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Development of NREL Performance Acceptance Test Guidelines for Large Commercial
Parabolic Trough Solar Fields
MENASOL 2011
CSP Today 4-5 May Morocco
Dr. David Kearney, K&A, USA Mark Mehos, NREL, USA
1 MENASOL 2011
Morocco K&A/NREL
Objectives
• Performance acceptance tests are required for the turnover of all major power plant equipment but as yet no formal codes exist for the solar field
• To fill this gap, NREL initiated development of performance
acceptance test Guidelines for the solar system, starting with parabolic troughs using oil HTF
• Solar system acceptance testing is unique due to: – variable nature of the energy source, and – necessity for a performance model to compare
results to measurements
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Scope
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• Thermal power or energy delivery of the solar system to the heat exchanger train (for steam production)
• Solar system is comprised of solar field & HTF system • Power block and BOP are not included in the Guidelines
• Thermal equilibrium (steady state) conditions are a critical test requirement • Uncertainty level in result equally critical
A sense of scale
• The capacity of parabolic trough projects under construction generally range from 50 to 250 MWe turbine net capacity
• A 250 MWe, with thermal storage, can have a total mirror aperture area of ≈1.8 million m2 covering a land area of about 540 hectares (1335 acres)
• This scale presents several challenges that will influence the level of uncertainty and transient errors in the test results
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Commercial Project Issues
• Testing parties can differ by virtue of different project structures, but the applicable codes remain unchanged. One example of parties would be EPC contractor accepting solar field from technology provider
• Top-level test procedures are set between the testing parties at contract signing
• Subsequently, but well before testing, detailed test procedures are laid down in a Test Plan. Examples include exactly where and how the measurements are made, the duration and number of tests, and pass/fail criteria.
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Considerable CSP industry input has gone into development of these Guidelines
• The process adopted by NREL was designed to include input from a wide spectrum of CSP stakeholders
• Advisory Committee was formed to periodically review and critique direction and progress. This 12-person group included EPCs, Technology Providers, Developers, Utilities, Independent Engineers, and Utilities.
• In parallel, U.S. ASME independently initiated a process to develop a Performance Test Code (PTC 52) for all CSP technologies, also restricted to thermal, not electrical, output. The NREL Guidelines will provide a jump-start to the ASME code development, which typically may take several years to complete
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• Short Duration Steady State Thermal Power Test – Objective is to measure the thermal power and efficiency under
clear sky conditions. – Multiple short-duration tests run sequentially over mid-day
time period, e.g., 0900 - 1500 – Satisfactory test runs (e.g., runs where steady-state conditions
exist) are extracted based on examination of the data. – Pattern can be repeated over multiple days based on agreement
between parties
• Governing Equations Thermal Power: Thermal Efficiency:
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Recommended Tests First
• Multi-Day Continuous Energy Test
– Objective is to collect continuous daily thermal energy output (integrated power output) for comparison against model projections
– Continuous 10-day test suggested (though this period to be set by agreement between parties).
– Both clear sky and partly cloudy conditions are acceptable – Additional information on system response to startup, shutdown,
and transient weather event to be collected over test period.
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Second
Attainment of Thermal Equilibrium
• Thermal equilibrium is a crucial test condition for acceptable results
• Analyses* have been carried out to evaluate the effects of gradients in the solar resource during a test period
• Important considerations are the transient effects on test results of a gradient in radiation input to the solar field and the transit time through the collector field header piping
* from Mike Wagner, NREL
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Attainment of Thermal Equilibrium (cont)
• Thermal equilibrium is a crucial test condition for acceptable results
• Analyses have been carried out to evaluate the effects of gradients in the solar resource during a test period
• Important considerations are the transient effects on test results of a gradient in radiation input to the solar field and the transit time through the collector field header piping
• Analyses for actual DNI data show that the disparity in results due to these effects are real, but small, and generally acceptable
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Other test issues
• Characterization of representative reflectivity of the mirrors for the model calculation
• Contribution of HTF properties to uncertainty • Solar field with high solar multiple
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• The methodology to evaluate test uncertainty is founded in ASME PTC 19.1 “Test Uncertainty”
• Sources of uncertainty are systematic (bias) and random (precision) errors, the former dominating the test results
• Major contributors are the measurements of HTF specific heat
and Direct Normal Radiation • Example uncertainty calculations give:
≈ 4% for the solar field power output and ≈ 5% for the solar field thermal efficiency
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Measurement Uncertainty
Future Work
• Expansion of guidelines to tower and linear Fresnel systems • Investigation of better methods for measuring average
reflectivity of large solar fields • Reduction of uncertainty contributions due to known issues,
such as HTF properties
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Thank you
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Summary Performance acceptance tests of large solar trough fields (and other CSP technologies) require careful attention to the unique effects of a varying energy source and the characteristics of the solar system This work represents an important step forward in providing a usable set of Guidelines for parabolic trough systems, while also identifying important issues that require further work to reduce test uncertainties