In Situ Time-Series Measurements of Subseafloor Sediment Properties     

Wheatcroft  R.A. Stevens  A.W. Johnson  R.V. 《Oceanic Engineering, IEEE Journal of》2007,32(4):862-871

The capabilities and diversity of subsurface sediment sensors lags significantly from what is available for the water column, thereby limiting progress in understanding time-dependent seabed exchange and high-frequency acoustics. To help redress this imbalance, a new instrument, the autonomous sediment profiler (ASP), is described herein. ASP consists of a four-electrode, Wenner-type resistivity probe and a thermistor that log data at 0.1-cm vertical intervals over a 58-cm vertical profile. To avoid resampling the same spot on the seafloor, the probes are moved horizontally within a 20 times 100-cm^-2 area in one of three preselected patterns. Memory and power capacities permit sampling at hourly intervals for up to 3-mo duration. The system was tested in a laboratory tank and shown to be able to resolve high-frequency sediment consolidation, as well as changes in sediment roughness. In a field test off the southern coast of France, the system collected resistivity and temperature data at hourly intervals for 16 d. Coupled with environmental data collected on waves, currents, and suspended sediment, the ASP is shown to be useful for understanding temporal evolution of subsurface sediment porosity, although no large depositional or erosional events occurred during the deployment. Following a rapid decrease in bottom-water temperature, the evolution of the subsurface temperature field was consistent with the 1-D thermal diffusion equation coupled with advection in the upper 3-4 cm. Collectively, the laboratory and field tests yielded promising results on time-dependent seabed change.  相似文献   

Data collection methodology for dynamic temperature model testing and corroboration     

B. T. Neilson  D. K. Stevens  S. C. Chapra  C. Bandaragoda 《水文研究》2009,23(20):2902-2914

This article describes a data collection approach for determining the significance of individual heat fluxes within streams with an emphasis on testing (i.e. identification of possible missing heat fluxes), development, calibration and corroboration of a dynamic temperature model. The basis for developing this approach was a preliminary temperature modelling effort on the Virgin River in southwestern Utah during a low‐flow period that suggested important components of the energy balance might be missing in the original standard surface‐flux temperature model. Possible missing heat fluxes were identified as bed conduction, hyporheic exchange, dead zone warming and exchange and poor representation of the amount of solar radiation entering the water column. To identify and estimate the relative importance of the missing components, a comprehensive data collection effort was developed and implemented. In particular, a method for measuring shortwave radiation behaviour in the water column and an in situ method for separating out bed conduction and hyporheic influences were established. The resulting data and subsequent modelling effort indicate that hyporheic and dead zone heat fluxes are important, whereas solar radiation reflection at the water surface was found to be insignificant. Although bed conduction can be significant in certain rivers, it was found to have little effect on the overall heat budget for this section of the Virgin River. Copyright © 2009 John Wiley & Sons, Ltd.  相似文献   

Scientific field training for human planetary exploration     

D.S.S. Lim  G.L. Warman  C.P. McKay  M.M. Marinova  D. Andersen  Z. Cardman  M.D. Delaney  A.L. Forrest  B.E. Laval  P. Nuytten  M. Reay  D. Schulze-Makuch  G.F. Slater 《Planetary and Space Science》2010,58(6):920-930

Forthcoming human planetary exploration will require increased scientific return (both in real time and post-mission), longer surface stays, greater geographical coverage, longer and more frequent EVAs, and more operational complexities than during the Apollo missions. As such, there is a need to shift the nature of astronauts’ scientific capabilities to something akin to an experienced terrestrial field scientist. To achieve this aim, the authors present a case that astronaut training should include an Apollo-style curriculum based on traditional field school experiences, as well as full immersion in field science programs. Herein we propose four Learning Design Principles (LDPs) focused on optimizing astronaut learning in field science settings. The LDPs are as follows:

(1)

LDP#1: Provide multiple experiences: varied field science activities will hone astronauts’ abilities to adapt to novel scientific opportunities

(2)

LDP#2: Focus on the learner: fostering intrinsic motivation will orient astronauts towards continuous informal learning and a quest for mastery

(3)

LDP#3: Provide a relevant experience—the field site: field sites that share features with future planetary missions will increase the likelihood that astronauts will successfully transfer learning

(4)

LDP#4: Provide a social learning experience—the field science team and their activities: ensuring the field team includes members of varying levels of experience engaged in opportunities for discourse and joint problem solving will facilitate astronauts’ abilities to think and perform like a field scientist.

The proposed training program focuses on the intellectual and technical aspects of field science, as well as the cognitive manner in which field scientists experience, observe and synthesize their environment. The goal of the latter is to help astronauts develop the thought patterns and mechanics of an effective field scientist, thereby providing a broader base of experience and expertise than could be achieved from field school alone. This will enhance their ability to execute, explore and adapt as in-field situations require.  相似文献   

New Urbanist developments in flood-prone areas: safe development,or safe development paradox?     

