scholarly journals Self-gravitating filament formation from shocked flows: velocity gradients across filaments

2020 ◽  
Vol 494 (3) ◽  
pp. 3675-3685 ◽  
Author(s):  
Che-Yu Chen ◽  
Lee G Mundy ◽  
Eve C Ostriker ◽  
Shaye Storm ◽  
Arnab Dhabal

ABSTRACT In typical environments of star-forming clouds, converging supersonic turbulence generates shock-compressed regions, and can create strongly magnetized sheet-like layers. Numerical magnetohydrodynamic simulations show that within these post-shock layers, dense filaments and embedded self-gravitating cores form via gathering material along the magnetic field lines. As a result of the preferred-direction mass collection, a velocity gradient perpendicular to the filament major axis is a common feature seen in simulations. We show that this prediction is in good agreement with recent observations from the CARMA Large Area Star Formation Survey (CLASSy), from which we identified several filaments with prominent velocity gradients perpendicular to their major axes. Highlighting a filament from the north-west part of Serpens South, we provide both qualitative and quantitative comparisons between simulation results and observational data. In particular, we show that the dimensionless ratio Cv ≡ Δvh2/(GM/L), where Δvh is half of the observed perpendicular velocity difference across a filament, and M/L is the filament’s mass per unit length, can distinguish between filaments formed purely due to turbulent compression and those formed due to gravity-induced accretion. We conclude that the perpendicular velocity gradient observed in the Serpens South north-west filament can be caused by gravity-induced anisotropic accretion of material from a flattened layer. Using synthetic observations of our simulated filaments, we also propose that a density-selection effect may explain observed subfilaments (one filament breaking into two components in velocity space) as reported in recent observations.

1979 ◽  
Vol 24 (5) ◽  
pp. 481-488 ◽  
Author(s):  
Burton G. Burton-Bradley

Arecaidinism, or betel-nut habituation, has existed since earliest recorded times. The custom is restricted to a large area to the north and north-west of Australia and enters into the daily life of well over 200 million people. The impropriety of interfering with other people's customs, however, has not prevented the imposition of alien values and many believe the practice must be stopped. The arguments advanced against arecaidinism are ostensibly esthetic, addictive and oncogenic in nature, but may have other origins. An account is given of the history, pharmacology, economic aspects, culture functions, psychiatric implications, and an alleged relationship to oral carcinoma in the associated research, all of which indicate a complex habit deeply rooted in the daily living of the peoples concerned. It is inextricably interwoven with the overall patterning of the psychological, social, cultural and economic behaviour. On the evidence there can be little doubt that the betel chewing mixture is a fairly harmless stimulant and addictive agent and that the esthetic and oncogenic arguments remain unsupported by studies with any significant degree of scientific rigour at the present time. The antagonists should look more deeply into their own underlying motivations, the true state of their knowledge and, in the unlikely event of their programs being successful, should ask themselves what is likely to take its place.


2021 ◽  
Vol 61 (2) ◽  
pp. 611
Author(s):  
Jarrad Grahame ◽  
Jianfeng Yao

The Davros-Typhon Multi-Client 3D surveys are located approximately 70km from the north-west coast of Australia, largely covering the NE trending Dampier Sub-basin and straddling the Rankin Trend within the Northern Carnarvon Basin. The basins within the North West Shelf formed as a result of seafloor spreading, associated with the breakup of the North West margin of East Gondwana. The combined, contiguous Davros-Typhon survey areas cover a number of significant discoveries and producing fields, which include both oil and gas accumulations. The key objective of the survey was to enhance the imaging of Triassic to Lower Cretaceous reservoir units and to develop a new interpretation framework, made possible by the modern broadband acquisition parameters and advanced processing techniques. Challenges associated with imaging and interpretation include the effects of high velocity carbonate overburden, steeply dipping structures, fault shadow and structural complexity at depth, which is critical for evaluation of reservoir targets. A major reprocessing effort was undertaken to further mitigate these issues, which included Davros and a number of adjacent existing 3D surveys, resulting in the Typhon Multi-Client 3D. CGG Multi-client and New Ventures geoscientists, in collaboration with CGG Seismic Imaging, have undertaken new interpretation and amplitude versus offset (AVO) inversion analysis using subsets of the Typhon 3D. The resulting volume-based attribute analysis and integration of new AVO inversion results demonstrates enhanced attribute quality for the reprocessed data and provides a platform for quantitative analysis over a large area of the Northern Carnarvon Basin.


