Temporal trends in abundance of fish in the tidal Delaware River

Water quality in the tidal Delaware River has improved dramatically over the last several decades. Areas near Philadelphia that were once anoxic and formed a pollution block to migratory fish passage now rarely experience dissolved oxygen concentrations less than 3 ppm. To assess whether these improvements in water quality led to increased abundance of juvenile fishes, data from a beach seine survey conducted annually since 1980 were examined. The number of species captured increased throughout the tidal river, but the increase was greatest in the areas downstream of Philadelphia, wheare water quality has improved the most. Abundance of juvenile striped bass and American shad, two important game species in the river whose migratory patterns make them susceptible to water quality problems, both increased more than, 1,000-fold during the last decade. Correlatations between the temporal abundance patterns of these species in the tidal Delaware River and in other East Coast systems were poor, suggesting that increases in their numbers were related more closely to improving conditions within the Delaware than to factors affecting coastal stocks.     

A radiative-conductive model for the prediction of radiation fog

A conductive-radiative model is used to predict the formation and growth of radiation fog. This is accomplished by solving numerically the heat and mass transport equations in conjunction with an approximate form of the radiative transfer equation. The equations of motion in simplified form are included in the physical system to make use of Blackadar's (1962) formulation of the exchange coefficient of the boundary layer.It is found for a number of hypothetical test cases that the model gives results which appear to represent real physical conditions. One actual situation is tested. Results show that the model reproduces better than qualitatively those parameters which are obtained from routine observations.     

The geology of part of an orogenic belt in western Sierra Leone,West Africa

Zusammenfassung Die Sierra Leone unterteilt sich in zwei Haupteinheiten. Die östliche ist ein Teil des festen präkambrischen westafrikanischen Kratons und besteht aus hochgradig metamorphem Gestein und Granitgneisen. Die Strukturen verlaufen in vorherrschend NE-Richtung. Der westliche Teil enthält Elemente eines orogenen Gürtels, nämlich der Rokeliden, die entweder im späten Präkambrium oder frühen Paläozoikum entstanden sind und nach NNW streichen. Die Gesteinsserien, die den orogenen Gürtel bilden, setzen sich aus dem Kasila-System, einer unbenannten Gneisgruppe östlich davon, den Rokel River Series und den Marampa Schists zusammen. Die sich an das Kasila-System, umbenannt in Kasila-Gruppe, anschließenden Gneise und wahrscheinlich auch die Kasila-Gruppe selbst können mit dem Gestein des Kratons verglichen werden, sind jedoch während der Entstehung der Rokeliden neu überprägt worden. Sie bilden die Basis der Mulde, die Sedimente und vulkanisches Gestein aus den Rokel River Series und den Marampa Schists enthält. Die Rokel River Series sind neu benannt und unterteilen sich in die Rokel River Gruppe mit sechs Formationen und in die Taban Formation, die aus nach-orogener Molasse besteht. Die Marampa Schists sind neu benannt in Marampa Formation. Das Ausmaß der Metamorphose steigert sich über die Rokeliden nach WSW, und die Marampa Formation ist der am stärksten metamorphisierte Teil der geosynklinalen Ausfüllung.

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Sierra Leone is divisible into two major structural units. The eastern one is part of the stable Precambrian West African craton and consists of high grade metamorphic rocks and granitic gneisses. The foliation has a dominantly NE trend. The western unit contains the elements of an orogenic belt named the Rokelides, which formed in either late Precambrian or early Palaeozoic, and trends NNW. The rock groups which comprise the orogenic belt are the Kasila System, an unnamed group of gneisses on the east of it, the Rokel River Series and the Marampa Schists. The gneisses adjacent to the Kasila System, renamed Kasila Group, and also, probably, the Kasila Group can be correlated with rocks in the craton, but were refoliated during the Rokelide orogenesis. They constituted the basement to the geosyncline which contained sediments and volcanic rocks of the Rokel River Series and Marampa Schists. The Rokel River Series is renamed, and divided into Rokel River Group which contains six formations, and the Taban Formation which is post-orogenic molasse. The Marampa Schists are renamed the Marampa Formation. The intensity of metamorphism and deformation increases across the Rokelides towards the WSW and the Marampa Formation is the most highly metamorphosed part of the geosynclinal infilling.

