The variation in the vegetation pattern reflects the change in the regional environment. Normalized Difference Vegetation Index (NDVI) data from 2000 to 2022 for the Upper Bhima sub-basin in Western India has been used to identify the response of vegetation to the El Niño-Southern Oscillations (ENSO) and Indian Ocean Dipole (IOD) events. As a novelty, the present study identifies the ENSO-sensitive and IOD-sensitive vegetation areas within the watershed using vegetation mean to difference anomalies. Monthly NDVI anomalies are used to determine sensitive pixels of vegetation using mean monthly NDVI. Local spatial autocorrelation (LISA) is performed to analyze the pattern of the NDVI anomalies and cluster maps are generated. The results of spatial variation show that NDVI is adversely affected in El Niño years. During La Niña years, the percentage area covered by dense vegetation is more than 80%, which is significantly higher than that of El Niño years in the monsoon and post-monsoon periods. Positive IOD years show significantly more sparse vegetation cover than negative IOD years. The results of LISA analysis show that the rainfall shadow zone in the study area has a cluster of negative sensitive pixels even in the monsoon and post-monsoon period except in negative IOD year.

  • Vegetation is adversely affected by El Niño and not affected during La Niña.

  • The novelty is to identify the ENSO-sensitive and IOD-sensitive vegetation areas.

  • A positive IOD has an adverse effect on vegetation compared to a negative IOD event.

  • Rainfall shadow zone has negative sensitive pixels cluster even in monsoon and post-monsoon period.

Vegetation cover over the Earth's surface changes rapidly due to several parameters including climatic factors like changes in precipitation and temperature. Various patterns of vegetation on the Earth's surface and the annual dynamics of the photosynthetic activity of vegetation cause variations in the phenology (Myneni et al. 1997; Claussen et al. 2003). Overall, it may not be possible for the vegetation to be uniformly distributed throughout as it is constrained by the availability of water and nutrients. Apart from many factors which cause variations in vegetation like Land Use Land Cover (LULC), topography, etc., climatic factors including water and moisture transport in the environment contribute to the variation of vegetation (Piao et al. 2019). The distinct climatic patterns like dry and wet climates in the semi-arid region are mainly due to the differences in large-scale ocean – atmospheric circulation and different climate feedbacks (Liang et al. 2022). Ummenhofer et al. (2011) have investigated the impacts of El Niño-Southern Oscillation (ENSO) and the Indian Ocean Dipole (IOD) on Australian rainfall and soil moisture at different time scales. The study finds that there are significant differences between the dominant drivers of drought at interannual and decadal time scales. On interannual time scales, both ENSO and IOD alter the Southeastern Australian soil moisture, with the driest conditions over the southeast and more broadly over large parts of Australia occurring during an El Niño and positive IOD event. The study performed by Liguori et al. (2022) also shows that the positive phases of ENSO and IOD often co-occur making it difficult to attribute observed rainfall anomalies in Australia to either of them individually. The study also concludes that understanding the independent contributions of ENSO and IOD to rainfall variability is important for improving seasonal rainfall forecasts.

This indicates that climatic patterns like ENSO and IOD have distinct impacts on rainfall and soil moisture which in turn controls vegetation. Vegetation studies conducted using satellite data generated by NDVI have been helpful for land management, planning, long-term sustainability and assessing the natural resources and agricultural production (Nemani et al. 2003). Normalized difference vegetation index (NDVI) data have been used to study the interconnections between climate and landscape ecosystems, to monitor the effects of natural as well as anthropogenic disasters such as floods, drought, fire and desertification (Myneni et al. 1997; Seelan et al. 2003).

The most critical environmental and climate issues facing the world today are climate extremes (Stocker 2014), such as droughts and floods (nowadays flash floods), which ultimately change the composition, cover, structure and functions of surface vegetation. The impacts of climate extremes events such as ENSO and IOD may also be appropriately investigated by studying the vegetation dynamics. El Niño (warm phase) and La Niña (cold phase) are the two phases of the ENSO, while positive IOD and negative IOD are the two phases of the IOD. Regardless of the significant correlation between ENSO and the IOD (Allan et al. 2001), it is still uncertain if the IOD is independent of ENSO (Feng & Meyers 2003; Cai et al. 2012). Future studies on these aspects will help understand the certainties and uncertainties between the ENSO and IOD events of climate change.

Numerous research studies have examined the monsoon rainfall variability and its connection to ENSO and IOD (Ghosh et al. 2009; Propastin et al. 2010; Bothale & Katpatal 2016; Rishma & Katpatal 2016; Shukla & Huang 2016; Hrudya et al. 2021). It is essential to research how ENSO and IOD affect vegetation because ENSO and IOD have an impact on the variability of monsoon precipitation, which is a significant driver of vegetation variation (Krishnaswamy et al. 2015). In addition, the global and regional hydrological balance affects vegetation due to the spatial and temporal variation in precipitation.

Few studies have studied the impact of IOD and ENSO on the country-level geographical area over Madagascar (Ingram & Dawson 2005) and South Africa (Anyamba et al. 2018). According to Ingram and Dawson's study of Madagascar, the moderate but significant correlation observed here does indicate that El Niño has a considerable impact on the greenness level of vegetation on the island. The analysis of the strongest El Niño event followed by a weak La Niña event was conducted by Anyamba et al. in 2018. Time series correlation analysis was carried out between Niño 3.4, the Dipole Mode Index (DMI), precipitation and NDVI. The study concluded that the ENSO and IOD contributed to the effect on NDVI and agricultural production.

However, very few studies have been carried out on the subsequent impact of ENSO on vegetation variation. The present study aims to evaluate how sensitive the vegetation is to ENSO and IOD events at watershed/regional levels rather than at the country level/global levels. First of all, the ENSO (El Niño and La Niña) and IOD (positive and negative IOD) events are identified based on Oceanic Niño Index (ONI) and DMI, respectively. Then the MODIS NDVI data were processed for the period of selected ENSO and IOD years. Finally, the spatial variation of the NDVI has been analyzed using the inverse distance weightage (IDW) interpolation using geospatial techniques. According to the spatial variation analysis results, El Niño events have a more negative effect on the vegetation than La Niña events when ENSO events are taken into account.

The NDVI anomalies are calculated for monthly NDVI data and are processed using Geographic Information System (GIS) tools to generate NDVI anomaly maps. Based on the extreme anomaly values, sensitive vegetation pixels are identified. There are 71 micro watersheds in the sub-basin. The global spatial autocorrelation and LISA has been performed to analyze the anomalies in the watershed. In local spatial autocorrelation (LISA) analysis, cluster maps and significant maps are generated in the Geo-Da tool to identify the most affected micro-watersheds within the sub-basin. The novelty of this study is it introduces the ENSO and IOD-sensitive vegetation areas within the watershed using vegetation means to difference anomalies. The study utilizes LISA to identify clusters of anomalous pixels showing areas sensitive to ENSO and IOD events. To identify the seasonal effects on NDVI, ENSO-sensitive and IOD-sensitive vegetation areas within the watershed have been identified for January February March (JFM), April May June (AMJ), July August September (JAS) and October November December (OND) months. The results of this study are important as the study area consists of a rainfall shadow zone which is a drought-prone area in western India with diversified hydrological characteristics.

