Nonlinear wave conversion in electron-positron plasmas

Wave conversion mechanisms causing large-frequency shifts are considered for an electron-positron plasma in a strong magnetic field. In particular, we discuss the effects of the nonlinear erenkov as well as the cyclotron resonances in order to associate pulsar radio-emissions with our present model for nonlinear conversion of high-frequency radiation into the low-frequency region.     

Review of Carboniferous-Permian volcanicity in Scotland

The main Carboniferous outcrop in Scotland is in the Midland Valley rift, though rocks of that age also occur farther south along the English Border. The cyclic sedimentary sequence comprises up to 3,000 m. of Dinantian (mainly Viséan) and 2,000 m. of Silesian beds which at one locality or another include lavas or tuffs almost at every level. The distribution of these volcanic rocks is known in exceptional detail because of mining and exploratory borings in the Viséan oil shale field and in the various Namurian and Westphalian coalfields.The lavas and tuffs form part of an alkaline (sodic) magma series. Their outpourings were greatest in volume during the Dinantian, with the formation of the extensive lava piles which now form the Clyde Plateau (maximum thickness c. 900 m.) in the west, the Garleton Hills (c. 600 m.) and Burntisland Anticline (c. 400 m.) in the east, and the Kelso Traps of the Tweed Basin (c. 120 m.), the Birrenswark Lavas of Dumfriesshire (c. 90 m.), the Kershopefoot Basalt of Liddesdale (c. 60 m.) and the Glencartholm Volcanic Beds (mostly tuffs) of Eskdale (c. 180 m.) to the south. Most of the lavas are varieties of olivine-basalt, but subordinate trachybasalts, trachytes and rhyolites are included in the upper parts of the Clyde Plateau and Garleton Hills successions. The areas covered by individual lava fields are difficult to assess because they varied from time to time and occasionally overlapped.By the end of the Dinantian this form of activity had ceased everywhere except in West Lothian, where it continued into early Namurian (E₁). Thereafter volcanicity continued periodically from scattered centres and gave rise to relatively short-lived ash-cones. They formed in Ayrshire (E₁ age) but were most abundant in Fife, occurring there almost throughout the Namurian succession. The highly explosive nature of this phase of volcanicity is apparent from the rarity of associated lavas (though minor basaltic intrusions occur in the necks) and from the presence within the surrounding sediments of thin layers of tuff representing fine ash carried for distances of up to 32 km from source. These layers, some of which are kaolinized and are a variety of tonstein, are of local use in correlation.The explosive phase is now known to have continued throughout Westphalian A and possibly into Westphalian B in Fife, but in Ayrshire volcanicity was more intermittent and is represented by two outpourings of basalt lavas, one late Namurian to early Westphalian in age and up to 150 m. thick, the other Stephanian in age and 90 to 237 m. thick. The Stephanian lavas and associated necks in Ayrshire, like some of the necks exposed on the classic Fife coastal section on the Firth of Forth, were until recently believed to be Permian, but there is now no positive evidence of Permian eruption in Scotland.Two groups of intrusions cut the Carboniferous rocks. The most extensive is of alkaline dolerites which are co-magmatic with the basaltic lavas and tuffs, and are of similar geographic distribution. They form sills up to 120 m. thick and are probably of various ages up to Stephanian. It is possible that some of them were high-level reservoirs from which diatremes issued. The other group is of quartz-dolerite or tholeiite which forms a series of east-west dykes and a sill-complex extending over an area of about 1500 km² and having a maximum thickness of 127 m. Their age is late Carboniferous.The distribution of the Carboniferous volcanic rocks is not apparently related to the rift-valley, but is clearly linked in places to the earlier Caledonoid structures which determined the pattern of sedimentation. The lavas and, to a lesser extent, the tuffs, influenced the sedimentary processes by partially enclosing basins, by causing local anomalies in cyclic sequences and by providing sources of atypical sediment.

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Zusammenfassung Im Midland Valley (Schottland) war der permokarbonische Alkali-(Na)-Vulkanismus besonders im Dinantium aktiv, wobei bis 900 m mächtige Laven (Olivinbasalte, untergeordnet Trachytandesite, Trachyte und Rhyolite) gefördert wurden. Gegen Ende des Dinantium hörte diese Art der Aktivität fast ganz auf, dafür setzte eine explosive, periodische Tätigkeit ein, die zu kurzlebigen Aschenkegeln führte. Ein Beweis für das früher angenommene permische Alter dieser Necks läßt sich nicht erbringen.Zwei Gruppen von Intrusiva sind in die karbonischen Sedimente eingedrungen. Die größere der beiden wird durch Alkali-Dolerite (Sills) gebildet, die co-magmatisch zu den Laven und Tuffen sind. Die andere besteht aus Quarz-Doleriten und Tholeyiten (vorwiegend Dykes), die spätkarbonisch bis frühpermischen Alters sind.Die Verbreitung der karbonischen Vulkanite ist nicht an das Midland Valley, sondern an frühere caledonische Strukturen gebunden und für den Sedimentationsprozeß von Bedeutung.

