The Experts below are selected from a list of 4242 Experts worldwide ranked by ideXlab platform
A. De Miguel - One of the best experts on this subject based on the ideXlab platform.
-
Spectral attenuation of global and Diffuse UV Irradiance and actinic flux by clouds
Quarterly Journal of the Royal Meteorological Society, 2014Co-Authors: David Mateos, A. De Miguel, A. Di Sarra, Julia Bilbao, Daniela Meloni, G. Pace, Giampietro CasasantaAbstract:Measurements of spectral global and Diffuse ultraviolet (UV) Irradiance, and of spectral actinic flux were made jointly with determinations of cloud properties during a two- month experimental campaign that took place in southern Italy in May–June 2010. The cloud modification factor (CMF) which is the ratio between the incoming radiation under cloudy and in cloud-free conditions, was obtained for the global (direct plus Diffuse) and Diffuse components of the Irradiance, and for the actinic flux in the UV spectral range for overcast conditions. Measurements of the Diffuse Irradiance and actinic flux CMFs are very scarce, and are particularly important to characterize the radiation field and verify the behaviour of radiative transfer models in cloudy conditions. In addition to measurements, one-dimensional radiative transfer simulations are used to investigate the cloud influence on the spectral solar UV radiation. The analysis shows that the wavelength dependence of CMF for the global Irradiance is mainly due to the normalization for cloud-free conditions. The CMF for the Diffuse Irradiance and for the actinic flux displays a strong dependence on the solar zenith angle. This dependence appears to be mainly driven by the large role played by the zenith radiation in overcast conditions. Radiative transfer model determinations of CMF satisfactorily reproduce observations.
-
global Diffuse direct and ultraviolet solar Irradiance recorded in malta and atmospheric component influences
Energy Procedia, 2014Co-Authors: Javier Bilbao, Charles Yousif, Ana Perezburgos, Roberto Román, A. De MiguelAbstract:Abstract Global and Diffuse shortwave (SW) and global erythemal (UVER) Irradiances were measured in Malta, in the middle of Mediterranean Sea. The effect of solar zenith angle on these Irradiances is studied using the measurements and simulations developed with a radiative transfer model. The role of ozone, scattering by gases, and aerosols is analyzed. Results show that ozone and Rayleigh scattering are the main drivers responsible for the behavior of UVER variations with SZA. In the case of global and Diffuse Irradiance, the role of aerosols is the principal determinant.
-
evaluation of the desert dust effects on global direct and Diffuse spectral ultraviolet Irradiance
Tellus B, 2013Co-Authors: Roberto Román, A. De Miguel, Javier Bilbao, F.j. Olmo, M Anton, A Valenzuela, J E Gil, H Lyamani, L AladosarboledasAbstract:This paper presents a study of a strong desert dust episode over the Iberian Peninsula, and its effect on the spectral ultraviolet (UV) Irradiance in Granada, Spain. Remote sensing measurements, forecast models, and synoptic analysis are used to identify a Saharan desert dust outbreak that affected the Iberian Peninsula starting 20 July 2009. Additionally, a Bentham DMc150 spectroradiometer is employed to obtain global, direct and Diffuse spectral UV Irradiances every 15 minutes in Granada. The desert dust caused a large attenuation of the direct UV Irradiance (up to 55%), while the Diffuse UV Irradiance increased up to 40% at 400 nm. The UVSPEC/LibRadtran radiative transfer model is used to study the spectral dependence of the experimental UV Irradiance ratios (ratios of spectral Irradiance for the day with the highest aerosol load to that measured in days with lowmoderate load). The spectral increase or decrease of the UV direct Irradiance ratios depends on a new parameter: a threshold wavelength. The spectral dependence of the UV Diffuse Irradiance ratio can be explained because under the influence of the intense dust outbreak, the Mie scattering by aerosols at shorter wavelengths is stronger than the Rayleigh scattering by gases. Finally, the sensitivity analysis of the aerosol absorption properties shows a substantial attenuation of UV spectral Irradiance with a weak spectral dependence. Keywords: spectral radiation, desert dust, ultraviolet, aerosol, Diffuse Irradiance, Bentham (Published: 18 January 2013) Citation: Tellus B 2013, 65 , 19578, http://dx.doi.org/10.3402/tellusb.v65i0.19578
-
measurement and comparison of Diffuse solar Irradiance models on inclined surfaces in valladolid spain
Energy Conversion and Management, 2005Co-Authors: M Diezmediavilla, A. De Miguel, J BilbaoAbstract:Abstract This paper presents the performance of 10 arithmetic models used to estimate Diffuse solar Irradiance on inclined surfaces in a comparative study with actual data readings made available on an hourly and a daily basis. The data readings have been taken from a south facing surface inclined at 42° in an area at some distance from the provincial capital in the Spanish province of Valladolid. In order to confirm the results, three statistical parameters have been used in the study; root mean square error (RMSE), mean bias error (MBE) and Stone’s t-statistic. The results obtained favour the Muneer model, followed by the Reindl model, for hourly as well as for daily values. The Temps–Coulson model gives rise to great discrepancies with respect to the values measured. The results for the Perez model are not good due to the use of parameters that are not specifically calculated for the area in this study, which underlines the need to take an area’s features into account so that predictions for Diffuse Irradiance measured on inclined surfaces may be as accurate as possible.