The paper is organized as follows: an overview of the data used in this study is presented in Section 2; the method used to identify the spatial variation, sensitive pixels and spatial autocorrelation is described in Section 3; the results and discussion are presented in Section 4, and conclusions are summarized in Section 5.

Materials and data used

Brief information about the study area used for the research and an overview of the data used in this study are presented in this section. The Upper Bhima Sub-basin lies in the semi-arid ecosystem of Western India. This sub-basin is an example of a unique combination of diverse agro-climatic zones. Sahyadri Mountain Range divides the study area into the Western Ghat zone, which receives the highest rainfall, and the Water Scarcity zone, which is a shadow zone of precipitation and receives the lowest rainfall in the sub-basin. This section also provides information about the MODIS NDVI data and the information on ENSO and IOD events used for the analysis.

Study area

The Bhima River is a major tributary of the Krishna River. The whole Krishna basin splits into seven sub-basins which represent different tributary systems. Of the total area of the Krishna basin, 17.58% (46,066 km2) is covered by the Upper Bhima sub-basin. The study area lies between latitude 17°10′ 48″ N to 19°14′ 24″ N and longitude 73°12′ E to 76°9′ E (Londhe & Katpatal 2020). The location map of the study area is shown in Figure 1.
Figure 1

Location map of the study area.

Figure 1

Location map of the study area.

Close modal

The hydrological characteristics of the Upper Bhima River Sub-basin are highly diverse, caused by the interaction between the monsoon and the Western Ghat mountain range. The Western Ghat zone is covered with thick forest and receives heavy rainfall, reaching a maximum of 4,500 mm/year. Rainfall decreases rapidly towards the eastern slopes and plateau areas, where it is less than 500 mm/year. It again increases towards the east; hence, the central part of the Upper Bhima receives the lowest rainfall (Garg et al. 2012).

NDVI data

The mathematical expression for NDVI is given in Equation (1). NDVI is the index which is a good indicator of growth stages and vegetation parameters, such as leaf area, green biomass yield, vegetation coverage rate and photosynthetically active vegetation, and so on (Piao et al. 2003; Stow et al. 2003; Morgan et al. 2020).

NDVI quantifies the vegetation by using the reflection in the near-infrared region which vegetation strongly reflects and the red region which vegetation absorbs. NDVI is an index of the vegetation greenness, i.e., the density and health of vegetation of each pixel in a satellite image. NDVI is often used worldwide to monitor drought, monitor and predict agricultural production, assist in predicting hazardous fire zones and map desert encroachment (Arjasakusuma et al. 2018).

Hence, NDVI is an index which reflects the density of green vegetation which covers low-dense to highly dense vegetation. NDVI data from different sources like MODIS NDVI, NOAA AVHRR NDVI and LANDSAT derived NDVI, and other sources from remote sensing have been widely used in vegetation studies at regional and global scales (Hou et al. 2019; Kim et al. 2021; Zhou et al. 2021). In this study, MODIS NDVI data product MOD13C2 has been used for the analysis. The data files for each month were obtained from NASA's Earthdata website (https://giovanni.gsfc.nasa.gov) from February 2000 to January 2022. MOD13C2 data are cloud-free composites of the 16-day MOD13C1 product, and MOD13C1 data product is a higher quality climate data product useful for climate modeling and time series analyses of Earth surface processes (Didan et al. 2015). MOD13C2 data product has a spatial resolution of 0.05° (5,600 m). These data were corrected for cloud-free global coverage and are processed by replacing the historical time series MODIS climatology record as the input data from the 16-day MOD13C1 product. The mathematical expression of NDVI as (1)
(1)
where, NIR is reflected value of near-infrared band;

R is reflected value of red band.

ENSO – El Niño and La Niña Phases

ENSO (El Niño-Southern Oscillation) is the oscillations between wind and sea surface temperature (SST) that occurs in the equatorial eastern Pacific, which is represented by the transition of El Niño and La Niña in the ocean and the Southern Oscillation in the atmosphere (McPhaden et al. 2006). The ENSO significantly impacts global climatic parameters and the hydrological cycle.

The intensity of ENSO events is generally defined as the strength of the SST anomaly or ONI (Huang et al. 2016; van Oldenborgh et al. 2021). In this study, ENSO events (El Niño and La Niña events) are decided by using ONI. An ENSO warm event, i.e., El Niño, will occur when the ONI is greater than 0.5 for five consecutive months, and an ENSO cold event, i.e., La Niña event, will occur when the ONI is less than −0.5 at least for five consecutive months. Figure 2 shows the time series of ONI for January 2000 to January 2022. Four El Niño years and four La Niña years are defined based on this criterion, and the NDVI analysis has been done in accordance with those years. The ENSO years and the details of the maximum ONI value for El Niño events and the minimum ONI value for La Niña events with their duration of the event in months are given in Table 1.
Table 1

ENSO events explaining El Niño and La Niña Events from 2000 to 2021

PeriodPhase (El Niño/La Niña)Maximum/minimum index
07-2002 to 05-2003 El Niño 1.3 
07-2004 to 05-2005 El Niño 0.7 
07-2009 to 05-2010 El Niño 1.6 
07-2015 to 05-2016 El Niño 2.6 
07-2007 to 05-2008 La Niña −1.6 
07-2010 to 05-2011 La Niña −1.7 
07-2011 to 05-2012 La Niña −1.1 
07-2020 to 05-2021 La Niña −1.3 
PeriodPhase (El Niño/La Niña)Maximum/minimum index
07-2002 to 05-2003 El Niño 1.3 
07-2004 to 05-2005 El Niño 0.7 
07-2009 to 05-2010 El Niño 1.6 
07-2015 to 05-2016 El Niño 2.6 
07-2007 to 05-2008 La Niña −1.6 
07-2010 to 05-2011 La Niña −1.7 
07-2011 to 05-2012 La Niña −1.1 
07-2020 to 05-2021 La Niña −1.3 
Figure 2

Plot showing the time series of Oceanic Niño Index (ONI) over the current study period (January 2000–January 2022). The red (green) horizontal line represents the threshold for El Niño (La Niña) event. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 2

Plot showing the time series of Oceanic Niño Index (ONI) over the current study period (January 2000–January 2022). The red (green) horizontal line represents the threshold for El Niño (La Niña) event. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Close modal

IOD – positive and negative IOD phases

The IOD is defined by the difference in SST between two areas or poles; a western pole in the Arabian Sea (Western Indian Ocean) and an eastern pole in the eastern Indian Ocean south of Indonesia; hence it is called as a dipole. The IOD affects the climate of Australia and other surrounding countries of the Indian Ocean and is a significant contributor to rainfall variability in this region (Cai et al. 2011; Min et al. 2013). As IOD affects the Indian Ocean surrounding countries and rainfall variability in those countries, it is essential to study its impact on the change in NDVI pattern.

