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64 ransome _the_best_pv_model_depends_on_the_reason_for_modelling

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www.steveransome.com 27-Oct-15 1 The 'best' PV Model Depends on the Reason for Modelling Steve Ransome (Independent PV consultant SRCL) and Juergen Sutterlueti (Gantner Instruments) 4th PV Performance Modelling Collaborative (PVPMC) Workshop TÜV Cologne, Germany (22-23 Oct 2015)
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Page 1: 64 ransome _the_best_pv_model_depends_on_the_reason_for_modelling

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The 'best' PV Model Depends on the Reason for Modelling

Steve Ransome (Independent PV consultant SRCL) and

Juergen Sutterlueti (Gantner Instruments)

4th PV Performance Modelling Collaborative (PVPMC) Workshop

TÜV Cologne, Germany (22-23 Oct 2015)

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Many reasons for modelling performance of PV modules/arrays

1) Production process optimisation (to minimise losses at Standard Test Conditions).

2) Determination of coefficients “PMAX vs. TMODULE”, “Efficiency vs. Irradiance” etc.

3) Overall system energy yield predictions vs. simulated weather inputs

4) Benchmarking different PV technologies (vs. differing PMAX, Low Light … coefficients)

5) Validation of instantaneous performance (prove module/array is working)

6) Fault finding (if under performance) – which model parameters are responsible ?

7) System output validation e.g. kWh/ year

8) Degradation rate vs. time, which parameters are degrading ?

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Which parameters limit PMAX at high and low light levels ?Typical clear morning CdTe at NREL :

06:15 | 0.07kW/m² | T_Mod 17C

10:45 | 0.95 kW/m² | T_Mod 56C

Locus of PMAX at VMP

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Which parameters limit PMAX at high and low light levels ?Typical clear morning CdTe at NREL :

• PMAX = ISC * FF * VOC

• ISC ~ GI, AOI, AM, soil , snow, ...

• VOC ~ TMOD, ln(GI) ...

• FF “Fill factor vs. irradiance” depends on module technology

(3) “PMAX @ high light”limited by ROC

(4) “PMAX @ low light” limited by VOC, RSC vs. GI

(2) “Resistance at VOC”ROC= -1/(dI/dV)|V=VOC

(1) “Resistance at ISC”RSC=-1/(dI/dV)|V=0

Locus of PMAX at VMP

06:15 | 0.07kW/m² | T_Mod 17C

10:45 | 0.95 kW/m² | T_Mod 56C

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Example PV Models and their fit types to IV curves

Full CurveFit

Points + Gradients

1-diode model 5-7 parametersused in most simulation programmes, extended from de Soto 2006Fits entire curve – answer depends on glitches, non optimum performance, point distribution and/or weighting e.g. more important nearest PMAX

Matrix method, IEC 61853, PVUSA, Empirical fits

ONLY knows PMAX

ISC, VOC etc. unknown

May know VDC

Sandia Array Performance Model Loss Factors Model SRCL/GI

Takes values at only certain places on the IV curve e.g. V=0, V=VMP, I=0 …

PMAX or Efficiency Only AC or DC

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IV curvesVs. Irradianceand TMOD

Matrix - PMAX onlyAvg Eff (GI, TMOD)

1 diode (Full curve)IPH RSH I0 RSE nf

LFM (Points and gradients)Described in next talk

From IV curves vs. GI and TMOD to the three model types

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LFMPoints+Gradients

Irradiance

Matrix Avg Eff onlyIrradiance Tmod

1 diode Full curve

Irradiance

good c-Si Good RSC + ROC good TF Poorer ROC poor TF Poor RSC and ROC

How models differentiate PV Technologies

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LFMPoints+Gradients

Irradiance

Matrix Avg Eff onlyIrradiance Tmod

1 diode Full curve

Irradiance

good TF Poorer ROC poor TF Poor RSC and ROC

IV curves

good c-Si Good RSC + ROC

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LFMPoints+Gradients

Irradiance

Matrix Avg Eff onlyIrradiance Tmod

1 diode Full curve

Irradiance

VMP

VMP

VMP

VMP

FF FFFF

VMP

VMP

good TF Poorer ROC poor TF Poor RSC and ROC

Io n

RSHUNT RSERIES RSHUNT

RSERIES

RSHUNT RSERIES

Io n

Eff@LowLight Eff@HighLight

Eff@High TmodEff@HighTmod

Eff@LowLight

Max Eff @Low T, Low G

Max Eff @Low T, High G

“flat” EffVs. T and G

PR=100%

PR=100

PR<100%PMAX < PMAX.REFPMAX. ~ PMAX.REF

Eff@HighTmod

nRSC nROC nROCnRSC

nIMP nVMP nVMPnIMP

nROC

nVMP

GOOD

MEDIUM

POOR

DIRECTION

KEY

Optimum= 1

good c-Si Good RSC + ROC

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good c-Si good TF poor TF

LFMPoints+Gradients

Irradiance

Matrix Avg Eff onlyIrradiance Tmod

1 diode Full curve

Irradiance

Needs for optimum modelling :