F.j. Olmo - One of the best experts on this subject based on the ideXlab platform.
-
evaluation of the desert dust effects on global direct and Diffuse spectral ultraviolet Irradiance
Tellus B, 2013Co-Authors: Roberto Román, A. De Miguel, Javier Bilbao, F.j. Olmo, M Anton, A Valenzuela, J E Gil, H Lyamani, L AladosarboledasAbstract:This paper presents a study of a strong desert dust episode over the Iberian Peninsula, and its effect on the spectral ultraviolet (UV) Irradiance in Granada, Spain. Remote sensing measurements, forecast models, and synoptic analysis are used to identify a Saharan desert dust outbreak that affected the Iberian Peninsula starting 20 July 2009. Additionally, a Bentham DMc150 spectroradiometer is employed to obtain global, direct and Diffuse spectral UV Irradiances every 15 minutes in Granada. The desert dust caused a large attenuation of the direct UV Irradiance (up to 55%), while the Diffuse UV Irradiance increased up to 40% at 400 nm. The UVSPEC/LibRadtran radiative transfer model is used to study the spectral dependence of the experimental UV Irradiance ratios (ratios of spectral Irradiance for the day with the highest aerosol load to that measured in days with lowmoderate load). The spectral increase or decrease of the UV direct Irradiance ratios depends on a new parameter: a threshold wavelength. The spectral dependence of the UV Diffuse Irradiance ratio can be explained because under the influence of the intense dust outbreak, the Mie scattering by aerosols at shorter wavelengths is stronger than the Rayleigh scattering by gases. Finally, the sensitivity analysis of the aerosol absorption properties shows a substantial attenuation of UV spectral Irradiance with a weak spectral dependence. Keywords: spectral radiation, desert dust, ultraviolet, aerosol, Diffuse Irradiance, Bentham (Published: 18 January 2013) Citation: Tellus B 2013, 65 , 19578, http://dx.doi.org/10.3402/tellusb.v65i0.19578
-
global and Diffuse shortwave Irradiance during a strong desert dust episode at granada spain
Atmospheric Research, 2012Co-Authors: M Anton, F.j. Olmo, A Valenzuela, J E Gil, H Lyamani, A Cazorla, J Fernandezgalvez, I Foyomoreno, L AladosarboledasAbstract:Abstract This paper studies the influence of a strong Saharan dust event on Diffuse and global (direct + Diffuse) shortwave Irradiance (0.305 to 2.800 μm) recorded at Granada (South Spain) during 6 September 2007. The contribution of coarse mineral dust particles to the aerosol load was evidenced from the large aerosol optical depth (AOD, between 0.8 and 1.5) and the small Angstrom exponent (between 0.1 and 0.25) values recorded by a sun-photometer. Global Irradiance on 6 September decreased about 20% compared to low-aerosol load days, while Diffuse Irradiance increased 200–400% around solar noon. On that day, the Diffuse component was nearly 60% of the global Irradiance at 12:00 UTC and therefore the direct component was substantially reduced. The aerosol forcing efficiency (radiative forcing per unit of AOD) during this strong event was higher than most of the desert dust forcing efficiencies reported in the literature; an increase of one unit in the AOD at 440 nm led to a decrease in global solar Irradiance at the surface of 123 W/m2. Additionally, low values of the single scattering albedo at 440 nm (mean value 0.90 ± 0.2) in relation to pure desert dust episodes were indicative of absorbing anthropogenic particles from the European and Mediterranean regions.