In this study, positive and negative IOD years are decided using DMI. The Australian Government Bureau of Meteorology lists positive/negative IOD events when the DMI index exceeds ± 0.4 (Verdon-Kidd et al. 2017). Several IOD reconstructions specify different number of IOD events but currently, there are no analyses explaining IOD variability that are based exclusively on SST anomalies in the Indian Ocean Dipole East Pole (IODE) region (Cahyarini et al. 2021). Figure 3 shows the time series of DMI for January 2000 to June 2021.
Figure 3

Plot showing the variation of Dipole Mode Index (DMI) over the current study period (January 2000–September 2021). The red (green) horizontal line represents the threshold for positive (negative) IOD phase. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 3

Plot showing the variation of Dipole Mode Index (DMI) over the current study period (January 2000–September 2021). The red (green) horizontal line represents the threshold for positive (negative) IOD phase. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Close modal

The Bureau of Meteorology, Australia has decided on three positive IOD years and three negative IOD years during the study period. NDVI analysis has been done in accordance with those IOD years. The list of IOD years considered for the analysis is given in Table 2.

Table 2

IOD years considered for the analysis from 2000 to 2021 (Bureau of Meteorology, Australia)

IOD phaseYears
Positive IOD years 2006, 2012, 2015 
Negative IOD years 2010, 2014, 2016 
IOD phaseYears
Positive IOD years 2006, 2012, 2015 
Negative IOD years 2010, 2014, 2016 

Methods

In this section, the methodology used for the study is briefly explained. The methodology includes the NDVI data processing and its representation in ArcGIS software, calculation of monthly NDVI anomalies for the study period, and spatial autocorrelation (global spatial autocorrelation and LISA) of monthly NDVI anomalies for 71 micro watersheds in Geo-Da software.

NDVI data processing and generation of spatial variation maps

The downloaded MOD13C2 NDVI data product has been processed in ArcGIS software. First, the raster data in the form of pixels are converted to vector data (points) to create spatial variation maps. Then, the point-converted NDVI data was used to generate spatial variation maps of NDVI. The IDW interpolation technique has been used to perform the interpolation analysis. The IDW interpolation technique is suitable for the sample points that are equidistant and in a grid format. So, as points are converted from the raster, all the points are equidistant and gridded. Then the generated NDVI variation maps are reclassified into three classes; less than 0.3, 0.3–0.5 and more than 0.5 based on NDVI value. Finally, the area covered by all three classes of NDVI has been calculated and analyzed.

Anomaly calculation to identify ENSO- and IOD-sensitive vegetation area

The monthly NDVI anomalies are calculated using the raster calculator tool in ArcGIS. Anomalies are the difference between actual monthly NDVI values and the average of long-term monthly NDVI values. Here in this study, the long-term average considered is the average of monthly NDVI values from February 2000 to January 2022. The mathematical expression for NDVI anomaly calculation is given in the following equation,
(2)
For example, the NDVI anomaly of January 2001 is calculated

where,

AnomalyNDVI is the monthly NDVI anomaly for January 2001;

X is the actual value of the average monthly NDVI January 2001 and

is the long-term average monthly NDVI for January (an average NDVI value of January month from 2001 to 2022)

After the monthly NDVI anomalies have been calculated, the pixels sensitive to ENSO and IOD events are identified based on the range of NDVI anomaly values. The threshold value considered in this study is +0.05 for positive anomalous pixels and −0.05 for negative anomalous pixels, i.e., all the pixels having monthly NDVI anomaly value greater than +0.05 are positive sensitive pixels and all the pixels having monthly NDVI anomaly value less than −0.05 are negative sensitive pixels. The threshold values were selected based on data distribution of anomalous pixels. Sample histograms of the normal distribution of anomalous pixels are shown in Figure S1. The number of anomalous pixels will vary if the threshold values change. More data points will probably be classified as positive or sensitive anomalous pixels when the threshold value is lowered, and vice versa. The NDVI anomaly values are analyzed for the El Niño, La Niña, Positive IOD and Negative IOD years, and the specific event-sensitive pixels are identified based on monthly NDVI anomaly values.

Spatial autocorrelation (global spatial autocorrelation and LISA)

This study uses spatial autocorrelation analysis to identify the growth and spatial features of the monthly NDVI anomaly over the Upper Bhima Sub-basin. Spatial autocorrelation indicates the interconnection between a specific attribute value at a regional level and the same attribute value in a neighboring geographical location. It is a metric of the degree of value aggregation in the spatial domain. This aggregation property is measured using Moran's I, divided into global spatial autocorrelation and LISA. The global spatial autocorrelation has been applied to the monthly NDVI anomalies, but the results of all the events show clustered patterns with zero or negligible p values. So, the LISA has been applied for the analysis.

Local Moran's I, also known as LISA Index has been used to indicate the specific accumulation area and spatial aggregation of NDVI anomalies in 71 micro watersheds. Local Moran's I determines the correlation of each spatial unit. For the ith area, Local Moran's I index is defined as follows:
(3)
where, is an attribute for feature i, is the mean of the corresponding attribute, is the spatial weight between feature i and j.
If ,
(4)
Moran's I's LISA statistics are tested using z-score:
(5)

The LISA coefficient is used to determine whether there is spatial clustering of NDVI anomaly. The LISA coefficient greater than 0 indicates that there is a positive spatial correlation between the local spatial unit and the nearby spatial unit, which is represented by ‘high–high’ or ‘low–low’; the LISA index less than 0 indicates ‘low–high’ or ‘high–low’. The performance of the aggregation is negatively correlated.

Spatial variation of NDVI/vegetation in ENSO and IOD events

The variation in the vegetation based on NDVI values has been estimated. The study area is primarily covered by agricultural area (58.43%) and barren land (19.16%) while forest land is 14.08%, water bodies are 1.35% and built-up area is 6.98%. The LULC map of the study area derived from the LANDSAT 8 image of November 2015 is shown as Figure 4.
Figure 4

LULC map of the study area.

Figure 4

LULC map of the study area.

Close modal
The spatial distribution of vegetation based on NDVI values in ENSO and IOD years are shown in Figures 58, respectively. The impacts of the El Niño and La Niña dominant cycles on the vegetation condition in the Upper Bhima Sub-basin may clearly be observed from Figures 5 and 6, respectively, and impacts of the positive and negative IOD events from Figures 7 and 8, respectively. The spatial distribution of NDVI-derived vegetation sensitive to ENSO and IOD varies due to variations in precipitation, temperature, topography and agricultural activities throughout sub-basins. In order to examine the regional variations in the area and pattern of ENSO- and IOD-sensitive vegetation, the percentage of areas covered by the three vegetation classes in the Upper Bhima Sub-basin was estimated and tabulated in Tables 35. The NDVI values were categorized into the same number of classes with the same range to make it simple to compare the results for El Niño and La Niña events in the case of ENSO and positive and negative IOD in the case of IOD years. The NDVI value range −1 to +1 is classified into three different classes where <0.3, 0.3–0.5 and >0.5 denote sparse vegetation (red), medium dense vegetation (yellow) and highly dense vegetation (green), respectively. In case of ENSO events, the results were analyzed by considering seasons as ENSO cycle starts from July to May for analyzing appropriate results. The IOD years, however, are taken as provided by the meteorological agency BOM Australia. To understand the variation of NDVI in accordance with the variation of precipitation and temperature for the same time periods, precipitation and temperature variation maps are generated and given as Figures S2 to S9. Spatial variation maps of precipitation and temperature have been generated by using Climate Research Unit (CRU) data.
Table 3

