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ISSN 0252-1075 Contribution from IITM Research Report No. RR-147 ESSO/IITM/MM/SR/01(2020)/199 Initiative to Develop a Forecasting System for Wind Energy over a complex terrain in India using Weather Research and Forecasting (WRF) Model Radhika Kanase 1 , Greeshma Mohan 1 , Madhuparna Halder 2 , Medha Deshpande 1 and P. Mukhopadhyay 1 Indian Institute of Tropical Meteorology (IITM) Ministry of Earth Sciences (MoES) PUNE, INDIA http://www.tropmet.res.in/ 0 100 200 300 400 0 2 4 6 8 10 12 14 T1 T16 T34 Observed power curve for the site over Maharashtra State in India. Wind Speed (m/s) Frequency distribution of observed wind speed (m/s) for the month of April 2015.

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ISSN 0252-1075 Contribution from IITM

Research Report No. RR-147 ESSO/IITM/MM/SR/01(2020)/199

Initiative to Develop a Forecasting System for Wind Energy over a complex terrain in India using Weather Research and Forecasting (WRF) Model

Radhika Kanase1, Greeshma Mohan1, Madhuparna Halder2, Medha Deshpande1 and P. Mukhopadhyay1

Indian Institute of Tropical Meteorology (IITM) Ministry of Earth Sciences (MoES)

PUNE, INDIA http://www.tropmet.res.in/

0

100

200

300

400

0 2 4 6 8 10 12 14

T1T16T34

Observed power curve for the site over Maharashtra State in India.

Wind Speed (m/s) Frequency distribution of observed wind speed (m/s) for the month of April 2015.

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ISSN 0252-1075 Contribution from IITM

Research Report No. RR-147 ESSO/IITM/MM /SR/01(2020)/199

Initiative to Develop a Forecasting System for Wind Energy over a complex terrain in India using Weather Research and Forecasting (WRF) Model

Radhika Kanase1, Greeshma Mohan1, Madhuparna Halder2,

Medha Deshpande1 and P. Mukhopadhyay1

1Indian Institute of Tropical Meteorology, Ministry of Earth Sciences, Pune-411008

2K. Banerjee Centre for Atmospheric and Oceanic Studies, University of Allahabad, Allahabad

*Corresponding Address:

Dr. P. Mukhopadhyay Indian Institute of Tropical Meteorology, Dr. Homi Bhabha Road, Pashan, Pune – 411008, India. E-mail: [email protected] Phone: +91-(0)20-25904221

Indian Institute of Tropical Meteorology (IITM) Ministry of Earth Sciences (MoES)

PUNE, INDIA http://www.tropmet.res.in/

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DOCUMENT CONTROL SHEET -------------------------------------------------------------------------------------------------------------------------------------

Ministry of Earth Sciences (MoES) Indian Institute of Tropical Meteorology (IITM)

ESSO Document Number

ESSO/IITM/SERP/SR/01(2020)/199

Title of the Report

Initiative to Develop a Forecasting System for Wind Energy over a complex terrain in India using Weather Research and Forecasting (WRF) Model Authors Radhika Kanase1, Greeshma Mohan1, Madhuparna Halder2, Medha Deshpande1 and P. Mukhopadhyay1

Type of Document Scientific Report Number of pages and figures 51, 17 Number of references 18 Keywords WRF, day ahead wind forecast, linear bias correction Security classification Open Distribution Unrestricted Date of Publication May 2020 Abstract

The increasing demand for energy and rapidly decreasing conventional fossil fuels are the main

drivers for the increasing interest in renewable energy resources (RES) especially Wind. Although

the demand for accurate solar and wind forecasting is increasing, there is still a huge gap in the

indigenous development as per the requirement. Keeping this in background, the objective of the

present study is to develop a reliable day-ahead (~ 48 hrs lead) forecasting system for wind energy

over specific locations. With the help of a cloud-resolving model, various science-based sensitivity

experiments are conducted. The correlation coefficient (r) between model and observation is

increased from 0.3 to 0.7 with these experiments. After implementing the bias correction method,

r is further increased to 0.95. This study highlights some of the forecast generation experiments

and evaluation of wind power forecast.

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Summary

With rapid decrease in the conventional fossil fuels, there is increasing interest in the renewable

energy resources (RES) especially wind. Although the demand for accurate wind forecasting is

increasing, there is still a huge gap in the indigenous development as per the requirement. In the

present study, a cloud resolving model i.e. WRF model is used for generating a day-ahead (~48hrs)

forecast of wind. With default configuration of different physical parameterizations, WRF model is

run for whole month of April-2015. With every day’s initial condition, model is run for 48hrs with

4 domains having resolution as 27-,9-,3- and 1km. Different verification metrics are calculated and

it is found that the correlation coefficient (r) of 0.3 is achieved with the default configuration. To

improve the model performance further, different sensitivity experiments such as PBL sensitivity,

LU/LC sensitivity experiments as well as model domain sensitivity experiments are conducted.

With the best model configuration obtained from different sensitivity experiments, r is increased

to 0.7. With the implementation of new linear bias correction method, r is reached up to 0.95. The

percentage error for bias corrected wind and power is hardly crossing 0.5% for the first 24 hours

which is a greater achievement. The future developmental work is progressing for generating high-

resolution forecasts as well as for improving the wind forecast.

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Contents

1. Introduction: ................................................................................................................................................. 1

2. Methodology: ............................................................................................................................................... 4

2.1 Model Configuration and Physical Options: .............................................................................. 4

2.2 Site Details: ................................................................................................................................ 4

2.3 Model Validation:....................................................................................................................... 5

2.3.1 Forecast Error (Bias) : ......................................................................................................... 5

2.3.2 Mean Absolute Error (MAE), and Root Mean Square Error (RMSE) : .............................. 5

2.3.3 Skill Scores: ......................................................................................................................... 6

2.3.4 Correlation Coefficient: ....................................................................................................... 7

3. Results and Discussions: ............................................................................................................................ 8

3.1 Preliminary Experiments and Results: ....................................................................................... 8

3.2 Sensitivity Studies: ................................................................................................................... 11

3.2.1 Model Initialization and Domain Sensitivity: .................................................................... 12

3.2.2 PBL sensitivity: ................................................................................................................. 13

3.2.3 Landuse and Land Cover (LU/LC) sensitivity: ................................................................. 13

3.2.4 Linear Bias Correction Method: ........................................................................................ 14

4. Conclusions: ............................................................................................................................................... 15

Acknowledgements: ...................................................................................................................................... 16

References: ..................................................................................................................................................... 16

List of Tables: ................................................................................................................................................. 19

Tables: ............................................................................................................................................................. 20

List of Figures: ............................................................................................................................................... 26

Figures: ............................................................................................................................................................ 28

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1. Introduction:

Electricity consumption increased during the last decade with a compound annual growth

rate (CAGR) of 7.39% (ENERGY STATISTICS 2019). Out of the total consumption of electricity

in 2017-18, industry sector accounted for the largest share (41.48%), followed by domestic

