Combined observations of meteors by image-orthicon television camera and multi-station radar

Observations from multiple sites of a radar network and by television of 29 individual meteors from February 1969 through June 1970 are reported. Only 12 of the meteors did not appear to fragment over all the observed portion of their trajectories. From these 12, the relation for the radar magnitude to the panchromatic absolute magnitude was found in terms of velocity of the meteor. A very tentative fit to the data on the duration of long enduring echoes versus visual absolute magnitude is made. The exponential decay characteristics of the later parts of several of the light curves are pointed out as possible evidence of mutual coalescence of droplets into which the meteoroid has completely broken

L’ambiente carsico e l’idrogeologia dei gessi di Sassalbo (MS)

Nel Canale dell’Acqua Torbida (Alta Lunigiana), si trova il maggiore affioramento di evaporiti triassiche della Toscana. Rispetto ai gessi dell’Alta val Secchia (RE), di cui sono il lembo meridionale, appaiono molto meno tettonizzati. L’area carsica, che comprende in prevalenza calcari cavernosi, ha una superficie complessiva di circa 2,2 km2 in cui sono ben rappresentate forme carsiche superficiali, sia macro che micro. Anche i fenomeni carsici sotterranei sembrano essere ben sviluppati: la loro genesi è stata attribuita a periodi di avanzata e arretramento dei ghiacciai durante l’ultimo glaciale. Attualmente nel catasto toscano sono registrate 5 cavità, di cui 4 rilevate. Nell’ambito del Progetto Trias II (studio interdisciplinare svolto dalla Società Speleologica Italiana per conto del Parco Nazionale dell’Appennino Tosco-Emiliano) è stato possibile studiare l’area dal punto di vista morfologico, speleologico e idrochimico, monitorando in continuo alcune delle principali risorgenti carsiche parallelamente ai torrenti cui esse potevano risultare connesse. Nel presente lavoro, dopo breve illustrazione delle morfologie epigee ed ipogee, vengono presentati i risultati del monitoraggio idrologico. Le analisi hanno permesso di evidenziare come in molti casi le acque del carso di Sassalbo siano chimicamente molto simili a quelle del sistema ad ansa ipogea del Tanone della Gacciolina in Alta val di Secchia. Fanno eccezione altre sorgenti, alimentate quasi esclusivamente dalla serie marnoso arenacea e dal macigno, che presentano comportamenti idrodinamici differenti in funzione dei loro specifici bacini di alimentazione.Karst and hydrology of the Sassalbo Gypsa (Massa Carrara – Italy) The largest triassic evaporitic outcrop of Tuscany is located inside the Acqua Torbida creek (Upper Lunigiana). They represent the southernmost and less tectonized part of the Upper Secchia Gypsa (RE). The karst area (some 2,2) consists mostly of limestone (Calcari Cavernosi) with well developed macro – and micro – forms. The underground phenomena are mainly related to the mouventes of glacial tongues during the last Glacial. 5 cavities are presently known and inserted in the Tuscany Cadaster, 4 of which mapped. In the framework of the Trias II Project (an interdisciplinary study sponsored by the Appennino Tosco-Emiliano National Park and performed by the Italian Speleological Society) this area has been investigated from the morphological, speleological, hydrochemical point of view while some of the major springs and related rivers were monitored. In the paper after a short description of the epigean and hypogean forms, the achieved result during the hydrological study are presented. This study evidenced that in many occurrences the behavior of the Sassalbo karst waters is very similar to that of the Tanone della Gacciolina cave in the Upper Secchia Valley. Only a few springs exhibit a different behavior being rather completely fed by the marnoso-arenacea and macigno formations

Direct evidence for efficient ultrafast charge separation in epitaxial WS2_2/graphene heterostructure

We use time- and angle-resolved photoemission spectroscopy (tr-ARPES) to investigate ultrafast charge transfer in an epitaxial heterostructure made of monolayer WS$_2$ and graphene. This heterostructure combines the benefits of a direct gap semiconductor with strong spin-orbit coupling and strong light-matter interaction with those of a semimetal hosting massless carriers with extremely high mobility and long spin lifetimes. We find that, after photoexcitation at resonance to the A-exciton in WS$_2$, the photoexcited holes rapidly transfer into the graphene layer while the photoexcited electrons remain in the WS$_2$ layer. The resulting charge transfer state is found to have a lifetime of $\sim1$\,ps. We attribute our findings to differences in scattering phase space caused by the relative alignment of WS$_2$ and graphene bands as revealed by high resolution ARPES. In combination with spin-selective excitation using circularly polarized light the investigated WS$_2$/graphene heterostructure might provide a new platform for efficient optical spin injection into graphene.Comment: 28 pages, 14 figure