Details of area covered by each class of the vegetation in El Niño years

El Niño yearsSeasonNDVI classArea (km2)% AreaEl Niño yearsSeasonNDVI classArea (km2)% Area
2002–2003 JAS <0.3 5,679.86 12.33 2009–10 JAS <0.3 633.64 1.38 
0.3–0.5 31,201.57 67.73 0.3–0.5 26,762.03 58.10 
>0.5 9,184.57 19.94 >0.5 18,670.33 40.53 
OND <0.3 6,052.82 13.14 OND <0.3 0.22 0.00 
0.3–0.5 36,278.03 78.75 0.3–0.5 29,696.91 64.47 
>0.5 3,735.15 8.11 >0.5 16,368.87 35.53 
JFM <0.3 31,839.43 69.12 JFM <0.3 8,809.18 19.12 
0.3–0.5 14,166.68 30.75 0.3–0.5 35,930.64 78.00 
>0.5 59.90 0.13 >0.5 1,326.19 2.88 
AMJ <0.3 38,901.79 84.45 AMJ <0.3 32,277.21 70.07 
0.3–0.5 7,164.21 15.55 0.3–0.5 13,758.85 29.87 
>0.5 0.00 0.00 >0.5 29.94 0.07 
2004–2005 JAS <0.3 708.65 1.54 2015–16 JAS <0.3 8,940.88 19.41 
0.3–0.5 34,143.56 74.12 0.3–0.5 25,973.49 56.38 
>0.5 11,213.80 24.34 >0.5 11,151.64 24.21 
OND <0.3 488.55 1.06 OND <0.3 924.37 2.00 
0.3–0.5 40,208.62 87.29 0.3–0.5 32,837.72 71.28 
>0.5 5,368.84 11.66 >0.5 12,303.91 26.71 
JFM <0.3 29,630.54 64.32 JFM <0.3 26,792.63 58.16 
0.3–0.5 16,127.97 35.01 0.3–0.5 18,538.08 40.24 
>0.5 307.50 0.67 >0.5 735.29 1.60 
AMJ <0.3 36,367.62 78.95 AMJ <0.3 37,204.05 80.76 
0.3–0.5 9,690.72 21.04 0.3–0.5 8,803.91 19.11 
>0.5 7.67 0.02 >0.5 58.04 0.13 
El Niño yearsSeasonNDVI classArea (km2)% AreaEl Niño yearsSeasonNDVI classArea (km2)% Area
2002–2003 JAS <0.3 5,679.86 12.33 2009–10 JAS <0.3 633.64 1.38 
0.3–0.5 31,201.57 67.73 0.3–0.5 26,762.03 58.10 
>0.5 9,184.57 19.94 >0.5 18,670.33 40.53 
OND <0.3 6,052.82 13.14 OND <0.3 0.22 0.00 
0.3–0.5 36,278.03 78.75 0.3–0.5 29,696.91 64.47 
>0.5 3,735.15 8.11 >0.5 16,368.87 35.53 
JFM <0.3 31,839.43 69.12 JFM <0.3 8,809.18 19.12 
0.3–0.5 14,166.68 30.75 0.3–0.5 35,930.64 78.00 
>0.5 59.90 0.13 >0.5 1,326.19 2.88 
AMJ <0.3 38,901.79 84.45 AMJ <0.3 32,277.21 70.07 
0.3–0.5 7,164.21 15.55 0.3–0.5 13,758.85 29.87 
>0.5 0.00 0.00 >0.5 29.94 0.07 
2004–2005 JAS <0.3 708.65 1.54 2015–16 JAS <0.3 8,940.88 19.41 
0.3–0.5 34,143.56 74.12 0.3–0.5 25,973.49 56.38 
>0.5 11,213.80 24.34 >0.5 11,151.64 24.21 
OND <0.3 488.55 1.06 OND <0.3 924.37 2.00 
0.3–0.5 40,208.62 87.29 0.3–0.5 32,837.72 71.28 
>0.5 5,368.84 11.66 >0.5 12,303.91 26.71 
JFM <0.3 29,630.54 64.32 JFM <0.3 26,792.63 58.16 
0.3–0.5 16,127.97 35.01 0.3–0.5 18,538.08 40.24 
>0.5 307.50 0.67 >0.5 735.29 1.60 
AMJ <0.3 36,367.62 78.95 AMJ <0.3 37,204.05 80.76 
0.3–0.5 9,690.72 21.04 0.3–0.5 8,803.91 19.11 
>0.5 7.67 0.02 >0.5 58.04 0.13 
Table 4

Details of area covered by each class of the vegetation in La Niña years

La Niña yearsSeasonNDVI classArea (km2)% AreaLa Niña yearsSeasonNDVI classArea (km2)% Area
2007–2008 JAS <0.3 7.64 0.02 2011–12 JAS <0.3 745.53 1.62 
0.3–0.5 20,376.25 44.23 0.3–0.5 25,944.58 56.32 
>0.5 25,682.11 55.75 >0.5 19,375.89 42.06 
OND <0.3 999.85 2.17 OND <0.3 2,532.12 5.50 
0.3–0.5 37,182.97 80.72 0.3–0.5 31,919.31 69.29 
>0.5 7,883.18 17.11 >0.5 11,614.57 25.21 
JFM <0.3 25,639.13 55.66 JFM <0.3 25,252.21 54.82 
0.3–0.5 20,382.34 44.25 0.3–0.5 20,736.43 45.05 
>0.5 44.53 0.09 >0.5 77.36 0.17 
AMJ <0.3 35,258.74 76.54 AMJ <0.3 33,169.71 72.01 
0.3–0.5 10,805.58 23.46 0.3–0.5 12,894.51 27.99 
>0.5 1.68 0.00 >0.5 1.78 0.00 
2010–2011 JAS <0.3 0.00 0.00 2020–21 JAS <0.3 0.00 0.00 
0.3–0.5 9,882.28 21.45 0.3–0.5 2,169.31 4.71 
>0.5 36,183.73 78.55 >0.5 43,896.69 95.29 
OND <0.3 0.00 0.00 OND <0.3 0.00 0.00 
0.3–0.5 17,547.52 38.09 0.3–0.5 14,946.37 32.45 
>0.5 28,518.48 61.91 >0.5 31,119.63 67.55 
JFM <0.3 9,873.11 21.43 JFM <0.3 2,407.05 5.23 
0.3–0.5 35,267.66 76.56 0.3–0.5 41,183.28 89.40 
>0.5 925.23 2.01 >0.5 2,475.68 5.37 
AMJ <0.3 30,870.00 67.01 AMJ <0.3 17,146.14 37.22 
0.3–0.5 15,144.43 32.88 0.3–0.5 27,567.51 59.84 
>0.5 51.57 0.11 >0.5 1,352.35 2.94 
La Niña yearsSeasonNDVI classArea (km2)% AreaLa Niña yearsSeasonNDVI classArea (km2)% Area
2007–2008 JAS <0.3 7.64 0.02 2011–12 JAS <0.3 745.53 1.62 
0.3–0.5 20,376.25 44.23 0.3–0.5 25,944.58 56.32 
>0.5 25,682.11 55.75 >0.5 19,375.89 42.06 
OND <0.3 999.85 2.17 OND <0.3 2,532.12 5.50 
0.3–0.5 37,182.97 80.72 0.3–0.5 31,919.31 69.29 
>0.5 7,883.18 17.11 >0.5 11,614.57 25.21 
JFM <0.3 25,639.13 55.66 JFM <0.3 25,252.21 54.82 
0.3–0.5 20,382.34 44.25 0.3–0.5 20,736.43 45.05 
>0.5 44.53 0.09 >0.5 77.36 0.17 
AMJ <0.3 35,258.74 76.54 AMJ <0.3 33,169.71 72.01 
0.3–0.5 10,805.58 23.46 0.3–0.5 12,894.51 27.99 
>0.5 1.68 0.00 >0.5 1.78 0.00 
2010–2011 JAS <0.3 0.00 0.00 2020–21 JAS <0.3 0.00 0.00 
0.3–0.5 9,882.28 21.45 0.3–0.5 2,169.31 4.71 
>0.5 36,183.73 78.55 >0.5 43,896.69 95.29 
OND <0.3 0.00 0.00 OND <0.3 0.00 0.00 
0.3–0.5 17,547.52 38.09 0.3–0.5 14,946.37 32.45 
>0.5 28,518.48 61.91 >0.5 31,119.63 67.55 
JFM <0.3 9,873.11 21.43 JFM <0.3 2,407.05 5.23 
0.3–0.5 35,267.66 76.56 0.3–0.5 41,183.28 89.40 
>0.5 925.23 2.01 >0.5 2,475.68 5.37 
AMJ <0.3 30,870.00 67.01 AMJ <0.3 17,146.14 37.22 
0.3–0.5 15,144.43 32.88 0.3–0.5 27,567.51 59.84 
>0.5 51.57 0.11 >0.5 1,352.35 2.94 
Table 5

