csp solar field quality assurance methods

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Solar Field Quality Assurance Methods Klaus Pottler CSP Services GmbH [email protected] https://es.linkedin.com/in/klauspottler http://www.researchgate.net/profile/Klaus_Pottler China International CSP Station Conference & CSPPLAZA 2015 Annual Meeting CPC2015, 25-26 June 2015, Beijing, China

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Page 1: CSP Solar Field Quality Assurance Methods

Solar Field Quality Assurance Methods

Klaus Pottler

CSP Services GmbH [email protected]

https://es.linkedin.com/in/klauspottler http://www.researchgate.net/profile/Klaus_Pottler

China International CSP Station Conference & CSPPLAZA 2015 Annual Meeting

CPC2015, 25-26 June 2015, Beijing, China

Page 2: CSP Solar Field Quality Assurance Methods

Introduction to CSP Services

CPC2015, 25-26 June 2015, Beijing, China 2

Almería, Spain

Cologne, Germany

Private company founded 2007, >20 Engineers Based in Germany, Office in Spain German Aerospace Center (DLR) Spin-Off Proximity to Plataforma Solar de Almería (PSA)

Page 3: CSP Solar Field Quality Assurance Methods

CSP Services Main Goals

CPC2015, 25-26 June 2015, Beijing, China 3

Implement R&D results in industry to improve CSP technologies

For power plant producers

• Lower investment risks

• Improve project performance

• Improved competitiveness

For Operators

• Increase solar power production

• Rise profitability

For Society and Environment

• Reduce solar electricity costs

• Reduce CO2 emissions

Heat the tube, not the surroundings

Page 4: CSP Solar Field Quality Assurance Methods

CSP Services Main Goals

CPC2015, 25-26 June 2015, Beijing, China 4

Implement R&D results in industry to improve CSP technologies

For power plant producers

• Lower investment risks

• Improve project performance

• Improved competitiveness

For Operators

• Increase solar power production

• Rise profitability

For Society and Environment

• Reduce solar electricity costs

• Reduce CO2 emissions

Stay warm but do not burn your feet

Page 5: CSP Solar Field Quality Assurance Methods

CSP Services Products & Clients

CPC2015, 25-26 June 2015, Beijing, China 5

http://www.cspservices.de

Page 6: CSP Solar Field Quality Assurance Methods

Solar field has a high share of total investment costs • Long-term investment

• Large extension (→ adjustments are expensive)

• Plant output strongly depends on collector field quality (3-10% field performance can be easily lost)

Quality assurance is necessary for

• Control of subcontractors

• Warranty claims

Quality assurance is indispensable and makes economic sense

Motivation for Quality Assurance

CPC2015, 25-26 June 2015, Beijing, China 6

Page 7: CSP Solar Field Quality Assurance Methods

Importance of High Quality Components Example: Possible degradation of mirror panels Based on • 200 MWel power plant, annual capacity factor 40%, revenue 0.14 US$/kWh

Exemplary degradation of mirrors • 0.3% less reflectance/year → 0.45% less thermal efficiency/year

→ ≈ 4% less energy production over 20 years Energy generation and losses • 200 MW · 8760 h/year · 40% · 20 years ≈ 14’000’000 MWh total generation • 14’000’000 MWh · 140 US$/GWh * 4% ≈ 78 Million US$ revenue loss

Loss of revenues of 78 Million US$ can be avoided with high quality and durable components

CPC2015, 25-26 June 2015, Beijing, China 7

Page 8: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 8

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Page 9: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 9

Resource assessment

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Page 10: CSP Solar Field Quality Assurance Methods

Resource Assessment

CPC2015, 25-26 June 2015, Beijing, China 10

Do we REALLY have 100% of DNI available?

