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The ongoing human-induced emission of carbon dioxide (CO2) threatens to change the earth's climate. One possible way of decreasing CO2 emissions is to apply CO2 removal, which involves recovering of carbon dioxide from energy conversion processes and storing it outside the atmosphere. Since the 1980's, the possibilities for recovering CO2 from thermal power plants received increasing attention.In this study possible techniques of recovering CO2 from large-scale industrial processes are assessed.In some industrial processes, e.g. ammonia production, CO2 is recovered from the process streams to prevent it from interfering with the production process. The CO2 thus recovered can easily be dehydrated and compressed, at low cost. In the iron and steel industry, carbon dioxide can be recovered from blast furnace gas. In the petrochemical industry CO2 can be recovered from flue gases, using low-temperature heat for the separation process.Carbon dioxide can be recovered from large-scale industrial processes and in some cases the cost of recovery is significantly less than CO2 recovery from thermal power plants. Therefore this option should be studied further and should be considered if carbon dioxide removal is introduced on a wide scale. 相似文献
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Features of atmospheric circulation and thermal structures are discussed using the NCAR/NCEP
data to reveal the reasons for the late onset and anomalous southward persistence of the South China Sea
Summer Monsoon (SCSSM) in 2005. The results show that three factors are crucial. First, a strong
Arabian High overlaps with a high-latitude blocking high and channels strong cold air to southern Asia.
Second, the Tibetan Plateau has a bigger snow cover than usual in spring and the melting of snow cools
down the surface. Third, the Somali Jet breaks out at a much later date, being not conducive to convection
over Indochina. The former two factors restrict atmospheric sensible heating over the Tibetan Plateau and
nearby regions while the third one limits latent heating over Indochina. All of the factors slow down
atmospheric warming and postpone the onset of SCSSM. Long after the onset of SCSSM, strong cold air
over India advances the Southwest Monsoon northward slowly, resulting in weaker convection and latent
heating over the Tibetan Plateau and nearby areas. The negative feedback conversely inhibits further
northward movement of Southwest Monsoon. 相似文献
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Philip Lah Jayaram N. Chengalur Frank H. Briggs Matthew Colless Roberto De Propris Michael B. Pracy W. J. G. de Blok Shinobu S. Fujita Masaru Ajiki Yasuhiro Shioya Tohru Nagao Takashi Murayama Yoshiaki Taniguchi Masafumi Yagi Sadanori Okamura 《Monthly notices of the Royal Astronomical Society》2007,376(3):1357-1366
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This paper discusses methodological issues relevant to the calculation of historical responsibility of countries for climate
change (‘The Brazilian Proposal’). Using a simple representation of the climate system, the paper compares contributions to
climate change using different indicators: current radiative forcing, current GWP-weighted emissions, radiative forcing from
increased concentrations, cumulative GWP-weighted emissions, global-average surface-air temperature increase and two new indicators:
weighted concentrations (analogue to GWP-weighted emissions) and integrated temperature increase. Only the last two indicators
are at the same time ‘backward looking’ (take into account historical emissions), ‘backward discounting’ (early emissions
weigh less, depending on the decay in the atmosphere) and ‘forward looking’ (future effects of the emissions are considered)
and are comparable for all gases. Cumulative GWP-weighted emissions are simple to calculate but are not ‘backward discounting’.
‘Radiative forcing’ and ‘temperature increase’ are not ‘forward looking’. ‘Temperature increase’ discounts the emissions of
the last decade due to the slow response of the climate system. It therefore gives low weight to regions that have recently
significantly increased emissions. Results of the five different indicators are quite similar for large groups (but possibly
not for individual countries): industrialized countries contributed around 60% to today’s climate change, developing countries
around 40% (using the available data for fossil, industrial and forestry CO2, CH4 and N2O). The paper further argues including non-linearities of the climate system or using a simplified linear system is a political
choice. The paper also notes that results of contributions to climate change need to be interpreted with care: Countries that
developed early benefited economically, but have high historical emission, and countries developing at a later period can
profit from developments in other countries and are therefore likely to have a lower contribution to climate change. 相似文献
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Eric F. Bell † W. J. G. de Blok ‡ 《Monthly notices of the Royal Astronomical Society》2000,311(4):668-672
We have assessed the significance of Tully and Verheijen's bimodal Ursa Major Cluster spiral galaxy near-infrared surface brightness distribution, focusing on whether this bimodality is simply an artefact of small number statistics. A Kolmogorov–Smirnov style of significance test shows that the total distribution is fairly represented by a single-peaked distribution, but that their isolated galaxy subsample (with no significant neighbours within a projected distance of ∼80 kpc) is bimodal at the 96 per cent level. We have also investigated the assumptions underlying the isolated galaxy surface brightness distribution, finding that the (often large) inclination corrections used in the construction of this distribution reduce the significance of the bimodality. We conclude that the Ursa Major Cluster data set is insufficient to establish the presence of a bimodal near-infrared surface brightness distribution: an independent sample of ∼100 isolated, low-inclination galaxies is required to establish bimodality at the 99 per cent level. 相似文献
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Meryl Waugh M. J. Drinkwater R. L. Webster L. Staveley-Smith V. A. Kilborn D. G. Barnes R. Bhathal W. J. G. de Blok P. J. Boyce M. J. Disney R. D. Ekers K. C. Freeman B. K. Gibson P. A. Henning H. Jerjen P. M. Knezek B. Koribalski M. Marquarding R. F. Minchin R. M. Price M. E. Putman † S. D. Ryder E. M. Sadler F. Stootman M. A. Zwaan 《Monthly notices of the Royal Astronomical Society》2002,337(2):641-656
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R. Auld R. F. Minchin J. I. Davies B. Catinella W. van Driel P. A. Henning S. Linder E. Momjian E. Muller K. O'Neil S. Sabatini S. Schneider G. Bothun L. Cortese M. Disney G. L. Hoffman M. Putman J. L. Rosenberg M. Baes W. J. G. de Blok A. Boselli E. Brinks N. Brosch J. Irwin I. D. Karachentsev V. A. Kilborn B. Koribalski K. Spekkens † 《Monthly notices of the Royal Astronomical Society》2006,371(4):1617-1640