1) Differentiate “offsets between technologies” from “product variability within a type”

2) Recreate these curves with simple models

3) Quantifyperformance loss or optimisation possible from sub standard modules

Need curves that are easy to fit

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Comparing residual errors from 1-diode, SAPM and LFMPVSEC Paris 2013 4CO-11.1

Cumulative distribution functions for residuals of 11 modules measured at Sandia

SAPM LFM CEC 1-diode

PMP

IMP

VMP

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Degradation : IV curve Analysis : Poor CIGS in ArizonaClear day IV measurements at 12:00 each month Corrected for Irradiance and Module temperature.

• IV curve Degradation/Failure Analysis

• ISC RSC IMP VMP ROC VOC

• Needs irradiance and temperature corrections

• Either fit 1-diode coefficients or analyse changes in shape of the curves - can be hard

• Glitches/imperfect behaviour make fitting difficult

ISC RSCIMP

VMP

ROC

VOC

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Degradation : Point/Gradient LFM Analysis : Poor CIGS in AZClear day IV measurements at 12:00 each month Corrected for Irradiance and Module temperature

• Residuals (enLFM = “measured-predicted”) of degrading CIGS module, no temperature correction needed

• Grey bars show residual < ±1%.

• Any fall in residual curve shows degradation

• It’s easy to determine rate and cause (note changes from April to October)

• Note: nIsc has more scatter as it has AOI and spectral and snow effects

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Using an Hourly energy simulation programvary losses and study performance change sensitivity at different climates

1. Sun tracking gain

2. Shading

3. Snow

4. Soil

5. AOI

6. Spectrum

7. Seasonal Annealing

8. Thermal loss (Gamma, NOCT)

9. DC constant loss

10. Efficiency vs. Irradiance (LLEC, I2.Rs)

11. Mismatch

12. DC I2R loss cabling

13. Inverter Wakeup

14. Mppt loss

15. Inverter Efficiency

16. AC Constant loss

17. Clipping

18. Transformer effiency

19. Tare

20. AC I2R loss cabling

Jan - Dec

Loss Gain

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Insolation distribution vs. Irradiance (kW/m²) and Tmodule (°C) for worldwide sites

Energy yield will be affected differently at sites worldwide

For example high RSERIES

causes loss at high light levels (right) which will lose more energy yield at high insolation sites (right)

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Energy yield sensitivity worldwide to finite changes in Gamma, NOCT (left) Low Light Efficiency, I².RSERIES (right)

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Conclusions

Recommendations• Normalise data to ensure easier understanding (e.g. ISC.MEAS/ISC.STC/GI)

• Use physically significant coefficients (e.g. nVOC)

• Ensure IV Scans are good quality, calibrated and believable with little scatter

• Simple kWh/kWp calculations, optimum sitesEfficiency only model may be enough

• Fast inline check, degradation/ non-optimum “points+gradients” models better

• For the ultimate understanding the full weighted point IV curves should be studied

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Acknowledgements• Gantner Instruments staff

• Bill Marion of NREL for data [email protected]

• This analysis and conclusions of NREL data based solely on available information

• Thank you for your attention !

For more information :

[email protected]

www.steveransome.com

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• Spare slides

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Model #2) Simplified normalised Loss Factors Model (LFM)26th EU PVSEC 2011 Hamburg 4AV.2.41

“6 physically significant normalised orthogonal parameters”

Easily Determine

Temperature and Irradiance Coefficients

Performance validation

Process optimisation (minimise losses)

Fault finding

Degradation rate and cause

I and V curvature parameters can detect

Cell mismatch/shading ([email protected]*VMP)

Non Ohmic back contacts ([email protected]*IMP)

PRDC = EffMEASURED/EffNOMINAL =

nISC * nRSC * nIMP * nVMP * nROC * nVOC


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