-
one minute kb and kd probability density distributions conditioned to the optical air mass
Solar Energy, 1999Co-Authors: J Tovar, F.j. Olmo, F J Batlles, L AladosarboledasAbstract:In this work we have analysed and modelled one-minute probability distribution function of solar direct and Diffuse Irradiance conditioned to the optical air mass. For this purpose, we have used one-minute data acquired in a radiometric station located in southeastern Spain (37.13° N, 3.63° W, 687 m a.m.s.l.). The study has been made over the dimensionless indices kb and kd. We have found marked bimodality in the kb distribution function and asymmetry associated with the unimodal function of one-minute kd values. In spite of these differences, we have modelled both distribution functions using a functional form based on Botlzmann's statistics. These functions have been used in a previous study devoted to modelling the clearness index for global radiation, kt. In order to model the asymmetry that is evident in the kd and kb distribution functions, the functional forms have been modified by the inclusion of an additional parameter. The adjustable parameters included in the model equations present a dependence on the optical air mass.
-
Solar radiation resource assessment by means of silicon cells
Solar Energy, 1995Co-Authors: Lucas Alados-arboledas, Francisco Javier Batlles, F.j. OlmoAbstract:Abstract To provide an accurate solar resource assessment, radiometric stations measuring global, Diffuse, and direct Irradiance must be widespread. Nevertheless, the high capital costs of thermopile instruments, usually used in pyranometry, represent an important obstacle. Therefore, silicon photovoltaic sensors have emerged as a more accessible alternative than standard thermopile sensors. However, their temperature and spectral responses must be taken into account in order to match silicon cells and thermopile responses. Global and Diffuse Irradiance have been measured from early 1990 to the end of 1992 in Almeria, southeastern Spain, by means of thermopile and photovoltaic sensor. Polar axis shadowbands were employed to measure the Diffuse Irradiance. These 10-minute coincident data sets, covering a complete range of atmospheric conditions, have been used to develop a correction procedure for the silicon detector measurements. Before the correction procedure was applied severe discrepancies were found, especially for the Diffuse Irradiance measurements performed under clear skies. Results of the correction method applied to an independent data set show a remarkable improvement. After correction, the comparison of silicon cell measurements with those obtained by means of thermopile pyranometers leads to a root mean square deviation of about 4% and 5% over the mean value of global and Diffuse horizontal Irradiance, respectively.
L Aladosarboledas - One of the best experts on this subject based on the ideXlab platform.
-
evaluation of the desert dust effects on global direct and Diffuse spectral ultraviolet Irradiance
Tellus B, 2013Co-Authors: Roberto Román, A. De Miguel, Javier Bilbao, F.j. Olmo, M Anton, A Valenzuela, J E Gil, H Lyamani, L AladosarboledasAbstract:This paper presents a study of a strong desert dust episode over the Iberian Peninsula, and its effect on the spectral ultraviolet (UV) Irradiance in Granada, Spain. Remote sensing measurements, forecast models, and synoptic analysis are used to identify a Saharan desert dust outbreak that affected the Iberian Peninsula starting 20 July 2009. Additionally, a Bentham DMc150 spectroradiometer is employed to obtain global, direct and Diffuse spectral UV Irradiances every 15 minutes in Granada. The desert dust caused a large attenuation of the direct UV Irradiance (up to 55%), while the Diffuse UV Irradiance increased up to 40% at 400 nm. The UVSPEC/LibRadtran radiative transfer model is used to study the spectral dependence of the experimental UV Irradiance ratios (ratios of spectral Irradiance for the day with the highest aerosol load to that measured in days with lowmoderate load). The spectral increase or decrease of the UV direct Irradiance ratios depends on a new parameter: a threshold wavelength. The spectral dependence of the UV Diffuse Irradiance ratio can be explained because under the influence of the intense dust outbreak, the Mie scattering by aerosols at shorter wavelengths is stronger than the Rayleigh scattering by gases. Finally, the sensitivity analysis of the aerosol absorption properties shows a substantial attenuation of UV spectral Irradiance with a weak spectral dependence. Keywords: spectral radiation, desert dust, ultraviolet, aerosol, Diffuse Irradiance, Bentham (Published: 18 January 2013) Citation: Tellus B 2013, 65 , 19578, http://dx.doi.org/10.3402/tellusb.v65i0.19578
