8 results on '"Röger, Marc"'
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2. Status update of the SolarPACES heliostat testing activities.
- Author
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Röger, Marc, Blume, Kristina, Schlichting, Tim, and Collins, Mike
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HELIOSTATS , *SOLAR receivers , *WIND pressure , *MIRRORS - Abstract
Power tower or central receiver systems use hundreds to ten thousands of two-axis tracking mirrors, so called heliostats, which reflect and focus the sunlight onto a receiver on top of a tower during the day. As basis for a well performing heliostat field, a single heliostat has to perform "correctly". In order to describe and measure the performance of a single heliostat, the SolarPACES Guideline for Heliostat Performance Testing has been developed by a group of R&D and industry experts during the last years. However, at the end, the performance of the whole field, which means the superposition and interaction of all heliostats determines the energy collected in the aperture of a solar central receiver. For that reason, a second guideline is currently outlined, the SolarPACES Guideline for Heliostat Field Performance Testing. Both guidelines aim to be commonly agreed protocols between R&D centers and industry in the field of heliostat performance testing. Recently, a third guideline activity has been started to improve and unify heliostat wind load design methods. The once finalized guidelines (or their concepts) should be included in international standards (e.g. IEC) and used by national organizations like DKE, AENOR, ASME, ASTM. This paper gives an update of the state of the three guidelines being developed in the SolarPACES task III-heliostat working group. [ABSTRACT FROM AUTHOR]
- Published
- 2022
- Full Text
- View/download PDF
3. Forty shades of black: A benchmark of high temperature sprayable black coatings applied on Haynes 230.
- Author
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Caron, Simon, Garrido, Jorge, Setien, Eneko, Harzallah, Ridha, Noč, Luka, Jerman, Ivan, Röger, Marc, Sutter, Florian, and Richter, Christoph
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HIGH temperatures ,SOLAR receivers ,SURFACE coatings ,THERMAL barrier coatings ,FURNACES - Abstract
The solar receiver coating opto-thermal efficiency has a significant impact on a central receiver system thermal final system efficiency. The development of durable high solar absorptance coatings with simple application process and minimal thermal treatment can directly improve the receiver efficiency, thus reducing the levelized cost of electricity. During the past years, innovative receiver coatings for solar thermal tower plants have been developed on various substrates and tested under isothermal load at different temperature levels. In this paper, eight commercial black coating formulations are sprayed on Haynes 230 metal coupons. Solar absorptance and thermal emittance are monitored before and after isothermal exposure. Mass deviations are also measured to pinpoint any oxidation or coating outgassing. Isothermal testing is performed at 700, 750 and 800 °C in a muffle furnace for 1000 hours. After 1000 hours isothermal exposure, Coterill 750 leads the benchmark in front of Pyromark 2500, while other black coatings degrade optically. Uncoated samples oxidize significantly and appear darker than some aged black coatings. [ABSTRACT FROM AUTHOR]
- Published
- 2020
- Full Text
- View/download PDF
4. Sunshape Measurements with Conventional Rotating Shadowband Irradiometers.
- Author
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Wilbert, Stefan, Röger, Marc, Csambor, Jonas, Breitbach, Moritz, Klinger, Florian, Nouri, Bijan, Hanrieder, Natalie, Wolfertstetter, Fabian, Schüler, David, Shaswattam, S., Goswami, Neeraj, Kumar, Sharad, Ghennioui, Abdellatif, Affolter, Roman, Geuder, Norbert, and Kraas, Birk
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SOLAR radiation , *SOLAR receivers , *RADIATION , *CALIBRATION , *ELECTRONIC data processing - Abstract
Because of forward scattered radiation in the atmosphere, the circumsolar region closely surrounding the solar disk looks very bright. The radiation coming from this region, the circumsolar radiation, is in large part included in direct normal irradiance (DNI) measurements at the usual 2.5° pyrheliometer opening half angle, but only partially intercepted by the receivers of focusing solar collectors. Therefore, circumsolar radiation measurements are recommended to be included in solar resource assessment. Circumsolar radiation can be characterized using the radial angular distribution of the radiance around the center of the sun - the so-called sunshape. Several sunshape measurement methods have been developed recently. Most approaches use cameras or pyrheliometers with different apertures which require daily maintenance. The Rotating Shadowband Irradiometer (RSI) based method discussed here uses a conventional RSI without any hardware modification to enable sunshape measurements without affecting the RSI's fundamental function as a DNI measurement device. Thus, it allows to measure circumsolar radiation without any additional hardware and with significantly lower maintenance requirements. The presented RSI-based sunshape measurement algorithm has been validated with four RSIs and more than two years of data. After a short description of the method to derive the circumsolar contribution, the validation results are shown. Then the required calibration method is discussed, followed by the results from the measurement campaigns at four sites in Spain, India and Morocco. It was found that no individual calibration is required per instrument and the algorithm can be used for automatic data processing so that common RSI stations can measure the sunshape with comparably low extra effort. Furthermore, we explain how to derive sunshapes from the RSI measurements. [ABSTRACT FROM AUTHOR]
- Published
- 2018
- Full Text
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5. Techno-Economic Analysis of Receiver Replacement Scenarios in a Parabolic Trough Field.
