云南高校图书馆联盟文献共享服务平台- CMES

CMES: 作品数：122被引量：337H指数：10; 导出分析报告; 相关领域：天文地球理学更多>>; 相关作者：杨其静辛大楞汪毓明肖明月吕品更多>>; 相关机构：西南财经大学中国人民大学安徽工业大学中国科学院国家天文台更多>>; 相关期刊：更多>>; 相关基金：国家自然科学基金国家重点基础研究发展计划国家社会科学基金浙江省哲学社会科学规划课题更多>>

Components and Anisotropy of 3D QFP Waves During the Early Solar Eruption: 《Research in Astronomy and Astrophysics》2024年第12期105-115,共11页Jialiang Hu Jing Ye Yuhao Chen Zhixing Mei Shanshan Xu Jun Lin; supported by Strategic Priority Research Program of the Chinese Academy of Sciences No. XDB0560000;National Key R&D Program of China No. 2022YFF0503804;NSFC grants 11933009, 12273107, U2031141 and 12073073;grants associated with the Yunling Scholar Project of Yunnan Province;the Yunnan Province Scientist Workshop of Solar Physics;the Yunnan Key Laboratory of Solar Physics and Space Exploration of Code 202205AG070009;the Special Project for the construction of science and technology innovation centers faced to South Asiaand Southeast Asia-Yunnan International Joint Innovation Platform: “China-Malaysia HF-VHF Advanced Radio Astronomy Technology International Joint Laboratory of Yunnan” (202303AP140003);the support by grants associated with the Yunnan Revitalization Talent Support Program;the Foundation of the Chinese Academy of Sciences (Light of West China Program)。; The propagation of disturbances in the solar atmosphere is inherently three-dimensional(3D), yet comprehensive studies on the spatial structure and dynamics of 3D wave fronts are scarce. Here we conduct high-resolutio...; 关键词：SUN corona-Sun coronal mass ejections(CMEs)-shock waves

A Special Kind of Interplanetary Coronal Mass Ejection: 《Research in Astronomy and Astrophysics》2024年第12期183-191,共9页H.Q.Feng Y.Zhao G.Q.Zhao H.B.Li L.Xiang J.M.Wang; support from the National Natural Science Foundation of China(NSFC,Grant Nos.41974197,41804162,and 42104158);supported by Central Plains Science and Technology Innovation Leading Talents of Henan Province under grant No.244200510012。; It is generally believed that coronal mass ejections(CMEs)have magnetic flux rope structures because of their helical shapes.However,only about 30%–40%of interplanetary CMEs(ICMEs)have a local magnetic flux rope stru...; 关键词：SUN coronal mass ejections(CMEs)-(Sun) solar wind-interplanetary medium

A New Approach of Data-driven Simulation and its Application to Solar Active Region 12673: 《Research in Astronomy and Astrophysics》2024年第12期43-52,共10页Zhi-Peng Liu Chao-Wei Jiang Xin-Kai Bian Qing-Jun Liu Peng Zou Xue-Shang Feng; supported by the National Natural Science Foundation of China (NSFC 42174200);Shenzhen Science and Technology Program (grant No. RCJC20210609 104422048);Shenzhen Key Laboratory Launching Project (No. ZDSYS20210702140800001);Guangdong Basic and Applied Basic Research Foundation (2023B1515040021);the Fundamental Research Funds for the Central Universities (grant No. HIT.OCEF.2023047)。; The solar coronal magnetic field is a pivotal element in the study of eruptive phenomena, and understanding its dynamic evolution has long been a focal point in solar physics. Numerical models, driven directly by obse...; 关键词：SUN coronal mass ejections(CMEs)-Sun flares-magnetohydrodynamics(MHD)-methods numerical

A Comprehensive Classification and Analysis of Geomagnetic Storms Over Solar Cycle 24: 《Research in Astronomy and Astrophysics》2024年第8期75-84,共10页Raja Adibah Raja Halim Shah Nurul Shazana Abdul Hamid Mardina Abdullah Adlyka Annuar Idahwati Sarudin Zahira Mohd Radzi Akimasa Yoshikawa; funding by Fundamental Research Grant Scheme(FRGS)under Ministry of Higher Education(KPT)Malaysia with the grant No.FRGS/1/2023/STG07/UKM/02/1;supported by Universiti Sains Malaysia through Short-Term Grant with project No.304/PFIZIK/6315730;supported by JSPS KAKENHI grant Nos.JP20H01961,JP22K03707,JP21H04518,JP22K21345。; A geomagnetic storm is a global disturbance of Earth?s magnetosphere,occurring as a result of the interaction with magnetic plasma ejected from the Sun.Despite considerable research,a comprehensive classification of s...; 关键词：(Sun)sunspots-Sun activity-(Sun)solar-terrestrial relations-Sun coronal mass ejections(CMEs)

