Space physics and astronomy research from Chinese polar stations: current and future directions  

作　　者：ZONG Qiugang HU Zejun LIU Jianjun JIANG Peng DU Yang ZHANG Wei 

机构地区：[1]Key Laboratory of Polar Science,MNR,Polar Research Institute of China,Shanghai 200136,China [2]Institute of Space Physics and Applied Technology,Peking University,Beijing 100871,China [3]Shanghai Institute of Satellite Engineering,Shanghai 201109,China

出　　处：《Advances in Polar Science》2023年第4期239-250,共12页极地科学进展（英文版）

基　　金：supported by the National Natural Science Foundation of China(Grant nos.42242406,42230202);Innovation Fund from Joint Innovation Center of Space Science(Aerospace Shanghai).

摘　　要：Space weather has a remarkable effect on modern human activities,e.g.,communication,navigation,space exploration etc.Space physics study from polar stations is as an important part of the entire solar-terrestrial space,and conducts quantitative research from the perspective of overall space plasma behavior.One of the most important issues is to identify the dominant processes that transfer plasma and momentum from the solar wind to Earth’s magnetosphere.Thus,it is necessary to carry out research for combination the observations from polar ground stations and spacecraft observations in the space.Observations at polar regions can be as a window to the space for satellite traffic controls.The operation of the observation chain―Zhongshan-Taishan-Kunlun Station could monitor polar space debris in a large area with high temporal and spatial resolution.Also,night-time measurements of astronomical seeing at Dome A in Antarctica make it less challenging to locate a telescope above it,thereby giving greater access to the free atmosphere because of a thinner boundary layer.

关 键 词：Great Wall Station Zhongshan Station Yellow River Station Kjell Henriksen Observatory China-Iceland Arctic Science Observatory Dome A 

分 类 号：P35[天文地球—空间物理学]