Direct evidence for efficient ultrafast charge separation in epitaxial WS₂/graphene heterostructures

We use time- and angle-resolved photoemission spectroscopy (tr-ARPES) to investigate ultrafast charge transfer in an epitaxial heterostructure made of monolayer WS2 and graphene. This heterostructure combines the benefits of a direct-gap semiconductor with strong spin-orbit coupling and strong light-matter interaction with those of a semimetal hosting massless carriers with extremely high mobility and long spin lifetimes. We find that, after photoexcitation at resonance to the A-exciton in WS2, the photoexcited holes rapidly transfer into the graphene layer while the photoexcited electrons remain in the WS2 layer. The resulting charge-separated transient state is found to have a lifetime of ∼1 ps. We attribute our findings to differences in scattering phase space caused by the relative alignment of WS2 and graphene bands as revealed by high-resolution ARPES. In combination with spin-selective optical excitation, the investigated WS2/graphene heterostructure might provide a platform for efficient optical spin injection into graphene

Integrated Nitrogen CAtchment model (INCA) applied to a tropical catchment in the Atlantic Forest, São Paulo, Brazil

International audienceStream-water flows and in-stream nitrate and ammonium concentrations in a small (36.7 ha) Atlantic Forest catchment were simulated using the Integrated Nitrogen in CAtchments (INCA) model version 1.9.4. The catchment, at Cunha, is in the Serra do Mar State Park, SE Brazil and is nearly pristine because the nearest major conurbations, São Paulo and Rio, are some 450 km distant. However, intensive farming may increase nitrogen (N) deposition and there are growing pressures for urbanisation. The mean-monthly discharges and NO3-N concentration dynamics were simulated adequately for the calibration and validation periods with (simulated) loss rates of 6.55 kg.ha?1 yr?1 for NO3-N and 3.85 kg.ha?1 yr?1 for NH4-N. To investigate the effects of elevated levels of N deposition in the future, various scenarios for atmospheric deposition were simulated; the highest value corresponded to that in a highly polluted area of Atlantic Forest in Sao Paulo City. It was found that doubling the atmospheric deposition generated a 25% increase in the N leaching rate, while at levels approaching the highly polluted São Paulo deposition rate, five times higher than the current rate, leaching increased by 240%, which would create highly eutrophic conditions, detrimental to downstream water quality. The results indicate that the INCA model can be useful for estimating N concentration and fluxes for different atmospheric deposition rates and hydrological conditions

A Study of the Radiative Ke3 Decay and Search for Direct Photon Emission with the KLOE Detector

We present a measurement of the ratio R = \Gamma(\keg;\Estar>30\mev,\qstar>20^\circ)$/$\Gamma(\kegf)$and a first measurement of the direct emission contribution in KL semileptonic decays. The measurement is done at the DAFNE phi-factory selecting phi->KL KS decays with the KLOE detector. We use 328 pb^{-1}$ of data corresponding to about 3.5 million Ke3(g) events and about 9000 radiative events. Our result is R=(924 +/- 23(stat) +/-16(syst)10^{-5} for the branching ratio and X=-2.3 +/- 1.3(stat) +/- 1.4(syst) for the parameter describing direct emission.Comment: 8 pages, 7 figure

SuperB: a linear high-luminosity B Factory

This paper is based on the outcome of the activity that has taken place during the recent workshop on "SuperB in Italy" held in Frascati on November 11-12, 2005. The workshop was opened by a theoretical introduction of Marco Ciuchini and was structured in two working groups. One focused on the machine and the other on the detector and experimental issues. The present status on CP is mainly based on the results achieved by BaBar and Belle. Estabilishment of the indirect CP violation in B sector in 2001 and of the direct CP violation in 2004 thanks to the success of PEP-II and KEKB e+e- asymmetric B Factories operating at the center of mass energy corresponding to the mass of the Y(4s). With the two B Factories taking data, the Unitarity Triangle is now beginning to be overconstrained by improving the measurements of the sides and now also of the angles alpha, and gamma. We are also in presence of the very intriguing results about the measurements of sin(2 beta) in the time dependent analysis of decay channels via penguin loops, where b --> s sbar s and b --> s dbar d. Tau physics, in particular LFV search, as well as charm and ISR physics are important parts of the scientific program of a SuperB Factory. The physics case together with possible scenarios for the high luminosity SuperB Factory based on the concepts of the Linear Collider and the related experimental issues are discussed.Comment: 22 pages, 22 figures, INFN Roadmap Repor