(24.20%), agriculture (18.08%) and commercial sectors (8.51%). This rapid increase in energy

demand has placed enormous pressure on its resources. The decreasing conventional fossil fuels and

increasing pollution due to the use of more energy, are the main drivers responsible for the

increasing interest in renewable energy resources (RES). Wind -, Hydro-, Biomass -, Solar Energy

are some of the renewable energy sources. Out of these RES, wind energy is considered to be one of

the attractive solutions for the power generation due to its lowest cost. In India, after solar power

(68%), wind energy (28%) has a higher potential for renewable power (Figure 1a). As shown in

figure 1b, Rajasthan (15 %) has a higher potential for renewable power followed by Gujarat (11%),

Maharashtra (10%), and Jammu & Kashmir (10%). The potential for wind power is higher in

Gujarat, followed by Karnataka, Maharashtra, Andhra Pradesh, and Tamil Nadu. The detailed state-

wise distribution of renewable power from each individual source is summarized in Table 1. As the

wind is inherently variable, wind power is also a fluctuating source of energy. Short-term forecasts

from 1hr up to 72 hrs are useful in power system planning. Medium Range forecasts from 3 days to

7 days are needed for maintaining the wind farms and energy storage operations. Accurate wind

power forecasting reduces the risk of uncertainty and allows for better grid planning and integration

of wind into power systems.

The forecasting models for wind power are of two types. The first type of model is based on

an analysis of historical time series of wind. These models use the statistical approach to forecast

mean hourly wind speed or to directly forecast power production. These types of models provide

good results in most of the cases such as estimation of mean monthly or even higher temporal scale

(quarterly, annual) wind speed. However in short-term scales (mean daily or hourly or even smaller

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2

wind speed forecasts), these models fail as atmospheric dynamics become dominant and more

important. Thus, the second type of model becomes essential for shorter time scales (daily, hourly

or even smaller). The second group uses forecasted values from a numerical weather prediction

(NWP) model as an input. In this approach, the use of a variable (called as an explanatory variable)

which is derived from a meteorological model is done for predicting the wind N-steps ahead. More

details of the wind power forecasting methods can be found in Foley et al 2012.

India is advancing towards the achievement of maximum green energy, which reflects in the

present position of the nation in power generation from renewable energy resources. Based on

power production during Jan-Dec 2018, in terms of wind energy, India is at 4th position in the world

with 7% of the global wind power (Figure 2a). The fiscal year cumulative capacity from 2005 to

2018 is shown in Figure 2b. There is a gradual increase in the cumulative capacity from 2005 and in

2018 India reached up to a cumulative capacity of - 36625 MW. Also India targets 175 GW from

renewable energy in which 60 GW is planned to be achieved from wind (RENEWABLES 2016

GLOBAL STATUS REPORT) by 2022. So it is necessary to develop a system that can predict the

wind speed for a site and which will be useful for efficient management of the electricity produced.

The forecasting of wind speed over a small area is a challenging task since the wind speed and

direction are highly random and uncontrollable. The wind over a particular location is dependent on

the local weather, obstacles such as trees, buildings, etc. and topology. Thus the performance of the

model is closely dependent on how well these factors are represented in the numerical model.

Various studies (Cardoso et al., 2012; Heikkila et al., 2011; Nachamkin and Hodur 2000;

etc) have shown that the model simulation can be improved over complex terrain by increasing the

resolution of the model. According to Carvalho et al. (2012) the model results can be improved by

increasing horizontal and vertical grid resolution through better representation of small scale

meteorological processes. He also emphasizes that this may not be true always because of the

uncertainties in the performance of the various physical parameterizations and their responses to

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grid resolution. Moreover, some of the assumptions used in these physical parameterization

schemes may result in an erroneous analysis (Awan et al., 2011). There can be other sources of

errors in the numerical model such as errors from different numerical solvers, domain sizes, site

location, initial and boundary conditions, grid resolution, terrain and vegetation characteristics etc.

(Awan et al. 2011). The representation of the terrain and vegetation characteristics are very

important since these features modify the surface fluxes and radiation balance which further

influences the local meteorology.

From the study on the impact of model resolution, initial conditions and boundary-layer set-

up on the sensitivity of nocturnal low-level jets and near-surface winds over the Sahel; Schepanski

et al. (2015) have shown that the choice of initial and boundary conditions have a greater impact on

NWP simulations than model grid resolution. Also, the physical processes have to be represented

well in the model through a better combination of physics parameterizations. In simulating low-

level winds PBL parameterization is having a crucial role. Carvalho et al. (2012) demonstrated that

it is important to determine the most appropriate scheme to simulate wind for an area. Several

studies have been found on the evaluation of parameterization schemes for simulating low-level

winds by using WRF (e.g. Carvalho et al. 2014; Carvalho et al. 2012; Balzarini et al. 2014; Hu et al.

2013). Krieger et al. (2009) have shown that the schemes are site-specific.

The present study concentrates on setting up a regional mesoscale model for short term (day

ahead: 48 h) prediction of wind at hub level (90 m). Thus, the main objectives of this study are-

1. To develop a short term wind forecasting NWP system for the energy management purpose

2. To check the sensitivity of the model in predicting wind by - using different initial conditions,

increased horizontal resolution, using different PBL parameterization schemes, and changing land

use/land cover (LU/LC) along with different model vertical resolution.

3. By adapting the best model configurations, study the model predictability for high and low wind

conditions during December 2016.

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4. Use of linear bias correction method to further reduce the error in a day-ahead wind forecast.

2. Methodology:

2.1 Model Configuration and Physical Options:

WRF version 3.7.1 has been used to conduct all the experiments in the present study. It has

the capability to run the global simulations at the spatial resolution of several kilometres and it can

also be used for weather simulations at a few hundred meters. Skamarock et al (2008) describe the

various physical parameterization schemes available for cumulus, microphysics, radiation and

planetary boundary layer schemes including surface Layer scheme (SL) and the land Surface

Models (LSM). Certain assumptions used in the physical parameterization schemes and their non-

linear interaction with the dynamical core may result in erroneous analysis (Awan et al 2011).

Besides these, there are other sources of errors in numerical models such as initial and boundary

conditions, domain sizes, site location, both horizontal and vertical grid resolution, terrain &

vegetation type etc. Topography will also affect the model performance by influencing the surface

heat flux and radiation reflected from the ground which in turn affects the wind speed and direction

significantly.

2.2 Site Details:

In the present study, we have chosen a site ‘Agaswadi’ which is located in the Maharashtra

state of India. Figure 3a shows the location of all 33 turbines (dots represent the number of

windmills) along with the terrain height (shaded) over the topographically complex region of

Agaswadi. This site is situated over hilly terrain with elevations ranging between 700 and 900 m

above mean sea level. Here the numbers of wind turbines are from T1-T9 and T16 to T39 (each

wind turbine separated by ~ 200m from each other). Hereafter, we use the same naming convention

for the wind turbines. All these wind mills are located at around 90m height above the surface and

thus observations of wind speed, wind direction and temperature are available at only 90m height.

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In this paper, the results are discussed at T1, T16, T34 wind turbines which are marked in yellow

circles in Figure 3a.

2.3 Model Validation:

Verification/Validation is the process of comparing the forecast to the relevant observations. It

measures the quality of the forecast and also tells about the goodness of the forecast. Thus the

forecast from any model should be verified with the observations due to inherent uncertainty in the

wind power forecasting. The verification is also important for identifying and correcting the model

flaws and deciding further strategies for forecast improvement. Forecast verification can be

evaluated by using a small number of sample statistical metrics listed below.