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Résumé Le principal affleurement carbonifère en Ecosse se trouve dans le graben du Midland Valley, quoiqu'on rencontre les roches de cet âge le long de la frontière anglaise. La succession du cycle sédimentaire comprend jusqu'à 3,000 m. de roches de l'âge Dinantien (principalement Viséen) et à 2,000 m. des couches Silésiennes qui dans une localité quelconque comprennent des laves ou des tufs à presque tous les niveaux. La distribution de ces roches volcaniques est bien connu dans tous les détails à cause des mines et des forages.Les laves et les tufs font partie d'une série alkaline (sodique) magma. Leurs éruptions atteignirent leur maximum en volume pendant Ie Dinantien, avec la formation du Plateau de Clyde (épaisseur maximum 900 m. env.) à l'ouest, les Collines de Garleton (600 m. env.) et l'anticlinal de Burntisland (400 m. env.) a l'est, et les Kelso Traps du bassin du Tweed (120 m. env.), les Birrenswark Lavas de Dumfriesshire (90 m. env.), le Kershopefoot Basait de Liddesdale (60 m. env.) et les Glencartholm Volcanic Beds (des tufs pour la plupart) d'Eskdale (180 m. env.) au sud. La plupart des laves sont des variétés de basalte-olivine, mais des quantié peu considérables de trachybasalte, trachytes et rhyolites sont comprises dans les parties supérieures dans les successions du Plateau de Clyde et des Collines de Garleton.A la fin du Dinantien, cette forme d'activité avait cessé partout excepté dans l'Ouest Lothian, où elle continuait jusqu'au commencement du Namurien. Après cela le volcanisme continua périodiquement des centres dispersés, et donna naissance à des cônes de cendre de relativement petite durée. Ceux-ci se formèrent en Ayrshire (age E₁), mais on les trouvait beaucoup plus souvent en Fife, et on les y rencontrait presque pendant toute la succession namurienne. La nature explosive de cette phase de volcanisme est apparente par la rareté des laves et par la présence dans le sédiment qui se trouve dans les couches étroites de tuf, résultat du cendre fin porté jusqu'à 32 km. de sa source. Ces couches-ci dont quelques-unes furent transformées en kaolin, sont une variété de tonstein qui s'emploie beaucoup en corrélation. La distribution des quelques cheminées volcaniques coïncide aux structures nord—est d'un âge précarbonifère.La phase explosive est maintenant connue d'avoir continué à travers toute la Westphalie «Äs» et possiblement d'avoir pénétré dans la Westphalie «B» en Fife, mais en Ayrshire le volcanisme était plus intermittent et est représenté par deux éruptions de lave basaltique, l'une pendant la fin du Namurien jusqu'au début du Westphalien et d'une épaisseur de 150 m., l'autre du Stéphanien et d'une épaisseur de 90 à 237 m. Les laves du Stéphanien et les cheminées associées étaient classées auparavant comme Permien, mais maintenant il n'y a aucune évidence positive d'éruption permianique en Ecosse.Deux groupes d'intrusions scindèrent les roches carbonifères. Le groupe le plus étendu est fait de dolérites alkalines qui sont co-magmatiques avec les laves basaltiques et les tufs, et sont de pareille distribution géographique. Elles forment des silles d'une épaisseur jusqu; à 120 m. et elles sont probablement d'âges variés jusqu'au Stéphanien. Il est possible que quelques-une d'entre elles furent des réservoirs de haut-niveau desquels des diatrèmes sortirent. L'autre groupe est fait de quartz-dolérite ou tholéiite qui forme une série de dikes est—ouest et une sille-complexe couvrant une étendue de 1,500 km² et ayant une épaisseur maximale de 127 km. Leur áge est de la fin du Carbonifère ou du début du Permien.

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Published by permission of the Director, Institute of Geological Sciences.     

