ENSO-neutral, and El Niño conditions vary seasonally, and are shown by the lines on the plot, and are given in a table at the bottom of this page for each 3-month season.
Caution is also advised in interpreting the forecast distribution from the Gaussian standard error as the actual probabilities, due to differing biases and performance of the different models. In particular, this approach considers only the mean of the predictions, and not the total range across the models, nor the ensemble range within individual models. At longer leads, the skill of the models degrades, and uncertainty in skill must be convolved with the uncertainties from initial conditions and differing model physics, which leads to more climatological probabilities in the long-lead ENSO Outlook than might be suggested by the suite of models. Furthermore, the expected skill of one model versus another has not been established using uniform validation procedures, which may cause a difference in the true probability distribution.
Season
La Nina
Neutral
El Nino
MAM
0
91
9
AMJ
0
53
47
MJJ
0
28
72
JJA
0
20
80
JAS
1
23
76
ASO
1
21
78
SON
2
20
78
OND
4
23
73
NDJ
5
22
73
ENSO Forecast
IRI ENSO Predictions Plume
Published: March 19, 2026
Note on interpreting model forecasts
The following graph and table show forecasts made by dynamical and statistical models for SST in the Nino 3.4 region
for nine overlapping 3-month periods. Note that the expected skills of the models, based on historical performance, are
not equal to one another. The skills also generally decrease as the lead time increases. Thirdly, forecasts made at some
times of the year generally have higher skill than forecasts made at other times of the year--namely, they are better when
made between June and December than when they are made between February and May. Differences among the forecasts of the
models reflect both differences in model design, and actual uncertainty in the forecast of the possible future SST scenario.
Interactive Chart
You can highlight a specific model by hovering over it either on the chart or the legend. Selecting An item on the legend will toggle
the visibility of the model on the page. You can also select DYN MODELS or STAT MODELS to toggle them all at once. Clicking on the "burger" menu
above the legend will give you options to download the image or expand to full screen. If you have any feedback on this new feature, please
let us know at webmaster@iri.columbia.edu.
Forecast SST Anomalies (deg C) in the Nino 3.4 Region
Seasons (2026 – 2026)
Model
MAM
AMJ
MJJ
JJA
JAS
ASO
SON
OND
NDJ
Dynamical Models
AUS-ACCESS
0.80
1.30
1.77
2.20
AUS-RELATIVE
0.47
1.00
1.40
1.77
BCC DIAP
0.12
0.46
0.75
0.98
1.20
1.34
1.48
1.59
1.74
CMC CANSIP
0.47
0.82
1.09
1.25
1.30
1.33
1.39
1.47
1.51
COLA CCSM4
0.40
0.73
1.07
1.45
1.79
2.03
2.17
2.22
2.21
CS-IRI-MM
0.28
0.53
0.76
1.05
1.31
1.62
IOCAS ICM
-0.15
-0.03
0.17
0.31
0.41
0.48
0.50
0.51
0.52
JMA
0.21
0.43
0.70
1.01
1.33
KMA
0.65
1.01
1.38
1.73
LDEO
0.07
0.29
0.43
0.47
0.49
0.60
0.81
1.01
1.10
MetFRANCE
0.18
0.53
0.96
1.09
1.19
NASA GMAO
0.33
0.66
1.07
1.47
1.90
2.32
2.72
NCEP CFSv2
0.26
0.60
0.88
1.07
1.27
1.46
1.63
SINTEX-F
0.30
0.64
0.98
1.26
1.41
1.47
1.53
1.61
1.64
UKMO
0.45
0.77
1.08
1.40
Average, Dynamical models
0.322
0.650
0.965
1.234
1.236
1.405
1.528
1.401
1.453
Statistical Models
BCC_RZDM
-0.02
0.03
0.05
0.03
-0.01
-0.04
-0.06
-0.08
-0.10
CPC MRKOV
-0.32
-0.20
-0.11
-0.04
0.04
0.14
0.25
0.38
0.52
CSU CLIPR
-0.12
0.01
0.14
0.27
0.32
0.38
0.43
0.46
0.49
IAP-NN
-0.03
0.13
0.28
0.41
0.50
0.55
0.57
0.57
0.57
NTU CODA
-0.04
0.03
0.17
0.42
0.49
0.59
0.62
0.72
0.76
TONGJI-ML
-0.24
-0.00
0.24
0.42
0.51
0.76
0.86
1.08
1.21
UCLA-TCD
0.57
0.89
1.14
1.32
1.44
1.50
1.52
1.50
1.42
UW PSL-CSLIM
0.37
0.68
0.92
1.06
1.15
1.24
1.34
1.41
1.41
UW PSL-LIM
0.24