2.3.1 Forecast Error (Bias):

Bias is defined as the difference between the forecast and the actual observations at any

point in time. This metric is useful in estimating the instantaneous performance. Bias signifies if the

method overestimates or underestimates the forecast variable

2.3.2 Mean Absolute Error (MAE), and Root Mean Square Error (RMSE):

These two metrics are commonly used to evaluate forecast performance for a time series

with n elements The MAE is obtained by taking the absolute value of all bias values and then taking

the mean of them. It gives the average magnitude of the errors over an entire dataset without

cancelling the effect of positive and negative errors, which occurs with a simple mean bias metric.

But the error directionality i.e. over-prediction or under-prediction which can be important when

large amounts of wind are integrated into the grid system, is lost in MAE.

RMSE can be a preferred metric for evaluating wind forecast errors. Due to the squared

nature of forecast errors, RMSE places more weight on the large error terms. But again this metric

comes at the expense of specifying error directionality.

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Each of the above metrics has its place in evaluating errors in wind power prediction. It is

well known that there is no single metric that can be used to completely describe forecast

performance. Thus, a combination of metrics is needed and each metric has its own importance.

2.3.3 Verification Metric:

For every forecast of wind and power, the number of correctly forecasted events(A), events

not correctly forecasted(B), events forecasted but not observed(C) and events not forecasted and

also not observed (D) is computed with respect to the contingency table 2. Based on these, five

verification metrics viz, Probability of detection (POD), False Alarm Ratio (FAR), Critical Success

Index (CSI), True Skill Statistics (TSS) and Hiedke Skill Score (HSS) are computed as shown in

Table 3.

POD is the ratio of events that are correctly forecasted to the total number of events (A+B).

FAR is the ratio of false alarm (C) to the total number of predicted events (A+C). CSI is the ratio of

the number of correctly forecasted events to the sum of the total number of events and false alarm

(A+B+C). Therefore CSI varies directly with the number of correct event forecasts and varies

inversely with both the number of incorrect event forecasts (false alarm) and the number of missed

events. However, CSI does not take into account the number of correct non-event forecasts (D). CSI

is a biased score that is dependent upon the frequency of the forecast events (Scheafer 1990). TSS is

the difference between the probability of detection of an event and the probability of detection of a

false event. The highest and lowest possible TSS score is 1 and -1. HSS is expressed as the ratio of

categorically correct forecast (A+D) above the expected number of the correct forecast by chance to

the total number of events also above the expected number of the correct forecast by chance. HSS is

defined such that a perfect set of forecast (all categorical hits) will show a score 1, a set of random

forecasts will be 0 and that having lesser hits compared to the forecast by chance will have a

negative score. Although CSI does not consider the number of correct non-event forecast, TSS and

HSS do consider that. But the limitation of TSS and HSS is that, if the number of correct forecasts

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(A) and the number of correct non-event forecasts (D) are interchanged the number of misses (B)

and the number of false alarms (C) is interchanged between each other, scores remain unchanged

whereas CSI score will change.

Due to this inherent advantage and disadvantage, Doswell et al. (1990) concluded that no

single measure of forecasting success can give a complete picture and it is desirable to include in

addition to HSS, the CSI, POD and FAR in any summary of forecasting verification. The

verification metrics computation is based on two different threshold limits such as 25% and 50%

chances of predicting the correct forecast (TH=25 and TH= 50) i.e. with different probability of

occurrence of the event. The results for all threshold values are presented in this paper.

2.3.4 Correlation Coefficient:

In addition to all the above skill scores, we have also computed the correlation coefficient

(r) between the actual and forecasted wind and power for day 1, day 2 and day 3 forecast periods. It

is the square root of the coefficient of determination, which provides an idea of how well a

predicted value of a time series matches the observed value. The formula for r is given by-

−=

−=

−−=

2

2

),(

)(

)(

))((

yyS

xxS

SS

yyxxR

iyy

ixx

yyxx

ii

yx

The x values represent the forecast data and the y-values represent the observed data. Correlation

coefficient r is commonly used in the regression analysis to determine the linear dependence of one

variable on another e.g. here the dependence of forecasted wind & power output on the observed

data. The correlation coefficient ranges between -1 to 1. r =1 means that with every positive

increase of 1 in one variable, there is a positive increase of 1 in the other variable and vice versa. for

r = -1. r =0 means that for every increase there isn’t a positive or negative increase and thus these

two variables aren’t related.

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3. Results and Discussions:

3.1 Preliminary Experiments and Results:

To check the model fidelity without any optimization, one-month simulation (Apr-2015)

with a day ahead forecast is carried out with the default physical parameterization options in the

WRF model. The model’s initial and boundary conditions are provided from GFS analysis data of

0.50 X 0.50. Here the month of April is chosen since the energy demands in India generally go high

in this month as summer season peaks in April and May. The WRF domain configuration remains

the same as shown in Figure 3b. The rest of the model configuration and experimental design is

summarized in Table 1. Here we have taken three representatives (T1, T16 & T34) for all 33 wind

mills and results for these three windmills will be discussed in detail.

The frequency distribution of observed wind speed (m s-1) for the month of April 2015 is

plotted in Figure 4a. It shows that maximum times the winds of magnitude 5-6 m s-1 are dominant

in the given region, whereas the frequency of higher winds is very low compared to the lower wind

speed. The relation between wind speed and power generated is given by

𝑃 = 0.5 ∗ 𝜌𝐴𝑣3 …(1)

Where 𝜌 is air density (kgm-3), A is the sweap area (πr2) in m2, v is the wind speed in ms-1

and P is the power generated in MW. From equation 1, it is clear that small variation in wind speed

will have a large variation in power generated.

The observed power curve for the present site also shows that the cut-off wind magnitude is

13ms-1 whereas the cut-in wind speed is 3 ms-1 (Figure 4b). The diurnal variation of wind as

observed in Turbine 1, 16 and 34 are plotted in Figure 4c and the model simulated wind is

compared. Even though there is an underestimation of the peak magnitude of wind by the model, it

reasonably captures the diurnal cycle in all the turbine's location. This further shows the model

fidelity in capturing the diurnal scale wind at wind turbine height.

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With the help of the wind-rose diagram, the observed wind speed and direction for the

month of April 2015 are shown in Figure 5 for wind turbines T1, T16 and T34 respectively. For T1,

the most prominent wind direction is North-East followed by the westerly with a wind speed of 6-

10 ms-1 in the same direction (Figure 5a). The wind speed of 6 or more than 6 ms-1 is more useful

for power generation. At this location, almost 19.3% of winds are calm during the whole month of

April 2015. For wind turbine T16, the strong winds of magnitude 6-8 ms-1 are frequently observed

almost in all directions except SE sectors. The turbine T16 is located over the terrain of 820-840 m

above MSL, where the prominent wind direction is West South-West and Westerly (Figure 5b) with

the strongest winds (10-12 ms-1) present in these directions. The occurrence of calm wind is around

11.3% at this location. The most productive winds (6-12 ms-1) are from West and West South-West,

whereas very weak winds are observed from the South and South South-East direction. T34 wind

turbine is located over the same terrain height as of T1 but in the eastern side of the orientation of

the western ghat. The prominent wind direction remains as easterlies or westerlies. The more

frequent occurrence of the strongest wind of speed 10 - 12 ms-1 is observed from West compared to

the East direction. In the case of T34, most of the winds are present in the North- East sector as well

as in West direction (Figure 5c). For the rest of the sectors, the winds higher than 6 ms-1 are less

frequently observed. Among these three turbines, T34 is having high occurrences of calm wind (~

16.9 %). This analysis indicates that even though the windmills are 200 m apart from each other,

there is a high fluctuation in wind speed and direction among the wind mills due to the complexity

of the terrain and thus different wind mills have different dominant wind directions.