2020 ◽  
Vol 494 (3) ◽  
pp. 3405-3412
Author(s):  
Xiao-Na Sun ◽  
Rui-Zhi Yang ◽  
Xiang-Yu Wang

ABSTRACT We report the Fermi Large Area Telescope (Fermi-LAT) detection of the γ-ray emission towards the young massive star cluster RSGC 1. Using the latest source catalogue and diffuse background models, we found that the diffuse γ-ray emission in this region can be resolved into three different components. The GeV γ-ray emission from the region HESS J1837-069 has a photon index of 1.83 ± 0.08. Combining with the HESS and MAGIC data, we argue that the γ-ray emission in this region likely originates from a pulsar wind nebula. The γ-ray emission from the north-west part (region A) can be modelled by an ellipse with the semimajor and semiminor axes of 0.5° and 0.25°, respectively. The GeV emission has a hard spectrum with a photon index of about −2 and partially coincides with the TeV source MAGIC J1835-069. The possible origin of the γ-ray emission in this region is the interaction of the cosmic rays (CRs) accelerated by SNR G24.7+0.6 or/and the OB cluster G25.18+0.26 with the surrounding gas clouds. The GeV γ-ray emission from the south-east region (region B) can be modelled as an ellipse with the semimajor and semiminor axes of 0.9° and 0.5°, respectively, and also reveals a hard γ-ray spectrum. We argue that the most probable origin is the interaction of the accelerated protons in the young massive star cluster RSGC 1 with ambient gas clouds, and the total CR proton energy is estimated to be as high as ${\sim}1\times 10^{50}\ \rm erg$.


Ocean Science ◽  
2009 ◽  
Vol 5 (4) ◽  
pp. 621-634 ◽  
Author(s):  
J. M. Huthnance ◽  
J. T. Holt ◽  
S. L. Wakelin

Abstract. We review mechanisms and studies of exchange between the north-east Atlantic and the adjacent shelf seas. Well-developed summer upwelling and associated filaments off Portugal and north-west Spain give exchange O(3 m2/s per unit length of shelf). Prevailing westerly winds further north drive exchange O(1 m2/s). Poleward flow along most of the upper slope has associated secondary circulation O(1 m2/s), meanders and eddies. Eddies are shed from slope waters into the Bay of Biscay, and local exchanges occur at shelf spurs and depressions or canyons (e.g. dense-water cascading of order 1 m2/s). Tidal transports are larger, but their reversal every six hours makes exchange largely ineffective except where internal tides are large and non-linear, as in the Celtic Sea where solitons carry water with exchange O(1 m2/s). These various physical exchanges amount to an estimated 2–3 m2/s per unit length of shelf, between ocean and shelf. A numerical model estimate is comparable: 2.5×106 m3/s onto and off the shelf from Brittany to Norway. Mixing controls the seasonal thermocline, affecting primary production and hence fluxes and fate of organic matter. Specifically, CO2 take-up by primary production, settling below the thermocline before respiration, and then off-shelf transport, make an effective shelf-sea "pump" (for CO2 from the atmosphere to the deep ocean). However, knowledge of biogeochemical fluxes is generally sparse, giving scope for more measurements, model validation and estimates from models.


1928 ◽  
Vol 65 (1) ◽  
pp. 12-25 ◽  
Author(s):  
F. Smithson

From the southern shores of Dublin Bay there stretches to the south-west a broad granite intrusion with rocks of supposed Ordovician age on both sides of it. These rocks are metamorphosed near the granite, and the belt of metamorphism is wider on the south-east than on the north-west side, indicating, no doubt, that the plane of junction dips more steeply on the latter side. Near Dublin the Lower Carboniferous rocks rest unaltered upon the granite. On the south-east side, in the northern part of the county of Wicklow, the belt of Ordovician rocks is only some 2 miles wide, and a large area of supposed Cambrian rocks lies between it and the sea. Around the hill of Carrickgollogan a. patch of similar rocks appears incongruously in the middle of the Ordovician belt. After a study of the region to the south of Dublin one seems to be naturally drawn towards this small area around Carrickgollogan, for it presents a problem, the key to which may explain the geological structure of a much wider area.


