The Oxford Principles     

Steve Rayner  Clare Heyward  Tim Kruger  Nick Pidgeon  Catherine Redgwell  Julian Savulescu 《Climatic change》2013,121(3):499-512

Scientific momentum is increasing behind efforts to develop geoengineering options, but it is widely acknowledged that the challenges of geoengineering are as much political and social as they are technical. Legislators are looking for guidance on the governance of geoengineering research and possible deployment. The Oxford Principles are five high-level principles for geoengineering governance. This article explains their intended function and the core societal values which they attempt to capture. Finally, it proposes a framework for their implementation in a flexible governance architecture through the formulation of technology-specific research protocols.  相似文献   

Radial and rotational velocities of young brown dwarfs and very low-mass stars in the Upper Scorpius OB association and the ρ Ophiuchi cloud core     

Ryuichi Kurosawa  Tim J. Harries  S. P. Littlefair 《Monthly notices of the Royal Astronomical Society》2006,372(4):1879-1887

We present the results of a radial velocity (RV) survey of 14 brown dwarfs (BDs) and very low-mass (VLM) stars in the Upper Scorpius OB association (UScoOB) and three BD candidates in the ρ Ophiuchi dark cloud core. We obtained high-resolution echelle spectra at the Very Large Telescope using the Ultraviolet and Visual Echelle Spectrograph (UVES) at two different epochs for each object, and measured the shifts in their RVs to identify candidates for binary/multiple systems in the sample. The average time separation of the RV measurements is 21.6 d, and our survey is sensitive to the binaries with separation <0.1 au. We found that four out of 17 objects (or 24⁺¹⁶₋₁₃ per cent by fraction) show a significant RV change in 4–33 d time-scale, and are considered as binary/multiple 'candidates'. We found no double-lined spectroscopic binaries in our sample, based on the shape of cross-correlation curves. The RV dispersion of the objects in UScoOB is found to be very similar to that of the BD and VLM stars in Chamaeleon I (Cha I). We also found the distribution of the mean rotational velocities ( v   sin   i ) of the UScoOB objects is similar to that of the Cha I, but the dispersion of v   sin   i is much larger than that of the Cha I objects.  相似文献   

A maximum-likelihood method for fitting colour–magnitude diagrams     

Tim Naylor  R. D. Jeffries 《Monthly notices of the Royal Astronomical Society》2006,373(3):1251-1263

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The effect of a dense atmosphere on the tidally induced potential of Titan     

Özgür Karatekin  Tim Van Hoolst 《Icarus》2006,183(1):230-232

The effect of the dense atmosphere of Titan on the tidal variations of the external gravitational potential of degree two is quantified. The atmospheric tides perturb the external gravitational potential of Titan in two ways. First, the atmosphere itself contributes directly to the external gravitational potential with a period of 15.945 days. Second, the variable loading of the atmosphere induces mass redistribution within Titan, which also changes the external gravitational potential. It is shown that the relative atmospheric contributions to the tides are most likely less than 2% and vanish almost completely for the most plausible models with a subsurface ocean. This suggest that atmospheric tidal perturbations will contribute only negligibly to Cassini measurements of Titan's gravitational field so that the tidal Love numbers derived from these observations can be directly interpreted in terms of the satellite's interior.  相似文献   

The Shear Testing Programme – I. Weak lensing analysis of simulated ground-based observations     

Catherine Heymans  Ludovic Van Waerbeke  David Bacon  Joel Berge  Gary Bernstein  Emmanuel Bertin  Sarah Bridle  Michael L. Brown  Douglas Clowe  Håkon Dahle  Thomas Erben  Meghan Gray  Marco Hetterscheidt  Henk Hoekstra  Patrick Hudelot  Mike Jarvis  Konrad Kuijken  Vera Margoniner  Richard Massey  Yannick Mellier  Reiko Nakajima  Alexandre Refregier  Jason Rhodes  Tim Schrabback  David Wittman 《Monthly notices of the Royal Astronomical Society》2006,368(3):1323-1339