Each wind power plant has its own optimized power curve. For Agaswadi, the observed

power curve is interpolated with respect to the observed wind. These interpolated power values are

used for the conversion of forecasted wind to forecasted power. We have calculated and plotted the

model generated winds (line) and power (bar) along with observations for all 33 wind turbines for

the month of April. One such plot for 1 Apr 2015 for T1 turbines over Agaswadi location is

presented in Figure 6. For day 1 and day 2, the line plots are almost overlapping with each other.

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The differences between the observed and forecasted wind continuously increase with time and

have a noticeable difference after ~40hrs and it continuously increases thereafter. Thus for

calculating different skill scores, we considered up to three-day forecasts and for each day

verification metrics are computed. The wind and power have a non-linear relation which is reflected

in the bar plots. The small changes in the wind forecast lead to large errors in the power forecast.

The wind and power forecast remains unchanged for all wind turbines as well as for each day of

April month (hence only one figure is shown here).

The different verification metrics for wind (Figure 7a-b) and power (Figure 7c-d) are

calculated for the whole month of April 2015 for all 33 wind turbines. The Figures are presented for

T1 wind turbines. For day 1, the probability of detecting the wind speed (Figure 7a) accurately is

almost one at threshold 25, which reduces further to 0.80 with an increased threshold limit of 50.

For day 2 and Day 3 Forecast, POD almost remains the same as day 1. With different threshold

values, the False Alarm Ratio (FAR) is almost 50% and remains the same for all three day forecast.

The CSI is approximately 0.5 for both thresholds and it decreases with time. The TSS and HSS for

wind forecast are on the negative side, which means that the false events are more compared to the

correct forecast events. With increased threshold, the number of false events increases and

continues to increase with time. Irrespective of the threshold limit, the correlation coefficient

remains unchanged ( r = 0.3). The value of r decreases with time.

For power forecasting (Figure 7b), the POD has an approximate score on all the days with

threshold 25, whereas for threshold 50, POD reduces remarkably compared with the wind. The

FAR has also increased for all forecast days compared with the wind, which further resulted in

decreased CSI score from 0.55 to 0.3 with TH=25 and from 0.4 to 0.2 with TH=50. The TSS and

HSS become positive for threshold 25, whereas both scores are negative with TH=50. The

correlation coefficient remains the same for wind and power forecast for day 1 and decreases

continuously as time progresses.

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The RMSE and Mean error variation for wind and power are plotted in Figure 7c and Figure

7d respectively. For Day 1, RMSE is 2.5 which slightly increases for day 2 and Day3 forecast. The

mean error variation also shows very little variation from 0.2 to 0.5 for all forecast days. In the case

of power forecast (Figure 7d), the RMSE varies from 260 to 290 but the mean error remains zero

for day 1 and day 2. All these results are shown for T1. Similarly, for all wind turbines, the skill

score remains broadly the same. So instead of considering individual wind turbines and evaluating

the skill score for each turbine, we have taken the area [ 74.6 -74.635 °E and 17.51 - 17.57 °N]

which includes all wind turbine and then calculated each skill score (Figure 8). All wind turbines

have improved skill scores for wind forecasts as well as power forecasts when compared with each

individual skill score for each turbine (Figure 7).The RMSE and Mean error variation for wind

forecast show that for day 1 and day 2 skill is better than day 3 forecast, The range of both the skill

scores is also found to be reduced than an individual wind turbine. Similarly for power forecast, the

mean error continuously increases when compared with the mean error of wind forecast.

3.2 Sensitivity Studies:

Prediction of wind over topographically complex terrain is a great challenge. With the default

model configuration, the correlation coefficient is 0.3 and other skill scores are also very less. To

further improve the model performance, different sensitivity experiments are carried out. These

experiments are summarized in Table 5 and the sequence of these experiments is explained in

Figure 9. Since the power generation rapidly increases from 8 ms-1 to 12 ms-1 ( Figure 4b), the

days are classified as high (low) wind days if the wind speed is more (less) than 10 ms-1 . Based on

the availability of the observations during the month of December 2016, three high wind, as well as

three low wind events, are selected for the study. They are :

High Wind Days Low Wind Days

1. 06 Dec 2016

2. 10 Dec 2016

3. 12 Dec 2016

1. 22 Dec 2016

2. 24 Dec 2016

3. 26 Dec 2016

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Figures 10 and figure 11 show observed and model-predicted wind speed for two low wind

(Figure 10) and two high wind (Figure 11) conditions. It is found that the peak wind speed during

high wind conditions (Figure 10a, b) is not captured by the model with the default configuration

used in Section 3.1. The low wind conditions are well predicted by the model whereas the low wind

conditions are well predicted by the model (Figure 11 a, b). Thus, the model finds it difficult to

simulate the high wind speed conditions. So for further improvement in the wind prediction,

different sensitivity experiments are conducted and results for high wind conditions of 06 Dec 2016

are presented here.

3.2.1 Model Initialization and Domain Sensitivity:

Initial and Boundary conditions to WRF model are provided from two different data sets (1)

National Centres for Environmental Prediction (NCEP) Global Forecast System (GFS) forecasts

with a horizontal resolution of 0.25° × 0.25° and (2) GFST1534 model with 0.125° × 0.125°

horizontal resolution at 0000 UTC 06 Dec 2016. The sensitivity to the horizontal resolution is

verified by configuring the model with 4 domains having resolutions 27-, 9-, 3- and 1 km and with

5 domains having resolutions 27-, 9-, 3-, 1-, and 0.333 km (Figure 12). It is noticed that the

simulated wind speed between GFST1534_4Dom and NCEP_GFS_4Dom are almost overlapping

throughout the simulation with very small variations among themselves. But GFST1534, being the

high resolution initial conditions it is decided to initialize the model with GFST1534 hereafter. We

have also done some experiments with ICs starting from 00UTC and 12 UTC of the respective day

(Figure not shown), but no remarkable improvement is seen in the results. When the model

resolution is increased from 1 km to 0.333 km (GFST1534_5Dom), the results are almost

overlapping with the 4th domain results with some criss-cross are seen in 5th domain winds. The

higher horizontal resolution requires longer computation time as well as more memory.

Improvements in the winds are also not remarkable; hence the model setup is constrained with 4

domains with innermost domain resolution of 1 km. Thus, it is noted that the model initialized with

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GFST1534 at 0000 UTC with 4 domains can be a better domain setup for the representation of wind

speed over Agaswadi.

