Ultrasoft narrow-line Seyfert 1 galaxies and X-ray surveys     

N. Brandt  T. Boller 《Astronomische Nachrichten》1998,319(3):163-166

Note from the editor: This article is a re-print of the original, which appeared in Astron. Nachr. 319 (1/2), 7 (1998). In the original version the figure was ruined in the process of paper production and the scientific content of the paper considerably degraded. Instead of printing only the correct figure, thus loosing the scientific context, we decided to re-print the whole article. We describe how recent X-ray surveys have led to advances in the understanding of ultrasoft narrow-line Seyfert 1 galaxies. The number of known ultrasoft narrow-line Seyfert 1s has increased greatly in recent years due to X-ray surveys, and it is now possible to obtian high quality 0.1–10 keV spectral and variability measurements for a large number of these galaxies. We generalize some of the correlations between X-ray properties and optical emission line properties,focusing on how the ROSAT band spectral slope appears to be directly connected to the Boroson & Green (1992) primary eigenvector. We discuss how ultrasoft narrow-line Seyfert 1s may well have extremal values of a primary physical parameter, and we describe new projects that should further improve our understanding of these extreme representatives of Seyfert activity.  相似文献   

Influence of the equatorial deep jets on the north equatorial countercurrent   总被引：1，自引：1，他引：0  

Jan-Dirk Matthießen  Richard J. Greatbatch  Peter Brandt  Martin Claus  Sven-Helge Didwischus 《Ocean Dynamics》2015,65(8):1095-1102

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The X-ray variability of the Seyfert 1 galaxy MCG–6-30-15 from long ASCA and RXTE observations     

Julia C. Lee  †  A. C. Fabian  Christopher S. Reynolds  ‡  W. N. Brandt  Kazushi Iwasawa 《Monthly notices of the Royal Astronomical Society》2000,318(3):857-874

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Compton-thick X-ray absorption in the Seyfert galaxies Tololo 0109383 and ESO 138G1     

M. J. Collinge  W. N. Brandt 《Monthly notices of the Royal Astronomical Society》2000,317(2):L35-L39

We present analyses of the ASCA X-ray spectra of two Seyfert galaxies, Tololo 0109383 and ESO 138G1. In both cases, spectral fitting reveals two statistically acceptable continuum models: Compton reflection and partial covering. Both spectra have strong iron K lines, with equivalent widths greater than 1.5 keV. These large equivalent widths are suggestive of heavier obscuration than that directly indicated by the partial-covering models (  210²³ cm^-2),  with the actual column densities being 'Compton-thick' (i.e.   N _H1.510²⁴ cm^-2).  We use the hard X-ray/[O  iii ] flux correlation for Seyferts and data from the literature to provide additional support for this hypothesis. Since Tololo 0109383 is known to have optical type 1 characteristics such as broad Balmer line components and Fe  ii emission, this result marks it as a notable object.  相似文献   

Wide field monitoring of the X-ray sky using Rotation Modulation Collimators     

Niels Lund  Søren Brandt 《Experimental Astronomy》1995,6(4):19-24

Wide field monitoring is of particular interest in X-ray astronomy due to the strong time-variability of most X-ray sources. Not only does the time-profiles of the persistent sources contain characteristic signatures of the underlying physical systems, but, additionally, some of the most intriguing sources have long periods of quiesense in which they are almost undetectable as X-ray sources, interspersed with relatively brief periods of intense outbursts, where we have unique opportunities of studying dynamical effects, in, for instance, the evolution of accretion discs. Another question for which wide field monitors may provide key information, is the origin and nature of the cosmic gamma ray bursts.Rotation Modulation Collimators (RMC's) were originally introduced in X-ray astronomy to provide accurate source localizations over extended fields. This role has since been taken over by the grazing incidence telescope systems. The potential of the RMC's as wide field monitors have recently been demonstrated by the WATCH instruments on GRANAT and EURECA. It now appears likely, that for use on large, 3-axis stabilized spacecraft, a pinhole camera system may provide better sensitivity than an RMC-system of corresponding physical dimensions. But due to its simplicity, low data rate, and ability to work on spin stabilized (micro)satellites, the RMC wide field monitor may still have a role to play in the X-ray astronomy of the future.  相似文献   