2009 ◽  
Vol 6 (2) ◽  
pp. 1061-1092 ◽  
Author(s):  
J. M. Huthnance ◽  
J. T. Holt ◽  
S. L. Wakelin

Abstract. We review mechanisms and studies of exchange between the north-east Atlantic and the adjacent shelf sea. Mechanisms include: well-developed summer upwelling and associated filaments off Portugal and north-west Spain giving exchange O(3 m2/s per unit length of shelf); prevailing westerly winds further north driving exchange O(1 m2/s); poleward flow along most of the upper slope with associated secondary circulation O(1 m2/s); meanders and eddies in this poleward flow; eddies shed from slope waters into the Bay of Biscay; local exchanges at shelf spurs and depressions or canyons (e.g. dense-water cascading of order 1 m2/s). Tidal transports are larger; their reversal every six hours makes exchange largely ineffective except where internal tides are large and non-linear, as in the Celtic Sea where solitons carry water with exchange O(1 m2/s). These various physical exchanges amount to an estimated 2–3 m2/s per unit length of shelf, between ocean and shelf; a numerical model estimate is comparable: 2.5×106 m3/s onto and off the shelf from Brittany to Norway. Mixing controls the seasonal thermocline, affecting primary production and hence fluxes and fate of organic matter. Specifically, CO2 take-up by primary production, settling below the thermocline before respiration, and then off-shelf transport, make an effective shelf-sea "pump" (for CO2 from the atmosphere to the deep ocean). However, knowledge of biogeochemical fluxes is generally sparse; there is scope for more measurements, model validation and estimates from models.


Author(s):  
Matthew J. Owen ◽  
Nicky H. Witt ◽  
Zyad Al-Hamdani ◽  
Niels Nørgaard-Pedersen ◽  
Katrine J. Andresen ◽  
...  

During August 2017, as part of the habitat mapping of Natura2000 areas, a geophysical survey of a large area within the Skagerrak was undertaken by the Geological Survey of Denmark and Greenland. In this article, we use the acquired data to discuss the geology of Tannis Bugt (Fig. 1), a large shallow bay at the north-west coast of Vendsyssel. The bay extends 40 km between Hirtshals in the west and Skagen in the east forming the northern-most Danish Skagerrak coast.


2012 ◽  
Vol 52 (1) ◽  
pp. 7 ◽  
Author(s):  
Thomas Bernecker

The Australian Government formally releases new offshore exploration areas at the annual APPEA conference. In 2012, 27 areas in nine offshore basins are being released for work program bidding. Closing dates for bid submissions are either six or twelve months after the release date, i.e. 8 November 2012 or 9 May 2013, depending on the exploration status in these areas and on data availability. As was the case in 2011, this year’s Release again covers a total offshore area of about 200,000 km2. The Release Areas are located in Commonwealth waters offshore Northern Territory, Western Australia, South Australia, Victoria and Tasmania (Fig. 1). Areas on the North West Shelf feature prominently again and include under-explored shallow water areas in the Arafura and Money Shoal basins and rank frontier deep water areas in the outer Browse and Roebuck basins as well as on the outer Exmouth Plateau. Following the recent uptake of exploration permits in the Bight Basin (Ceduna and Duntroon sub-basins), Australia’s southern margin is well represented in the 2012 Acreage Release. Three new areas in the Ceduna Sub-basin, four areas in the Otway Basin, one large area in the Sorell Basin and two areas in the eastern Gippsland Basin are on offer. Multiple industry nominations for this Acreage Release were received, confirming the healthy status of exploration activity in Australia. The Australian government continues to support these activities by providing free access to a wealth of geological and geophysical data.


