The aim of this study is to perform a comparative analysis of Italian and Spanish regulations for construction and demolition (C&D) waste management, to produce recycled aggregates (RAs). Furthermore, this study seeks to compare the results derived from the examination of leaching test results from RAs collected in both countries to identify the most critical pollutants. Our research involved a comprehensive comparison and analysis of waste management regulations in Italy and Spain, highlighting both commonalities and disparities.
View Article and Find Full Text PDFCompared to other age groups, 18- to 25-year olds (young adults) are more likely to engage in heavy alcohol use and inconsistent contraceptive use, increasing their susceptibility to sexually transmitted infections (STIs) and unintended pregnancy. The Studying Alcohol and Related Risks (STARR) intervention was efficacious in reducing young adult alcohol-related risky sexual behavior, including reducing the number of casual sexual partners and alcohol use prior to sex. We conducted a qualitative study to guide the adaptation of the STARR intervention to include additional content on contraceptive use and prepare for dissemination of the intervention to a community audience.
View Article and Find Full Text PDFIntroduction: Ovarian cancer (OC) is the eighth most common cancer in women, with a poor prognosis, particularly in older women. The aim of this study was to describe an octogenarian population with OC and to examine the differences in net survival (NS) according to age.
Material And Methods: In this retrospective observational population-based study from a gynecological cancer registry, patients aged > 18 years with an identified epithelial ovarian cancer stage IA to IVB diagnosed between 1998 and 2018 were included.
Based on decades of single-spacecraft measurements near 1 au as well as data from heliospheric and planetary missions, multi-spacecraft simultaneous measurements in the inner heliosphere on separations of 0.05-0.2 au are required to close existing gaps in our knowledge of solar wind structures, transients, and energetic particles, especially coronal mass ejections (CMEs), stream interaction regions (SIRs), high speed solar wind streams (HSS), and energetic storm particle (ESP) events.
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