0.52
0.76
0.94
1.06
1.10
1.08
1.03
0.96
XRO
-0.06
0.08
0.26
0.45
0.61
0.79
1.00
1.22
1.39
Average, Statistical models
0.035
0.217
0.385
0.527
0.612
0.701
0.761
0.829
0.864
Average, All models
0.207
0.477
0.733
0.951
0.939
1.035
1.102
1.044
1.085
Discussion of Current Forecasts
The CCSR/IRI ENSO prediction plume indicates a high likelihood of ENSO-neutral conditions during March–May 2026 (91% probability). The multimodel mean of statistical and dynamical models predict a decline in ENSO-neutral probability during February–April 2026 (53% chance), with a corresponding increase in El Niño probability to 47%.Going forward, El Niño is predicted to dominate with probabilities of 72–80%, while ENSO-neutral probabilities drop into the 20s and La Niña chances remain below 5% throughout the forecast period. Note that long-lead ENSO forecasts are highly uncertain, especially when crossing the spring predictability barrier.Based on the multi-model mean (Dynamical and Statistical models) prediction, and the expected skill of the models by start time and lead time, the probabilities (in %) for La Niña, ENSO-neutral and El Niño conditions (using -0.5 °C and 0.5 °C thresholds) over the coming 9 seasons are:
Season
La Nina
Neutral
El Nino
MAM
0
91
9
AMJ
0
53
47
MJJ
0
28
72
JJA
0
20
80
JAS
1
23
76
ASO
1
21
78
SON
2
20
78
OND
4
23
73
NDJ
5
22
73
Summary of forecasts issued over last 22 months
The following interactive plot shows the model forecasts issued not only from the current month (as in the plot above),
but also from the 21 months previous to this month. The observations are shown up to the most recently completed
3-month period. The plots allow comparison of plumes from the previous start times, or examination of the forecast
behavior of a given model over time.
Hovering over any single model will highlight that particular model in the chart.
Clicking a particular model will hide/show that model in the chart.
At the bottom of the plot, you can select which models to show in the chart:
all the models, the dynamical models only, or the statistical models only.
Notes on the data
Only models producing forecasts on a monthly basis are included. This means that some models whose forecasts appear in the Experimental Long-Lead Forecast Bulletin (produced by COLA) do not appear in the table.
Once an IRI ENSO probability forecast has been published, the results stand even if a model reports an error and changes their data.
When this happens we will update the plume with the model's correct values even though our forecast hasn't changed.
What this means is that our forecast is always the same, but the underlying data may be different from what we based our forecast on.
The SST anomaly forecasts are for the 3-month periods shown, and are for the Nino 3.4 region (120-170W, 5N-5S). Often, the anomalies are provided directly in a graph or a table by the respective forecasting centers for the Nino 3.4 region. In some cases, however, they are given for 1-month periods, for 3-month periods that skip some of the periods in the above table, and/or only for a region (or regions) other than Nino 3.4. In these cases, the following means are used to obtain the needed anomalies for the table:
Temporal averaging
Linear temporal interpolation
Visual averaging of values on a contoured map
The anomalies shown are those with respect to the base period used to define the normals, which vary among the groups producing model forecasts. They have not been adjusted to anomalies with respect to a common base period. Discrepancies among the climatological SST resulting from differing base periods may be as high as a quarter of a degree C in the worst cases. Forecasters are encouraged to use the standard 1991-2020 period as the base period, or a period not very different from it.
