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| 1 | The enhanced X-ray Timing and Polarimetry mission—eXTP显示文摘In this paper we present the enhanced X-ray Timing and Polarimetry mission—eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources.The paper provides a detailed description of:(1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload;(2) the elements and functions of the mission, from the spacecraft to the ground segment. | ShuangNan Zhang Andrea Santangelo Marco Feroci YuPeng Xu FangJun Lu Yong Chen Hua Feng Shu Zhang Sφren Brandt Margarita Hernanz Luca Baldini Enrico Bozzo Riccardo Campana Alessandra De Rosa YongWei Dong Yuri Evangelista Vladimir Karas Norbert Meidinger Aline Meuris Kirpal Nandra Teng Pan Giovanni Pareschi Piotr Orleanski QiuShi Huang Stephane Schanne Giorgia Sironi Daniele Spiga Jiri Svoboda Gianpiero Tagliaferri Christoph Tenzer Andrea Vacchi Silvia Zane Dave Walton ZhanShan Wang Berend Winter Xin Wu Jean J.M.in't Zand Mahdi Ahangarianabhari Giovanni Ambrosi Filippo Ambrosino Marco Barbera Stefano Basso Jörg Bayer Ronaldo Bellazzini Pierluigi Bellutti Bruna Bertucci Giuseppe Bertuccio Giacomo Borghi XueLei Cao Franck Cadoux Francesco Ceraudo TianXiang Chen Yu Peng Chen Jerome Chevenez Marta Civitani Wei Cui WeiWei Cui Thomas Dauser Ettore Del Monte Sergio Di Cosimo Sebastian Diebold Victor Doroshenko Michal Dovciak YuanYuan Du Lorenzo Ducci QingMei Fan Yannick Favre Fabio Fuschino JoséLuis Ga'lvez Min Gao MingYu Ge Olivier Gevin Marco Grassi QuanYing Gu YuDong Gu DaWei Han Bin Hong Wei Hu Long Ji ShuMei Jia WeiChun Jiang Thomas Kennedy Ingo Kreykenbohm Irfan Kuvvetli Claudio Labanti Luca Latronico Gang Li MaoShun Li Xian Li Wei Li ZhengWei Li Olivier Limousin HongWei Liu XiaoJing Liu Bo Lu Tao Luo Daniele Macera Piero Malcovati Adrian Martindale Malgorzata Michalska Bin Meng Massimo Minuti Alfredo Morbidini Fabio Muleri Stephane Paltani Emanuele Perinati Antonino Picciotto Claudio Piemonte JinLu Qu Alexandre Rachevski Irina Rashevskaya Jerome Rodriguez Thomas Schanz ZhengXiang Shen LiZhi Sheng JiangBo Song LiMing Song Carmelo Sgro Liang Sun Ying Tan Phil Uttley Bo Wang DianLong Wang GuoFeng Wang Juan Wang LangPing Wang YuSa Wang Anna L.Watts XiangYang Wen Jörn Wilms ShaoLin Xiong JiaWei Yang Sheng Yang YanJi Yang Nian Yu WenDa Zhang Gianluigi Zampa Nicola Zampa Andrzej A.Zdziarski AiMei Zhang ChengMo Zhang Fan Zhang Long Zhang Tong Zhang Yi Zhang XiaoLi Zhang ZiLiang Zhang BaoSheng Zhao ShiJie Zheng Yu Peng Zhou Nicola Zorzi J.Frans Zwart | 2019 | Science China(Physics,Mechanics & Astronomy)2019，62，2： | 11 |
| 2 | Photospheric shear flows along the magnetic neutral line of active region 10486 prior to an X10 flare 显示文摘 | Guo Yang Yan Xu Wenda Cao | 2004 | The Astrophysical Journal2004，617，： | 1 |
| 3 | Subunit composition and chromophore content of R-phycocyanin and allophycocyanin from Porphyra haitanensis显示文摘SubunitcompositionandchromophorecontentofR-phycocyaninandallophycocyaninfromPorphyrahaitanensis￥GaoHongfeng;CaoWendaandJiMing... | Gao Hongfeng Cao Wenda and Ji Minghou | 1994 | Acta Oceanologica Sinica1994，13，2： | 0 |
| 4 | Magneto-acoustic oscillations observed in a solar plage region显示文摘We gave an extensive study for the quasi-periodic perturbations on the time profiles of the line of sight(LOS) magnetic field in 10 × 10 sub-areas in a solar plage region(corresponds to a facula on the photosphere).The perturbations are found to be associated with the enhancement of He I 10830 A absorption in a moss region,which is connected to loops with million-degree plasma.FFT analysis to the perturbations gives a kind of spectrum similar to that of Doppler velocity:a number of discrete periods around 5 minutes.The amplitudes of the magnetic perturbations are found to be proportional to magnetic field strength over these sub-areas.In addition,magnetic perturbations lag behind a quarter of the cycle in the phase with respect to the p-mode Doppler velocity.We show that the relationships can be well explained with an MHD solution for the magneto-acoustic oscillations in high-β plasma.Observational analysis also shows that,for the two regions with the stronger and weaker magnetic field,the perturbations are always anti-phased.All findings show that the magnetic perturbations are actually magneto-acoustic oscillations on the solar surface,the photosphere,powered by p-mode oscillations.The findings may provide a new diagnostic tool for exploring the relationship between magneto-acoustic oscillations and the heating of the solar upper atmosphere,as well as their role in helioseismology. | Haisheng Ji Parida Hashim Zhenxiang Hong Zhe Xu Jinhua Shen Kaifan Ji Wenda Cao | 2021 | Research in Astronomy and Astrophysics2021，21，7： | 0 |
