Matches in SemOpenAlex for { <https://semopenalex.org/work/W2109308722> ?p ?o ?g. }
- W2109308722 endingPage "7404" @default.
- W2109308722 startingPage "7395" @default.
- W2109308722 abstract "Abstract. Particulate matter mass concentrations measured in the city of Rome (Italy) in the period 2001–2004 have been cross-analysed with concurrent Saharan dust advection events to infer the impact these natural episodes bear on the standard air quality parameter PM10 observed at two city stations and at one regional background station. Natural events such as Saharan dust advections are associated with a definite health risk. At the same time, the Directive 2008/50/EC allows subtraction of PM exceedances caused by natural contributions from statistics used to determine air quality of EU sites. In this respect, it is important to detect and characterise such advections by means of reliable, operational techniques. To assess the PM10 increase we used both the regional-background method suggested by EC Guidelines and a local background method, demonstrated to be most suited to this central Mediterranean region. In terms of exceedances, the two approaches provided results within ~20% of each other at background sites, and at ~50% of each other in traffic conditions. The sequence of Saharan advections over the city has been either detected by Polarization Lidar (laser radar) observations or forecast by the operational numerical regional mineral dust model BSC-DREAM8b of the Barcelona Supercomputing Centre. Lidar observations were also employed to retrieve the average physical properties of the dust clouds as a function of height. Over the four-year period, Lidar measurements (703 evenly distributed days) revealed Saharan plumes transits over Rome on 28.6% of the days, with minimum occurrence in wintertime. Dust was observed to reach the ground on 17.5% of the days totalling 88 episodes. Most (90%) of these advections lasted up to 5 days, averaging to ~3 days. Median time lag between advections was 7 days. Typical altitude range of the dust plumes was 0–6 km, with the centre of mass at ~3 km a.g.l. BSC-DREAM8b model simulations (1461 days) predicted Lidar detectable (532 nm extinction coefficient > 0.005 km−1) dust advections on 25.9% of the days, with ground contacts on 13% of the days. As in the Lidar case, the average dust centre of mass was forecast at ~3 km. Along the 703 day Lidar dataset, model forecast and Lidar detection of the presence of dust coincided on 80% of the cases, 92% coincidences are found within a ±1 day window. Combination of the BSC-DREAM8b and Lidar records leads to about 21% of the days being affected by presence of Saharan dust at the ground. This combined dataset has been used to compute the increase in PM with respect to dust-unaffected previous days. This analysis has shown Saharan dust events to exert a meaningful impact on the PM10 records, causing average increases of the order of 11.9 μg m−3. Conversely, PM10 increases computed relying only on the Lidar detections (i.e., presence of dust layers actually observed) were of the order of 15.6 μg m−3. Both analyses indicate the annual average contribution of dust advections to the city PM10 mass concentrations to be of the order of 2.35 μg m−3. The number of exceedances attributable to Saharan advections at the three station types addressed in this study (urban traffic, urban background and regional background) were found to be 25%, 30% and 43%, respectively. These results confirm Saharan advections in the central Mediterranean as important modulators of PM10 loads and exceedances." @default.
- W2109308722 created "2016-06-24" @default.
- W2109308722 creator A5009310025 @default.
- W2109308722 creator A5014234058 @default.
- W2109308722 creator A5024130572 @default.
- W2109308722 creator A5038802603 @default.
- W2109308722 creator A5043390065 @default.
- W2109308722 creator A5046180240 @default.
- W2109308722 creator A5083196794 @default.
- W2109308722 creator A5089279246 @default.
- W2109308722 date "2013-08-01" @default.
- W2109308722 modified "2023-09-29" @default.
- W2109308722 title "Changes in particulate matter physical properties during Saharan advections over Rome (Italy): a four-year study, 2001–2004" @default.
- W2109308722 cites W1965151843 @default.
- W2109308722 cites W1968167049 @default.
- W2109308722 cites W1970618731 @default.
- W2109308722 cites W1978753385 @default.
- W2109308722 cites W1995217561 @default.
- W2109308722 cites W2003786604 @default.
- W2109308722 cites W2007871967 @default.
- W2109308722 cites W2024973929 @default.
- W2109308722 cites W2026943903 @default.
- W2109308722 cites W2030554824 @default.