ENSO Forecast
Forecast Probability Distribution Based on the IRI ENSO Prediction Plume
Published: March 19, 2026
The plots on this page show predictions of seasonal (3-month average) sea surface temperature (SST)
anomaly in the Niño3.4 region in the east-central tropical Pacific (5°N-5°S, 120°-170°W),
covering the nine overlapping seasons beginning with the current month. The predictions are based on the large (20+)
set of dynamical and statistical models in the plume of model ENSO predictions.
Figure 5
Predictions of ENSO are probabilistic. The ensemble mean prediction is only a best single guess. On either side of that prediction, there is a substantial uncertainty distribution, or error tolerance. The second plot (Figure 2) shows the estimated probability distribution of the predictions, showing a set of percentiles within that distribution for each lead time. The distribution is modeled as a normal (Gaussian) distribution, so that the overall mean forecast represents the center, or 50 percentile, in the distribution. The overall mean is formed using equal weighting among all models. On either side, other percentile values are shown symmetrically, ranging from 1 to 99 and including some intermediate percentiles (5 and 95, 15 and 85, and 25 and 75). The plot enables a user to estimate the probability of the Niño3.4 SST anomaly to be greater or less than some critical value, or within some interval. If, for example, the 85 percentile falls at 1.8° C above average, the probability of the SST exceeding 1.8° C can be estimated at 15%. Probabilities for exceeding or not exceeding values not exactly on percentile line can be roughly interpolated by eye. The overall width of the probability distribution is derived from the historical skill of the hindcasts of the models, from 1982 to present, for the specific forecast start time and lead time. This method of defining the probability distribution represents one of two general approaches, the other approach being a direct counting of ensemble members within each of the percentile bands. This second approach assumes that the ensemble spreads of the models are true representations of the uncertainty. Individual model spreads have often been found to be somwehate narrower than they should be, although in multi-model ensembles this tendency has been shown to be milder or even eliminated.
Figure 6
Figure 6, sometimes called a spaghetti diagram, shows synthetically generated prediction scenarios that are equally likely. Here, 100 scenarios are shown; any number can be generated for such a diagram. Each scenario is produced using a random number generator, combined with knowledge of the mean forecast and its uncertainty, as well as the amount of persistence of anomalies. The degree of persistence of anomalies is based on the correlation of prediction errors from one lead time to another. In other words, the individual lines are designed to show the correct amount of persistence as expected in nature, rather than jumping around more randomly from one lead time to the next. The uncertainty and persistence statistics are based on the set of 7 NMME (North American Multimodel Ensemble) models, as it is assumed that these statistics are approximately applicable to all of the models. Sometimes the “spaghetti density” may appear asymmetric about the mean of all the forecasts or outside of the 85 and 15 percentile lines. This is purely sampling variability, and would not occur if many thousands of such lines were plotted. But with that many lines, most of the plot would be too crowded to get a sense of the behavior of the lines near the center of the distribution. The main purpose of the diagram is to serve users who want to assess realistic individual scenarios of ENSO behavior rather than statistical summaries of the forecast like the percentiles shown in the second plot.
IOD Forecast
Published: March 19, 2026
Note: The Dipole Mode Index is calculated based on the ERSSTv5 data. To account for evolving background conditions and long-term warming, SST anomalies were calculated relative to a sliding monthly climatology. For each month in the time series, the climatology was computed as the mean SST for that calendar month over the prior 30 years. The Dipole Mode Index (DMI) is then defined as the difference in sea surface temperature anomalies between the western equatorial Indian Ocean (50°E–70°E, 10°S–10°N) and the southeastern equatorial Indian Ocean (90°E–110°E, 10°S–0°), and is used to quantify the strength and phase of the Indian Ocean Dipole (IOD).
Current Conditions
In Feb 2026, the observed Dipole Mode Index was +0.25, indicating neutral IOD conditions across the Indian Ocean. According to the CCSR@NASA-GISS/IRI’s criteria for defining positive and negative Indian Ocean Dipole (IOD) events, a positive IOD phase is defined when the DMI exceeds +0.4 °C, and a negative IOD when it falls below −0.4 °C. The IOD is considered inactive (neutral) when the DMI lies between −0.4 °C and +0.4 °C.