Details of area covered by each class of the vegetation in positive and negative IOD years

Positive IOD yearsSeasonNDVI classArea (km2)% AreaNegative IOD yearsSeasonNDVI classArea (km2)% Area
2006 JFM <0.3 26,357.32 57.22 2010 JFM <0.3 8,809.18 19.12 
0.3–0.5 19,597.88 42.54 0.3–0.5 35,930.64 77.00 
>0.5 110.80 0.24 >0.5 1,326.19 2.88 
AMJ <0.3 27,333.72 59.34 AMJ <0.3 23,497.28 51.01 
0.3–0.5 18,603.64 40.39 0.3–0.5 22,442.44 48.72 
>0.5 128.64 0.28 >0.5 126.28 0.27 
JAS <0.3 599.12 1.30 JAS <0.3 0.00 0.00 
0.3–0.5 23,804.24 51.67 0.3–0.5 9,882.28 21.45 
>0.5 21,662.64 47.03 >0.5 36,183.73 78.55 
OND <0.3 0.58 0.00 OND <0.3 0.00 0.00 
0.3–0.5 28,246.93 61.32 0.3–0.5 17,547.52 38.09 
>0.5 17,818.49 38.68 >0.5 28,518.48 61.91 
2012 JFM <0.3 25,252.21 54.82 2014 JFM <0.3 13,160.25 28.57 
0.3–0.5 20,736.43 45.02 0.3–0.5 30,950.06 67.19 
>0.5 77.36 0.17 >0.5 1,955.70 4.25 
AMJ <0.3 32,178.08 69.85 AMJ <0.3 25,780.63 55.97 
0.3–0.5 13,867.96 30.11 0.3–0.5 18,997.64 41.24 
>0.5 19.97 0.04 >0.5 1,287.73 2.80 
JAS <0.3 8,117.07 17.62 JAS <0.3 62.70 0.14 
0.3–0.5 25,829.77 56.07 0.3–0.5 28,180.94 61.18 
>0.5 12,119.16 26.31 >0.5 17,822.36 38.69 
OND <0.3 489.03 1.06 OND <0.3 3.39 0.01 
0.3–0.5 33,489.62 72.70 0.3–0.5 30,847.22 66.96 
>0.5 12,087.35 26.24 >0.5 15,215.39 33.03 
2015 JFM <0.3 12,905.87 28.02 2016 JFM <0.3 26,792.63 58.16 
0.3–0.5 31,930.66 69.32 0.3–0.5 18,538.08 40.24 
>0.5 1,229.47 2.669 >0.5 735.29 1.60 
AMJ <0.3 24,643.01 53.50 AMJ <0.3 34,403.10 74.68 
0.3–0.5 20,698.32 44.93 0.3–0.5 11,520.86 25.01 
>0.5 724.66 1.57 >0.5 142.02 0.30 
JAS <0.3 8,940.88 19.41 JAS <0.3 0.00 0.00 
0.3–0.5 25,973.49 56.38 0.3–0.5 16,862.50 36.61 
>0.5 11,151.64 24.21 >0.5 29,203.50 63.40 
OND <0.3 924.37 2.01 OND <0.3 15.00 0.03 
0.3–0.5 32,837.72 71.28 0.3–0.5 34,652.52 75.22 
>0.5 12,303.91 26.71 >0.5 11,398.48 24.74 
Positive IOD yearsSeasonNDVI classArea (km2)% AreaNegative IOD yearsSeasonNDVI classArea (km2)% Area
2006 JFM <0.3 26,357.32 57.22 2010 JFM <0.3 8,809.18 19.12 
0.3–0.5 19,597.88 42.54 0.3–0.5 35,930.64 77.00 
>0.5 110.80 0.24 >0.5 1,326.19 2.88 
AMJ <0.3 27,333.72 59.34 AMJ <0.3 23,497.28 51.01 
0.3–0.5 18,603.64 40.39 0.3–0.5 22,442.44 48.72 
>0.5 128.64 0.28 >0.5 126.28 0.27 
JAS <0.3 599.12 1.30 JAS <0.3 0.00 0.00 
0.3–0.5 23,804.24 51.67 0.3–0.5 9,882.28 21.45 
>0.5 21,662.64 47.03 >0.5 36,183.73 78.55 
OND <0.3 0.58 0.00 OND <0.3 0.00 0.00 
0.3–0.5 28,246.93 61.32 0.3–0.5 17,547.52 38.09 
>0.5 17,818.49 38.68 >0.5 28,518.48 61.91 
2012 JFM <0.3 25,252.21 54.82 2014 JFM <0.3 13,160.25 28.57 
0.3–0.5 20,736.43 45.02 0.3–0.5 30,950.06 67.19 
>0.5 77.36 0.17 >0.5 1,955.70 4.25 
AMJ <0.3 32,178.08 69.85 AMJ <0.3 25,780.63 55.97 
0.3–0.5 13,867.96 30.11 0.3–0.5 18,997.64 41.24 
>0.5 19.97 0.04 >0.5 1,287.73 2.80 
JAS <0.3 8,117.07 17.62 JAS <0.3 62.70 0.14 
0.3–0.5 25,829.77 56.07 0.3–0.5 28,180.94 61.18 
>0.5 12,119.16 26.31 >0.5 17,822.36 38.69 
OND <0.3 489.03 1.06 OND <0.3 3.39 0.01 
0.3–0.5 33,489.62 72.70 0.3–0.5 30,847.22 66.96 
>0.5 12,087.35 26.24 >0.5 15,215.39 33.03 
2015 JFM <0.3 12,905.87 28.02 2016 JFM <0.3 26,792.63 58.16 
0.3–0.5 31,930.66 69.32 0.3–0.5 18,538.08 40.24 
>0.5 1,229.47 2.669 >0.5 735.29 1.60 
AMJ <0.3 24,643.01 53.50 AMJ <0.3 34,403.10 74.68 
0.3–0.5 20,698.32 44.93 0.3–0.5 11,520.86 25.01 
>0.5 724.66 1.57 >0.5 142.02 0.30 
JAS <0.3 8,940.88 19.41 JAS <0.3 0.00 0.00 
0.3–0.5 25,973.49 56.38 0.3–0.5 16,862.50 36.61 
>0.5 11,151.64 24.21 >0.5 29,203.50 63.40 
OND <0.3 924.37 2.01 OND <0.3 15.00 0.03 
0.3–0.5 32,837.72 71.28 0.3–0.5 34,652.52 75.22 
>0.5 12,303.91 26.71 >0.5 11,398.48 24.74 
Figure 5

