| Research Progress of Interplanetary Physics in Mainland China |
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| 作者姓名： | ZHAO Xinhua SHEN Chenglong HE Jiansen NING Hao |
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| 作者单位： | 1. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190; |
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| 基金项目： | Supported by the B-type Strategic Priority Research Program of Chinese Academy of Sciences (XDB41000000), the National Natural Science Foundation of China (41531073, 41731067, 41861164026, 41874202, 41474153), the Youth Innovation Promotion Association of Chinese Academy of Sciences (2016133) and Chinese Academy of Sciences Research Fund for Key Development Directions |
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| 摘 要： | Significant progress has been made by Chinese scientists in research of interplanetary physics during the recent two years (2018-2020). These achievements are reflected at least in the following aspects:Activities in solar corona and lower solar atmosphere; solar wind and turbulence; filament/prominence, jets, flares, and radio bursts; active regions and solar eruptions; coronal mass ejections and their interplanetary counterparts; other interplanetary structures; space weather prediction methods; magnetic reconnection; Magnetohydrodynamic (MHD) numerical modeling; solar energetic particles, cosmic rays, and Forbush decreases; machine learning methods in space weather and other aspects. More than one hundred and forty papers in the academic journals have been published in these research directions. These fruitful achievements are obtained by Chinese scholars in solar physics and space physics either independently or through international collaborations. They greatly improve people's understanding of solar activities, solar eruptions, the corresponding space weather effects, and the Sun-Earth relations. Here we will give a very brief review on the research progress. However, it must be pointed out that this paper may not completely cover all achievements in this field due to our limited knowledge.
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| 关 键 词： | Solar wind Solar eruptions Energetic particles Interplanetary transients Space weather |
| 收稿时间： | 2020-03-27 |
Research Progress of Interplanetary Physics in Mainland China |
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| ZHAO Xinhua,SHEN Chenglong,HE Jiansen,NING Hao.Research Progress of Interplanetary Physics in Mainland China[J].Chinese Journal of Space Science,2020,40(5):732-777. |
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| Institution: | 1. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing 100190;2. CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei 230026;3. School of Earth and Space Sciences, Peking University, Beijing 100871;4. Institute of Space Sciences, Institute of Frontier and Interdisciplinary Science, Shandong University, Weihai 264209 |
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| Abstract: | Significant progress has been made by Chinese scientists in research of interplanetary physics during the recent two years (2018-2020). These achievements are reflected at least in the following aspects:Activities in solar corona and lower solar atmosphere; solar wind and turbulence; filament/prominence, jets, flares, and radio bursts; active regions and solar eruptions; coronal mass ejections and their interplanetary counterparts; other interplanetary structures; space weather prediction methods; magnetic reconnection; Magnetohydrodynamic (MHD) numerical modeling; solar energetic particles, cosmic rays, and Forbush decreases; machine learning methods in space weather and other aspects. More than one hundred and forty papers in the academic journals have been published in these research directions. These fruitful achievements are obtained by Chinese scholars in solar physics and space physics either independently or through international collaborations. They greatly improve people's understanding of solar activities, solar eruptions, the corresponding space weather effects, and the Sun-Earth relations. Here we will give a very brief review on the research progress. However, it must be pointed out that this paper may not completely cover all achievements in this field due to our limited knowledge. |
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