• High quality ground data & long-time satellite data necessary to get correct weather data time series

• Rotating Shadowband Irradiometer (RSI) often better than Pyrheliometer (due to lower soiling)

• Excellent maintenance on site is essential

Suggestion: Use economic RSI-Stations, ask for frequent maintenance and high-quality data service

Satellite map of beam irradiance Pyrheliometer station Rotating Shadowband Irradiometer (RSI)

CSPS

SolarGIS

CSPS

Page 11: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 11

Resource assessment

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Page 12: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 12

Resource assessment

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 13: CSP Solar Field Quality Assurance Methods

Collector Design Efficiency influenced by

• Cosine effects

• Incidence angle modifier (IAM)

• Shading / blocking

• End losses

• Intercept factor

Suggestion

• Use mature designs

• Adapt to local production possibilities

• Cross-check drawings

• Build full-scale prototypes

• Perform extensive geometric, structural and thermal tests

CPC2015, 25-26 June 2015, Beijing, China 13

from: Geyer et al.: “EuroTrough - Parabolic Trough Collector “ SolarPACES-Conference, Sept. 4-6, 2002, Zurich, Switzerland

LS3 Design Torque Tube Design Torque Box Design

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Page 14: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 14

Resource assessment

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 15: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 15

Resource assessment

Mirror panels

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 16: CSP Solar Field Quality Assurance Methods

Mirror Panels (1) Efficiency influenced by

• Specular reflectance

• Shape accuracy (“focus deviation”)

• Degradation

State of the art (for RP3 mirror panel)

• Specular reflectance: > 94 % (solar weighted, 15°, 12.5 mrad)

• Focus Deviation (FDx): < 7 mm (RMS)

CPC2015, 25-26 June 2015, Beijing, China 16

Hemispherical Reflectance

0,0

0,1

0,2

0,3

0,4

0,5

0,6

0,7

0,8

0,9

1,0

250 500 750 1000 1250 1500 1750 2000 2250 2500

wavelength [nm]

Rh

em

0

0,001

0,002

0,003

0,004

0,005

0,006

0,007

0,008

0,009

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rela

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glass-mirror ρSWH=0.94

polymerfoil ρSWH=0.92

aluminum ρSWH=0.87

Solar Norm G173

Page 17: CSP Solar Field Quality Assurance Methods

Mirror Panels (2)

Price reduction and quality improvement of solar mirrors

from: R. Pitz-Paal, Kosten und Wert von CSP Solarstrom, 18. Sonnenkolloquium, Cologne, May 2015

http://www.dlr.de/sf/desktopdefault.aspx/tabid-10498

CPC2015, 25-26 June 2015, Beijing, China 17

Page 18: CSP Solar Field Quality Assurance Methods

Mirror Panels (3) Suggestions

• Specify “state of the art” in tender documents

• Claim long term warranty in procurement

• Evaluate offers in respect to costs and quality

• Confirm technical data through expert laboratories

• Claim frequent sample measurements in fabrication with traceable documentation

CPC2015, 25-26 June 2015, Beijing, China 18

QDec System QDec Test Report

Page 19: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 19

Resource assessment

Mirror panels

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 20: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 20

Resource assessment

Receivers

Mirror panels

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 21: CSP Solar Field Quality Assurance Methods

Receivers (1) Efficiency influenced by

• Transmittance of glass cover tube

• Absorptance of steel tube

• Heat loss

• Bellow design

• Degradation

State of the art (for Ø70 mm tube)

• Optical Efficiency: ≈ 106% (relative to DLR OptiRec artificial reference)

• Transmittance: > 96 %

• Heat Loss: ≈ 150 W/m (@350 °C)

≈ 230 W/m (@400 °C)

CPC2015, 25-26 June 2015, Beijing, China 21

DLR OptiRec System

Page 22: CSP Solar Field Quality Assurance Methods

Receivers (2) Suggestions

• Specify “state of the art” in tender documents

• Claim long term warranty in procurement

• Evaluate offers in respect to costs and quality

• Confirm technical data through expert laboratories

• Claim frequent sample measurements in fabrication with traceable documentation

CPC2015, 25-26 June 2015, Beijing, China 22

http://www.dlr.de/sf/quarz/test-reports

ThermoRec System ThermoRec Test Report

Page 23: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 23

Resource assessment

Receivers

Mirror panels

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 24: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 24

Resource assessment

Receivers

Mirror panels

Assembly&Installation

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 25: CSP Solar Field Quality Assurance Methods

Assembly & Installation (1) Efficiency influenced by intercept factor

• 3D-Accuracy of Concentrator Structures

• Concentrator Shape Accuracy

• 3D-Deformation (tracking angle, wind)

• Receiver and Module Alignment

• Tracking Accuracy

State of the art (for EuroThrough geometry)

• Mirror support bracket position -> mirror tilt deviation: < 0.8 mrad (RMS)

• Mirror support bracket angle -> effect on mirror geometry: < 1.0 mrad (RMS)

