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Atmospheric heating rate due to black carbon aerosols: Uncertainties and impact factors 期刊论文
ATMOSPHERIC RESEARCH, 2020, 240
作者:  Lu, Qiao;  Liu, Chao;  Zhao, Delong;  Zeng, Chen;  Li, Jing;  Lu, Chunsong;  Wang, Jiandong;  Zhu, Bin
收藏  |  浏览/下载:36/0  |  提交时间:2020/08/18
Black carbon  Radiative forcing  Heating rate  Vertical distribution  
In Situ Observations of Ionospheric Heating Effects: First Results from a Joint SURA and NorSat-1 Experiment 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (13)
作者:  Chernyshov, A. A.;  Chugunin, D., V;  Frolov, V. L.;  Clausen, L. B. N.;  Miloch, W. J.;  Mogilevsky, M. M.
收藏  |  浏览/下载:9/0  |  提交时间:2020/06/16
active experiments  ionospheric heating  ionosphere  ionospheric irregularities  plasma instabilities  
Constraining Global Changes in Temperature and Precipitation From Observable Changes in Surface Radiative Heating 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (9)
作者:  Dhara, Chirag
收藏  |  浏览/下载:10/0  |  提交时间:2020/07/02
surface energy balance  surface radiative heating  surface temperature response  precipitation change  climate change projections  GCM biases  
Atmospheric Circulation Response to Short-Term Arctic Warming in an Idealized Model 期刊论文
JOURNAL OF THE ATMOSPHERIC SCIENCES, 2020, 77 (2) : 531-549
作者:  Hell, Momme C.;  Schneider, Tapio;  Li, Camille
收藏  |  浏览/下载:6/0  |  提交时间:2020/07/02
Arctic  Dynamics  Heating  Stratospheric circulation  Stratosphere-troposphere coupling  Intraseasonal variability  
Gram-scale bottom-up flash graphene synthesis 期刊论文
NATURE, 2020, 577 (7792) : 647-651
作者:  Long, Haizhen;  Zhang, Liwei;  Lv, Mengjie;  Wen, Zengqi;  Zhang, Wenhao;  Chen, Xiulan;  Zhang, Peitao;  Li, Tongqing;  Chang, Luyuan;  Jin, Caiwei;  Wu, Guozhao;  Wang, Xi;  Yang, Fuquan;  Pei, Jianfeng;  Chen, Ping;  Margueron, Raphael;  Deng, Haiteng;  Zhu, Mingzhao;  Li, Guohong
收藏  |  浏览/下载:14/0  |  提交时间:2020/07/03

Most bulk-scale graphene is produced by a top-down approach, exfoliating graphite, which often requires large amounts of solvent with high-energy mixing, shearing, sonication or electrochemical treatment(1-3). Although chemical oxidation of graphite to graphene oxide promotes exfoliation, it requires harsh oxidants and leaves the graphene with a defective perforated structure after the subsequent reduction step(3,4). Bottom-up synthesis of high-quality graphene is often restricted to ultrasmall amounts if performed by chemical vapour deposition or advanced synthetic organic methods, or it provides a defect-ridden structure if carried out in bulk solution(4-6). Here we show that flash Joule heating of inexpensive carbon sources-such as coal, petroleum coke, biochar, carbon black, discarded food, rubber tyres and mixed plastic waste-can afford gram-scale quantities of graphene in less than one second. The product, named flash graphene (FG) after the process used to produce it, shows turbostratic arrangement (that is, little order) between the stacked graphene layers. FG synthesis uses no furnace and no solvents or reactive gases. Yields depend on the carbon content of the source  when using a high-carbon source, such as carbon black, anthracitic coal or calcined coke, yields can range from 80 to 90 per cent with carbon purity greater than 99 per cent. No purification steps are necessary. Raman spectroscopy analysis shows a low-intensity or absent D band for FG, indicating that FG has among the lowest defect concentrations reported so far for graphene, and confirms the turbostratic stacking of FG, which is clearly distinguished from turbostratic graphite. The disordered orientation of FG layers facilitates its rapid exfoliation upon mixing during composite formation. The electric energy cost for FG synthesis is only about 7.2 kilojoules per gram, which could render FG suitable for use in bulk composites of plastic, metals, plywood, concrete and other building materials.


Flash Joule heating of inexpensive carbon sources is used to produce gram-scale quantities of high-quality graphene in under a second, without the need for a furnace, solvents or reactive gases.


  
An orbital water-ice cycle on comet 67P from colour changes 期刊论文
NATURE, 2020, 578 (7793) : 49-+
作者:  Oh, Myoung Hwan;  Cho, Min Gee;  Chung, Dong Young;  Park, Inchul;  Kwon, Youngwook Paul;  Ophus, Colin;  Kim, Dokyoon;  Kim, Min Gyu;  Jeong, Beomgyun;  Gu, X. Wendy;  Jo, Jinwoung;  Yoo, Ji Mun;  Hong, Jaeyoung;  McMains, Sara;  Kang, Kisuk;  Sung, Yung-Eun;  Alivisatos, A. Paul;  Hyeon, Taeghwan
收藏  |  浏览/下载:52/0  |  提交时间:2020/07/03

Solar heating of a cometary surface provides the energy necessary to sustain gaseous activity, through which dust is removed(1,2). In this dynamical environment, both the coma(3,4) and the nucleus(5,6) evolve during the orbit, changing their physical and compositional properties. The environment around an active nucleus is populated by dust grains with complex and variegated shapes(7), lifted and diffused by gases freed from the sublimation of surface ices(8,9). The visible colour of dust particles is highly variable: carbonaceous organic material-rich grains(10) appear red while magnesium silicate-rich(11,12) and water-ice-rich(13,14) grains appear blue, with some dependence on grain size distribution, viewing geometry, activity level and comet family type. We know that local colour changes are associated with grain size variations, such as in the bluer jets made of submicrometre grains on comet Hale-Bopp(15) or in the fragmented grains in the coma(16) of C/1999 S4 (LINEAR). Apart from grain size, composition also influences the coma'  s colour response, because transparent volatiles can introduce a substantial blueing in scattered light, as observed in the dust particles ejected after the collision of the Deep Impact probe with comet 9P/Tempel 1(17). Here we report observations of two opposite seasonal colour cycles in the coma and on the surface of comet 67P/Churyumov-Gerasimenko through its perihelion passage(18). Spectral analysis indicates an enrichment of submicrometre grains made of organic material and amorphous carbon in the coma, causing reddening during the passage. At the same time, the progressive removal of dust from the nucleus causes the exposure of more pristine and bluish icy layers on the surface. Far from the Sun, we find that the abundance of water ice on the nucleus is reduced owing to redeposition of dust and dehydration of the surface layer while the coma becomes less red.