Long-term radial velocity variations in some Be stars

All the radial velocities (RV) available in the literature since the beginning of the century for the Be stars EW Lac, 28 Tau, Tau, KX And, KY And, CX Dra and 88 Her, are assembled. When possible, a periodogram analysis has been performed to search for eventual periodic phenomena.The following conclusions have been drawn: EW Lac could be a spectroscopic binary with a period of about 40 years; 28 Tau shows some indications of regular long-term RV variations on the time scale of decades; a probable recurrent shell activity of Tau could be hypothesized. Some useful indications for KX and KY And are given, whereas it is not possible to draw any conclusion for CX Dra and 88 Her owing to the lack of data.     

Spectrographic observations of omicron andromedae from 1967 to 1976

The results of qualitative analysis and radial velocity (RV) determinations from 1967 to 1976 are given. These analyses show sometimes the presence of a thin variable shell also in the years 1967–1974, before the appearance of the envelope. Intensity variations of the metallic lines seem to indicate that in the same period changes of temperature and/or electron pressure may occur in the photospheric layers. In the period 1975–76, the considerable range ofRV and the variability of the shell features show that the shell is rather active. Some conspicuousRV variations seem to be correlated to brightness changes. TheRV do not confirm the periods suggested by the photometric observations. A periodogram analysis givesRV curves with a poor evidence of periodicity. However, the periodP=1^d.5845 obtained from this analysis, close to that of Schmidt, seems to confirm Schmidt's hypothesis of a contact binary system. The periodogram analysis of theRV during the years 1900–1976 and some physical arguments, suggest a probable photospheric activity or an invisible companion with the observed shell period of 30 yr. The duplicity, suggested by Kí and Harmanec (1975) for all the Be stars, could be yet questioned foro And.Thesis for the degree of Applied Physics.     

Imaging and modelling the subsurface structure of volcanic calderas with high-resolution aeromagnetic data at Vulcano (Aeolian Islands,Italy)

In this paper, we present a magnetic model of the subsurface structure of Vulcano island based on high-resolution aeromagnetic data. Three profiles across the most intense magnetic anomalies over the Piano and Fossa calderas were selected for the magnetic modelling, which was constrained by structural and volcanological data, previous geophysical models, paleomagnetic data, and borehole stratigraphy obtained from two deep wells. The interpretation of the magnetic sources represents a significant contribution to the understanding of the Piano and Fossa calderas’ underlying structure, providing us with evidence of the lateral discontinuity between them at depth. We propose that the positive magnetic anomalies in the Piano caldera area are caused by: (a) the remnants of an early submarine volcano; (b) an outcropping dyke swarm related to the feeding system of the Primordial Vulcano phase (beneath Mt. Saraceno); and (c) the presence of a non-outcropping dyke system intruded along a NE–SW-oriented intra-caldera fault (beneath the eastern part of the Piano caldera). Offshore, to the west, the magnetic anomaly map suggests the presence of a submarine volcanic structure, not revealed by bathymetric data, which could represent the eruptive centre, the presence of which has been indirectly deduced from the outcrop of eastern-dipping lavas on the western seashore. Magnetic modelling of the Fossa caldera points to the presence of a highly magnetized cone-like body inside the Fossa cone, centred beneath the oldest crater rims. We interpret this body as a pile of tephritic lavas emplaced in an early phase of activity of the Fossa cone, suggesting that the volume of mafic lavas that erupted at the beginning of the construction of the Fossa edifice was more significant than has previously been deduced. Furthermore, the presence of a magnetized body inside the Fossa cone implies that high temperatures are contained in very limited spaces, do not affect its bulk inner structure, and are restricted to fumarolic conduits and vents. In addition, structures beneath the western and northern part of the Fossa caldera are revealed to have null or low magnetization, which can be ascribed to the presence of pyroclasts and hyaloclastites in this area as well as to a large volume of hydrothermally altered materials. This suggests that the hydrothermal system, with a very limited extension at present, affected a larger area in the past, especially beneath the western part of the caldera.     