-
global and Diffuse shortwave Irradiance during a strong desert dust episode at granada spain
Atmospheric Research, 2012Co-Authors: M Anton, F.j. Olmo, A Valenzuela, J E Gil, H Lyamani, A Cazorla, J Fernandezgalvez, I Foyomoreno, L AladosarboledasAbstract:Abstract This paper studies the influence of a strong Saharan dust event on Diffuse and global (direct + Diffuse) shortwave Irradiance (0.305 to 2.800 μm) recorded at Granada (South Spain) during 6 September 2007. The contribution of coarse mineral dust particles to the aerosol load was evidenced from the large aerosol optical depth (AOD, between 0.8 and 1.5) and the small Angstrom exponent (between 0.1 and 0.25) values recorded by a sun-photometer. Global Irradiance on 6 September decreased about 20% compared to low-aerosol load days, while Diffuse Irradiance increased 200–400% around solar noon. On that day, the Diffuse component was nearly 60% of the global Irradiance at 12:00 UTC and therefore the direct component was substantially reduced. The aerosol forcing efficiency (radiative forcing per unit of AOD) during this strong event was higher than most of the desert dust forcing efficiencies reported in the literature; an increase of one unit in the AOD at 440 nm led to a decrease in global solar Irradiance at the surface of 123 W/m2. Additionally, low values of the single scattering albedo at 440 nm (mean value 0.90 ± 0.2) in relation to pure desert dust episodes were indicative of absorbing anthropogenic particles from the European and Mediterranean regions.
-
one minute kb and kd probability density distributions conditioned to the optical air mass
Solar Energy, 1999Co-Authors: J Tovar, F.j. Olmo, F J Batlles, L AladosarboledasAbstract:In this work we have analysed and modelled one-minute probability distribution function of solar direct and Diffuse Irradiance conditioned to the optical air mass. For this purpose, we have used one-minute data acquired in a radiometric station located in southeastern Spain (37.13° N, 3.63° W, 687 m a.m.s.l.). The study has been made over the dimensionless indices kb and kd. We have found marked bimodality in the kb distribution function and asymmetry associated with the unimodal function of one-minute kd values. In spite of these differences, we have modelled both distribution functions using a functional form based on Botlzmann's statistics. These functions have been used in a previous study devoted to modelling the clearness index for global radiation, kt. In order to model the asymmetry that is evident in the kd and kb distribution functions, the functional forms have been modified by the inclusion of an additional parameter. The adjustable parameters included in the model equations present a dependence on the optical air mass.
M Diezmediavilla - One of the best experts on this subject based on the ideXlab platform.
-
shadow band radiometer measurement of Diffuse solar Irradiance calculation of geometrical and total correction factors
Solar Energy, 2016Co-Authors: Miguel De Simonmartin, M Diezmediavilla, Cristina AlonsotristanAbstract:Abstract Among the various methods of measuring Diffuse solar Irradiance, shadowing devices are ones of the most commonly used in solar research all over the world. These instruments work with a basic pyranometer, properly calibrated for the measurement of solar Irradiance, with a shadowing element, which can be a disk or a band (Drummond’s shadow-band), that prevents the direct incidence of solar beam Irradiance on the sensor. This method is capable of precise measurements, but sensor outputs have to be corrected, so as to quantify the amount of Diffuse Irradiance that the band blocks from reaching the sensor. Several authors have advanced different expressions for this correction factor, most of which only apply to horizontal and equator-oriented tilting pyranometers. In this work, we present a general approach to calculate the geometrical correction factor for a tilted sensor, oriented towards all possible azimuth and zenith angles, which permits the measurement of solar Diffuse Irradiance on any tilted and oriented surfaces. Furthermore, five total correction models are adapted for measurement in any given direction and evaluated on vertical walls pointing the four cardinal directions. Our results show that geometrical correction improves the Mean Bias Difference (MBD), the Root Mean Squared Difference (RMSD) and the μ 0.99 statistics by 60%, 62% and 56%, respectively, in contrast with the raw data. The LeBaron et al. model gives the most accurate figure for total correction according to MBD, RMSD and μ 0.99 statistics, with promising average performances of 97%, 91%, and 96%, respectively.
