The Chinese Hα Solar Explorer (CHASE) mission: An overview
The Chinese Hα Solar Explorer (CHASE), dubbed “Xihe”—Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration (CNSA). The CHASE mission is designed to test a newly developed satellite platform and to acquire the spectroscopic observ...
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| Veröffentlicht in: | Science China. Physics, mechanics & astronomy mechanics & astronomy, 2022-08, Vol.65 (8), p.289602, Article 289602 |
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| creator | Li, Chuan Fang, Cheng Li, Zhen Ding, MingDe Chen, PengFei Qiu, Ye You, Wei Yuan, Yuan An, MinJie Tao, HongJiang Li, XianSheng Chen, Zhe Liu, Qiang Mei, Gui Yang, Liang Zhang, Wei Cheng, WeiQiang Chen, JianXin Chen, ChangYa Gu, Qiang Huang, QingLong Liu, MingXing Han, ChengShan Xin, HongWei Chen, ChangZheng Ni, YiWei Wang, WenBo Rao, ShiHao Li, HaiTang Lu, Xi Wang, Wei Lin, Jun Jiang, YiXian Meng, LingJie Zhao, Jian |
| description | The Chinese Hα Solar Explorer (CHASE), dubbed “Xihe”—Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration (CNSA). The CHASE mission is designed to test a newly developed satellite platform and to acquire the spectroscopic observations in the Hα waveband. The Hα Imaging Spectrograph (HIS) is the scientific payload of the CHASE satellite. It consists of two observational modes: raster scanning mode and continuum imaging mode. The raster scanning mode obtains full-Sun or region-of-interest spectral images from 6559.7 to 6565.9 Å; and from 6567.8 to 6570.6 Å with 0.024 Å pixel spectral resolution and 1 min temporal resolution. The continuum imaging mode obtains photospheric images in continuum around 6689 Å with the full width at half maximum of 13.4 Å. The CHASE mission will advance our understanding of the dynamics of solar activity in the photosphere and chromosphere. In this paper, we present an overview of the CHASE mission including the scientific objectives, HIS instrument overview, data calibration flow, and first results of on-orbit observations. |
| doi_str_mv | 10.1007/s11433-022-1893-3 |
| format | Article |
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The CHASE mission is designed to test a newly developed satellite platform and to acquire the spectroscopic observations in the Hα waveband. The Hα Imaging Spectrograph (HIS) is the scientific payload of the CHASE satellite. It consists of two observational modes: raster scanning mode and continuum imaging mode. The raster scanning mode obtains full-Sun or region-of-interest spectral images from 6559.7 to 6565.9 Å; and from 6567.8 to 6570.6 Å with 0.024 Å pixel spectral resolution and 1 min temporal resolution. The continuum imaging mode obtains photospheric images in continuum around 6689 Å with the full width at half maximum of 13.4 Å. The CHASE mission will advance our understanding of the dynamics of solar activity in the photosphere and chromosphere. In this paper, we present an overview of the CHASE mission including the scientific objectives, HIS instrument overview, data calibration flow, and first results of on-orbit observations.</description><identifier>ISSN: 1674-7348</identifier><identifier>EISSN: 1869-1927</identifier><identifier>DOI: 10.1007/s11433-022-1893-3</identifier><language>eng</language><publisher>Beijing: Science China Press</publisher><subject>Astronomy ; Chinese space program ; Chromosphere ; Classical and Continuum Physics ; H alpha line ; Imaging ; Observations and Techniques ; Photosphere ; Physics ; Physics and Astronomy ; Raster ; Raster scanning ; Solar activity ; Space missions ; Spectral resolution ; Temporal resolution</subject><ispartof>Science China. Physics, mechanics & astronomy, 2022-08, Vol.65 (8), p.289602, Article 289602</ispartof><rights>Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2022</rights><rights>Science China Press and Springer-Verlag GmbH Germany, part of Springer Nature 2022.