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Probing the IRC+10 ° 216 circumstellar envelope using spectroscopic observations of background stars     

Tim Kendall  Nicolas Mauron  June McCombie  Peter Sarre 《Astrophysics and Space Science》2004,289(3-4):203-206

A unique and novel set of observations has been undertaken to study the circumstellar envelope (CSE) of the nearby (130 pc) carbon star IRC +10° 216 using optical absorption spectroscopy towards twobackground stars lying beyond the envelope.The primary aim of the observations is to search for diffuse band (DIB)carriers in the CSE. The circumstellar H+2H₂column density expected along the line of sight towards the targets islarge compared to that derived from the small interstellar reddening inthis region, E _B-V< 0.03 mag. We summarise our mainfindings, already reported in Kendall et al. (2002): The 6284Å DIB is detected in the VLT/UVES spectrum of one target, but clearly arises inthe foreground ISM. No other DIB is seen. Hence the DIB carriers, if present in the CSE, have a low abundance relative to H in the C-rich envelope of IRC +10°216, in comparison with this ratio in theISM. An important new result, previously unreported, concerns the detectionof circumstellar C₂ via absorption of the Phillips bandnear 8760Å.  相似文献   

Three-dimensional dust radiative-transfer models: the Pinwheel Nebula of WR 104     

Tim J. Harries  John D. Monnier  Neil H. Symington  Ryuichi Kurosawa 《Monthly notices of the Royal Astronomical Society》2004,350(2):565-574

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A comparison between cokriging and ordinary kriging: Case study with a polymetallic deposit     

Guocheng Pan  Dave Gaard  Ken Moss  Tim Heiner 《Mathematical Geology》1993,25(3):377-398

Cokriging is applied to the estimation of mineral resources in a polymetallic deposit. Several major steps, which should be taken in using cokriging, are highlighted as necessary practical considerations. The case study is related to an ultramafic copper-nickel deposit. Six elements, Cu, Ni, Au, Ag, Pt, and Pd, occurring in the deposit, are partitioned into three subgroups and the elements within each group are simultaneously estimated on the basis of over 4000 drill assays. A comparison was made between ordinary kriging and cokriging methods through cross-validation. The results show that cokriging has significantly improved the estimates of resources by reducing the overall estimation error by over 15% and the variance of error by over 20%.  相似文献   

cDNA cloning and expression of a cytochrome P450 1A (CYP1A) gene from the hermaphroditic fish Rivulus marmoratus     

Lee YM  Williams TD  Jung SO  Lee JS 《Marine pollution bulletin》2005,51(8-12):769-775

We previously described the genomic structure of the cytochrome P450 1A (CYP1A) gene from the hermaphroditic fish Rivulus marmoratus [Kim, I.-C., Kim, Y.J., Yoon, Y.-D, Kawamura, S., Lee, Y.-S., Lee, J.-S., 2004a. Cloning of cytochrome P450 1A (CYP1A) genes from the hermaphroditic fish Rivulus marmoratus and the Japanese medaka Oryzias latipes. Mar. Environ. Res. 58, 125–129]. To further characterize R. marmoratus CYP1A, we cloned the cDNA sequence of a CYP1A gene from this species and also expressed its recombinant protein in an E. coli system. We exposed R. marmoratus to 4-nonylphenol, and found a small induction of CYP1A mRNA in the treated animals. In this paper, we discuss the characteristics of R. marmoratus CYP1A gene as well as its potential use in a biomonitoring assay.  相似文献   

Geography and global health     

Brown T  Moon G 《The Geographical journal》2012,178(1):13-17

In the wake of the report of the World Health Organisation's Commission on the Social Determinants of Health, Closing the gap in a generation (Marmot 2008), this invited commentary considers the scope for geographical research on global health. We reflect on current work and note future possibilities, particularly those that take a critical perspective on the interplay of globalisation, security and health.  相似文献