Spatial distribution of NDVI over Upper Bhima sub-basin during El Niño years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 5

Spatial distribution of NDVI over Upper Bhima sub-basin during El Niño years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

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Figure 6

Spatial distribution of NDVI over Upper Bhima sub-basin during La Niña years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 6

Spatial distribution of NDVI over Upper Bhima sub-basin during La Niña years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

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Figure 7

Spatial distribution of NDVI over Upper Bhima sub-basin for positive IOD years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 7

Spatial distribution of NDVI over Upper Bhima sub-basin for positive IOD years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

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Figure 8

Spatial distribution of NDVI over Upper Bhima sub-basin for negative IOD years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 8

Spatial distribution of NDVI over Upper Bhima sub-basin for negative IOD years. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

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El Niño and La Niña events of ENSO

The spatial distribution of NDVI during El Niño and La Niña events have been generated for JAS, OND, JFM and AMJ months and are shown in Figures 5 and 6, respectively. The total area covered by the sparse, medium dense and highly dense vegetation during El Niño and La Niña events is tabulated in Tables 3 and 4, respectively.

It has been observed that in AMJ months during both the ENSO phenomenon, the spatial variation shows a similar pattern and a majority of the area is covered by sparse vegetation (NDVI < 0.3). The percentage area covered by sparse vegetation in AMJ months of El Niño events are 84.45 (2002–2003), 78.95 (2004–2005), 70.07 (2009–2010) and 80.76 (2015–2016) and for La Niña events are 76.54 (2007–2008), 67.01 (2010–2011), 72 (2011–2012) and 37.22 (2020–2021). This illustrates that ENSO has no impact on vegetation during AMJ.

The micro-watersheds from the western and southern regions of the sub-basin are most vulnerable to El Niño events as this region shows sparse vegetation during El Niño events. The central, eastern and southern region of the sub-basin is already in the rainfall shadow zone.

The impact of ENSO on NDVI is clearly observed during JAS and OND months as shown in Figures 5 and 6. The percentage area covered by dense vegetation (NDVI > 0.5) during La Niña years in JAS and OND is more as compared to El Niño years. The percentage area covered by dense vegetation during El Niño events in JAS months are 19.94 (2002–2003), 24.34 (2004–2005), 40.53 (2009–2010) and 24.21 (2015–2016) and in OND months are 8.11 (2002–2003), 11.66 (2004–2005), 35.53 (2009–2010) and 26.71 (2015–2016). While, percentage area covered by dense vegetation during La Niña years in JAS months are 55.75 (2007–2008), 78.55 (2010–2011), 42.06 (2011–2012) and 95.29 (2020–2021) in OND months are 17.11 (2007–2008), 61.91 (2010–2011), 25.21 (2011–2012) and 67.55 (2020–2021). This variation in the percentage of area covered by highly dense vegetation shows how ENSO has a significant influence on the vegetation during JAS and OND months. The impacts of ENSO on the spatial variation of NDVI are also observed during JFM months. The area covered by sparse vegetation in JFM months during El Niño years is more than that of La Niña years. The results related to the impact of El Niño and La Niña year on vegetation match with the study conducted in Haryana state in India by Chauhan et al. (2022). The study analyzed the vegetation for monsoon only and concluded that vegetation in monsoon during La Niña is higher than in El Niño.

The western region within the study area has a dense vegetation cover due to geographical factors and the Sahyadri mountain range. According to the fluctuations in temperature and precipitation, El Niña is a warm phase, whereas La Niña is the cold phase of ENSO and the El Niño event has less rainfall in India than the La Niña event (Wang et al. 2014).

The results show a distinct dipole pattern that is reversed between El Niño and La Niña and shows that vegetation conditions are highly connected with ENSO climatic phenomenon. In the Upper Bhima sub-basin, ENSO events are controlled due to the oscillations between wind and SST controlling the amount of monsoon rainfall in the sub-basin. This results in less rainfall during El Niño events and excessive rainfall during La Niña events, which is evident from the regional vegetation growth pattern.

Positive and negative IOD events

Sustained changes in the difference between sea surface temperatures of the tropical western and eastern Indian Oceans are known as the Indian Ocean Dipole or IOD. According to the fluctuations in SST, the IOD event is considered a positive (negative) IOD when the Western Indian Ocean is warmer (cooler) than the Eastern Indian Ocean. The rise in temperature in a particular geographical region causes a rise in convection which ultimately causes an increase in the rainfall in that region. As a result, the countries surrounding the Indian Ocean are affected by the IOD events. There are many studies and research on the impact of IOD events on African countries surrounding the Eastern Indian Ocean (Anyamba et al. 2018), concluding that IOD has significant impacts such as the incidence of severe floods due to an increase in convection in that area. As India is geographically located between the Eastern and Western Indian Oceans, it is very complicated to decide whether IOD events affect India's monsoon cycle.

The spatial distribution of vegetation derived NDVI values in positive and negative IOD events is shown in Figures 7 and 8, respectively. To analyze the regional variations and change in the pattern of vegetation during positive and negative IOD events, the area covered by the three vegetation classes (sparse vegetation, medium vegetation and highly dense vegetation) in the Upper Bhima Sub-basin, is shown in Table 5. During IOD events also, the NDVI variation has been analyzed for JFM, AMJ, JAS and OND months to understand the seasonal variation.

It has been observed that in AMJ months during both the positive and negative IOD events, the spatial variation shows a similar pattern and the majority of the area is covered by sparse vegetation (NDVI < 0.3). The percentage area covered by sparse vegetation in AMJ months during positive IOD events are 59.34 (2006), 69.85 (2012) and 53.50 (2015) and of negative IOD events are 51.01 (2010), 55.97 (2014) and 74.68 (2016). This similarity in the percentage area covered by sparse vegetation in AMJ months during both positive and negative IOD events illustrates that IOD has much less impact on the vegetation in AMJ months.

The impact of IOD on NDVI is clearly observed during JAS and OND months as shown in Figures 7 and 8. The percentage area covered by dense vegetation (NDVI > 0.5) during negative IOD events in JAS and OND is more as compared to positive IOD events. The percentage area covered by dense vegetation during positive IOD events in JAS months are 47.03 (2006), 26.31 (2012) and 24.21 (2015) and in OND months are 38.68 (2006), 26.24 (2012) and 26.71 (2015). While, the percentage of area covered by dense vegetation during negative IOD events in JAS months are 78.55 (2010), 38.69 (2014) and 63.40 (2016) and in OND months are 61.91 (2010), 33.03 (2014) and 24.74 (2016). Also, the sparse vegetation is not even present in JAS and OND months during negative IOD events and is present up to 20% in JFM. This difference in the area covered by dense vegetation illustrates that a positive IOD event has a major adverse impact on the vegetation during JAS and OND months than a negative IOD event.

