@Article{CeballosPorfOricPoss:2022:ChAnRe,
author = "Ceballos, Juan Carlos and Porfirio, Anthony Carlos Silva and
Oricchi, Patricio Alberto and Posse, Gabriela",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and Instituto de Clima y
Agua, Centro de Investigaci{\'o}n de Recursos Naturales (CIRN)
and Instituto de Clima y Agua, Centro de Investigaci{\'o}n de
Recursos Naturales (CIRN)",
title = "Characterization of the annual regime of surface solar irradiance
over Argentine Pampean Region using GL1.2 satellite-based data",
journal = "Renewable Energy",
year = "2022",
volume = "194",
pages = "526--537",
month = "July",
keywords = "Argentine pampa, GL model, Satellite-based data, Shortwave
radiation climate, Solar radiation, Time series periodicities.",
abstract = "Detailed description of the solar resource (spatial distribution
and temporal variations) is highly desirable in the context of
climate monitoring, agricultural planning and energy technologies;
however, one shortcoming is the low density of solarimetric
networks in many extended regions. Satellite-based estimations
have become a potential key tool, provided their data show
adequate temporal frequency, high resolution and acceptable
accuracy. GL1.2 Model currently runs at Brazilian National
Institute for Space Research (CPTEC/INPE), based on GOES VIS
channel imagery. It was tested for characterizing solar radiation
regime over Pampa Region in Argentina, which extends over more
than 600,000 km2. Comparison with time series of nine stations of
the Pampa network in the period 20112018 showed close agreement
for daily mean irradiance using 10-days as well as monthly values
(mean bias error generally |MBE| < 6 W m-2 standard deviation STD
\≈ 10-15 W m-2 and resulting root mean square error RMSE
\≈ 1016 W m\−2). Completeness of GL time series and
high spatial definition (0.04°) allowed further time and space
analysis of solar radiation regime. It confirmed that Pampean
region is rather homogeneous with annual mean GL increasing from
185 W m\−2 on coastal region up to 220 W m\−2 on the
western and northern limits. In addition, GL data detects sharper
variations in a scale of few kilometers, such as transition
between ground and water in oceanic coast or large rivers.
Regional interannual variability is low: COV \≈ 34%. All
stations in Pampa network show a well definite annual cycle,
closely followed by GL estimates. Fourier analysis for GL monthly
series shows a dominant deterministic one year signal (H8
harmonic), accounting for 9395% of variance for all stations and
throughout the Pampa region, in phase with the end of Southern
Hemisphere spring. The H8 amplitude varies from 100 W m\−2
along inner continental boundary up to 120 in southwestern and
coastal bound. It is concluded that GL 1.2 model data can be used
to accurately describe time series of daily mean irradiance, for
10-days and monthly scales and 4 km resolution, providing a Test
Reference Year (TRY). This is precious in order to describe
spatial-temporal patterns of regional solar climate. An otherwise
random signal of 20 W m\−2 is associated to transient
meteorological phenomena with durations shorter than 10-days, such
as cold fronts or convective activity. Their deterministic and/or
statistical structure could be improved by the combined analysis
of short-time scales Pampa network and GL data (daily, hourly or
even minutely).",
doi = "10.1016/j.renene.2022.05.038",
url = "http://dx.doi.org/10.1016/j.renene.2022.05.038",
issn = "0960-1481",
language = "en",
targetfile = "1-s2.0-S0960148122006796-main.pdf",
urlaccessdate = "06 jun. 2024"
}