Space Weather Related to Solar Eruptions With the ASO-S Mission
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 Magne...
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Frontiers Media S.A.
2020-03-01
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Series: | Frontiers in Physics |
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Online Access: | https://www.frontiersin.org/article/10.3389/fphy.2020.00045/full |
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record_format |
Article |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
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 |
spellingShingle |
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 Space Weather Related to Solar Eruptions With the ASO-S Mission Frontiers in Physics Sun: solar-terrestrial relations Sun: magnetic fields Sun: coronal mass ejections (CMEs) Sun: flares Sun: filaments Sun: prominences |
author_facet |
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 |
author_sort |
Li Feng |
title |
Space Weather Related to Solar Eruptions With the ASO-S Mission |
title_short |
Space Weather Related to Solar Eruptions With the ASO-S Mission |
title_full |
Space Weather Related to Solar Eruptions With the ASO-S Mission |
title_fullStr |
Space Weather Related to Solar Eruptions With the ASO-S Mission |
title_full_unstemmed |
Space Weather Related to Solar Eruptions With the ASO-S Mission |
title_sort |
space weather related to solar eruptions with the aso-s mission |
publisher |
Frontiers Media S.A. |
series |
Frontiers in Physics |
issn |
2296-424X |
publishDate |
2020-03-01 |
description |
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. |
topic |
Sun: solar-terrestrial relations Sun: magnetic fields Sun: coronal mass ejections (CMEs) Sun: flares Sun: filaments Sun: prominences |
url |
https://www.frontiersin.org/article/10.3389/fphy.2020.00045/full |
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doaj-a25ca1539a14446fae824b71724412852020-11-25T02:34:55ZengFrontiers Media S.A.Frontiers in Physics2296-424X2020-03-01810.3389/fphy.2020.00045510684Space Weather Related to Solar Eruptions With the ASO-S MissionLi Feng0Li Feng1Weiqun Gan2Weiqun Gan3Siqing Liu4Huaning Wang5Hui Li6Hui Li7Long Xu8Weiguo Zong9Xiaoxing Zhang10Yaguang Zhu11Haiyan Wu12Anqin Chen13Yanmei Cui14Xinghua Dai15Juan Guo16Han He17Xin Huang18Lei Lu19Lei Lu20Qiao Song21Jingjing Wang22Qiuzhen Zhong23Ling Chen24Zhanle Du25Xingliang Guo26Yu Huang27Yu Huang28Hu Li29Ying Li30Ying Li31Senlin Xiong32Shenggao Yang33Beili Ying34Beili Ying35Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaKey Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, ChinaKey Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, ChinaState Key Laboratory of Astronautic Dynamics, Xi'an, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaSchool of Physics and Information Engineering, Shanxi Normal University, Linfen, ChinaKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaKey Laboratory of Space Weather, National Center for Space Weather, China Meteorological Administration, Beijing, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, ChinaState Key Laboratory of Astronautic Dynamics, Xi'an, ChinaKey Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaKey Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaNational Space Science Center, Chinese Academy of Sciences, Beijing, ChinaState Key Laboratory of Astronautic Dynamics, Xi'an, ChinaKey Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, ChinaSchool of Astronomy and Space Science, University of Science and Technology of China, Hefei, ChinaThe 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.https://www.frontiersin.org/article/10.3389/fphy.2020.00045/fullSun: solar-terrestrial relationsSun: magnetic fieldsSun: coronal mass ejections (CMEs)Sun: flaresSun: filamentsSun: prominences |