TY - JOUR A1 - Cheng, Shifeng A1 - van den Bergh, Erik A1 - Zeng, Peng A1 - Zhong, Xiao A1 - Xu, Jiajia A1 - Liu, Xin A1 - Hofberger, Johannes A1 - de Bruijn, Suzanne A1 - Bhide, Amey S. A1 - Kuelahoglu, Canan A1 - Bian, Chao A1 - Chen, Jing A1 - Fan, Guangyi A1 - Kaufmann, Kerstin A1 - Hall, Jocelyn C. A1 - Becker, Annette A1 - Bräutigam, Andrea A1 - Weber, Andreas P. M. A1 - Shi, Chengcheng A1 - Zheng, Zhijun A1 - Li, Wujiao A1 - Lv, Mingju A1 - Tao, Yimin A1 - Wang, Junyi A1 - Zou, Hongfeng A1 - Quan, Zhiwu A1 - Hibberd, Julian M. A1 - Zhang, Gengyun A1 - Zhu, Xin-Guang A1 - Xu, Xun A1 - Schranz, M. Eric T1 - The Tarenaya hassleriana Genome Provides insight Into Reproductive Trait and Genome Evolution of Crucifers JF - The plant cell N2 - The Brassicaceae, including Arabidopsis thaliana and Brassica crops, is unmatched among plants in its wealth of genomic and functional molecular data and has long served as a model for understanding gene, genome, and trait evolution. However, genome information from a phylogenetic outgroup that is essential for inferring directionality of evolutionary change has been lacking. We therefore sequenced the genome of the spider flower (Tarenaya hassleriana) from the Brassicaceae sister family, the Cleomaceae. By comparative analysis of the two lineages, we show that genome evolution following ancient polyploidy and gene duplication events affect reproductively important traits. We found an ancient genome triplication in Tarenaya (Th-alpha) that is independent of the Brassicaceae-specific duplication (At-alpha) and nested Brassica (Br-a) triplication. To showcase the potential of sister lineage genome analysis, we investigated the state of floral developmental genes and show Brassica retains twice as many floral MADS (for MINICHROMOSOME MAINTENANCE1, AGAMOUS, DEFICIENS and SERUM RESPONSE FACTOR) genes as Tarenaya that likely contribute to morphological diversity in Brassica. We also performed synteny analysis of gene families that confer self-incompatibility in Brassicaceae and found that the critical SERINE RECEPTOR KINASE receptor gene is derived from a lineage-specific tandem duplication. The T. hassleriana genome will facilitate future research toward elucidating the evolutionary history of Brassicaceae genomes. Y1 - 2013 U6 - https://doi.org/10.1105/tpc.113.113480 SN - 1040-4651 VL - 25 IS - 8 SP - 2813 EP - 2830 PB - American Society of Plant Physiologists CY - Rockville ER - TY - JOUR A1 - Luo, Xiaomin A1 - Xiong, Chao A1 - Gu, Shengfeng A1 - Lou, Yidong A1 - Stolle, Claudia A1 - Wan, Xin A1 - Liu, Kangkang A1 - Song, Weiwei T1 - Geomagnetically conjugate observations of equatorial plasma irregularities from swarm constellation and ground-based GPS stations JF - Journal of geophysical research: Space physics N2 - The near-polar orbit satellites of Swarm mission provide a good opportunity to investigate the conjugacy of equatorial plasma irregularities (EPIs) since their trajectories at low latitudes are basically aligned with fixed geographical longitude. However, the Swarm in situ electron density occasionally shows EPIs at only one hemisphere at this longitude. In this study, we provide detailed analysis of such EPI events from the in situ electron densities and onboard global positioning system (GPS) measurements of Swarm low pair satellites, and simultaneous GPS data from two geomagnetically conjugate ground stations at the Africa longitudes. The result indicates that when Swam in situ electron density sometime shows EPIs at only one hemisphere, the GPS scintillations are still observed from the Swarm onboard receiver and by the two conjugate ground stations. It implies that the EPIs should generally elongate along the geomagnetic flux tube. More than two-year statistic results show that the onset time of scintillation in the northern station is on average 16 and 18 min earlier than that in the southern station for September equinox and December solstice in 2015, while for March equinox in 2016 the onset time of scintillation of northern station is about 11 min later than that of southern station, which indicates the asymmetry features of EPIs along the flux tube. Further analysis of nearly three-year GPS data from two conjugate stations at the Asia longitudes, we find that during solar maximum years the local sunset time plays an important role for causing the difference of onset time of scintillation between two conjugate stations. Y1 - 2019 U6 - https://doi.org/10.1029/2019JA026515 SN - 2169-9380 SN - 2169-9402 VL - 124 IS - 5 SP - 3650 EP - 3665 PB - Wiley CY - Hoboken ER - TY - JOUR A1 - Sheng, Gui-Lian A1 - Basler, Nikolas A1 - Ji, Xue-Ping A1 - Paijmans, Johanna L. A. A1 - Alberti, Federica A1 - Preick, Michaela A1 - Hartmann, Stefanie A1 - Westbury, Michael V. A1 - Yuan, Jun-Xia A1 - Jablonski, Nina G. A1 - Xenikoudakis, Georgios A1 - Hou, Xin-Dong A1 - Xiao, Bo A1 - Liu, Jian-Hui A1 - Hofreiter, Michael A1 - Lai, Xu-Long A1 - Barlow, Axel T1 - Paleogenome reveals genetic contribution of extinct giant panda to extant populations JF - Current biology N2 - Historically, the giant panda was widely distributed from northern China to southwestern Asia [1]. As a result of range contraction and fragmentation, extant individuals are currently restricted to fragmented mountain ranges on the eastern margin of the Qinghai-Tibet plateau, where they are distributed among three major population clusters [2]. However, little is known about the