3.2.2 PBL sensitivity:

Different PBL sensitivity experiments are conducted for a high wind case on 06 Dec 2016

(Figure 13). The PBL schemes used for these experiments are - Bougeault-Lacarrére (BouLac),

Mellor-Yamada-Nakanishi and Niino Level 3 (MYNN3), Quasi-Normal Scale Elimination (QNSE),

Yonsei University (YSU), Mellor-Yamada-Janjic (MYJ), Total Energy – Mass Flux (TEMF), UW

(Bretherton and Park) Scheme (UW), Asymmetric Convective Model (ACM2), Shin Hong and

MRF. It is found that none of the experiments can capture the high wind speed conditions. All PBL

schemes could capture the low wind speed conditions very well (Figure not shown). As YSU is

following the mean wind speed, for further experiments, YSU as PBL is used.

3.2.3 Landuse and Land Cover (LU/LC) sensitivity:

Surface winds are highly dependent on PBL processes. The PBL processes are closely related to

the land surface features such as vegetation, soil types, soil moisture, land-sea contrast, inland water

bodies, snow cover etc. So the representation of LULC has a major role in modulating the PBL

processes. Three LULC data sets are used in the present study. They are: 1) USGS: This dataset is

developed by the United States Geological Survey's (USGS) National Center for Earth Resources

Observation and Science (EROS), the University of Nebraska-Lincoln (UNL) and the Joint

Research Centre of the European Commission. It has been derived from AVHRR satellite data

spanning April 1992 through March 1993 using a resolution of 1km (schicker, 2011; Serteletal,

2009) and it has 20 land use categories. 2) MODIS: This dataset has been derived from one year

Terra and Aqua data collected during 2001-2005. It includes 20 land use categories defined by the

International Geosphere Biosphere Programme (IGBP). 3) NRSC: This data set is modified by

replacing LULC over the Indian region of USGS data with AWiFS derived data and made

compatible to MM5 & WRF models. This dataset is being updated at an annual basis for the time

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period 2004-2005 to 2012-2013 (9 cycles). The LULC categories of these datasets are enlisted in

Table. 6. Further, these LULC has been used to study the sensitivity of the model to predict wind

speed for low wind (26 Dec 2016) days and high wind (06 Dec 2016) as shown in Figure 14a,b. The

LULC data with resolutions 10 min, 5 min, 2 min, and 30 s are used in domains 1, 2, 3, and 4

respectively. From Figure 14a it is clear that experiments with NRSC LU/LC are able to predict the

wind speed much better than MODIS and USGS. But for high wind conditions as shown in Figure

14b, MODIS, USGS, and NRSC go hand in hand and it's difficult to find the impact of LU/LC .

Simultaneously one more experiment of vertical resolution is carried out for all three LU/LC

datasets and results are shown in the same Figure 14. It is noticed that the increase in the model

vertical resolution of 31, 45 and 52 levels, doesn’t guarantee the improvement in the winds at 90 m

height. Careful examination of Figure 14 shows that when the atmosphere is represented in 45

vertical levels with 7 levels in the boundary layer and remaining above PBL, the observed and

predicted winds are very close to each other. This can be due to the PBL processes are well

represented in the experiments with the increased number of vertical levels. Thus, from all the

above sensitivity experiments as well as from CU and MP sensitivity (as mentioned in Table 5 but

not explained in the present report), GFST1534 as an initial condition, YSU as PBL, KF as

Cumulus, Morrison as Microphysics with 45 vertical levels and MODIS and NRSC as LU/LC is the

best combination we found which enhanced the correlation coefficient from 0.3 to 0.7.

3.2.4 Linear Bias Correction Method:

We have observed that with sensitivity experiments, there is a time lag/lead between the

observations and model predicted winds. There are different methods to correct the predicted winds

(Rangaraj et al. 2019; Sweeny et al. 2013). One such method i.e. Short term Bias Correction

(STBC) explained in Rangaraj et al. (2019) is modified and called linear bias correction (LBC).

The only difference between these two methods is the time window. In the Linear Bias Correction

method, it is assumed that today’s wind pattern is the same as yesterday’s wind. The time window

used in LBC is yesterday’s observations at t-1, t-2, and t-3 (where t is present time step) with each

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time step separated by 15-minute interval. Bias is calculated at these time steps with respect to

yesterday’s observations at the same time. The mean of the bias is either added or subtracted from

the model forecasted wind at time step ‘t’. This method is explained in Figure 15. The linear Bias

correction method can be used to correct the lead/lag in the model predicted winds. With the best

model configuration (we found with all the above experiments) along with NRSC, USGS and

MODIS LU/LC, we implemented a linear bias correction method as shown in Figure 16 for high

and low wind conditions. The results are very promising as the errors of lead/lag are removed and

the predicted wind follows the observed wind. Now, with the bias correction method the correlation

coefficient is increased from 0.7 to 0.9547, 0.9547 and 0.9554 in low wind case and 0.950, 0.9443,

0.9411 in high wind case for MODIS, NRSC and USGS respectively. Also, it is found that during

the model integration period, in both high and low wind cases mostly the error is below 15 % and

MODIS is having lesser error than NRSC and USGS.

The percentage error for power is shown in Figure 17. The remarkable improvement is seen

in bias-corrected winds which are not retained in power percentage error due to the non-linear

relation between wind and power. The non-bias corrected power shows higher error compared with

the bias-corrected power. The percentage error with bias correction hardly crossed 0.5 for the first

24 hours, whereas it is more than 1 for non-bias corrected power.

4. Conclusions:

In the present study, a new approach of numerical weather prediction of wind with a cloud-

resolving model is tested with different experiments such as PBL sensitivity; LU/LC sensitivity

experiments, as well as model domain sensitivity experiments, are conducted. The best model setup

is used for a few cases of high and low wind conditions and thus the approximate correlation

coefficient of 0.7 is achieved. It is also observed that the model faced difficulties in forecasting the

high wind conditions. To further improve the forecast, we have implemented a linear bias correction

method. With this method, for low as well as high wind conditions the correlation coefficient

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reached up to 0.95. The percentage error for power from newly bias-corrected winds is hardly

crossing 0.5% for the first 24 hours which is a greater achievement.

The future developmental work is progressing for generating high-resolution forecasts as

well as for improving the wind forecast.

Acknowledgments:

IITM is an autonomous research institution, fully supported by the Ministry of Earth Sciences

(MoES), Govt. of India, New Delhi. The observational data is provided by TATA POWER under

the pilot project to test the model forecast fidelity for Wind power forecasting. We acknowledge

the help of Mr. Rajiv B. Samant, Mr. Manish S Gupte, Mr. Mahesh D Paranjpe and Mr. Mahadev

Udachan from TATA Power in the project. The WRF model is run on the ‘Aaditya’ MoES high

power computing system located at IITM, Pune. The authors are thankful to Dr. M. Rajeevan for

initiating the work and constant guidance throughout the period. Prof. Toumi Ralf, Reading

University, UK and Prof D. Niyogi, Perdue University, are thankfully acknowledged for their

suggestions. All authors are grateful to the Director, IITM for the encouragement and support.