Mark R. Stevens  Yan Song  Philip R. Berke 《Natural Hazards》2010,53(3):605-629

Government policies intended to reduce flood losses can increase the potential for catastrophe by stimulating development inside the floodplain, a phenomenon referred to as the “safe development paradox.” New Urbanist design has the potential to both exacerbate and alleviate flood risks. Because they are built at relatively high densities, New Urbanist developments can exacerbate risk by placing more people and property in harm’s way. Conversely, New Urbanist design features theoretically better enable designers of New Urbanist developments to avoid floodplain portions of project sites than designers of conventional subdivisions. Using a sample of New Urbanist developments in the US that contain floodplain portions within their boundaries, this paper focuses on whether and why these developments locate built structures inside the floodplain. The authors find that roughly 30% of the developments locate structures inside the floodplain, and that the odds of locating structures inside the floodplain increase with the proportion of the project site located inside the floodplain and decrease with the presence of government policies that prohibit residential development in the floodplain. The authors also identify confusion among government planners regarding the distinction between pre and postconstruction floodplain boundaries. A subset of New Urbanist developments is found to have built structures located outside the postconstruction floodplain boundary, but inside the preconstruction floodplain boundary. This finding is cited as an example of the “safe development paradox” in action. The authors recommend changes in New Urbanist design codes and local government floodplain management to increasingly direct new development away from the floodplain.  相似文献   

An ultraluminous X-ray microquasar in NGC 5408?     

R. Soria  R. P. Fender  D. C. Hannikainen  A. M. Read  I. R. Stevens 《Monthly notices of the Royal Astronomical Society》2006,368(4):1527-1539

We studied the radio source associated with the ultraluminous X-ray source in NGC 5408  ( L _X≈ 10⁴⁰ erg s⁻¹)  . The radio spectrum is steep (index  ≈−1  ), consistent with optically thin synchrotron emission, not with flat-spectrum core emission. Its flux density (≈0.28 mJy at 4.8 GHz, at a distance of 4.8 Mpc) was the same in the March 2000 and December 2004 observations, suggesting steady emission rather than a transient outburst. However, it is orders of magnitude higher than expected from steady jets in stellar-mass microquasar. Based on its radio flux and spectral index, we suggest that the radio source is either an unusually bright supernova remnant, or, more likely, a radio lobe powered by a jet from the black hole (BH). Moreover, there is speculative evidence that the source is marginally resolved with a radius ∼30 pc. A faint H  ii region of similar size appears to coincide with the radio and X-ray sources, but its ionization mechanism remains unclear. Using a self-similar solution for the expansion of a jet-powered electron–positron plasma bubble, in the minimum-energy approximation, we show that the observed flux and (speculative) size are consistent with an average jet power  ≈ 7 × 10³⁸ erg s⁻¹∼ 0.1 L _X∼ 0.1 L _Edd  , an age ≈10⁵ yr, a current velocity of expansion ≈80 km s⁻¹. We briefly discuss the importance of this source as a key to understand the balance between luminosity and jet power in accreting BHs.  相似文献   

Dust in spiral galaxies: global properties     

J. A. Stevens  M. Amure  W. K. Gear 《Monthly notices of the Royal Astronomical Society》2005,357(1):361-380

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A phase-resolved XMM–Newton campaign on the colliding-wind binary HD 152248     

H. Sana  I. R. Stevens  E. Gosset  G. Rauw  J.-M. Vreux 《Monthly notices of the Royal Astronomical Society》2004,350(3):809-828

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Radio observations of super star clusters in dwarf starburst galaxies     

Ian R. Stevens  Duncan A. Forbes  Ray P. Norris 《Monthly notices of the Royal Astronomical Society》2002,335(4):1079-1084

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Probing the wind–wind collision in γ² Velorum with high-resolution Chandra X-ray spectroscopy: evidence for sudden radiative braking and non-equilibrium ionization     

David B. Henley  Ian R. Stevens  Julian M. Pittard 《Monthly notices of the Royal Astronomical Society》2005,356(4):1308-1326

We present a new analysis of an archived Chandra HETGS X-ray spectrum of the WR+O colliding wind binary γ² Velorum. The spectrum is dominated by emission lines from astrophysically abundant elements: Ne, Mg, Si, S and Fe. From a combination of broad-band spectral analysis and an analysis of line flux ratios we infer a wide range of temperatures in the X-ray-emitting plasma (∼4–40 MK). As in the previously published analysis, we find the X-ray emission lines are essentially unshifted, with a mean FWHM of  1240 ± 30 km s⁻¹  . Calculations of line profiles based on hydrodynamical simulations of the wind–wind collision predict lines that are blueshifted by a few hundred  km s⁻¹  . The lack of any observed shift in the lines may be evidence of a large shock-cone opening half-angle (>85°), and we suggest this may be evidence of sudden radiative braking. From the R and G ratios measured from He-like forbidden-intercombination-resonance triplets we find evidence that the Mg  xi emission originates from hotter gas closer to the O star than the Si  xiii emission, which suggests that non-equilibrium ionization may be present.  相似文献   

TOPOGRAPHIC SHADING AND GEOGRAPHICAL PATTERNS OF DIRECT SOLAR RADIATION IN MOUNTAINOUS REGIONS*     

Dale J. Stevens  Alan H. Grey 《The Professional geographer》1986,38(4):383-390

Topographic shading curtails the period and complicates the geographic patterns of insolation in mountainous areas. Maps derived from oblique aerial photographs of shadow lines cast by the irregular, mountainous east horizon in Provo, Utah are used as a case study to illustrate an alternative to existing techniques of solar radiation data collection. For study areas of several hundred square kilometers, this method may be superior in resolution and at the same time more error free and economically feasible than other methods. Measurement of solar inputs received at sample stations scattered through the mapped area show that the phenomenon of topographically delayed sunrise has a distinct effect on daily totals of radiation in the manner suggested by the maps.  相似文献