Model-Based IOD Outlook: Deterministic Forecasts from the NMME
Forecasts from the latest set of operational models in the North American Multi-Model Ensemble (NMME) project are used to construct deterministic IOD forecasts from each individual model using its ensemble mean DMI to form an IOD forecast plume. The IOD plume plot shows the latest set of predictions from CESM1, CFSv2, CanESM5, GEM-NEMO, and NASA along with their equally weighted multi-model mean (MME). The observed DMI (shown in black) rose steadily from its negative-phase peak in October 2025, gradually weakening through the end of the year and returning to neutral IOD conditions by February 2026. Forecasts for March 2026 from two models, NASA and CFSv2, predict DMI values exceeding the +0.4°C threshold, while other models remain within the neutral range. The MME, overall, favors positive IOD conditions (DMI exceeding +0.4°C) for March 2026. Looking further ahead, most models show a gradual decrease in DMI values, particularly during April, May, and June. However, for July, August, and September, the MME mean points toward the development of positive IOD conditions.
Probabilistic IOD Forecasts from the NMME
Based on March 2026 initialization data, the model-based probabilistic forecast of the Indian Ocean Dipole was generated by CCSR@NASA-GISS/IRI to assess potential phase developments. Probabilities are computed using an ensemble-member counting method, where all ensemble members from the contributing models (92 in this case), are pooled to determine the likelihood of a negative, neutral, or positive IOD phase for the upcoming months. Climatological probabilities for each IOD phase, based on historical data, are shown as dotted lines for reference. In March 2026, the odds favor positive IOD (62%), while IOD-neutral is estimated at 38%. For April, May, and June, IOD-neutral is the dominant category, although the odds of positive IOD gradually increase. By July 2026, the chances for IOD-neutral and positive IOD become nearly equal. In the final two months of the forecast period, August and September, the odds shift strongly in favor of positive IOD, consistent with CCSR/IRI’s ENSO forecasts, with the probability remaining above 60%.
In summary, March 2026 favors positive IOD, with neutral conditions dominating during the first half of the forecast period. Positive IOD conditions gradually increase in the second half, particularly from July to September.
All data from this website is covered under the
Creative Commons Attribution 4.0 License.
When citing IRI ENSO images or data, please use "Images [or Data] provided by The International Research Institute for Climate and Society, Columbia University Climate School",
with a link to https://iri.columbia.edu/ENSO.
The official CPC ENSO probability forecast, based on a consensus of CPC and IRI forecasters.
It is updated during the first half of the month, in association with the
Official CPC ENSO Diagnostic Discussion.
It is based on observational and predictive information from early in the month and from the previous month.
It uses human judgment in addition to model output, while the forecast shown in Fig. 3 relies solely on model output.
Figure 1 is updated on this page on the second Thursday of every month.
NOAA/CPC ENSO Forecast Graphic, courtesy of NOAA/CPC
A purely objective ENSO probability forecast, based on regression, using as input the model predictions from the plume of dynamical and
statistical forecasts shown in Fig. 4. Each of the forecasts is weighted equally. It is updated near or just after the middle of the month, using
forecasts from the plume models that are run in the first half of the month. It does not use any human interpretation or judgment.
Figure 3 is updated on the third Thursday of every month.
Plume of forecasts of the Nino3.4 SST anomaly from dynamical and statistical models that are run during the first half of the month. A probability
forecast is generated using all the models in Fig. 4, and is shown in Fig. 3. The average of the forecasts of the dynamical models is shown by the
thick yellow line, and of the statistical models by the thick green line. The average of the four models run at the NOAA Climate Prediction center (CPC)
is shown by the thick pink line. This figure is updated on the third Thursday of every month. Because forecasts from some models of Fig. 4
are not yet available when the official CPC ENSO probability forecast (Fig. 1) is made, the official forecast uses the previous month's Fig. 4
as one of its inputs, which is shown in the CPC ENSO Diagnostic Discussion.