-
new device for the simultaneous measurement of Diffuse solar Irradiance on several azimuth and tilting angles
Solar Energy, 2015Co-Authors: Miguel De Simonmartin, Cristina Alonsotristan, D Gonzalezpena, M DiezmediavillaAbstract:Abstract A device is proposed for the measurement of Diffuse solar Irradiance on tilted surfaces pointing-to as well as fixed on the equatorial direction. Most commercial devices are not designed for this purpose. Here, we present a specific design for a system based on a single multi-lobe shadow-ring that allows us to measure Diffuse Irradiance with several tilted pyranometers – from 60 to 90 degrees from the horizontal plane – and on different azimuth angles. This first prototype allows us to measure in the four cardinal directions. The ring is designed to minimize the covered celestial dome observed by each sensor. Moreover, the complete device needs a very small installation area and its simplicity means it is inexpensive and easy to operate. The measurements have subsequently to be corrected with a geometrical correction factor that takes into account the portion of the sky vault blocked by the shadow-ring. These measurements are essential for estimating solar potential on tilted surfaces – such as building facades – and for improving current anisotropic solar models, among many other applications.
-
measurement and comparison of Diffuse solar Irradiance models on inclined surfaces in valladolid spain
Energy Conversion and Management, 2005Co-Authors: M Diezmediavilla, A. De Miguel, J BilbaoAbstract:Abstract This paper presents the performance of 10 arithmetic models used to estimate Diffuse solar Irradiance on inclined surfaces in a comparative study with actual data readings made available on an hourly and a daily basis. The data readings have been taken from a south facing surface inclined at 42° in an area at some distance from the provincial capital in the Spanish province of Valladolid. In order to confirm the results, three statistical parameters have been used in the study; root mean square error (RMSE), mean bias error (MBE) and Stone’s t-statistic. The results obtained favour the Muneer model, followed by the Reindl model, for hourly as well as for daily values. The Temps–Coulson model gives rise to great discrepancies with respect to the values measured. The results for the Perez model are not good due to the use of parameters that are not specifically calculated for the area in this study, which underlines the need to take an area’s features into account so that predictions for Diffuse Irradiance measured on inclined surfaces may be as accurate as possible.
Thomas Stoffel - One of the best experts on this subject based on the ideXlab platform.
-
solar and infrared radiation measurements
2012Co-Authors: Frank Vignola, Joseph J. Michalsky, Thomas StoffelAbstract:Measuring Solar and Infrared Radiation Solar Resource Definitions and Terminology Introduction The Sun Extraterrestrial Radiation Solar Coordinates Zenith, Azimuth, and Hour Angles Solar, Universal, and Local Standard Time Solar Position Calculation Sunrise and Sunset Times Global, Direct Normal, and Diffuse Irradiance Solar Radiation on Tilted Surfaces Spectral Nature of Solar Radiation Fundamentals of Thermodynamics and Heat Transfer Photodiodes and Solar Cell Prerequisites Models Historic Milestones in Solar and Infrared Radiation Measurement Introduction Earliest Observations of the Sun and the Nature of Light Nineteenth-Century Radiometers Operational Radiometers of the Twentieth Century Recent Advances in Solar Measurements Direct Normal Irradiance Overview of Direct Normal Irradiance Pyrheliometer Geometry Operational Thermopile Pyrheliometers Absolute Cavity Radiometers Uncertainty Analysis for Pyrheliometer Calibration Uncertainty Analysis for Operational Thermopile Pyrheliometers Uncertainty Analysis for Rotating Shadowband Radiometer Measurements of Direct Normal Irradiance Direct Normal Irradiance Models Historical and Current Surface-Measured Direct Normal Irradiance Data Measuring Global Irradiance Introduction to Global Horizontal Irradiance Measurements Black-Disk Thermopile Pyranometers Black-and-White Pyranometers Photodiode-Based Pyranometers Calibration of Pyranometers Pyranometer Calibration Uncertainties Diffuse Irradiance Introduction The Measurement of Diffuse Irradiance Calibration of Diffuse Pyranometers Value of Accurate Diffuse Measurements Rotating Shadowband