Authors are also thankful to the anonymous reviewers and the members of IITM Library

committee for their insightful comments and suggestions that helped to improve the report.

References:

1. Awan N K, Gobiet A and Truhetz H (2011) Parameterization induced error-characteristics

of MM5 and WRF operated in climate mode over the Alpine Region: an ensemble based

analysis. J. Clim. 24, pp. 3107-3123.

2. Balzarini A, Angelini F, Ferrero L, Moscatelli M et al (2014) Comparing WRF PBL

schemes with experimental data over Northern Italy. Air Pollution Modeling and its

Application XXIII, Springer , pp. 545-549

3. Cardoso R M, Soares P M M, Miranda P M A and Belo-Pereira M (2012) WRF high

resolution simulation of Iberian mean and extreme precipitation climate. Int. J. Climatol.,

33, pp. 2591-2608.

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17

4. Carvalho D, Rocha A, Moncho G-G and Santos C. (2012) A sensitivity study of the WRF

model in wind simulation for an area of high wind energy. Environ. Model. Softw., 33, pp.

23-34.

5. Carvalho D, Rocha A, Moncho G-G and Santos C. (2014) Sensitivity of the WRF model

wind simulation and wind energy production estimates to planetary boundary layer

parameterizations for onshore and offshore areas in the Iberian Peninsula. Appl. Energy,

135, pp. 234-246.

6. Doswell C A III, Robert D-J and Keller D L (1990) On summary of skill in rare event

forecasting based on contingency tables. Wea. and Forecast, 5, pp. 576-585.

7. Foley A M, Leahy P G, Marvuglia A and McKeogh E J (2012) Current methods and

advances in forecasting of wind power generation. Renewable Energy, 37, pp. 1-8.

8. Heikkila U, Sandvik A and Sorterberg A (2011) Dynamical downscaling or ERA-40 in

complex terrain using WRF regional climate model. Clim. Dyn., 37, pp. 1551-1564.

9. Hu X M, Klein P M and Xue M (2013) Evaluation of the updated YSU planetary boundary

layer scheme within WRF for wind resource and air quality assessments. J. Geophys. Res.

Atmos., 118, pp. 10490-10505.

10. Krieger J R, Zhang J, Atkinson D E, Shulski M D and Zhang X (2009) Sensitivity of WRF

model forecasts to different physical parameterizations in the beaufort sea region. Eighth

Conference on Coastal Atmospheric and Oceanic Prediction and Processes, P1.2.

11. Nachamkin J E and Hodur R M (2008) Verification of short-term forecasts from the Navy

COAMPS over the Mediterranean. 15 th Conference on Statistics and Probability in the

Atmospheric Sciences, Asheville, North Carolina, 8-11 May 2008.

12. Rangaraj A G, Srinath Y, Boopathi K, Sheelarani N, Kumar S and Balaraman K (2019)

Validation and bias correction techniques to improve Numerical Weather Prediction wind

speed data 2nd Int'l Conference on Large-Scale Grid Integration of Renewable Energy in

India| New Delhi, India 4-6 Sep 2019.

13. RENEWABLES 2019 GLOBAL STATUS REPORT, (2019) downloaded from

https://www.ren21.net/wp-content/uploads/2019/05/gsr_2019_full_report_en.pdf

14. Schaefer J T (1990) The Critical Success index as an Indicator of Warning Skill. Wea. and

Forecast., 5, pp. 570-575.

15. Schepanski K, Knippertz O, Fiedler S, Timouk F and Demarty J (2015) The sensitivity of

nocturnal low-level jets and near-surface winds over the Sahel to model resolution, initial

conditions and boundary-layer set-up. Q. J. R. Meteorol. Soc., 141, pp. 1442-1456

doi:10.1002/qj.2453

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16. Skamarock W C, Klemp J B, Dudhia J, Gill D O, Barker D M, Duda M G, Huang X Y,

Wang W and Powers J G (2008) A Description of the Advanced Research WRF Version 3.

NCAR Technical Note, NCAR/TN-475+STR. Mesoscale and Microscale Meteorology

Division, National Center for Atmospheric Research, Boulder.

17. Sweeney C P, Peter L and Nolan P (2013) Reducing errors of wind speed forecasts by an

optimal combination of post-processing methods. Meteorol. Appl., 20, 32-40.

18. Technical Report on IRS-P6 AWiFS Derived Gridded Land Use/Land Cover Data

Compatible to Mesoscale Models (MM5 and WRF) Over Indian Region downloaded from

https://bhuvan-

app3.nrsc.gov.in/data/download/tools/document/AWiFS_LULC4Mesoscale%20Modeling_ACSG_24

April2014.pdf

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List of Tables:

Table 1. Sourcewise and Statewise Estimated Potential of Renewable Power in India as on

31.03.2018.

Table 2 Contingency Table.

Table 3. Description of different Verification Metrics.

Table 4. WRF Model Configuration for April 2015 over ‘Agaswadi’ site.

Table 5. Different sensitivity Experiments conducted to increase the model performance over

Agaswadi (Maharashtra) Site (Bold letters indicate the final chosen configuration from

different experiments).

Table. 6. Different land use categories in USGS, MODIS, and NRSC (Based on the information

from Technical Report on IRS-P6 AWiFS Derived Gridded Land Use/Land Cover Data

Compatible to Mesoscale Models (MM5 and WRF) Over Indian Region).

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Tables:

Table 1. Sourcewise and Statewise Estimated Potential of Renewable Power in India as on

31.03.2018

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Table 2 Contingency Table.

Prediction

Event Predicted Event not Predicted

Observation

Event observed A

(Hits)

B

(Misses)

Event not observed C

(False Alarm)

D

(Non event Hits)

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Table 3. Description of different Verification Metrices.

Skill Score Code References Equation Limits

Probability of Detection POD Donaldson et al.(1975) POD=A/(A+B) 0 ≤ POD ≤ 1

False Alarm Ratio FAR Donaldson et al.(1975) FAR=C/(A+C) 0 ≤ FAR ≤ 1

Critical Success Index CSI Donaldson et al.(1975) CSI=A/(A+B+C) 0 ≤ CSI ≤ 1

True Skill Statistics TSS Hansen & Kuipers (1965) TSS=(A/(A+B))-(c/(C+D)) -1 ≤ TSS ≤ 1

Hiedke Skill Score HSS Brier & Allen (1952) HSS=(CF-E)/(N-E) -1 ≤ HSS ≤ 1

CF=Total No. of correct Forecasts=A+D

N=Total Number of events=A+B+C+D

A+C=Total number of forecast for the vent

A+B=Total number of observed events

C+D= Total number of observed non-event

B+D= Total number of forecast for the non-event

E=Expected number of correct forecast by chance= (A+C)(A+B)+ (C+D)(B+D)/N

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Table 4. WRF Model Configuration for April 2015 over ‘Agaswadi’ site.

Domains & Resolution 4 domains with 27km, 9km, 3km and 1km resolution

Initial Conditions GFS analysis data of 0.5o X 0.5o

Start time of Integration

Total Period of Integration

00UTC 1Apr 2015, 00UTC 2Apr2015,…., 00UTC

25Apr2015

5 days from each initial condition

Model Output At 30 min interval for inner domain of 1km

Cumulus Parameterization Grell-Freitas Ensemble Scheme

Microphysics Morrison Scheme

Planetary Boundary Layer Yonsei University (YSU) Scheme

Radiation Scheme RRTM for Long Wave and Dhudhia for Short Wave

Observed Data Used Wind and Temperature for Agaswadi provided by TATA

Power Ltd.