1936 ◽  
Vol 16 (3) ◽  
pp. 295-320 ◽  
Author(s):  
B. H. St. J. O'Neil

Mynydd Craig-goch, the westernmost height of a rocky ridge of the Snowdon mountains, slopes gently down to a watershed at the head of the Afon Dwyfach, over which run the railway and the main road from Criccieth and Portmadoc to Caernarvon. Between the ninth and tenth milestones from Caernarvon, immediately to the east of the road and thus on the lowest part of the mountain slope, there lie the remains of a most extensive primitive agricultural settlement. It is not marked on the Ordnance Survey map (6 in. 26 NE.), but was known locally, and the farm within which most of it lies bears the significant name Caerau. Its recognition as a site of great possibilities on account of its excellent state of preservation is due to Mr. W. J. Hemp, F.S.A. The settlement must originally have extended north and south for a distance of about half a mile. It may, indeed, have been contiguous with other settlements on the north and north-west, thus forming part of a large area of cultivated land, since there exists in excellent preservation a house or hut-group of the same type with at least one typical field about one mile to the west on the farm of Cefn Graianog. This point, however, cannot now be determined on account of more recent agricultural developments around the farm of Bodychain.


1964 ◽  
Vol 55 (2) ◽  
pp. 289-304 ◽  
Author(s):  
W. Klassen ◽  
B. Hocking

The influence of a deep river valley system on the distribution of dispersing Aedes mosquitos was studied during 1958–59 in the vicinity of Edmonton, Alberta, Canada. Mosquito breeding within an area extending two to three miles beyond the city limits was prevented by anti-larval measures, and almost the only remaining breeding places were situated on the plains several miles to the north-west and south-east, yet considerable numbers of mosquitos appeared every spring in that part of the city included in the valley-ravine system of the North Saskatchewan River. Previous work had suggested that mosquitos dispersing across the plains were collected by the valley-ravine system and entered the city by passing down the main valley. The present paper attempts to account for this directed dispersal in terms of the behaviour of Aedes mosquitos in response to certain physical factors in the environment. The species mainly concerned were Aedes cataphylla Dyar, A. fitchii (Felt & Young), A. excrucians (Wlk.) and A. stimulans (Wlk.).The initiation of dispersal flight downwind across the plains at twilight was observed. This took place soon after emergence and was not prevented by moderate winds. It was shown experimentally that neither high wind speeds nor turbulence inhibited the flight of newly emerged Aedes mosquitos, but that individuals several days old were reluctant to take flight in turbulent conditions. Since wind speeds on the plains were generally higher than those in the valleys, these reactions would tend to confine older mosquitos to the valleys while not preventing dispersal of newly emerged mosquitos across the plains.The direction of the initial dispersal flights from the breeding places was observed in mosquitos escaping from rearing cages. Take-off was characteristically into the wind, but re-orientation downwind took place when the mosquitos began to be blown backwards in flight. It was shown experimentally, by releasing mosquitos in the field when the wind was very light, that the preferred direction of flight uninfluenced by wind was towards the lowest part of the horizon, both on the plains and in the valley. This response would tend to cause mosquitos on the plain to fly into ravines and valleys, and thence down-stream within them. Dispersing mosquitos would thus tend to be held by any valleys or ravines in their path.Swarming was never observed near the pools from which the mosquitos emerged, but was mainly seen in the valley or on the edge of the valley and ravines. Swarming of A. cataphylla took place during the evenings after the initial dispersal. The swarms were predominantly male but mating occurred during swarming. A cohesive factor seemed to be involved in the behaviour of the swarms, and further dispersal also seemed to occur gregariously; the movement of large male swarms down the river valley was observed.By the application of optomotor theories of insect flight to previously published data on the flight speed and behaviour of A. aegypti (L.) and A. punctor (Kby.), the relationships between wind speed and permissible heights of flight of these species upwind and downwind were calculated. These relationships were consistent with the observations on dispersal of Aedes mosquitos in the Edmonton area, and could largely explain the mechanism by means of which deep valleys attracted and held dispersing mosquitos.In contrast to the open plains, the wooded river valley provides a more favourable environment for adult mosquitos. The supply of nectar is greater, saturation deficiency and wind speeds are lower and less variable, and shaded resting sites are more abundant.Observations on mosquitos in chambers with either vertical or horizontal humidity gradients suggested that the behaviour of Aedes mosquitos is not greatly influenced by humidity.


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