• Receiver alignment -> lateral deviation of receiver position: < 3.0 mm (RMS)

• Module alignment -> deviation to drive: < 1.0 mrad (RMS)

• Collector torsion -> torsion between drive and all modules: < 1.0 mrad (RMS)

• Tracking accuracy -> deviation of optical axis: < 1.0 mrad (RMS)

CPC2015, 25-26 June 2015, Beijing, China 25

Page 26: CSP Solar Field Quality Assurance Methods

Side note: Intercept Factor Check (1)

CPC2015, 25-26 June 2015, Beijing, China 26

Intercept factor measurement of a parabolic trough collector with Camera-Target-Method

Page 27: CSP Solar Field Quality Assurance Methods

Side note: Intercept Factor Check (2)

CPC2015, 25-26 June 2015, Beijing, China 27

Camera-Target-Methode (CTM): Measurement pictures for evaluation of intercept factor

Page 28: CSP Solar Field Quality Assurance Methods

Side note: Intercept Factor Check (3)

CPC2015, 25-26 June 2015, Beijing, China 28

Intercept factor of a trough collector before and after optimization measures

Page 29: CSP Solar Field Quality Assurance Methods

Assembly & Installation (2) Suggestions

• Specify “state of the art” in tender documents

• Claim long term warranty in procurement

• Evaluate offers in respect to costs and quality

• Check prototypes by independent experts

• Elaborate suitable process descriptions for assembly and solar field installation

• Check all components during solar field fabrication

• Frequently check metal structures by adequate 3D-measurement methods in assembly hall

• Check solar field installation quality

Details are given in this paper K. Pottler et al: Ensuring Performance by Geometric Quality Control and Specifications for Parabolic Trough Solar Fields http://www.sciencedirect.com/science/article/pii/S187661021400684531)

CPC2015, 25-26 June 2015, Beijing, China 29

Page 30: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 30

Resource assessment

Receivers

Mirror panels

Assembly&Installation

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 31: CSP Solar Field Quality Assurance Methods

Efficiency Chain for Parabolic Trough

CPC2015, 25-26 June 2015, Beijing, China 31

Resource assessment

Cleaning, M&O

Receivers

Mirror panels

Assembly&Installation

Exemplary numbers for parabolic trough for normal incidence Note: current collectors usually perform better

Total optical efficiency

Collector design

Page 32: CSP Solar Field Quality Assurance Methods

European Testing Centers (Selection) German Aerospace Center: DLR QUARZ Center, Germany

• Component laboratory tests (e.g. Receivers, Mirror Panels)

German Aerospace Center: DLR KONTAS Test Bench, Spain

• Full scale test for parabolic through modules under real sun conditions

CIEMAT and DLR: PSA OPAC Laboratory, Spain

• Accelerated Aging Tests

CSP Services: Germany and Spain

• Quality Inspection Systems

• Solar Field Expert Services

CPC2015, 25-26 June 2015, Beijing, China 32

Page 33: CSP Solar Field Quality Assurance Methods

Testing (1): DLR QUARZ Center Mirror Panel Performance Tests

• Shape accuracy: QDec

• Specular reflectance

• Spectral hemispheric reflectance

Receiver Performance Tests

• Optical efficiency: OptiRec

• Thermal power loss: ThermoRec

• Overheating & thermal cycling

• Bellow fatigue tests

• Operability tests under real solar conditions: KONTAS

CPC2015, 25-26 June 2015, Beijing, China 33

Page 34: CSP Solar Field Quality Assurance Methods

Testing (1): DLR QUARZ Center Mirror Panel Performance Tests

• Shape accuracy: QDec

• Specular reflectance

• Spectral hemispheric reflectance

Receiver Performance Tests

• Optical efficiency: OptiRec

• Thermal power loss: ThermoRec

• Overheating & thermal cycling

• Bellow fatigue tests

• Operability tests under real solar conditions: KONTAS

CPC2015, 25-26 June 2015, Beijing, China 34

Temperature

control unit

23 m

Eurotrough 12m

Page 35: CSP Solar Field Quality Assurance Methods

Testing (2): PSA OPAC Laboratory Accelerated Aging Tests

ISO 6270-2CH: Thermal Cycling with Humidity

ISO 9227: Neutral Salt Spray Test (NSS)