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Table 5. Different sensitivity Experiments conducted to increase the model performance over

Agaswadi (Maharashtra) Site (Bold letters indicate the final chosen configuration from different

experiments)

Initial Condition

Sensitivity

1. GFS Analysis (0. 50 X 0.50)

2. GFS Forecast (0.250 X 0.250)

3. GFST1534 Forecast (0.1250 X 0.1250)

Planetary Boundary Layer

Scheme

1. Yonsei University (YSU)

2. Mellor-Yamada-Janjic(MYJ)

3. Quasi-Normal Scale Elimination(QNSE)

4. Mellor-Yamada-Nakanishi &Niino Level 2.5

(MYNN2.5)

5. MYNN3 scheme

6. Bougeault-Lacarrere (BouLac )

7. University of Washington (UW) PBL Scheme

8. Total Energy Mass Flux(TEMF)

9. Shin Hong scale aware scheme

10. MRF

Microphysics Sensitivity 1. Morrison

2. Thompson

3. WDM6

Cumulus Sensitivity 1. Kain Fritsch(KF)

2. Betts-Miller-Janjic (BMJ)

3. Grell-Freitas Ensemble (GF)

No of vertical levels 1. 31

2. 45

3. 52

LU/LC data 1. USGS

2. MODIS

3. NRSC

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Table. 6. Different land use categories in USGS, MODIS, and NRSC (Based on the information from Technical

Report on IRS-P6 AWiFS Derived Gridded Land Use/Land Cover Data Compatible to Mesoscale Models

(MM5 and WRF) Over Indian Region)

Cate

gory USGS MODIS NRSC

1 Urban and Built-up Land Evergreen Needleleaf Forest

Settlement

2 Dryland Cropland and Pasture Evergreen Broadleaf Forest Kharif Crop only

3 Irrigated Cropland and Pasture Deciduous Needleleaf Forest

Rabi Crop/ Zaid/ double/ triple Crop

4 Mixed Dryland/ Irrigated

Cropland and Pasture Deciduous Broadleaf Forest Mixed Dryland/ Irrigated Cropland and Pasture

5 Cropland/ Grassland Mosaic Mixed Forests Current Fallow

6 Cropland/ Woodland Mosaic Closed Shrublands Cropland/ Woodland Mosaic

7 Grassland Open Shrublands Grassland

8 Shrubland Woody Savannas Scrub/ Deg.Forest/ Shrubland

9 Mixed Shrubland/ Grassland Savannas Mixed Shrubland/ Grassland

10 Savanna Grasslands Savanna

11 Deciduous Broadleaf Forest Permanent Wetlands Deciduous Forest

12 Deciduous Needleleaf Forest Croplands Deciduous Needle leaf Forest

13 Evergreen Broadleaf Urban and Built-Up Evergreen Forest

14 Evergreen Needleleaf Cropland/ Natural Vegetation Mosaic

Evergreen forest (Himalayan region)

15 Mixed Forest Snow and Ice Plantations/ orchards/ shifting cultivation

16 Water Bodies Barren or Sparsely Vegetated

Water bodies

17 Herbaceous Wetland Water Herbaceous Wetland

18 Wooden Wetland Wooded Tundra Littoral Swamp (Mangrove)

19 Barren or Sparsely Vegetated Mixed Tundra Other Wasteland/ Gullied/ Rann

20 Herbaceous Tundra Barren Tundra Herbaceous Tundra

21 Wooded Tundra Wooded Tundra

22 Mixed Tundra Mixed Tundra

23 Bare Ground Tundra Bare Ground Tundra

24 Snow or Ice Snow cover

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List of Figures:

Figure 1a) Source wise Estimated Potential of Renewable Power in India as on 31.03.2018 b)

Statewise Potential of Renewable Power in India as on 31.3.2018.

Figure 2 (a) Top 10 new installed capacity Jan-Dec 2018 (source: https://www.power-

technology.com/features/wind-energy-by-country/ (b) Fiscal year cumulative capacity in MW (

https://gwec.net/wp-content/uploads/2019/04/GWEC-Global-Wind-Report-2018.pdf ) )

Figure 3a. Terrain Height in meter (shaded) at Agaswadi (Maharashtra state) wind Farm site in

India. The dots represent the location of each wind turbine over the topographically complex site of

Agaswadi. The dotted lines represent the model grid at 1km and yellow circles show location of T1,

T16 and T34 wind mills.

Figure 3b. Domain of integration for WRF model. First Domain’s horizontal resolution is 27km,

Second domain 9km, 3rd domain 3km and innermost 4th domain 1km.

Figure 4a. Frequency distribution of observed wind speed (m/s) for the month of April 2015. The

blue colour is for wind turbine T1, Orange colour for T16 and Green colour is for T34.

Figure 4b. Observed power curve for the complex terrain site over Maharashtra State in India.

Figure 5. Wind rose diagram for the observed wind direction for wind turbines a) T1, b) T16 and c)

T34 for the month of April 2015. Shade represents the different bins of wind speed in m/s.

Figure 6 The wind speed (m/s) and power (KW) forecast from the model compared with the

observation for 1 Apr 2015 for wind turbine T1 over Agaswadi Region. The black line is observed

wind and pink line is forecasted wind in m/s. The green bars represent observed power and blue

bars as forecasted power in KW.

Figure 7 (a-c) Different skill scores for wind and power with varying threshold values and RMSE

and mean error variation (b-d) for wind turbine T1.

Figure 8 (a-d) Same as Figure 6 , but for all wind turbines for area averaged over 74.6 - 74.635 °E

and 17.51 - 17.57 °N .

Figure 9 Flow chart of different sensitivity experiment conducted for obtaining best model

configuration.

Figure 10 Comparison of high wind conditions on (a) 10 Dec 2016, (b) 12 Dec 2016 with observed

wind speed .

Figure 11 Same as Figure 10 but for low wind conditions on (c) 24 Dec 2016, (d) 26 Dec 2016 .

Figure 12 Comparison of simulated wind speed with different model grid resolutions

(GFST1534_4dom: innermost domain resolution is 1 km; GFST1534_5dom: innermost domain

resolution is 333.33 m) with 0000 UTC 06 Dec 2016 from GFST1534 and NCEP_GFS.

Figure 13 Sensitivity of the model to simulate wind speed with different PBL scheme.

Figure 14 Model vertical level & land use land cover sensitivity of the model to simulate wind

speed during (a) low wind condition and (b) high wind condition.

Figure 15. Flow chart explaining Linear Bias correction method for wind prediction.

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Figure 16 Comparison of wind speed simulated with different LULC data with observation (a) low

wind case and (b) high wind case without bias correction (solid lines) and with bias correction

(dashed lines).

Figure 17 Comparison of Percentage error (%) of power for low wind case without bias correction

(solid lines) and with bias correction (dashed lines).