Are Solar Active Regions Born with Neutralized Currents?: 《Research in Astronomy and Astrophysics》2024年第7期79-88,共10页Aiying Duan Yaoyu Xing Chaowei Jiang; supported by the National Natural Science Foundation of China(NSFC)U2031108;Yunnan Key Laboratory of Solar Physics and Space Science under the number YNSPCC202213。; Solar active regions(ARs)are formed by the emergence of current-carrying magnetic flux tubes from below the photosphere.Although for an isolated flux tube the direct and return currents flowing along the tube should b...; 关键词：SUN magnetic fields-Sun flares-Sun corona-Sun coronal mass ejections(CMEs)

A Revised Graduated Cylindrical Shell Model and its Application to a Prominence Eruption: 《Research in Astronomy and Astrophysics》2023年第12期63-72,共10页Qing-Min Zhang Zhen-Yong Hou Xian-Yong Bai; supported by the National Key R&D Program of China 2022YFF0503003(2022YFF0503000),2021YFA1600500(2021YFA1600502);the National Natural Science Foundation of China(No.12373065);Yunnan Key Laboratory of Solar Physics and Space Science under the No.YNSPCC202206;NSFC under grant No.12373065。; In this paper,the well-known graduated cylindrical shell(GCS)model is slightly revised by introducing longitudinal and latitudinal deflections of prominences originating from active regions(ARs).Subsequently,it is app...; 关键词：SUN flares-Sun filaments-prominences-Sun coronal mass ejections(CMEs)

Global Energetics of Solar Powerful Events on 2017 September 6: 《Research in Astronomy and Astrophysics》2023年第9期180-193,共14页Dong Li Alexander Warmuth Jincheng Wang Haisheng Zhao Lei Lu Qingmin Zhang Nina Dresing Rami Vainio Christian Palmroos Miikka Paassilta Annamaria Fedeli Marie Dominique; funded by the National Key R&D Program of China 2022YFF0503002(2022YFF0503000);the National Natural Science Foundation of China(NSFC,Grant Nos.11973092,12073081,12003064,12103090 and U1938102);the Strategic Priority Research Program on Space Science,CAS,grant Nos.XDA15052200 and XDA15320301;supported by the Specialized Research Fund for State Key Laboratories;LYRA is a project of the Centre Spatial de Liege,the Physikalisch-Meteorologisches Observatorium Davos and the Royal Observatory of Belgium funded by the Belgian Federal Science Policy Office(BELSPO);by the Swiss Bundesamt für Bildung und Wissenschaft;Part of this work was performed in the framework of the SERPENTINE project,which has received funding from the European Union’s Horizon 2020 research and innovation program under grant agreement No.101004159;support by the Turku Collegium for Science,Medicine and Technology of the University of Turku,Finland;support from the Belgian Federal Science Policy Office(BELSPO)in the framework of the ESA-PRODEX program,grant No.4000134474.; Solar flares and coronal mass ejections(CMEs)are thought to be the most powerful events on the Sun.They can release energy as high as~10^(32)erg in tens of minutes,and also can release solar energetic particles(SEPs)i...; 关键词：SUN flares-Sun magnetic fields-Sun coronal mass ejections(CMEs)

Breaking of Large-Scale Filament due to Magnetic Reconnection and Consequent Partial Eruption: 《Research in Astronomy and Astrophysics》2023年第9期194-206,共13页Kaifeng Kang Yang Guo Yan Li Jingxing Wang Jun Lin; supported by the National Key R&D Program of China No.2022YFF0503804;the Strategic Priority Research Programme of the Chinese Academy of Sciences with grant XDA17040507;the National Natural Science Foundation of China (NSFC) grant 11 933 009;grants associated with the Yunling Scholar Project of Yunnan Province,the Yunnan Province Scientist Workshop of Solar Physics.; Following our previous work,we studied the partial eruption of a large-scale horse-shoe-like filament that had beenobserved in a decaying active region on the solar disk for more than 4.5 days.The filament became acti...; 关键词：SUN activity-Sun filaments-prominences-Sun coronal mass ejections(CMEs)-Sun flares-Sun magnetic fields

Investigation on the Formation of Herringbone Structure in TypeⅡSolar Radio Bursts: 《Research in Astronomy and Astrophysics》2023年第5期101-109,共9页Z.Z.Abidin A.N.Zulkiplee V.Epin F.A.M.Pauzi; the Faculty of Science,University of Malaya(grant No.GPF081-2020)for their funding。; We report detailed observation of the“herringbone”of a Type II solar radio burst that occurred on 2010 November 3rd.Data from the Space Weather Prediction Center,National Oceanic and Atmospheric Administration,e-CAL...; 关键词：SUN activity-Sun corona-Sun coronal mass ejections(CMEs)-Sun magnetic fields-Sun radio radiation

Analysis of Ground Level Enhancement Events of 1989 September 29;2001April 15 and 2005 January 20: 《Research in Astronomy and Astrophysics》2022年第10期86-102,共17页R.E.Ugwoke A.A.Ubachukwu J.O.Urama O.Okike J.A.Alhassan A.E.Chukwude; We present the results of analyses of the ground level enhancements(GLEs)of cosmic ray(CR)events on 1989September 29;2001 April 15 and 2005 January 20.This involves examination of hourly raw CR counts of an array of n...; 关键词：SUN coronal mass ejections(CMEs)-Sun flares-Sun particle emission

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