- Author
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Röger, Marc, Lüpfert, Eckhard, Caron, Simon, and Dieckmann, Simon
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SOLAR receivers , *PARABOLIC troughs , *HEAT losses , *SOLAR power plants , *TEMPERATURE effect , *ANTIREFLECTIVE coatings - Abstract
The heat loss of an evacuated parabolic trough receiver of solar thermal power plants ranges typically between values below 150 and 200 W/m at 350?C. Defects, such as glass breakage by wind events and coating degradation, antireflection coating degradation or hydrogen accumulation in the annulus, decrease the annual electricity production. This study examines the effect of different receiver performance loss scenarios on the energetic and economic output of a modern 150-MWel-parabolic trough plant with 7.5-hours molten-salt storage, located in Ma'an, Jordan over the whole lifetime by modeling it in an extended version of the software greenius. Compared to the reference scenario, a wind event in year 5 (10, 15) causing glass envelope breakage and consequential degradation of the selective coating of 5.6% of the receivers reduces the electricity output by 5.1% (3.8%, 2.5%), the net present value is reduced by 36.5% (23.1%,13.1%). The payback time of receiver replacement is only 0.7 years and hence this measure is recommended. The highest negative impact on performance and net present value of a project has the hydrogen accumulation scenario (50% of field affected) in event year 5 (10,15) reducing net electric output by 10.7% (8.1%, 5.4%) and the net present value by 77.0% (48.7%, 27.6%). Replacement of the receivers or even better an inexpensive repair solution is an energetically and economically sensible solution. The option of investing in premium receivers with Xe-capsule during the construction phase is a viable option if the surplus cost for premium receivers is lower than 10 to 20 percent. [ABSTRACT FROM AUTHOR]
- Published
- 2016
- Full Text
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6. Efficiency determination of tubular solar receivers in central receiver systems.
- Author
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Ebert, Miriam, Benitez, Daniel, Röger, Marc, Korzynietz, Roman, and Brioso, José Antonio
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SOLAR receivers , *ACTINIC flux , *SOLAR gas turbines , *THERMORECEPTORS , *SOLAR energy - Abstract
This paper describes a method for the efficiency determination of a cavity receiver using the example of the solar hybrid gas turbine system SOLUGAS. Major focus is given on the improvement of a new approach of the solar flux density determination based on a measurement-supported simulation technique where an acceptable uncertainty of the solar input power of −1.3%…+6.3% is achieved. For the thermal evaluation an uncertainty of 2.4% is determined that leads to an overall uncertainty of the thermal receiver efficiency of −2.8%…+7.7%. Detailed uncertainty propagation is presented and conclusions discussed. [ABSTRACT FROM AUTHOR]
- Published
- 2016
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7. Intercomparison of opto-thermal spectral measurements for concentrating solar thermal receiver materials from room temperature up to 800 °C.