genetic consequences of this dramatic range contraction. For example, were regions where giant pandas previously existed occupied by ancestors of present-day populations, or were these regions occupied by genetically distinct populations that are now extinct? If so, is there any contribution of these extinct populations to the genomes of giant pandas living today? To investigate these questions, we sequenced the nuclear genome of an similar to 5,000-year-old giant panda from Jiangdongshan, Teng-chong County in Yunnan Province, China. We find that this individual represents a genetically distinct population that diverged prior to the diversification of modern giant panda populations. We find evidence of differential admixture with this ancient population among modern individuals originating from different populations as well as within the same population. We also find evidence for directional gene flow, which transferred alleles from the ancient population into the modern giant panda lineages. A variable proportion of the genomes of extant individuals is therefore likely derived from the ancient population represented by our sequenced individual. Although extant giant panda populations retain reasonable genetic diversity, our results suggest that this represents only part of the genetic diversity this species harbored prior to its recent range contractions. Y1 - 2019 U6 - https://doi.org/10.1016/j.cub.2019.04.021 SN - 0960-9822 SN - 1879-0445 VL - 29 IS - 10 SP - 1695 EP - 1700 PB - Cell Press CY - Cambridge ER - TY - JOUR A1 - Chen, You-Peng A1 - Lu, Yong-Ping A1 - Li, Jian A1 - Liu, Zhi-Wei A1 - Chen, Wen-Jing A1 - Liang, Xu-Jing A1 - Chen, Xin A1 - Wen, Wang-Rong A1 - Xiao, Xiao-Min A1 - Reichetzeder, Christoph A1 - Hocher, Berthold T1 - Fetal and maternal angiotensin (1-7) are associated with preterm birth JF - Journal of hypertension N2 - Background: Recent studies show that preterm birth is associated with hypertension in later life. The renin-angiotensin system (RAS) during pregnancy influences fetal growth and development. In the current study, we investigated the impact of fetal as well as maternal angiotensin (1-7) [Ang (1-7)] and angiotensin II (Ang II) plasma concentrations on the risk of preterm birth. Methods: Three hundred and nine pregnant women were prospectively included into the study. The pregnant women were divided into two groups, for example, preterm birth of lower than 37 gestational weeks (n = 17) and full-term birth of 37 gestational weeks or more (n = 292). Maternal and neonatal plasma Ang (1-7) and Ang II concentrations were analyzed at birth from maternal venous blood and umbilical cord blood, respectively. Risk factors for premature birth were determined by multiple logistic regression analysis. Results: Fetal and maternal plasma Ang (1-7) concentrations in the preterm group were lower than those of the term group fetal Ang (1-7) preterm birth: 486.15 +/- 337.34 ng/l and fetal Ang (1-7) term birth: 833.84 +/- 698.12 ng/l and maternal Ang (1-7) preterm birth: 399.86 +/- 218.93 ng/l; maternal Ang (1-7) term birth: 710.34 +/- 598.22 ng/l. Multiple logistic regression analysis considering confounding factors revealed that preeclampsia (P < 0.001), premature rupture of membranes (P = 0.001), lower concentration of maternal Ang (1-7) (P = 0.013) and fetal plasma Ang (1-7) (P = 0.032) were independently associated with preterm birth. We could furthermore demonstrate that the maternal Ang (1-7)/Ang II ratio is independently associated with gestational hypertension or preeclampsia, factors causing preterm birth. Conclusions: Lower concentrations of maternal and fetal Ang (1-7) are independently associated with preterm birth - a risk factor of hypertension in later life. KW - angiotensin (1-7) KW - angiotensin II KW - cardiovascular disease KW - fetal programming KW - intrauterine fetal growth KW - pregnancy KW - preterm delivery Y1 - 2014 U6 - https://doi.org/10.1097/HJH.0000000000000251 SN - 0263-6352 SN - 1473-5598 VL - 32 IS - 9 SP - 1833 EP - 1841 PB - Lippincott Williams & Wilkins CY - Philadelphia ER - TY - JOUR A1 - Xue, Zhike A1 - Yan, Xiaoli A1 - Cheng, Xin A1 - Yang, Liheng A1 - Su, Yingna A1 - Kliem, Bernhard A1 - Zhang, Jun A1 - Liu, Zhong A1 - Bi, Yi A1 - Xiang, Yongyuan A1 - Yang, Kai A1 - Zhao, Li T1 - Observing the release of twist by magnetic reconnection in a solar filament eruption JF - Nature Communications N2 - Magnetic reconnection is a fundamental process of topology change and energy release, taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory. However, observational evidence has been relatively rare and typically only partial. Here we present evidence of fast reconnection in a solar filament eruption using high-resolution H-alpha images from the New Vacuum Solar Telescope, supplemented by extreme ultraviolet observations. The reconnection is seen to occur between a set of ambient chromospheric fibrils and the filament itself. This allows for the relaxation of magnetic tension in the filament by an untwisting motion, demonstrating a flux rope structure. The topology change and untwisting are also found through nonlinear force-free field modelling of the active region in combination with magnetohydrodynamic simulation. These results demonstrate a new role for reconnection in solar eruptions: the release of magnetic twist. Y1 - 2016 U6 - https://doi.org/10.1038/ncomms11837 SN - 2041-1723 VL - 7 PB - Nature Publ. Group CY - London ER -