richard perez - gw solar symposium 2012

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SOLAR ENERGY: A Path to Energy Significance 4/12/12 DISPERSED PV GENERATION: SOLAR RESOURCE VARIABILITY Richard Perez Tom Hoff

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Page 1: Richard Perez - GW Solar Symposium 2012

SOLAR ENERGY: A Path to Energy Significance 4/12/12

DISPERSED PV GENERATION: SOLAR RESOURCE VARIABILITY

Richard Perez Tom Hoff

Page 2: Richard Perez - GW Solar Symposium 2012

DISPERSED PV GENERATION: SOLAR RESOURCE VARIABILITY

SPATIAL

© R. Perez & T. Hoff

Page 3: Richard Perez - GW Solar Symposium 2012

TEMPORAL TIME SCALE

© R. Perez & T. Hoff

Page 4: Richard Perez - GW Solar Symposium 2012

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One-Minute Global Irradiance (W/sq.m)

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One-Minute Global Irradiance (W/sq.m)

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100%Minute-to-Minute Change (% maximum yield)

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0%

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60%

80%Minute-to-Minute Change (% maximum yield)

SINGLE LOCATION

20 UNCORRELATED LOCATIONS

© R. Perez et al

Relative Variability = 1/√N N locations

© Richard Perez / Tom Hoff

Variability = σ(∆kt*)

Page 5: Richard Perez - GW Solar Symposium 2012

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One-Minute Global Irradiance (W/sq.m)

-80%

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0%

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80%Minute-to-Minute Change (% maximum yield)

20 UNCORRELATED LOCATIONS

© R. Perez et al

© Richard Perez / Tom Hoff

Relative Variability = 1/√N N locations

Page 6: Richard Perez - GW Solar Symposium 2012

© Richard Perez / Tom Hoff

16 Months of data -- 40 million data points

© R. Perez & T. Hoff

Page 7: Richard Perez - GW Solar Symposium 2012

Virtual Networks Time space = f (cloud speed)

© Richard Perez / Tom Hoff

400x400km satellite-derived hi-resolution one-minute data

16 Months of data -- 40 million data points 16 Months of data -- 4 Billion data points

Very high density modular networks

66 stations

Page 8: Richard Perez - GW Solar Symposium 2012

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∆K

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Site-pair distance distance (km)

One minute

One minute

© Richard Perez / Tom Hoff

Page 9: Richard Perez - GW Solar Symposium 2012

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© Richard Perez / Tom Hoff

Page 10: Richard Perez - GW Solar Symposium 2012

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© Richard Perez / Tom Hoff

Page 11: Richard Perez - GW Solar Symposium 2012

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© Richard Perez / Tom Hoff

Page 12: Richard Perez - GW Solar Symposium 2012

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One minute5-minutes15-minutes30-minutesOne Hour

HAWAII LAND Nov 2011 CLOUD SPEED 13 km/h

© Richard Perez / Tom Hoff

Page 13: Richard Perez - GW Solar Symposium 2012

NEVADA Jun 1998 CLOUD SPEED 24 km/h

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© Richard Perez / Tom Hoff

Page 14: Richard Perez - GW Solar Symposium 2012

HAWAII Dec 2010 CLOUD SPEED 26 km/h

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Site-pair distance distance (km)

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© Richard Perez / Tom Hoff

Page 15: Richard Perez - GW Solar Symposium 2012

CENT. CALIFORNIA Mar 1998 CLOUD SPEED 30 km/h

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© Richard Perez / Tom Hoff

Page 16: Richard Perez - GW Solar Symposium 2012

SOUTH GT. PLAINS Dec 2010 CLOUD SPEED 44 km/h

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Site-pair distance distance (km)

One minute5-minutes15-minutes30-minutesOne Hour

© Richard Perez / Tom Hoff

Page 17: Richard Perez - GW Solar Symposium 2012

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Site-pair distance distance (km)

© R. Perez & T. Hoff

Page 18: Richard Perez - GW Solar Symposium 2012

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Corr

elat

ion

Zero

Cro

ssov

er D

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nce

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Fluctuation Delta T (minutes)

