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  • 1
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    Observed climate change hot-spots (2015)
    Wiley
    Details
    Publication Date: 2015-04-10
    Description: We quantify climate change hot-spots from observations, taking into account the differences in precipitation and temperature statistics (mean, variability and extremes) between 1981-2010 and 1951-1980. Areas in the Amazon, the Sahel, tropical West Africa, Indonesia and central eastern Asia emerge as primary observed hot-spots. The main contributing factors are the global increase in mean temperatures, the intensification of extreme hot-season occurrence in low-latitude regions and the decrease of precipitation over central Africa. Temperature and precipitation variability have been substantially stable over the past decades, with only a few areas showing significant changes against the background climate variability. The regions identified from the observations are remarkably similar to those defined from projections of global climate models under a “business-as-usual” scenario, indicating that climate change hot-spots are robust and persistent over time. These results provide a useful background to develop global policy decisions on adaptation and mitigation priorities over near-time horizons.
    Print ISSN: 0094-8276
    Electronic ISSN: 1944-8007
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 2
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    Precipitation in the Hindu-Kush Karakoram Himalaya: Observations and future scenarios (2013)
    Wiley
    Details
    Publication Date: 2013-01-17
    Description: [1]  We study the properties of precipitation in the Hindu-Kush Karakoram Himalaya (HKKH) region using currently available data sets. We consider satellite rainfall estimates (Tropical Rainfall Measuring Mission), reanalyses (ERA-Interim), gridded in situ rain gauge data (Asian Precipitation Highly Resolved Observational Data Integration Towards Evaluation of Water Resources, Climate Research Unit, and Global Precipitation Climatology Centre), and a merged satellite and rain gauge climatology (Global Precipitation Climatology Project). The data are compared with simulation results from the global climate model EC-Earth. All data sets, despite having different resolutions, coherently reproduce the mean annual cycle of precipitation in the western and eastern stretches of the HKKH. While for the Himalaya only a strong summer precipitation signal is present, associated with the monsoon, the data indicate that the Hindu-Kush Karakoram, which is exposed to midlatitude “western weather patterns”, receives water inputs in winter. Time series of seasonal precipitation confirm that the various data sets provide a consistent measurement of interannual variability for the HKKH. The longest observational data sets indicate a statistically significant decreasing trend in Himalaya during summer. None of the data sets gives statistically significant precipitation trends in Hindu-Kush Karakoram during winter. Precipitation data from EC-Earth are in good agreement with the climatology of the observations (rainfall distribution and seasonality). The evolution of precipitation under two different future scenarios (RCP 4.5 and RCP 8.5) reveals an increasing trend over the Himalaya during summer, associated with an increase in wet extremes and daily intensity and a decrease in the number of rainy days. Unlike the observations, the model shows an increasing precipitation trend also in the period 1950–2009, possibly as a result of the poor representation of aerosols in this type of GCMs.
    Print ISSN: 0148-0227
    Topics: Geosciences , Physics
    Published by Wiley on behalf of American Geophysical Union (AGU).
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  • 3
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    GRB 090423 at a redshift of z approximately 8.1 (2009)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2009-10-30
    Description: Gamma-ray bursts (GRBs) are produced by rare types of massive stellar explosion. Their rapidly fading afterglows are often bright enough at optical wavelengths that they are detectable at cosmological distances. Hitherto, the highest known redshift for a GRB was z = 6.7 (ref. 1), for GRB 080913, and for a galaxy was z = 6.96 (ref. 2). Here we report observations of GRB 090423 and the near-infrared spectroscopic measurement of its redshift, z = 8.1(-0.3)(+0.1). This burst happened when the Universe was only about 4 per cent of its current age. Its properties are similar to those of GRBs observed at low/intermediate redshifts, suggesting that the mechanisms and progenitors that gave rise to this burst about 600,000,000 years after the Big Bang are not markedly different from those producing GRBs about 10,000,000,000 years later.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Salvaterra, R -- Valle, M Della -- Campana, S -- Chincarini, G -- Covino, S -- D'Avanzo, P -- Fernandez-Soto, A -- Guidorzi, C -- Mannucci, F -- Margutti, R -- Thone, C C -- Antonelli, L A -- Barthelmy, S D -- De Pasquale, M -- D'Elia, V -- Fiore, F -- Fugazza, D -- Hunt, L K -- Maiorano, E -- Marinoni, S -- Marshall, F E -- Molinari, E -- Nousek, J -- Pian, E -- Racusin, J L -- Stella, L -- Amati, L -- Andreuzzi, G -- Cusumano, G -- Fenimore, E E -- Ferrero, P -- Giommi, P -- Guetta, D -- Holland, S T -- Hurley, K -- Israel, G L -- Mao, J -- Markwardt, C B -- Masetti, N -- Pagani, C -- Palazzi, E -- Palmer, D M -- Piranomonte, S -- Tagliaferri, G -- Testa, V -- England -- Nature. 2009 Oct 29;461(7268):1258-60. doi: 10.1038/nature08445.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉INAF, Osservatorio Astronomico di Brera, Via E. Bianchi 46, 23807 Merate (LC), Italy. salvaterra@mib.infn.it〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19865166" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
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  • 4
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    The unusual gamma-ray burst GRB 101225A explained as a minor body falling onto a neutron star (2011)
    Nature Publishing Group (NPG)
    Details
    Publication Date: 2011-12-02
    Description: The tidal disruption of a solar-mass star around a supermassive black hole has been extensively studied analytically and numerically. In these events, the star develops into an elongated banana-shaped structure. After completing an eccentric orbit, the bound debris falls into the black hole, forming an accretion disk and emitting radiation. The same process may occur on planetary scales if a minor body passes too close to its star. In the Solar System, comets fall directly into our Sun or onto planets. If the star is a compact object, the minor body can become tidally disrupted. Indeed, one of the first mechanisms invoked to produce strong gamma-ray emission involved accretion of comets onto neutron stars in our Galaxy. Here we report that the peculiarities of the 'Christmas' gamma-ray burst (GRB 101225A) can be explained by a tidal disruption event of a minor body around an isolated Galactic neutron star. This would indicate either that minor bodies can be captured by compact stellar remnants more frequently than occurs in the Solar System or that minor-body formation is relatively easy around millisecond radio pulsars. A peculiar supernova associated with a gamma-ray burst provides an alternative explanation.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Campana, S -- Lodato, G -- D'Avanzo, P -- Panagia, N -- Rossi, E M -- Della Valle, M -- Tagliaferri, G -- Antonelli, L A -- Covino, S -- Ghirlanda, G -- Ghisellini, G -- Melandri, A -- Pian, E -- Salvaterra, R -- Cusumano, G -- D'Elia, V -- Fugazza, D -- Palazzi, E -- Sbarufatti, B -- Vergani, S D -- England -- Nature. 2011 Nov 30;480(7375):69-71. doi: 10.1038/nature10592.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉INAF - Osservatorio Astronomico di Brera, Via E. Bianchi 46, I-23807 Merate, Italy. sergio.campana@brera.inaf.it〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22129725" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
    Published by Nature Publishing Group (NPG)
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