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地球所遭受的高碰撞率导致晚太古代大气氧化延迟及变化 快报文章
地球科学快报,2021年第21期
作者:  王晓晨
Microsoft Word(13Kb)  |  收藏  |  浏览/下载:754/0  |  提交时间:2021/11/10
high collision  atmospheric oxidation  
Crustal Scale Imaging of the Arabia-Central Iran Collision Boundary Across the Zagros Suture Zone, West of Iran 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (8)
作者:  Dashti, F.;  Lucente, F. P.;  Motaghi, K.;  Bianchi, I.;  Najafi, M.;  Govoni, A.;  Shabanian, E.
收藏  |  浏览/下载:1/0  |  提交时间:2020/07/02
Zagros suture zone  receiver function  collision boundary  exhumation  
Fate of Forearc Lithosphere at Arc-Continent Collision Zones: Evidence From Local Earthquake Tomography of the Sunda-Banda Arc Transition, Indonesia 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (6)
作者:  Supendi, P.;  Nugraha, A. D.;  Widiyantoro, S.;  Abdullah, C., I;  Rawlinson, N.;  Cummins, P. R.;  Harris, C. W.;  Roosmawati, N.;  Miller, M. S.
收藏  |  浏览/下载:7/0  |  提交时间:2020/07/02
tomography  subduction  collision  earthquakes  Indonesia  
Lateral Variations of Shear-Wave Velocity in the D '' Layer Beneath the Indian-Eurasian Plate Collision Zone 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2020, 47 (6)
作者:  Li, Guohui;  Bai, Ling;  Ritsema, Jeroen
收藏  |  浏览/下载:6/0  |  提交时间:2020/07/02
D  Indian-Eurasian plate collision zone  3-D synthetic waveform  ScS and S phases  compositional heterogeneity  long-term subduction  
Collisional cooling of ultracold molecules 期刊论文
NATURE, 2020, 580 (7802) : 197-+
作者:  Wang, Qinyang;  Wang, Yupeng;  Ding, Jingjin;  Wang, Chunhong;  Zhou, Xuehan;  Gao, Wenqing;  Huang, Huanwei;  Shao, Feng;  Liu, Zhibo
收藏  |  浏览/下载:11/0  |  提交时间:2020/07/03

Since the original work on Bose-Einstein condensation(1,2), the use of quantum degenerate gases of atoms has enabled the quantum emulation of important systems in condensed matter and nuclear physics, as well as the study of many-body states that have no analogue in other fields of physics(3). Ultracold molecules in the micro- and nanokelvin regimes are expected to bring powerful capabilities to quantum emulation(4) and quantum computing(5), owing to their rich internal degrees of freedom compared to atoms, and to facilitate precision measurement and the study of quantum chemistry(6). Quantum gases of ultracold atoms can be created using collision-based cooling schemes such as evaporative cooling, but thermalization and collisional cooling have not yet been realized for ultracold molecules. Other techniques, such as the use of supersonic jets and cryogenic buffer gases, have reached temperatures limited to above 10 millikelvin(7,8). Here we show cooling of NaLi molecules to micro- and nanokelvin temperatures through collisions with ultracold Na atoms, with both molecules and atoms prepared in their stretched hyperfine spin states. We find a lower bound on the ratio of elastic to inelastic molecule-atom collisions that is greater than 50-large enough to support sustained collisional cooling. By employing two stages of evaporation, we increase the phase-space density of the molecules by a factor of 20, achieving temperatures as low as 220 nanokelvin. The favourable collisional properties of the Na-NaLi system could enable the creation of deeply quantum degenerate dipolar molecules and raises the possibility of using stretched spin states in the cooling of other molecules.


NaLi molecules are cooled to micro- and nanokelvin temperatures through collisions with ultracold Na atoms by using molecules and atoms in stretched hyperfine spin states and applying two evaporation stages.


  
The wide-binary origin of (2014) MU69-like Kuiper belt contact binaries 期刊论文
NATURE, 2020, 580 (7804) : 463-+
作者:  Jiao, Lin;  Howard, Sean;  Ran, Sheng;  Wang, Zhenyu;  Rodriguez, Jorge Olivares;  Sigrist, Manfred;  Wang, Ziqiang;  Butch, Nicholas P.;  Madhavan, Vidya
收藏  |  浏览/下载:66/0  |  提交时间:2020/07/03

Following its flyby and first imaging of the Pluto-Charon binary, the New Horizons spacecraft visited the Kuiper belt object (KBO) 2014 MU69 (also known as (486958) Arrokoth). The imaging showed MU69 to be a contact binary that rotates at a low spin period (15.92 hours), is made of two individual lobes connected by a narrow neck and has a high obliquity (about 98 degrees)(1), properties that are similar to those of other KBO contact binaries inferred through photometric observations(2). However, all scenarios suggested so far for the origins of such configurations(3-5) have failed to reproduce these properties and their probable frequent occurrence in the Kuiper belt. Here we show that semi-secular perturbations(6,7) operating on only ultrawide KBO binaries close to their stability limit can robustly lead to gentle, slow binary mergers at arbitrarily high obliquities but low rotational velocities, reproducing the characteristics of MU69 and other similar oblique contact binaries. Using N-body simulations, we find that approximately 15 per cent of all ultrawide binaries with a cosine-uniform inclination distribution(5,9) are likely to merge through this process. Moreover, we find that such mergers are sufficiently gentle to deform the shape of the KBO only slightly. The semi-secular contact binary formation channel not only explains the observed properties of MU69, but may also apply to other Kuiper belt or asteroid belt binaries and in the Solar System and extra-solar moon systems.


The high obliquity and low rotation period of the Kuiper belt object (2014) MU69 and other similar contact binaries is successfully reproduced from the collision and post-collision characteristics of initially wide binaries.


  
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.


  
An Experimental Study on Splash Functions of Natural Sand-Bed Collision 期刊论文
JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 2019, 124 (13) : 7226-7235
作者:  Chen, Youxing;  Zhang, Jie;  Huang, Ning;  Xu, Bin
收藏  |  浏览/下载:1/0  |  提交时间:2019/11/27
sand-bed collision  high-speed photograph  splash function  
Little Geodetic Evidence for Localized Indian Subduction in the Pamir-Hindu Kush of Central Asia 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2019, 46 (1) : 109-118
作者:  Perry, M.;  Kakar, N.;  Ischuk, A.;  Metzger, S.;  Bendick, R.;  Molnar, P.;  Mohadjer, S.
收藏  |  浏览/下载:7/0  |  提交时间:2019/04/09
continental collision  tectonics  Hindu Kush  geodesy  
Indirect Influence of Humidity on Atmospheric Spectra Near 4 mu m 期刊论文
GEOPHYSICAL RESEARCH LETTERS, 2018, 45 (22) : 12593-12601
作者:  Hartmann, J. -M.;  Armante, R.;  Toon, G. C.;  Scott, N.;  Tran, H.;  Crevoisier, C.;  Chedin, A.;  Capelle, V.
收藏  |  浏览/下载:6/0  |  提交时间:2019/04/09
atmospheric spectra  4 mu m region  influence of humidity  N-2 collision-induced absorption  CO2 line wings  surface temperature retrievals