© Richard Perez / Tom Hoff

∆t

Zero

Cor

rella

tion

Dist

ance

Page 19: Richard Perez - GW Solar Symposium 2012

BASE GENERATION

VARIABLE GENERATION

SOLAR GENERATION STORAGE

CRITICAL TIME SCALE

Seconds Minutes Half Hour Hour

Small PV

Large PV or dist. feeder

Utility

Balancing Area

Application

Technical Solutions

Interconnection Hardware

Voltage reg. devices

Storage

Load Management, contingency variable generation

SolarAnywhere High Resolution

SolarAnywhere Standard Resolution

© R. Perez & T. Hoff

Page 20: Richard Perez - GW Solar Symposium 2012

CRITICAL TIME SCALE

Seconds Minutes Half Hour Hour

SolarAnywhere High Resolution

SolarAnywhere Standard Resolution

© R. Perez & T. Hoff

Measured and simulated 10 second fleet output for a 4 km x 4 km region

Page 21: Richard Perez - GW Solar Symposium 2012

© R. Perez & T. Hoff.

© Richard Perez / Tom Hoff

Page 22: Richard Perez - GW Solar Symposium 2012

-1

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Delta

Kt*

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lta K

t*

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Delta

Kt*

single point

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Delta

Kt*

single point

20-Second fluctuations

1-minute fluctuations

5-minute fluctuations

15-minute fluctuations

SINGLE POINT

© Richard Perez / Tom Hoff

Page 23: Richard Perez - GW Solar Symposium 2012

-1

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Delta

Kt*

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lta K

t*

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Delta

Kt*

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Delta

Kt*

20-Second fluctuations

1-minute fluctuations

5-minute fluctuations

15-minute fluctuations

SINGLE POINT

40x40 km AREA

© Richard Perez / Tom Hoff

Page 24: Richard Perez - GW Solar Symposium 2012

Hourly Variability divided by 5

3-Hour Variability divided by 5

6-Hour Variability divided by 5

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Corr

elat

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ssov

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nce

(km

)

Fluctuation Delta T (minutes)

∆t = 24 hours

Source: Marc Perez, Columbia University

∆t

Zero

Cor

rella

tion

Dist

ance

Page 25: Richard Perez - GW Solar Symposium 2012

Perez et al., ASRC

Page 26: Richard Perez - GW Solar Symposium 2012

100oF

80oF

20oF

40oF

60oF

© Richard Perez, ASRC

Page 27: Richard Perez - GW Solar Symposium 2012

Early 2012 Heat Wave

0 30 60 100

© R. Perez & T. Hoff

Page 28: Richard Perez - GW Solar Symposium 2012

0.10 0.23 0.28 0.33 0.38 0.43 0.48 0.53 0.58 0.63 0.68 0.73 0.78 0.83 0.88 0.93 0.98 10 x10 km 0.3% 0.2% 0.2% 0.1% 0.1% 0.2% 0.2% 0.2% 0.3% 0.2% 0.5% 0.4% 0.6% 1.7% 3.9% 11.6% 79.2%

Clearness IndexDistributed

resource footprint

30x30 km 0.0% 0.0% 0.1% 0.1% 0.1% 0.1% 0.2% 0.3% 0.3% 0.4% 0.3% 0.4% 1.0% 1.9% 2.9% 7.5% 84.3%

70x70 km 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.6% 0.4% 0.8% 3.9% 94.4%90x90 km 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.1% 2.0% 97.8%

110x110 km 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 2.7% 97.3%

50x50 km 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.0% 0.1% 0.4% 0.2% 0.4% 1.2% 97.6%

A/C Solar Peak Shaving Guarantee increases with resource distribution

15-year Clearness Index distribution for all hours with T >88F, Central CA

Probability of having less than a 90% ideal solar resource: ZERO

10x10km 30x30km 50x50km 70x70km 90x90km 110x110km

© R. Perez & T. Hoff

Page 29: Richard Perez - GW Solar Symposium 2012

More intense cloud impact

More intense turbidity impact

FLAT PLATE vs. CONCENTRATION

Capa

city

fact

or

© R. Perez & T. Hoff

Page 30: Richard Perez - GW Solar Symposium 2012

Thank you

Page 31: Richard Perez - GW Solar Symposium 2012

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