Stefania Argentini

Dr. Stefania Argentini

Consiglio Nazionale delle Ricerche, Piazzale Aldo Moro, 7 - 00185 Roma, Italy

Research Focus & Metrics

Academic Career Length

39Years (1988-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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5 March 2010 in Journal of Geophysical Research: Atmospheres
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CGChristophe Genthon
Christophe Genthon
MTMichael S. Town
Michael S. Town
DSDelphine Six
Delphine Six
VFVincent Favier
Vincent Favier
Stefania ArgentiniStefania Argentini
Stefania Argentini
APAndrea Pellegrini
Andrea Pellegrini

19 January 2006 in Journal of Geophysical Research: Atmospheres
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JKJ. C. King
J. C. King
Stefania ArgentiniStefania Argentini
Stefania Argentini
PAP. S. Anderson
P. S. Anderson
The Antarctic research stations of Dome C and Halley lie at similar latitudes (∼75°S) and are thus subject to similar diurnal variation of solar radiation at the top of the atmosphere. However, the response of the atmospheric boundary layer to this diurnally varying forcing differs greatly at the two stations. At Dome C during summer there is a strong diurnal cycle in near‐surface temperature and wind speed, and a shallow (∼350 m) convective boundary layer is observed to grow in response to diurnal heating. At Halley, diurnal variations in temperature and wind speed are smaller than those at Dome C, and there is no clear diurnal variability in boundary layer depth. Analysis of the summertime surface energy budget for both stations indicates that the main reason for the different diurnal variability at the two stations is the greater partitioning of available energy into latent heat flux at the warmer Halley station. We argue that the diurnally varying convective boundary layer observed at Dome C will not be typical of the whole of the East Antarctic plateau.

1 September 2001 in Meteorology and Atmospheric Physics
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HBH. J. Beine
H. J. Beine
Stefania ArgentiniStefania Argentini
Stefania Argentini
AMalberto maurizi
alberto maurizi
AVAngelo P. Viola
Angelo P. Viola
GMG. Mastrantonio
G. Mastrantonio

1 June 2005 in Boundary-Layer Meteorology
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Stefania ArgentiniStefania Argentini
Stefania Argentini
AVAngelo P. Viola
Angelo P. Viola
ASA. M. Sempreviva
A. M. Sempreviva
Igor PetenkoIgor Petenko
Igor Petenko

12 December 2017 in Atmosphere
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francesca costabilefrancesca costabile
francesca costabile
HAHoney Alas
Honey Alas
MAMichaela Aufderheide
Michaela Aufderheide
Pasquale AvinoPasquale Avino
Pasquale Avino
FAFulvio Amato
Fulvio Amato
EPEttore Petralia
Ettore Petralia
In February 2017 the “Carbonaceous Aerosol in Rome and Environs (CARE)” experiment was carried out in downtown Rome to address the following specific questions: what is the color, size, composition, and toxicity of the carbonaceous aerosol in the Mediterranean urban background area of Rome? The motivation of this experiment is the lack of understanding of what aerosol types are responsible for the severe risks to human health posed by particulate matter (PM) pollution, and how carbonaceous aerosols influence radiative balance. Physicochemical properties of the carbonaceous aerosol were characterised, and relevant toxicological variables assessed. The aerosol characterisation includes: (i) measurements with high time resolution (min to 1–2 h) at a fixed location of black carbon (eBC), elemental carbon (EC), organic carbon (OC), particle number size distribution (0.008–10 μ m), major non refractory PM1 components, elemental composition, wavelength-dependent optical properties, and atmospheric turbulence; (ii) 24-h measurements of PM10 and PM2.5 mass concentration, water soluble OC and brown carbon (BrC), and levoglucosan; (iii) mobile measurements of eBC and size distribution around the study area, with computational fluid dynamics modeling; (iv) characterisation of road dust emissions and their EC and OC content. The toxicological assessment includes: (i) preliminary evaluation of the potential impact of ultrafine particles on lung epithelia cells (cultured at the air liquid interface and directly exposed to particles); (ii) assessment of the oxidative stress induced by carbonaceous aerosols; (iii) assessment of particle size dependent number doses deposited in different regions of the human body; (iv) PAHs biomonitoring (from the participants into the mobile measurements). The first experimental results of the CARE experiment are presented in this paper. The objective here is to provide baseline levels of carbonaceous aerosols for Rome, and to address future research directions. First, we found that BC and EC mass concentration in Rome are larger than those measured in similar urban areas across Europe (the urban background mass concentration of eBC in Rome in winter being on average 2.6 ± 2.5 μ g · m − 3 , mean eBC at the peak level hour being 5.2 (95% CI = 5.0–5.5) μ g · m − 3 ). Then, we discussed significant variations of carbonaceous aerosol properties occurring with time scales of minutes, and questioned on the data averaging period used in current air quality standard for PM 10 (24-h). Third, we showed that the oxidative potential induced by aerosol depends on particle size and composition, the effects of toxicity being higher with lower mass concentrations and smaller particle size. Albeit this is a preliminary analysis, findings reinforce the need for an urgent update of existing air quality standards for PM 10 and PM 2.5 with regard to particle composition and size distribution, and data averaging period. Our results reinforce existing concerns about the toxicity of carbonaceous aerosols, support the existing evidence indicating that particle size distribution and composition may play a role in the generation of this toxicity, and remark the need to consider a shorter averaging period (<1 h) in these new standards.

4 October 2013 in Boundary-Layer Meteorology
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IPIlaria Pietroni
Ilaria Pietroni
Stefania ArgentiniStefania Argentini
Stefania Argentini
Igor PetenkoIgor Petenko
Igor Petenko
In 2005 the Study of Stable Boundary Layer Environment at Dome C (STABLEDC) experimental campaign was conducted at the plateau station of Concordia at Dome C, Antarctica. Temperature profiles measured with a microwave radiometer were used to study the characteristics of surface-based temperature inversions over the course of a year. Statistics of temperature profiles for every month are discussed; the difference between daytime and nocturnal cases observed during the summer months disappears during winter. Surface-based temperature inversions occurred in 70 % of the time during summer, and almost all of the time during winter. During winter the occurrence of warming events leads to a decrease in the temperature difference between the top and the base of the inversion (i.e. the inversion strength). The inversion strength maxima ranged between \(3\,^{\circ }\mathrm{C}\) (December) and \(35\,^{\circ }\mathrm{C}\) (August) corresponding to gradients of 0.1 and \(0.3\,^{\circ }\mathrm{C}\, \mathrm{m}^{-1}\) , respectively. The average surface-based inversion height presents a daily cycle during the summer months with values up to 200 m in the morning hours, while it affects a layer always deeper than 100 m during the winter months. The relationships between inversion strength and the downward longwave radiative flux, absolute temperature, and wind speed are examined. The inversion strength decreases as the longwave radiation increases. A clear anti-correlation between inversion strength and near-surface temperature is evident throughout the year. During the winter, the largest inversion strength values were observed under low wind-speed conditions; in contrast, a clear dependence was not found during the summer.