327 research outputs found

    Key drivers of India’s African engagement

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    Daniel Large explains why Indian government and businesses are increasingly prioritising engagement with different parts of Africa. This post is an excerpt from “India’s African Engagement”, a chapter in the recent LSE IDEAS report on Emerging Powers in Africa. Click here for all India At LSE coverage of India-Africa ties

    The limits of Modi-fying India’s Africa engagement

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    Last month’s India-Africa Forum and Summit saw African leaders welcomed with unprecedented levels of ceremony and political theatre. But Daniel Large writes that underneath new branding were old questions about how what was witnessed in Delhi in October will be followed through on in substantive ways, and the extent to which these will catalyse relations beyond political level

    China’s Sudan engagement: changing Northern and Southern political trajectories in peace and war

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    China has developed a more consequential role in Sudan over the past two decades, during which it has become bound up in the combination of enduring violent internal instability and protracted external adversity that has characterized the politics of the central state since the 1989 Islamist revolution. Two inter-related political trajectories of China’s Sudan engagement are examined here. The first concerns Beijing’s relations with the ruling National Congress party in incorporating China into its domestic politics and foreign relations amidst war in Darfur, to which Beijing has responded through a more engaged political role. The second confronts the practical limitations of China’s sovereignty doctrine and exclusive reliance upon relations with the central state. Following the peace agreement of 2005 that ended the North–South war, and motivated by political imperatives linked to investment protection concerns, China has developed new relations with the semi-autonomous Government of Southern Sudan, thus seeking to position itself to navigate Sudan’s uncertain political future

    Suppression-Induced Forgetting on a Free-Association Test

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    The repeated suppression of thoughts in response to cues for their expression leads to forgetting on a subsequent test of cued recall (Anderson & Green, 2001). We extended this effect by using homograph cues and presenting them for free association following suppression practice. Cue-target pairs were first learned under integrating imagery instructions; then in the think/no-think phase students practiced suppressing thoughts connected to some homograph cues, with or without the assistance of thought substitutes that changed their meaning. Below-baseline forgetting on the subsequent free-association test was found in the production of suppressed targets. Following aided suppression, this effect was also obtained in the production of other responses denoting the target-related meaning of the homograph cues. Discussion emphasizes the ecological value of the test; rarely do people deliberately attempt recall of unwanted thoughts

    Does pyrite act as an important host for molybdenum in modern and ancient euxinic sediments?

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    Molybdenum (Mo) is a popular paleoproxy for tracking the spatiotemporal pattern of euxinic (anoxic and sulfidic) conditions in the ancient ocean, yet surprisingly little is known about the processes leading to its fixation under sulfidic conditions. Pyrite has been proposed to be the main host phase for Mo sequestration. To clarify the role played by pyrite, and thus to refine the utility of this paleoproxy, modern and ancient samples from six different study sites were analyzed, all representing euxinic conditions, using laser ablation-inductively coupled plasma-mass spectrometry (LA-ICP-MS). Although pyrite often shows substantial enrichments relative to average crust and even matrix samples of similar size, our results show that most of the Mo in euxinic muds and shales is found in the non-pyrite matrix (80–100%) and not in the pyrite grains (0–20%)—simply because the volume of matrix dominates the bulk sediments/rocks. A relationship between the percent of Mo hosted by pyrite and the sulfur isotope composition of that pyrite is observed and can be linked to post-depositional alteration. Specifically, the oldest, typically most altered samples, show the highest δ^(34)S values because of limited sulfate availability at the time of their formation in the early ocean. In these old samples, the relatively small amount of Mo sequestered initially within pyrite is more likely to have been released to the matrix during the strong recrystallization overprints that these rocks have disproportionately suffered. Despite the universal importance of appreciable H_2S availability during Mo uptake, we conclude that pyrite should be viewed as a nontrivial sink for Mo but clearly not the primary host in most euxinic shales and rather suggest that other burial pathways should be emphasized in future studies of the mechanisms of Mo sequestration in such settings

    The New Generation Atlas of Quasar Spectral Energy Distributions from Radio to X-rays

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    We have produced the next generation of quasar spectral energy distributions (SEDs), essentially updating the work of Elvis et al. (1994) by using high-quality data obtained with several space and ground-based telescopes, including NASA's Great Observatories. We present an atlas of SEDs of 85 optically bright, non-blazar quasars over the electromagnetic spectrum from radio to X-rays. The heterogeneous sample includes 27 radio-quiet and 58 radio-loud quasars. Most objects have quasi-simultaneous ultraviolet-optical spectroscopic data, supplemented with some far-ultraviolet spectra, and more than half also have Spitzer mid-infrared IRS spectra. The X-ray spectral parameters are collected from the literature where available. The radio, far-infrared, and near-infrared photometric data are also obtained from either the literature or new observations. We construct composite spectral energy distributions for radio-loud and radio-quiet objects and compare these to those of Elvis et al., finding that ours have similar overall shapes, but our improved spectral resolution reveals more detailed features, especially in the mid and near-infrared.Comment: 46 pages, 10 figures, 10 tables, Accepted by ApJS. Composite SED data files for radio-loud and radio-quiet quasars (rlmsedMR.txt, rqmsedMR.txt) are included in the source (Other formats -> Source). Supplemental figures are not include
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