Recent channel adjustments in alluvial rivers of Tuscany,central Italy

Drastic channel adjustments have affected the main alluvial rivers of Tuscany (central Italy) during the 20th century. Bed‐level adjustments were identified both by comparing available topographic longitudinal profiles of different years and through field observations. Changes in channel width were investigated by comparing available aerial photographs (1954 and 1993–98). Bed incision represents the dominant type of vertical adjustment, and is generalized along all the fluvial systems investigated. The Arno River system is the most affected by bed‐level lowering (up to 9 m), whereas lower incision (generally less than 2 m) is observed along the rivers of the southern part of the region. Human disturbances appear to be the dominant factors of adjustments: the main phase of vertical change occurred during the period 1945–80, in concomitance with the phase of maximum sediment mining activity at the regional scale. The second dominant type of adjustment that involved most of the rivers in the region consists of a narrowing of the active channel. Based on measurements of channel width conducted on aerial photographs, 38% of the reaches analysed experienced a narrowing greater than 50% of the initial channel width. The largest values of channel narrowing were observed along initially braided or sinuous with alternate bars morphologies in the southern portion of the region. A regional scheme of channel adjustments is derived, based on initial channel morphology and on the amounts of incision and narrowing. Different styles of channel adjustments are described. Rivers that were originally sinuous with alternate bars to braided generally became adjusted by a moderate incision and a moderate to intense narrowing; in contrast, sinuous‐meandering channels mainly adjusted vertically, with a minor amount of narrowing. Copyright © 2003 John Wiley & Sons, Ltd.     

Paleo-environmental and volcano-tectonic evolution of the southeastern flank of Mt. Etna during the last 225 ka inferred from the volcanic succession of the ‘Timpe’, Acireale, Sicily

The tectonic escarpments locally known as ‘Timpe’ cut a large sector of the eastern flank of Etna, and allow an ancient volcanic succession dating back to 225 ka to be exposed. Geological and volcanological investigations carried out on this succession have allowed us to recognize relevant angular unconformities and volcanic features which are the remnants of eruptive fissures, as well as important changes in the nature, composition and magmatic affinity of the exposed volcanics. In particular, the recognition in the lower part of the succession of important and unequivocal evidence of ancient eruptive fissures led us to propose a local origin for these volcanics and to revise previous interpretations which attributed their westward-dipping to the progressive tectonic tilting of strata. These elements led us to reinterpret the main features of the volcanic activity occurring since 250 ka BP and their relationship with tectonic structures active in the eastern flank of Etna. We propose a complex paleo-environmental and volcano-tectonic evolution of the southeastern flank of Mt. Etna, in which the Timpe fault system played the role of the crustal structure that allowed the rise and eruption of magmas in the above considered time span.     

Pre-alpine and alpine evolution of the South-alpine basement of the Orobic Alps

New K-Ar age determinations on the gneisses and schists of the south-Alpine basement of the Orobic Alps and their separated minerals have been carried out to supplement and support the previous study ofBocchio et al. (1981).The cooling ages of biotites and muscovites range from 218 to 331 my and from 170 to 330 my respectively, according to a bimodal distribution with modes at 222 and 298 my for biotite, 182 and 322 my for muscovite. The whole rock ages spread from 43 to 402 my with no significant cluster. Only a few samples give statistically significant internal isochrones, and these suggest two periods of equilibration, at 226–245 and 312–368 my.These age determinations support the conclusion drawn from regional petrologic studies (Bocchio et al., 1980;Crespi et al., 1980), that the south-Alpine basement underwent two main phases of metamorphism, now preferentially preserved in different areas: an old, Hercynian phase under a regime of intermediate pressure (staur-ky type), and a young, post-Hercynian phase under a regime of low pressure (staur-sill type) reactivated by the cover of the thick sedimentary pile on top of the basement. Furthermore, radiometric ages also point out the widespread but irregularly distributed occurence of an alpine overprint under the conditions of a very low metamorphic regime, that is documented by the growth of post-kinematic stilpnomelane in rocks of suitable bulk composition (Crespi et al., 1981, 1982), as well as by fine-grained phengite.