The results show a similar dipole pattern as seen in ENSO events. The vegetation patterns in positive and negative IOD occurrences indicate that it is connected to the IOD climate phenomenon. Positive and negative IOD events caused by changes in SST in the Indian Oceans regulate rainfall in the Upper Bhima sub-basin, impacting the regional vegetation pattern.

Identification of ENSO- and IOD-sensitive pixels

The ENSO and IOD-sensitive pixels are identified by using monthly NDVI anomalies. Instead of finding the sensitive pixels annually, for better understanding, the seasonal anomalies of the data variables are derived through a simple compilation of their monthly values. The seasons are categorized into January–March (JFM), April–June (AMJ), July–September (JAS), and October–December (OND). The ENSO- and IOD-sensitive pixels for JFM, AMJ, JAS and OND are shown in Figure 9. Green pixels represent positive anomaly pixels, while red pixels represent negative anomaly pixels.
Figure 9

Sensitive vegetation pixels identified by calculating NDVI anomalies for El Niño, La Niña, positive IOD and negative IOD events. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Figure 9

Sensitive vegetation pixels identified by calculating NDVI anomalies for El Niño, La Niña, positive IOD and negative IOD events. Please refer to the online version of this paper to see this figure in colour: http://dx.doi.org/10.2166/wcc.2023.010.

Close modal

The pixels sensitive to ENSO and IOD events are determined based on the range of NDVI anomaly values. Based on the NDVI anomaly range, the threshold value considered in this study is +0.05 for positive anomalous pixels and −0.05 for negative anomalous pixels. Positive anomaly pixels have a monthly NDVI anomaly value larger than +0.05, whereas negative anomaly pixels have a monthly NDVI anomaly value less than −0.05.

In the El Niño and La Niña events for JFM and AMJ, the area covered by negative sensitive pixels is much less than positive anomaly pixels. All positive anomaly pixels in El Niño and La Niña events during the JFM and AMJ seasons are dispersed throughout the study area and are not concentrated in any specific region. Also, during JAS and OND seasons, i.e., during the monsoon and post-monsoon period, El Niño and La Niña events show the opposite results. JAS and OND seasons have maximum negative sensitive pixels in El Niño events and maximum positive anomaly pixels in La Niña events. Hence, it may be concluded that El Niño has an adverse effect on the monsoon rainfall, which can be identified from the presence of a large number of negative anomaly pixels during the post-monsoon period (JAS and OND). The study conducted by et al. (2012) analyzed the El Niño and La Niña sensitive vegetation and concluded that the area of El Niño sensitive vegetation was much larger than the area of La Niña sensitive vegetation, although the study was conducted for specific El Niño and La Niña events without considering the seasonality.

In case of IOD events, positive anomaly pixels are almost absent in the JFM season of positive IOD events and are very few in JFM and AMJ in negative IOD events. Also, there are very few negative anomaly pixels in all seasons of positive IOD events. However, during JAS, i.e., during monsoon in positive IOD event, negative anomaly pixels are concentrated in the southern region of the study area, which is a drought-prone area due to the rainfall shadow zone and all positive anomaly pixels are distributed throughout the study area. This concludes that negative IOD events have a negative impact during JFM and AMJ seasons, and the rainfall shadow zone is also affected adversely during JAS of positive IOD events.

LISA analysis

The concentration and significance of monthly NDVI anomaly within a specific region can be clearly expressed through LISA analysis.

The references to high and low in the results of LISA are relative to the variable's mean and should not be taken as fact. In this study, the high–high indicates that the monthly NDVI anomaly having higher values is clustered in the red color area, and the low–low indicates that the monthly NDVI anomaly having lower values is clustered in the blue color area, as shown in cluster maps. The significant areas of high–high, low–low, low–high, and high–low in the 71 micro watersheds of the Upper Bhima Sub-basin during El Niño, La Niña, positive IOD and negative IOD are shown in Figures 1013, respectively. These are the cluster maps, including the significance levels of the p-value as 0.05, 0.01 and 0.001, as shown in the figures. The region's significant high–high and low–low distribution indicate spatial clusters, and high–low and low–high indicate spatial outliers.
Figure 10

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in El Niño year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in El Niño year (b). (Maps are created by Geo-da, version 1.14.0. https://geodacenter.github.io/.).

Figure 10

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in El Niño year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in El Niño year (b). (Maps are created by Geo-da, version 1.14.0. https://geodacenter.github.io/.).

Close modal
Figure 11

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in La Niña year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in La Niña year (b). (Maps are created by Geoda, version 1.14.0. https://geodacenter.github.io/.).

Figure 11

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in La Niña year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in La Niña year (b). (Maps are created by Geoda, version 1.14.0. https://geodacenter.github.io/.).

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Figure 12

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in positive IOD year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in positive IOD year (b). (Maps are created by Geoda, version 1.14.0. https://geodacenter.github.io/.).

Figure 12

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in positive IOD year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in positive IOD year (b). (Maps are created by Geoda, version 1.14.0. https://geodacenter.github.io/.).

Close modal
Figure 13

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in negative IOD year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in negative IOD year (b). (Maps are created by Geoda, version 1.14.0. https://geodacenter.github.io/.).

Figure 13

LISA cluster map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in negative IOD year (a), LISA significance map of NDVI anomaly in 71 micro-watersheds in JFM, AMJ, JAS and OND in negative IOD year (b). (Maps are created by Geoda, version 1.14.0. https://geodacenter.github.io/.).

Close modal

In accordance with Table 6, the spatial clusters (high–high and low–low) in the total study area are higher than that of spatial outliers for all the ENSO and IOD events. However, El Niño and La Niña cluster maps reveal contrasting results. In El Niño events, the Western Ghat region and surrounding region show a cluster of high anomaly values and a cluster of low anomaly values in the study area's eastern and northeastern parts throughout the year except JFM. In JFM, the cluster of high and low anomaly values is present in an irregular pattern, as shown in Figure 10.

Table 6

LISA types of monthly NDVI anomaly for ENSO and IOD events in 71 micro watersheds in study area

Spatial autocorrelation typeMonthsHigh–highLow–lowLow–highHigh–lowNeighborlessNon-significantTotal
El Niño JFM 53 71 
AMJ 13 14 42 71 
JAS 16 16 37 71 
OND 20 23 25 71 
La Niña JFM 11 10 48 71 
AMJ 16 19 34 71 
JAS 18 16 35 71 
OND 50 71 
Positive IOD JFM 56 71 
AMJ 62 71 
JAS 14 46 71 
OND 17 45 71 
Negative IOD JFM 19 16 35 71 
AMJ 11 14 45 71 
JAS 11 17 42 71 
OND 58 71 
Spatial autocorrelation typeMonthsHigh–highLow–lowLow–highHigh–lowNeighborlessNon-significantTotal
El Niño JFM 53 71 
AMJ 13 14 42 71 
JAS 16 16 37 71 
OND 20 23 25 71 
La Niña JFM 11 10 48 71 
AMJ 16 19 34 71 
JAS 18 16 35 71 
OND 50 71 
Positive IOD JFM 56 71 
AMJ 62 71 
JAS 14 46 71 
OND 17 45 71 
Negative IOD JFM 19 16 35 71 
AMJ 11 14 45 71 
JAS 11 17 42 71 
OND 58 71 

The Moran index for all the events lies within an 0–1 interval indicating that the monthly NDVI anomaly of 71 micro watersheds has significant spatial autocorrelation. Local Moran's I of 71 watersheds in the study area are given in Table 7. Moran's I autocorrelation values of JFM, AMJ, JAS and OND in El Niño events are 0.387, 0.626, 0.779 and 0.809, respectively, and in La Niña events, 0.449, 0.707, 0.701 and 0.562, respectively.