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Résumé Le Sierra Leone peut se diviser en deux principales sections structurales. La section orientale fait partie du craton stable précambrien de l'Afrique occidentale, formé de roches métamorphiques de haute qualité et de gneiss de granit. La foliation a principalement une direction NE. La section occidentale contient les éléments d'une ceinture orogénique appelée les Rokelides qui ont été formées soit vers la fin de la période précambrienne, soit au début de la période paléozoique et en direction NNW. Les groupes rocheux qui comprennent la ceinture orogénique sont le Kasila System, un groupe de gneiss sans nom situé à son côté est, la Rokel River Series et les Marampa Schists. Les gneiss avoisinant le Kasila System, renommé Kasila Group et en toute probilité le Kasila Group également peuvent être rattachés aux roches du craton mais auraient été refoliés pendant l'orogenèse Rokelide. Ils ont formé la base du géosynclinal qui contient des sédiments et des roches volcaniques de la Rokel River Series et des Marampa Schists. La Rokel River Series a été renommée et divisée en Rokel River Group qui contient six formations et la Taban Formation qui est la mollasse post-orogénique. Les Marampa Schists ont été renommés la Marampa Formation. L'intensité du métamorphisme et de la déformation augmente vers WSW à travers les Rokelides, et la Marampa Formation est la partie la plus métamorphosée de l'accumulation géosynclinale.

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Constructing the Coronal Magnetic Field By Correlating Parameterized Magnetic Field Lines With Observed Coronal Plasma Structures

A method is presented for constructing the coronal magnetic field from photospheric magnetograms and observed coronal loops. A set of magnetic field lines generated from magnetogram data is parameterized and then deformed by varying the parameterized values. The coronal flux tubes associated with this field are adjusted until the correlation between the field lines and the observed coronal loops is maximized. A mathematical formulation is described which ensures that (i) the normal component of the photospheric field remains unchanged, (ii) the field is given in the entire corona over an active region, (iii) the field remains divergence-free, and (iv) electric currents are introduced into the field. It is demonstrated that a parameterization of a potential field, comprising a radial stretching of the field, can provide a match for a simple bipolar active region, AR 7999, which crossed the central meridian on 1996 November 26. The result is a non-force-free magnetic field with the Lorentz force being of the order of 10^–5.5 g cm s^–2 resulting from an electric current density of 0.079 A m^–2. Calculations show that the plasma beta becomes larger than unity at a relatively low height of 0.25 r supporting the non-force-free conclusion. The presence of such strong non-radial currents requires large transverse pressure gradients to maintain a magnetostatic atmosphere, required by the relatively persistent nature of the coronal structures observed in AR 7999. This scheme is an important tool in generating a magnetic field solution consistent with the coronal flux tube observations and the observed photospheric magnetic field.     

A need for incentivizing field hydrology,especially in an era of open data: discussion of “The role of experimental work in hydrological sciences – insights from a community survey”*

ABSTRACT

The sharing of data and collection of new data are both essential, but they are not inherently complementary. When data are openly available, researchers may be motivated to use those data rather than collect more because field work has costs and risks. The competitive advantage to those who do not put resources towards fieldwork may discourage field hydrology. Allocating efforts towards generating field data, which benefits hydrological sciences, is not necessarily best for individual hydrologists, especially in an era of open data. The objective of this work is to open a conversation on whether individuals’ best interests may contrast with the community’s desire for new observations. If the community wants new field observations, there is a need to consider the shifting balance of incentives and disincentives for pursuing field studies in hydrology.