| 5 | An Interpretation of a Radiation Damage Phenomenon of the Solar-A CCD显示文摘High energy radiation exists in the space natural radiation environment may cause the degradation of the performance of charge coupled devices used in space. The Solar A satellite was launched in 1991. Since then, radiation damage effected phenomena have been reported. The flatband voltage shift resulted from the trapped holes within the insulator layer between the CCD gates and bulk silicon may throw light on the interpretation of some of the radiation damage phenomena. | Song Qian, Cao Wenda (Yunnan Observatory, The Chinese Academy of Sciences, Kunming 650011, China) (National Astronomical Observatories, The Chinese Academy of Sciences, Beijing 100012, E mail: qiansong@163. net) | 1999 | 天文研究与技术1999，，S1： | 0 |
| 6 | Effect of Magnetized Water on the Mice Given High Doses of Antineoplastic Drugs显示文摘To broaden the applications of magnetized water(MW) in medical science, the possible detoxicative effect of MW to anticancer drugs in vivo were studied. After being given ip with cyclophosphomide (CTX) 500 mg/kg, cisplatin (DDP) 40 mg/kg, harringtonine (HA) 20 mg/kg, mitomycin C (MMC) 8 mg/kg, lycobetaine (Lyc) 200 mg/kg, respectively, the mice were given MW ip 0.2 ml for 7 days. The average life span was calculated for each group. After being given subacutely lower doses of anticancer drugs ( CTX 100 mg/kg, HA 3 mg/kg ) ip 3 times, the mice were given MW ip 0.2 ml for 7 days and the blood white cells were counted as routine. It was shown that the mice in MW groups after ip anticancer drugs survived longer than those without MW. The effects of various anticancer drugs on life span were different. The white cell numbers of groups with MW were higher than that of the groups without MW. So it is possible that MW can remarkably extend the life span of mice and attenuate the leukopenia by mitigating the toxicity of anticancer drugs in vivo . | Lu Dayong Shen Wenda * Cao Jingyi Lu Tingren Cui Baoyi Fu Zhiyu (School of Life Sciences, *College of Sciences, Shanghai University) | 1999 | Advances in Manufacturing1999，，1： | 0 |
| 7 | Model of Spectral Fluxes for Solar Spectrograph显示文摘Taking use of the solar spectrograph in Yunnan Observatory, we built a model to estimate the spectral fluxes of solar spectrograph with computer and confirmed the result by observations. The spectral fluxes in visible and near infrared bands were calculated for the solar spectrograph of Yunnan Observatory. | Cao Wenda, Song Qian (Yunnan Observatory, The Chinese Academy of Sciences, Kunming 650011, China) (National Astronomical Observatories, The Chinese Academy of Sciences, Beijing 100012, China) | 1999 | 天文研究与技术1999，，S1： | 0 |
| 8 | Effect of pressure cooking on phenolic compounds of quinoa显示文摘Due to good nutritional properties and potential health benefits,quinoa has gained an increasing attention.The study aimed to analyze the effect of pressure cooking on the composition,antioxidant activity,antibacterial activity and bioavailability of phenolic compounds in four types of quinoa,and to evaluate the correlation between phenolics and its biological activities by correlation analysis.The results showed that different varieties of quinoa contained different phenolic components and their biological activities were different.Pressure cooking could significantly increase(P<0.05)the phenolic contents of quinoa,and decrease in vitro digestibility of protein.The antioxidant activity,antibacterial activity and bioavailability of quinoa were also enhanced which were positively related with phenolic contents.HPLC analysis indicated that at least twelve phenolic compounds were found in quinoa,and hyperoside,sinapic acid,rutin and ferulic acid occupied a majority of them.Correlation analysis suggested that hyperoside,quercetin,sinapic acid,ferulic acid and gallic acid made the key contribution to antioxidant and antibacterial activities of phenolic compounds of quinoa.The results provided valuable information for quinoa processing with phenolics as functional ingredient. | Qianwei Ma Zhixiang Li Thanutchaporn Kumrungsee Wenda Huang Ruge Cao | 2023 | Grain & Oil Science and Technology2023，6，3： | 0 |
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