Simulation of the size distribution and erosivity of raindrops and throughfall drops     

C. Jane Brandt 《地球表面变化过程与地形》1990,15(8):687-698

This paper presents a model that simulates the size distribution and erosivity of raindrops and throughfall drops. It utilizes existing models of rainfall drop size distribution and fall velocity and combines them with newly collated evidence of throughfall drop size distributions. A sensitivity analysis reveals that the model is sensitive to parameters that are easily measured or estimated: rainfall intensity, the mean volume drop diameter of the intercepted throughfall, canopy cover, and canopy height. The results of the model may be used at two levels. Firstly, to calculate specifically the size and fall velocity of individual drops, parameters that are needed in studies examining the response of soil surfaces to forces applied by rainfall. Secondly, to produce erosivity indices, based on rainfall intensity but which take account of the effects of a vegetation canopy. The paper shows that while the kinetic energy of rainfall (E(0), J mm^?1 m^?2) may be calculated from an equation of the familiar form: the kinetic energy of throughfall under any canopy may be calculated by combining this equation with another that relates the energy of drops under a 100 per cent canopy cover (E(100)) and the canopy height: .  相似文献   

An experimental study of two-dimensional atmospheric gas dispersion near two objects     

S. Kim  H. Brandt  B. R. White 《Boundary-Layer Meteorology》1990,52(1-2):1-16

Two-dimensional gas dispersion in the atmosphere was investigated experimentally using an atmospheric boundary-layer wind tunnel. Argon gas, which is one and one half times heavier than air, was injected two-dimensionally and uniformly near two square objects at the rates of 3.55 and 4.93 m³/min per lateral meter from the bottom of the wind tunnel floor through a porous metal plate. The gas injection source was located at one object distance upstream of the first square object. Gas concentrations and velocities of the flow field were measured using an aspirating hot-film probe and a low velocity flow analyzer, respectively. The gas was dispersed no higher than approximately 2.0 object heights near the objects, and dispersed no higher than 3.5 object heights at the location of downwind distances of nine object lengths for the injection rates tested. The gas concentrations between the injection source and the first object were about 4 to 5 times higher than the gas concentrations of the other locations. The gas concentrations were 2 to 3% in the recirculation zone between the two objects, and were less than 2% behind the second object. The air-gas mixtures in the recirculation zone between the two objects and within the wake recirculation bubble behind the second object were well mixed and no gravitational settlement was detected in those regions. However, as the mixture moved down-stream, the gravitational settlement occurred beyond the wake recirculation bubble. This paper demonstrates that it is possible to model a two-dimensional heavy gas release in the atmosphere using wind-tunnel simulation with properly matched similitude parameters.  相似文献   

Spatial and Temporal Variability in Estuary Habitat Use by American Alligators     

Ikuko Fujisaki  Kristen M. Hart  Michael S. Cherkiss  Frank J. Mazzotti  Jeff S. Beauchamp  Brian M. Jeffery  Laura A. Brandt 《Estuaries and Coasts》2016,39(5):1561-1569

Estuarine habitat occupied by Alligator mississippiensis, a primarily freshwater species, is spatially and temporally heterogeneous largely due to a salinity gradient that fluctuates. Using long-term night light survey data, we examined seasonal patterns in alligators’ habitat use by size classes in midstream and downstream estuary zones of Shark River, Everglades National Park, in southern Florida. We observed predominantly large-sized alligators (total length?≥?1.75 m); observations of alligators in the small size classes (0.5 m?≤?total length?<?1.25 m) were rare especially in the higher-salinity downstream zone. The density of alligators in the downstream zone was lower than that of the midstream zone during the dry season when salinity increases due to reduced precipitation. Conversely, the density of the large size alligators was higher in the downstream zone than in the midstream zone during the wet season, likely because of reduced salinity. We also found a significant declining trend over time in the number of alligators in the dry season, which coincides with the reported decline in alligator relative density in southern Florida freshwater wetlands. Our results indicated high adaptability of alligators to the fluctuating habitat conditions. Use of estuaries by alligators is likely driven in part by physiology and possibly by reproductive cycle, and our results supported their opportunistic use of estuary habitat and ontogenetic niche shifts.  相似文献   