Table 7

Local Moran's I of 71 watersheds in study area

Spatial autocorrelation typeMonthsMoran's I
El Niño JFM 0.387 
AMJ 0.626 
JAS 0.779 
OND 0.809 
La Niña JFM 0.449 
AMJ 0.707 
JAS 0.701 
OND 0.562 
Positive IOD JFM 0.386 
AMJ 0.275 
JAS 0.584 
OND 0.585 
Negative IOD JFM 0.825 
AMJ 0.681 
JAS 0.666 
OND 0.367 
Spatial autocorrelation typeMonthsMoran's I
El Niño JFM 0.387 
AMJ 0.626 
JAS 0.779 
OND 0.809 
La Niña JFM 0.449 
AMJ 0.707 
JAS 0.701 
OND 0.562 
Positive IOD JFM 0.386 
AMJ 0.275 
JAS 0.584 
OND 0.585 
Negative IOD JFM 0.825 
AMJ 0.681 
JAS 0.666 
OND 0.367 

Whereas in La Niña events (Figure 11), high anomaly values are clustered in the eastern and central part of the study area, and low anomaly values are clustered in Western Ghat and the surrounding region for the whole year except OND. Here, in the La Niña event during the post-monsoon period, i.e., in OND, both high and low clusters are concentrated in the eastern part of the study area, and the low–low cluster is located precisely at the rainfall shadow zone. This indicates that, even if precipitation is higher during a La Niña year, the rainfall shadow zone does not receive adequate water.

In positive IOD events, significantly fewer micro watersheds show significant clusters generated after LISA analysis compared to the ENSO events (Figure 12). This indicates that a positive IOD event does not affect the monthly NDVI anomaly. However, the central region of the study area in JAS and OND during positive IOD events shows a cluster of high NDVI anomaly values, and negative anomaly pixels are clustered in the southern part, which is a drought-prone area during the post-monsoon period (OND).

In negative IOD events, JFM and AMJ seasons have high anomaly values clustered in the western region and low anomaly pixels are clustered in the central and southern regions (Figure 13). During the post-monsoon period, very few micro watersheds have high and low clusters. As far as the IOD events are considered, the negative IOD event has more effect on monthly vegetation anomaly clusters than the positive IOD event.

The outcome of this study will be helpful to key stakeholders such as farmers, the Water Resource Department in the state of Maharashtra, the Central Water Commission of India and policymakers. The study provides extensive information on the response of vegetation to climate change events that can be used for the implementation and planning of farming-related activities to resolve the problems faced by farmers during extreme events like floods and droughts. The study also gives information about the impact of ENSO and IOD events on vegetation cover and the location of vegetation clusters in the study area, i.e., it can also be used for assessment and planning of agricultural activities. For example, seasonal variation can be mapped in relation to ENSO and IOD events in the agricultural region (Figure 9). Vulnerable micro watersheds will be given more priority for future planning of water supply and demand management (Figures 1013).

This study presents a complete assessment of vegetation sensitivity to ENSO and IOD events over the Upper Bhima Sub-basin, Western Maharashtra, India, from 2000 to 2022. MODIS NDVI data were used to represent vegetation, and the ENSO and IOD events were defined. El Niño and La Niña events of ENSO are identified using the Southern Oscillation Index (SOI), and positive and negative IOD is identified using DMI. This study identifies ENSO and IOD-sensitive vegetation regions for selected ENSO and IOD events from 2000 to 2022 monthly NDVI anomalies. The following conclusions can be drawn based on this work:

  • 1.

    Seasonality affects the vegetation variation during all the events due to the rainfall and temperature variation which are predominant parameters causing vegetation variation at the regional level.

  • 2.

    The effect of ENSO on NDVI is noticeable and observed during JAS and OND months as percentage area covered by dense vegetation during El Niño event is less than 30% and that of during the La Niña event is more than 50%. Therefore, when ENSO events are considered, most of the vegetation in the watershed is adversely affected during El Niño which is the warm phase of the ENSO event while higher NDVI values are observed during the La Niña events as expected. Hence, a dipole pattern is seen during ENSO events.

  • 3.

    The vegetation patterns in positive and negative IOD events indicate that vegetation is connected to the IOD climate phenomenon. Positive and negative IOD events caused by changes in SST in the Indian Oceans regulate rainfall in the Upper Bhima sub-basin, impacting the regional vegetation development pattern. The percentage area covered by dense vegetation is more in negative IOD events than positive IOD events during JAS and OND, i. e. during monsoon and post-monsoon periods. Hence it can be concluded that a positive IOD event has an adverse effect on vegetation growth compared to a negative IOD event. The lowest vegetation has been seen in the drought-prone areas which is the rainfall shadow zone in the watershed.

  • 4.

    The identification of positive and negative sensitive anomaly pixels shows that El Niño has a negative impact on the monsoon rainfall which can be identified from the presence of a large number of negative sensitive pixels in post-monsoon period (JAS and OND) during El Niño events and a large number of negative sensitive pixels are recognized in post-monsoon period (JAS and OND) during La Niña events.

  • 5.

    The negative IOD events have a negative impact during JFM and AMJ seasons, and the rainfall shadow zone is also affected negatively during JAS of positive IOD events.

  • 6.

    The cluster map and outliers of the monthly NDVI anomalies are identified using LISA analysis in Geo-da. The results of the LISA analysis also show that the El Niño and La Niña events affect the vegetation in the watershed. During El Niño events, the micro watersheds in the eastern region show lower anomaly clusters and the western region shows high anomaly clusters. The micro watersheds in the central and eastern regions during La Niña events shows high anomaly clusters and the western region shows low anomaly clusters. This shows that the central and eastern region which is the draught prone areas is predominantly affected due to the ENSO phases.

  • 7.

    According to the LISA analysis, the rainfall shadow zone in the study area has a cluster of negative sensitive pixels even in the monsoon and post-monsoon periods except for negative IOD events.

The limitation of the study is that it focuses only on the response of vegetation to ENSO and IOD events and does not consider other meteorological and local influencing factors that may affect vegetation dynamics. As a future scope of the study, the analysis conducted in the present study can also be performed by using Enhanced Vegetation Index. The analysis can also be performed by dividing the study area into multiple LULC classes. However, the study recommends a novel method that analyzes the impact of ENSO and IOD events to identify vulnerable regions which helps in the effective planning and management of water in agricultural basins. The methodology proposed in this study has been applied to the upper Bhima sub-basin, although it can be applied to any other basin worldwide.

We thank the anonymous editors and reviewers for suggestions on the manuscript. This research received no specific grant from any funding agency in the public, commercial or not-for-profit sectors.

All relevant data are included in the paper or its Supplementary Information.

The authors declare there is no conflict.

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