ISO 9227: Copper Accelerated Salt Spray Test (CASS)

ISO 11507: UV + Water Test

ISO 21207: Corrosion Test (NO2, SO2)

IEC 61215: Thermal Cycling Test

IEC 62108: Damp Heat Test & Humidity Freeze Test

MIL-STD 810G / ISO 11998 / DIN ISO 9211-4: Abrasion Tests

DIN 50018 / ISO 6988: Kesternich Test (SO2)

CPC2015, 25-26 June 2015, Beijing, China 35

OPAC outdoor test sites in Spain and Morocco

Page 36: CSP Solar Field Quality Assurance Methods

Testing (3): CSP Services Measurement Systems

• MHP / MDI: Automatic Weather Stations

• QDec: Mirror Shape Check Station

• QFoto: Concentrator Frame 3D Check Station

• QRec: Receiver Optical & Thermal Check Stations

(On-Site) Expert Services

• Handling Measurement Services for DLR QUARZ Center

• Weather Data Check, TMY

• Solar Field Expert Consulting

• 3D-Accuracy of Prototype Collectors, Concentrator Shape

• Alignment Measurements: Mirror, Receiver, Module

• Local Intercept Factor Measurement

• Thermal Efficiency Measurement

CPC2015, 25-26 June 2015, Beijing, China 36

Page 37: CSP Solar Field Quality Assurance Methods

Standards and Guidelines Active Standards • EN 12975:2006 Thermal solar systems and components - Solar collectors (for low and middle temperature range)

• ISO 9488:1999 Solar energy - Vocabulary

• ISO 9806:2013 Solar energy - Solar thermal collectors - Test methods

• UNE 206009:2013 Solar thermal electric plants. Terminology (in Spanish)

• UNE 206011:2014 Solar thermal electric plants. Procedure for Generating a Representative Solar Year (in Spanish)

• UNE 206010:2015 Tests for the […] performance of […] plants with parabolic trough collector technology (in Spanish)

General Information (open web access) • IEC 62862 / Technical Committee TC 117: Solar thermal electric plants (standard under development)

http://www.iec.ch/dyn/www/f?p=103:7:0::::FSP_ORG_ID:7851

• QAiST: A Guide to the Standard EN 12975, May 2012 http://www.estif.org/projects/completed_projects/qaist/project_summary/wp2_solar_thermal_collectors

• SolarPACES Guideline: Official Reflectance Guideline Version 2.5, 2013 http://www.solarpaces.org/tasks/task-iii-solar-technology-and-advanced-applications/reflectance-measurement-guideline

• NREL/TP-5D00-63112: Best Practices Handbook for the Collection and Use of Solar Resource Data for Solar Energy Applications, 2015 http://www.nrel.gov/docs/fy15osti/63112.pdf

• NREL/SR-5500-57272: Utility-Scale Power Tower solar Systems: Performance Acceptance Test Guidelines, 2013 http://www.nrel.gov/docs/fy11osti/52467.pdf

• DLR-QUARZ: Test and Qualification Center for Concentrating Solar Power Technologies http://www.dlr.de/sf/desktopdefault.aspx/tabid-7236

• K. Pottler et al: Ensuring Performance by Geometric Quality Control and Specifications for Parabolic Trough Solar Fields http://www.sciencedirect.com/science/article/pii/S187661021400684531)

CPC2015, 25-26 June 2015, Beijing, China 37

Page 38: CSP Solar Field Quality Assurance Methods

Summary Quality Assurance is necessary and possible • Prevents financial losses and improves profits • Testing Infrastructure available • First Standards & Guidelines available, International Standards under development

Quality Assurance includes • Resource Assessment • Collector & Solar Field Design • Component Qualification • Assembly & Installation • Operation & Maintenance

CPC2015, 25-26 June 2015, Beijing, China 38

Page 39: CSP Solar Field Quality Assurance Methods

Summary Quality Assurance is necessary and possible • Prevents financial losses and improves profits • Testing Infrastructure available • First Standards & Guidelines available, International Standards under development

Quality Assurance includes • Resource Assessment • Collector & Solar Field Design • Component Qualification • Assembly & Installation • Operation & Maintenance

CPC2015, 25-26 June 2015, Beijing, China 39

Don’t produce just paperwork -> Implement QA efficiently

Correctly implemented Quality Assurance saves money in the long run