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Figures:

Figure 1a) Source wise Estimated Potential of Renewable Power in India as on 31.03.2018 b) Statewise Potential of Renewable Power in India as on 31.3.2018.

Wind Power28.00%

Solar Power68.00%

Hydro Power1.76%

Biomass Power1.56%

Cogeneration bagasse0.44%Waste to energy0.24%

Other4.00%

Wind Power Solar Power Hydro Power

Biomass Power Cogeneration bagasse Waste to energy

15%

16%

11%

10%10%

8%

8%

7%5%3%3%2%2%

Statewise Potential of Renewable Power in India as on 31.3.2018Rajasthan

Others**GujaratMaharashtraJammu & KashmirAndhra PradeshKarnatakaMadhya PradeshTamil NaduHimachal PradeshOdishaUttar PradeshTelangana

Source : Ministry of New and Renewable Energy

a) b)

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Figure 2 (a) Top 10 new installed capacity Jan-Dec 2018 (source: https://www.power-technology.com/features/wind-energy-by-country/ (b) Fiscal year cumulative

capacity in MW ( https://gwec.net/wp-content/uploads/2019/04/GWEC-Global-Wind-Report-2018.pdf )

43%

19%

12%

7%

5%

4%3%

3%2%2% China

USA

Germany

india

spain

UK

France

Brazil

Canada

Italy

0

5000

10000

15000

20000

25000

30000

35000

40000

2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016 2017 2018

Fisc

al Y

ear

En

d C

um

ula

tive

Cap

acit

y (M

W)

Year

a)

b)

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Figure 3a. Terrain Height in meter (shaded) at Agaswadi (Maharashtra

state) wind Farm site in India. The dots represent the location of each

wind turbine over the topographically complex site of Agaswadi. The

dotted lines represent the model grid at 1km and yellow circles show

location of T1, T16 and T34 wind mills.

Figure 3b. Domain of integration for WRF model. First Domain’s

horizontal resolution is 27km, Second domain 9km, 3rd domain 3km and

innermost 4th domain 1km.

a) b)

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31

Figure 4a. Frequency distribution of observed wind speed (m/s) for the

month of April 2015. The blue colour is for wind turbine T1, Orange

colour for T16 and Green colour is for T34.

Figure 4b. Observed power curve for the complex terrain site over

Maharashtra State in India.

0

50

100

150

200

250

300

350

0 2 4 6 8 10 12 14

Freq

uen

cy

Wind Speed (m/s)

T1

T16

T34

a)

b)

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Figure 4c Diurnal variation of observed and forecasted wind speed(m/s) for the month of April . The blue colour is for wind turbine T1,

Red colour for T16 and Green colour is for T34.

0

1

2

3

4

5

6

7

08:30 11:30 14:30 17:30 20:30 23:30 02:30 05:30

Win

d (

m/s

)

TIme

Diurnal Variation

Obs_wind_T01

Model_wind_T01

Obs_wind_T16

Model_wind_T16

Obs_wind_T34

Model_wind_T34

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Figure 5. Wind rose diagram for the observed wind

direction for wind turbines a) T1, b) T16 and c) T34 for

the month of April 2015. Shade represents the different

bins of wind speed in m/s.

b. T16 a. T1

c. T34 N

E

S

W

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34

Figure 6 The wind speed (m/s) and power (KW) forecast from the model compared with the observation for 1 Apr 2015 for wind turbine T1 over Agaswadi

Region. The black line is observed wind and pink line is forecasted wind in m/s. The green bars represent observed power and blue bars as forecasted

power in KW.

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Figure 7 (a-c) Different skill scores for wind and power with varying threshold values and RMSE and mean error variation (b-d) for wind turbine T1.

b

a c

d

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Figure 8 (a-d) Same as Figure 6 , but for all wind turbines for area averaged over 74.6 - 74.635 °E and 17.51 - 17.57 °N .

b

a c

d

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Figure 9 Flow chart of different sensitivity experiment conducted for obtaining best model configuration.

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Figure 10 Comparison of high wind conditions on (a) 10 Dec 2016, (b) 12 Dec 2016 with observed wind speed.

a)

b)

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Figure 11 Same as Figure 10 but for low wind conditions on (c) 24 Dec 2016, (d) 26 Dec 2016.

a)

b)

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Figure 12 Comparison of simulated wind speed with different model grid resolutions (GFST1534_4dom: innermost domain resolution is 1 km;

GFST1534_5dom: innermost domain resolution is 333.33 m) with 0000 UTC 06 Dec 2016 from GFST1534 and NCEP_GFS

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Figure 13 Sensitivity of the model to simulate wind speed with different PBL scheme

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Figure 14 Model vertical level & land use land cover sensitivity of the model to simulate wind speed during (a) low wind condition and (b) high wind condition

a)

b)

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Using yesterday’s observations, calculate error

(bias) in winds as Model (today)- obs (y’day) for a day ahead forecast

Average earlier three consecutive times error and

note this as ∆ at time ‘t’

Depending on the sign of ∆, add or subtract it from

model predicted winds at time ‘t’

These bias corrected winds now can be used as

forecast.

Figure 15. Flow chart explaining Linear Bias correction

method for wind prediction

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Figure 16 Comparison of wind speed simulated with different LULC data with observation (a) low wind case and (b) high wind case

without bias correction (solid lines) and with bias correction (dashed lines).

a)

b)

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Figure 17 Comparison of Percentage error (%) of power for low wind case without bias correction (solid lines) and with bias correction (dashed lines).

0

0.5

1

1.5

2

2.5

3

26-1

2-2

016

11

:30

26-1

2-2

016

12

:20

26-1

2-2

016

16

:40

26-1

2-2

016

17

:30

26-1

2-2

016

18

:20

26-1

2-2

016

19

:20

26-1

2-2

016

20

:10

26-1

2-2

016

21

:10

26-1

2-2

016

22

:10

26-1

2-2

016

23

:00

26-1

2-2

016

23

:50

27-1

2-2

016

00

:50

27-1

2-2

016

01

:50

27-1

2-2

016

02

:40

27-1

2-2

016

03

:30

27-1

2-2

016

04

:20

27-1

2-2

016

05

:10

27-1

2-2

016

06

:10

27-1

2-2

016

07

:20

27-1

2-2

016

09

:00

27-1

2-2

016

09

:50

27-1

2-2

016

10

:50

27-1

2-2

016

11

:40

27-1

2-2

016

12

:30

27-1

2-2

016

13

:30

27-1

2-2

016

14

:20

27-1

2-2

016

15

:20

27-1

2-2

016

16

:10

27-1

2-2

016

17

:00

27-1

2-2

016

17

:50

27-1

2-2

016

18

:40

27-1

2-2

016

19

:30

27-1

2-2

016

22

:40

27-1

2-2

016

23

:30

28-1

2-2

016

00

:30

28-1

2-2

016

01

:20

28-1

2-2

016

02

:10

28-1

2-2

016

03

:00

28-1

2-2

016

04

:00

28-1

2-2

016

04

:50

Pe

rce

nta

ge E

rro

r (%

)

Date & Time

USGS_Vert45_T1

MODIS_vert45_T1

NRSC_vert45_T1

USGS_45_Bias_corrected

MODIS_45_Bias_corrected

NRSC_45_Bias_corrected