Water availability and land subsidence in the Central Valley,California, USA     

Claudia C. Faunt  Michelle Sneed  Jon Traum  Justin T. Brandt 《Hydrogeology Journal》2016,24(3):675-684

The Central Valley in California (USA) covers about 52,000 km² and is one of the most productive agricultural regions in the world. This agriculture relies heavily on surface-water diversions and groundwater pumpage to meet irrigation water demand. Because the valley is semi-arid and surface-water availability varies substantially, agriculture relies heavily on local groundwater. In the southern two thirds of the valley, the San Joaquin Valley, historic and recent groundwater pumpage has caused significant and extensive drawdowns, aquifer-system compaction and subsidence. During recent drought periods (2007–2009 and 2012-present), groundwater pumping has increased owing to a combination of decreased surface-water availability and land-use changes. Declining groundwater levels, approaching or surpassing historical low levels, have caused accelerated and renewed compaction and subsidence that likely is mostly permanent. The subsidence has caused operational, maintenance, and construction-design problems for water-delivery and flood-control canals in the San Joaquin Valley. Planning for the effects of continued subsidence in the area is important for water agencies. As land use, managed aquifer recharge, and surface-water availability continue to vary, long-term groundwater-level and subsidence monitoring and modelling are critical to understanding the dynamics of historical and continued groundwater use resulting in additional water-level and groundwater storage declines, and associated subsidence. Modeling tools such as the Central Valley Hydrologic Model, can be used in the evaluation of management strategies to mitigate adverse impacts due to subsidence while also optimizing water availability. This knowledge will be critical for successful implementation of recent legislation aimed toward sustainable groundwater use.  相似文献   

Bathymetric distribution patterns of Southern Ocean macrofaunal taxa: Bivalvia, Gastropoda, Isopoda and Polychaeta     

Angelika Brandt  Katrin Linse  Myriam Schüller   《Deep Sea Research Part I: Oceanographic Research Papers》2009,56(11):2013-2025

The aim of this study is to compare the depth distributions of four major Southern Ocean macrobenthic epi- and infaunal taxa, the Bivalvia, Gastropoda, Isopoda, and Polychaeta, from subtidal to abyssal depth. All literature data up to summer 2008, as well as the unpublished data from the most recent ANDEEP I–III (Antarctic benthic deep-sea biodiversity: colonisation history and recent community patterns) expeditions to the Southern Ocean deep sea are included in the analysis. Benthic invertebrates in the Southern Ocean are known for their wide bathymetric ranges. We analysed the distributions of four of the most abundant and species-rich taxa from intertidal to abyssal (5200 m) depths in depth zones of 100 m. The depth distributions of three macrofaunal classes (Bivalvia, Gastropoda, Polychaeta) and one order (Isopoda) showed distinct differences. In the case of bivalves, gastropods and polychaetes, the number of species per depth zone decreased from the shelf to the slope at around 1000 m depth and then showed stable low numbers. The isopods showed the opposite trend; they were less species rich in the upper 1000 m but increased in species numbers from the slope to bathyal and abyssal depths. Depth ranges of families of the studied taxa (Bivalvia: 31 families, Gastropoda: 60, Isopoda: 32, and Polychaeta: 46 families) were compiled and illustrated. At present vast areas of the deep sea in the Southern Ocean remain unexplored and species accumulation curves showed that only a fraction of the species have been discovered to date. We anticipate that further investigations will greatly increase the number of species known in the Southern Ocean deep sea.  相似文献