- W2109308722 cites W2030696112 @default.
- W2109308722 cites W2035204328 @default.
- W2109308722 cites W2035211183 @default.
- W2109308722 cites W2048269024 @default.
- W2109308722 cites W2072154930 @default.
- W2109308722 cites W2075105262 @default.
- W2109308722 cites W2081107827 @default.
- W2109308722 cites W2087240094 @default.
- W2109308722 cites W2088063495 @default.
- W2109308722 cites W2099633906 @default.
- W2109308722 cites W2103608831 @default.
- W2109308722 cites W2109662368 @default.
- W2109308722 cites W2137895123 @default.
- W2109308722 cites W2140705068 @default.
- W2109308722 cites W2143063774 @default.
- W2109308722 cites W2145943926 @default.
- W2109308722 cites W2155843311 @default.
- W2109308722 cites W2157386516 @default.
- W2109308722 cites W2158636480 @default.
- W2109308722 cites W2166786685 @default.
- W2109308722 cites W2168373839 @default.
- W2109308722 cites W2171980762 @default.
- W2109308722 cites W4246953547 @default.
- W2109308722 cites W2144836630 @default.
- W2109308722 doi "https://doi.org/10.5194/acp-13-7395-2013" @default.
- W2109308722 hasPublicationYear "2013" @default.
- W2109308722 type Work @default.
- W2109308722 sameAs 2109308722 @default.
- W2109308722 citedByCount "32" @default.
- W2109308722 countsByYear W21093087222013 @default.
- W2109308722 countsByYear W21093087222015 @default.
- W2109308722 countsByYear W21093087222016 @default.
- W2109308722 countsByYear W21093087222017 @default.
- W2109308722 countsByYear W21093087222018 @default.
- W2109308722 countsByYear W21093087222019 @default.
- W2109308722 countsByYear W21093087222020 @default.
- W2109308722 countsByYear W21093087222021 @default.
- W2109308722 countsByYear W21093087222022 @default.
- W2109308722 countsByYear W21093087222023 @default.
- W2109308722 crossrefType "journal-article" @default.
- W2109308722 hasAuthorship W2109308722A5009310025 @default.
- W2109308722 hasAuthorship W2109308722A5014234058 @default.
- W2109308722 hasAuthorship W2109308722A5024130572 @default.
- W2109308722 hasAuthorship W2109308722A5038802603 @default.
- W2109308722 hasAuthorship W2109308722A5043390065 @default.
- W2109308722 hasAuthorship W2109308722A5046180240 @default.
- W2109308722 hasAuthorship W2109308722A5083196794 @default.
- W2109308722 hasAuthorship W2109308722A5089279246 @default.
- W2109308722 hasBestOaLocation W21093087221 @default.
- W2109308722 hasConcept C121332964 @default.
- W2109308722 hasConcept C126314574 @default.
- W2109308722 hasConcept C127313418 @default.
- W2109308722 hasConcept C153294291 @default.
- W2109308722 hasConcept C160529264 @default.
- W2109308722 hasConcept C166957645 @default.
- W2109308722 hasConcept C178790620 @default.
- W2109308722 hasConcept C185592680 @default.
- W2109308722 hasConcept C205649164 @default.
- W2109308722 hasConcept C24245907 @default.
- W2109308722 hasConcept C2779345167 @default.
- W2109308722 hasConcept C39432304 @default.
- W2109308722 hasConcept C4646841 @default.
- W2109308722 hasConcept C49204034 @default.
- W2109308722 hasConcept C5072599 @default.
- W2109308722 hasConcept C51399673 @default.
- W2109308722 hasConcept C62649853 @default.
- W2109308722 hasConcept C91586092 @default.
- W2109308722 hasConcept C97355855 @default.
- W2109308722 hasConceptScore W2109308722C121332964 @default.
- W2109308722 hasConceptScore W2109308722C126314574 @default.
- W2109308722 hasConceptScore W2109308722C127313418 @default.
- W2109308722 hasConceptScore W2109308722C153294291 @default.
- W2109308722 hasConceptScore W2109308722C160529264 @default.
- W2109308722 hasConceptScore W2109308722C166957645 @default.
- W2109308722 hasConceptScore W2109308722C178790620 @default.