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Zusammenfassung Neue Kali-Argon-Datierungen von Gneisen und Schiefern und ihrer abgetrennten Minerale des südalpinen Grundgebirges wurden in Ergänzung der Studie vonBocchio et al., 1981 durchgeführt. Die Abkühlungsalter der Biotite und Muskovite reichen von 218 bis 331 ma und von 170 bis 330 ma entsprechend einer bimodalen Entwicklung mit Modalwerten bei 222 und 298 ma für Biotit und 182 und 322 ma für Muskovit. Die Gesamtgesteinsalter reichen von 43–402 ma ohne signifikante Häufung. Nur wenige Proben geben eine statistisch signifikante Isochrone, woraus sich zwei Gleichgewichtsperioden zwischen 226–245 ma und 312–368 ma ablesen lassen.Diese Altersbestimmungen unterstützen die Schlußfolgerungen, die aus regional-petrologischen Studien (Bocchio et al., 1980;Crespi et al., 1980) gezogen wurden und die Aussagen, daß das südalpine Grundgebirge zwei Hauptphasen der Metamorphose mitgemacht hat, die heute in verschiedenen Gebieten erhalten sind: eine ältere herzynische Phase unter mittleren Druckbedingungen (Staur-Ky) und eine jüngere postherzynische Phase unter niedrigem Druck (Staur-Sil), die unter der Überdeckung einer mächtigen Sedimentserie über dem Grundgebirge reaktiviert wurde. Darüber hinaus deuten die radiometrischen Alter auf einen weit verteilten, aber unregelmäßig auftretenden alpinen Einfluß hin, der unter den Bedingungen einer sehr niedrigen Metamorphose aufgeprägt wurde. Dies wird dokumentiert durch das Wachstum postkinematischer Stilpnomelane in Gesteinen mit einer entsprechenden Zusammensetzung (Crespi et al., 1981, 1982) sowie von feinkörnigen Phenigiten.

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Résumé De nouvelles déterminations d'âge par la méthode K-Ar ont été effectuées sur les gneiss et les schistes du socle sudalpin des Alpes Orobiques, ainsi que sur certains de leurs minéraux, en complément aux travaux antérieurs deBocchio et al. (1981).L'âge du refroidissement des biotites s'étend de 210 à 331 Ma et celui des muscovites de 170 à 330 Ma, selon une distribution bimodale: modes à 222 à 298 Ma pour la biotite et à 183 et 322 Ma pour la muscovite. Les âges mesurés sur roche totale vont de 43 à 402 Ma sans concentration significative autour d'une valeur. Un petit nombre d'échantillons seulement fournissent des isochrones statistiquement significatives; elles suggèrent deux périodes de mise en équilibre, à 226–245 Ma et à 312–368 Ma.Ces déterminations d'âge appuient les conclusions d'études pétrologiques régionales antérieures (Bocchio et al. 1980;Crespi et al. 1980), à savoir que le socle sud-alpin a subi deux phases principales de métamorphisme, conservées aujourd'hui dans de régions différentes: une phase ancienne, hercynienne, de pression intermédiaire (type staurotide-disthène) et une phase jeune, post-hercynienne, de basse pression (type staurotide-sillimanite) réactivée sous la couverture sédimentaire épaisse reposant sur le socle. De plus, les âges radiométriques mettent en évidence une reprise alpine, d'extension régionale mais irrégulièrement distribuée, dans les conditions d'un métamorphisme de très faible degré. Cette reprise s'exprime par la croissance de stilpnomélane post-cinématique dans les roches de composition appropriée (Crespi et al. 1981, 1982) ainsi que par le développement de phengite finement grenue.

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. (1981), K/Ar-. 218 331 170 330 , 222 298 182 322 . 43–402 - . , 226–245 312–368 . . (1980) . (1980) , - : , , (Staur-Ky) , , (StaurSil) , . , , . ( ., 1981, 1982), .

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Paper presented at the Second E.U.G. Meeting at Strasbourg, April 23–26, 1983     

Impact of Heterogeneity on Oxygen Transfer in a Fluctuating Capillary Fringe

We performed quasi‐two‐dimensional flow through laboratory experiments to study the effect of a coarse‐material inclusion, located in the proximity of the water table, on flow and oxygen transfer in the capillary fringe. The experiments investigate different phases of mass transfer from the unsaturated zone to anoxic groundwater under both steady‐state and transient flow conditions, the latter obtained by fluctuating the water table. Monitoring of flow and transport in the different experimental phases was performed by visual inspection of the complex flow field using a dye tracer solution, measurement of oxygen profiles across the capillary fringe, and determination of oxygen fluxes in the effluent of the flow‐through chamber. Our results show significant effects of the coarse‐material inclusion on oxygen transfer during the different phases of the experiments. At steady state, the oxygen flux across the unsaturated/saturated interface was considerably enhanced due to flow focusing in the fully water‐saturated coarse‐material inclusion. During drainage, a zone of higher water saturation formed in the fine material overlying the coarse lens. The entrapped oxygen‐rich aqueous phase contributed to the total amount of oxygen supplied to the system when the water table was raised back to its initial level. In case of imbibition, pronounced air entrapment occurred in the coarse lens, causing oxygen to partition between the aqueous and gaseous phases. The oxygen mass supplied to the anoxic groundwater following the imbibition event was found to be remarkably higher (approximately seven times) in the heterogeneous system compared with a similar experiment performed in a homogeneous porous medium.