- Author
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Caron, Simon, Farchado, Meryem, San Vicente, Gema, Morales, Angel, Ballestrín, Jesus, Carvalho, Maria Joao, Pascoa, Soraia, le Baron, Estelle, Disdier, Angela, Guillot, Emmanuel, Escape, Christophe, Sans, Jean-Louis, Binyamin, Yaniv, Baidossi, Mubeen, Sutter, Florian, Röger, Marc, and Manzano-Agugliaro, Francisco
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SOLAR receivers , *SURFACE finishing , *SOLAR energy , *SILICON carbide , *TEMPERATURE , *STANDARD deviations - Abstract
An intercomparison of opto-thermal spectral measurements has been performed for some relevant receiver materials in concentrating solar thermal applications, from room temperature up to 800°C. Five European laboratories performed spectral measurements at room temperature, while two laboratories performed infrared spectral measurements at operating temperature up to 800 °C. Relevant materials include Haynes 230 (oxidized, Pyromark 2500 and industrial black coating) and silicon carbide. Two key figures of merit were analyzed: i) solar absorptance α sol at room temperature, over the spectral range [0.3 – 2.5] μm, ii) thermal emittance ε th (T), over the common spectral range [2-14] μm, derived from spectral measurements performed from room temperature up to 800 °C. Oxidized H230 reached an α sol value of 90.9±1.0%. Pyromark 2500 reached an α sol value of 96.3±0.5%, while the industrial black coating achieved an α sol value of 97.0±0.4%. Silicon carbide reached an α sol value of 93.5±1.1%. Low standard deviations in α sol indicate reproducible measurements at room temperature. For oxidized H230, the ε th,calc (T) value varied from 55% at room temperature up to 81% at 800 °C. For Pyromark 2500 and the industrial black coating, ε th,calc (T) fluctuated between 90% and 95%, with a weak temperature dependence. For silicon carbide, ε th,calc (T) varied from 70% at room temperature up to 86% at 800 °C. The typical standard deviation among participating laboratories is about 3%. ε th,meas (T) values derived from spectral measurements at operating temperature were consistent within a few percentage points in comparison to ε th,calc (T) values derived from spectral measurements at room temperature. • Spectral measurements of receiver materials for Concentrating Solar Power are performed from room temperature up to 800 °C. • Material substrates include H230 and SiC. Three different surface finishes are investigated for H230 (oxide, black coatings). • Solar absorptance is analyzed at room temperature, while thermal emittance is analyzed from room temperature up to 800°C. [ABSTRACT FROM AUTHOR]
- Published
- 2024
- Full Text
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8. Laboratory intercomparison of solar absorptance and thermal emittance measurements at room temperature.
- Author
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Caron, Simon, Herding, Leslie, Binyamin, Yaniv, Baidossi, Mubeen, Vinetsky, Yelena, Morales, Angel, Hildebrandt, Christina, Reoyo-Prats, Reine, Faugeroux, Olivier, Agüero, Alina, Rodriguez, Sergio, Sutter, Florian, Röger, Marc, and Manzano-Agugliaro, Francisco
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SPECTROPHOTOMETERS , *TEMPERATURE measurements , *REFLECTANCE measurement , *SOLAR energy , *SOLAR receivers , *SOLAR spectra , *REFLECTOMETER - Abstract
Solar thermal absorber coatings play an important role in the opto-thermal efficiency of receivers in Concentrated Solar Power (CSP). Two standard figures of merit are the solar absorptance α sol and thermal emittance ε th , derived from spectral directional hemispherical reflectance measurements at room temperature. These two figures of merit allow comparing coating formulations in terms of performance and durability. In this study, a black coating and a solar selective coating are optically characterized by different laboratories to compare spectral datasets, solar absorptance α sol and thermal emittance ε th calculations. The comparison includes various benchtop spectrophotometers operating in the UV-VIS-NIR and Infrared spectral ranges as well as three commercial portable reflectometers/emissometers. A good agreement is found between the nine parties participating in this intercomparison campaign. The black coating α sol value is 96.6 ± 0.2%, while the solar selective coating α sol value is 94.5 ± 0.4%. For the thermal emittance, spectral data is concatenated and integrated from 0.3 to 16 μm. The black coating ε th value calculated at 650 °C is 80.8 ± 3.8%, while the solar selective coating ε th value calculated at 650 °C is 25.0 ± 0.5%. • Spectral measurements of absorber coatings are compared at room temperature. • Spectral mismatch from 1.5 to 2.5 μm is analyzed for spectrophotometers. • Solar absorptance and thermal emittance calculations are homogenized. • The uncertainty propagation on the coating opto-thermal efficiency is evaluated. [ABSTRACT FROM AUTHOR]
- Published
- 2022
- Full Text
- View/download PDF
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