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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

Development of NREL Performance Acceptance Test … · • The capacity of parabolic trough projects under construction ... code development, which typically may take several years

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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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Solar Field Test Schematic

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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