Frontiers in Physics (Mar 2020)
Space Weather Related to Solar Eruptions With the ASO-S Mission
- Li Feng,
- Li Feng,
- Weiqun Gan,
- Weiqun Gan,
- Siqing Liu,
- Huaning Wang,
- Hui Li,
- Hui Li,
- Long Xu,
- Weiguo Zong,
- Xiaoxing Zhang,
- Yaguang Zhu,
- Haiyan Wu,
- Anqin Chen,
- Yanmei Cui,
- Xinghua Dai,
- Juan Guo,
- Han He,
- Xin Huang,
- Lei Lu,
- Lei Lu,
- Qiao Song,
- Jingjing Wang,
- Qiuzhen Zhong,
- Ling Chen,
- Zhanle Du,
- Xingliang Guo,
- Yu Huang,
- Yu Huang,
- Hu Li,
- Ying Li,
- Ying Li,
- Senlin Xiong,
- Shenggao Yang,
- Beili Ying,
- Beili Ying
Affiliations
- Li Feng
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Li Feng
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- Weiqun Gan
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Weiqun Gan
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- Siqing Liu
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Huaning Wang
- Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
- Hui Li
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Hui Li
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- Long Xu
- Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
- Weiguo Zong
- Key Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, China
- Xiaoxing Zhang
- Key Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, China
- Yaguang Zhu
- State Key Laboratory of Astronautic Dynamics, Xi'an, China
- Haiyan Wu
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Anqin Chen
- Key Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, China
- Yanmei Cui
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Xinghua Dai
- School of Physics and Information Engineering, Shanxi Normal University, Linfen, China
- Juan Guo
- Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
- Han He
- Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
- Xin Huang
- Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
- Lei Lu
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Lei Lu
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- Qiao Song
- Key Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, China
- Jingjing Wang
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Qiuzhen Zhong
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Ling Chen
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Zhanle Du
- Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China
- Xingliang Guo
- State Key Laboratory of Astronautic Dynamics, Xi'an, China
- Yu Huang
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Yu Huang
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- Hu Li
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Ying Li
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Ying Li
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- Senlin Xiong
- National Space Science Center, Chinese Academy of Sciences, Beijing, China
- Shenggao Yang
- State Key Laboratory of Astronautic Dynamics, Xi'an, China
- Beili Ying
- Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, China
- Beili Ying
- School of Astronomy and Space Science, University of Science and Technology of China, Hefei, China
- DOI
- https://doi.org/10.3389/fphy.2020.00045
- Journal volume & issue
-
Vol. 8
Abstract
The Advanced Space-based Solar Observatory (ASO-S) is a mission aiming at exploring solar flares, coronal mass ejections (CMEs), solar magnetic field and their relationships. To fulfill its major scientific objectives, ASO-S has three elaborately-designed payloads onboard: the Full-disk vector MagnetoGraph (FMG), the Lyman-alpha Solar Telescope (LST), and the Hard X-ray Imager (HXI) dedicated to observe vector magnetic fields, CMEs, and flares, respectively. Beside the scientific objectives, we have an operational objective to observe solar eruptions and magnetic field for making related space weather forecasts. More specifically, we have set a priority for the downlink of CME data observed by LST, and will distribute those data to different space weather prediction centers in China within 2 h once the Science Operation and Data Center (SODC) of ASO-S receive the data. After data downlink and archiving, different automatic detection, tracking, and cataloging procedures are planned to run for the most critical solar eruptive features. On the other hand, based on the distributed and downloaded data, different space weather prediction centers are to activate their forecast systems for the ASO-S observed solar eruption events. Our particular interests are currently focused on nowcast of different eruption events, prediction of CME arrivals, forecast of solar flares and the onset of solar eruptions. We are also working on further forecast potentials using the ASO-S data to make contributions to other possible important issues of space weather.
Keywords
- Sun: solar-terrestrial relations
- Sun: magnetic fields
- Sun: coronal mass ejections (CMEs)
- Sun: flares
- Sun: filaments
- Sun: prominences