Changes in the circulation of Tampa Bay due to Hurricane Frances as recorded by ADCP measurements and reproduced with a numerical Ocean model

Hurricane Frances is shown to greatly alter the hydrodynamics within Tampa Bay, Florida, and the exchange of water with the Gulf of Mexico in both observational data and a realistic numerical circulation model of the Tampa Bay estuary. Hurricane Frances hit Tampa Bay on September 5, 2004 with surface winds peaking twice near 22 m s⁻¹. There were three stages to the hydrodynamic effect of Frances on Tampa Bay. The first stage included the approach of Frances up to the first wind peak. The winds were to the south and southeast. During this stage sea level was maintained below mean sea level (MSL) and the residual current (demeaned, detided) was weak. The second stage began as the winds turned to the east and northeast, as the eye passed near the bay, and ended as the second wind peak appeared. During this stage the residual currents were strongly positive (into the bay), raising sea level to 1.2 m above MSL at St. Petersburg. The measured residual circulation peaked at over +0.7 m s⁻¹ near the surface. The model shows this velocity peak yielded a maximum volume flux into the bay of +44,227 m³ s⁻¹, displacing a total volume of 1.5 billion m³ in just a few hours, about 42% of the bay volume. In the third stage a strong negative flow developed as the wind and sea level relaxed to near normal levels. The ADCP measured a peak outflow of −0.8 m s⁻¹ during this time. Model results indicate a maximum flux of −37,575 m³ s⁻¹, and that it took about 50 h to drain the extra volume driven into the bay by Hurricane Frances.     

Observations on the asexual reproductive activities of the sessile stages of the sea nettleChrysaora quinquecirrha (Scyphozoa)

Twenty-seven colonies of wild scyphistomae ofChrysaora quinquecirrha were observed for a period of ten weeks during the summer. Asexual activities of individual organisms were recorded several times each week. Polyps most often proceeded to strobilate in mid-June and then strobilate a second time 18 days later. They then detached and changed position by means of stolons and then produced podocysts. Initial cysts first excysted and the resulting polyps then strobilated. A second strobilation was not generally observed. The developmental implications of these activities are discussed.     

High-Resolution Simulations of Nonhelical MHD Turbulence

According to the kinematic theory of nonhelical dynamo action, the magnetic energy spectrum increases with wavenumber and peaks at the resistive cutoff wavenumber. It has previously been argued that even in the dynamical case, the magnetic energy peaks at the resistive scale. Using high resolution simulations (up to 1024³ meshpoints) with no large-scale imposed field, we show that the magnetic energy peaks at a wavenumber that is independent of the magnetic Reynolds number and about five times larger than the forcing wavenumber. Throughout the inertial range, the spectral magnetic energy exceeds the kinetic energy by a factor of two to three. Both spectra are approximately parallel. The total energy spectrum seems to be close to k ^?3/2, but there is a strong bottleneck effect and we suggest that the asymptotic spectrum is instead k ^?5/3. This is supported by the value of the second-order structure function exponent that is found to be ζ₂ = 0.70, suggesting a k ^?1.70 spectrum. The third-order structure function scaling exponent is very close to unity,—in agreement with Goldreich–Sridhar theory. Adding an imposed field tends to suppress the small-scale magnetic field. We find that at large scales the magnetic energy spectrum then follows a k ^?1 slope. When the strength of the imposed field is of the same order as the dynamo generated field, we find almost equipartition between the magnetic and kinetic energy spectra.     

Kinematic Subsystems of the Ionized Gas in the Central Region of NGC 1068 Inferred from the [O III] λλ 4959, 5007 and [S III] λ 9069 Emission Lines

We discuss the multi-Gaussian decomposition of the [O III] λλ 4959,5007 emission line profiles from 2-D spectroscopy. We found that a model based on five main gaseous components can reproduce the observed line profiles consistently. The morphology of the intensity maps of some of these gaseous subsystems seems bipolar. This is in better agreement with current ideas about the alignment of the ionization in AGNs than the relatively amorphous morphology seen in filter images. The centre of the inter-pole region is sited ~ 2″ NE of the optical nucleus, close to the origin of the strong outflow of ionized gas recently reported (Arribas et al. 1996). This suggests that the putative hidden nucleus of NGC 1068 could be sited near to this point.     

The use of 18O/16O ratios to study the formation and chemical origin of coal

The ${}^{18}\text{O}{}^{16}\text{O}$ ratios of some New Zealand peat, lignite and coal samples were measured and compared with those of various coal precursors (cellulose, lignin and plant resins). The results showed that the major source of oxygen in all cases (except that of high rank coal) was from cellulose with the contribution from lignin and plant resins being insignificant.