Radiometers Introduction The Rotating Shadowband Radiometer The Multifilter Rotating Shadowband Radiometer Measuring Solar Radiation on a Tilted Surface Introduction Effect of Tilt on Single Black Detector Pyranometers Effect of Tilt on Black-and-White Pyranometers Effect of Tilt on Photodiode Pyranometers Recommendations for Tilted Irradiance Measurements Notes on Modeling PV System Performance with Photodiode Pyranometers Albedo Introduction Broadband Albedo Spectral Albedo Bidirectional Reflectance Distribution Function Albedo Measurements Infrared Measurements Introduction Pyrgeometers Calibration Improved Calibrations Other Pyrgeometer Manufacturers Operational Considerations Net Radiation Measurements Introduction Single-Sensor (All-Wave) Net Radiometers Two-Sensor Net Radiometers Four-Sensor Net Radiometers Accuracy of Net Radiometers A Better Net Radiation Standard Net Radiometer Sources Solar Spectral Measurements Introduction The Extraterrestrial Solar Spectrum Atmospheric Interactions Broadband Filter Radiometry Narrow-Band Filter Radiometry Spectrometry Meteorological Measurements Introduction Ambient Temperature Wind Speed and Wind Direction Relative Humidity Pressure Recommended Minimum Accuracies for Operational Instruments Setting Up a Solar Monitoring Station Introduction Choosing a Site Grounding and Shielding Data Logger and Communications Measurement Interval Cleaning and Maintenance Record Keeping Importance of Reviewing Data Quality Control of Data Field Calibrations Physical Layout of a Solar-Monitoring Station Appendix A: Modeling Solar Radiation Appendix B: Solar Radiation Estimates Derived from Satellite Measurements Appendix C: Sun Path Charts Appendix D: Solar Position Algorithms Appendix E: Useful Conversion Factors Appendix F: Sources for Equipment Appendix G: BORCAL Report Appendix H: Sunshine Duration Appendix I: Failure Modes
-
further developments in closure experiments for surface Diffuse Irradiance under cloud free skies at a continental site
Geophysical Research Letters, 2004Co-Authors: Rangasayi N Halthore, Donald W Slater, Mark A Miller, J A Ogren, Patrick J Sheridan, Thomas StoffelAbstract:[1] Direct and Diffuse surface Irradiances measured with the shaded and ventilated Black and White Eppley pyranometer under cloud-free skies at a continental site are compared with radiative transfer model calculated values. For the measurements in 2002, calculations of Irradiance utilizing surface-measured aerosol single scattering albedo (SSA) agree with that measured to within the mutual uncertainties. For the days in 2001 and 2003, the modeled Irradiance values agree with that measured only if highly absorbing aerosols of SSA ∼0.7, well below surface-measured SSA, are used. Modeled Diffuse/direct Irradiance ratios continue to exceed those measured in the visible and near-IR using silicon detector-based radiometers, suggesting problems with measurements and/or model estimates of atmospheric, most likely, aerosol, absorption. A detailed study is therefore required to establish the role of aerosol absorption in shortwave radiative transfer.
-
measurement of broadband Diffuse solar Irradiance using current commercial instrumentation with a correction for thermal offset errors
Journal of Atmospheric and Oceanic Technology, 2001Co-Authors: Ellsworth G Dutton, Thomas Stoffel, J J Michalsky, Bruce W Forgan, John R Hickey, Donald W Nelson, Timothy L Alberta, Ibrahim RedaAbstract:Abstract Diffuse-sky solar Irradiance is an important quantity for radiation budget research, particularly as it relates to climate. Diffuse Irradiance is one component of the total downwelling solar Irradiance and contains information on the amount of downward-scattered, as opposed to directly transmitted, solar radiation. Additionally, the Diffuse component is often required when calibrating total Irradiance radiometers. A variety of pyranometers are commonly used to measure solar Diffuse Irradiance. An examination of some instruments for measuring Diffuse Irradiance using solar tracking shade disks is presented, along with an evaluation of the achieved accuracy. A data correction procedure that is intended to account for the offset caused by thermal IR exchange between the detector and filter domes in certain common Diffuse pyranometers is developed and validated. The correction factor is derived from outputs of a collocated pyrgeometer that measures atmospheric infrared Irradiance.