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c359t-106ff0d945ff738c66a3a6ab1e2dbdcc2a21f8784dc77a150becdac6f7e4c7af3</citedby><cites>FETCH-LOGICAL-c359t-106ff0d945ff738c66a3a6ab1e2dbdcc2a21f8784dc77a150becdac6f7e4c7af3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s11433-022-1893-3$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s11433-022-1893-3$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,778,782,27907,27908,41471,42540,51302</link.rule.ids></links><search><creatorcontrib>Li, Chuan</creatorcontrib><creatorcontrib>Fang, Cheng</creatorcontrib><creatorcontrib>Li, Zhen</creatorcontrib><creatorcontrib>Ding, MingDe</creatorcontrib><creatorcontrib>Chen, PengFei</creatorcontrib><creatorcontrib>Qiu, Ye</creatorcontrib><creatorcontrib>You, Wei</creatorcontrib><creatorcontrib>Yuan, Yuan</creatorcontrib><creatorcontrib>An, MinJie</creatorcontrib><creatorcontrib>Tao, HongJiang</creatorcontrib><creatorcontrib>Li, XianSheng</creatorcontrib><creatorcontrib>Chen, Zhe</creatorcontrib><creatorcontrib>Liu, Qiang</creatorcontrib><creatorcontrib>Mei, Gui</creatorcontrib><creatorcontrib>Yang, Liang</creatorcontrib><creatorcontrib>Zhang, Wei</creatorcontrib><creatorcontrib>Cheng, WeiQiang</creatorcontrib><creatorcontrib>Chen, JianXin</creatorcontrib><creatorcontrib>Chen, ChangYa</creatorcontrib><creatorcontrib>Gu, Qiang</creatorcontrib><creatorcontrib>Huang, QingLong</creatorcontrib><creatorcontrib>Liu, MingXing</creatorcontrib><creatorcontrib>Han, ChengShan</creatorcontrib><creatorcontrib>Xin, HongWei</creatorcontrib><creatorcontrib>Chen, ChangZheng</creatorcontrib><creatorcontrib>Ni, YiWei</creatorcontrib><creatorcontrib>Wang, WenBo</creatorcontrib><creatorcontrib>Rao, ShiHao</creatorcontrib><creatorcontrib>Li, HaiTang</creatorcontrib><creatorcontrib>Lu, Xi</creatorcontrib><creatorcontrib>Wang, Wei</creatorcontrib><creatorcontrib>Lin, Jun</creatorcontrib><creatorcontrib>Jiang, YiXian</creatorcontrib><creatorcontrib>Meng, LingJie</creatorcontrib><creatorcontrib>Zhao, Jian</creatorcontrib><title>The Chinese Hα Solar Explorer (CHASE) mission: An overview</title><title>Science China. Physics, mechanics & astronomy</title><addtitle>Sci. China Phys. Mech. Astron</addtitle><description>The Chinese Hα Solar Explorer (CHASE), dubbed “Xihe”—Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration (CNSA). The CHASE mission is designed to test a newly developed satellite platform and to acquire the spectroscopic observations in the Hα waveband. The Hα Imaging Spectrograph (HIS) is the scientific payload of the CHASE satellite. It consists of two observational modes: raster scanning mode and continuum imaging mode. The raster scanning mode obtains full-Sun or region-of-interest spectral images from 6559.7 to 6565.9 Å; and from 6567.8 to 6570.6 Å with 0.024 Å pixel spectral resolution and 1 min temporal resolution. The continuum imaging mode obtains photospheric images in continuum around 6689 Å with the full width at half maximum of 13.4 Å. The CHASE mission will advance our understanding of the dynamics of solar activity in the photosphere and chromosphere. In this paper, we present an overview of the CHASE mission including the scientific objectives, HIS instrument overview, data calibration flow, and first results of on-orbit observations.</description><subject>Astronomy</subject><subject>Chinese space program</subject><subject>Chromosphere</subject><subject>Classical and Continuum Physics</subject><subject>H alpha line</subject><subject>Imaging</subject><subject>Observations and Techniques</subject><subject>Photosphere</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Raster</subject><subject>Raster scanning</subject><subject>Solar activity</subject><subject>Space missions</subject><subject>Spectral resolution</subject><subject>Temporal resolution</subject><issn>1674-7348</issn><issn>1869-1927</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>AFKRA</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kM1OAjEUhRujiQR5AHdN3Oii2r9pp7oiExQTEhfguimdVobAFFtAfCxfxGeyZExceTf3Ls45N-cD4JLgW4KxvEuEcMYQphSRUjHETkCPlEIhoqg8zbeQHEnGy3MwSGmJ8zCFueQ98DBbOFgtmtYlB8ffX3AaVibC0WGzCtFFeF2Nh9PRDVw3KTWhvYfDFoa9i_vGfVyAM29WyQ1-dx-8Po5m1RhNXp6eq-EEWVaoLSJYeI9rxQvvJSutEIYZYebE0XpeW0sNJb6UJa-tlIYUeO5sbazw0nErjWd9cNXlbmJ437m01cuwi21-qanKPUlRsCKrSKeyMaQUndeb2KxN_NQE6yMm3WHSGZM-YtIse2jnSVnbvrn4l_y_6QfY4Wl3</recordid><startdate>20220801</startdate><enddate>20220801</enddate><creator>Li, Chuan</creator><creator>Fang, Cheng</creator><creator>Li, Zhen</creator><creator>Ding, MingDe</creator><creator>Chen, PengFei</creator><creator>Qiu, Ye</creator><creator>You, Wei</creator><creator>Yuan, Yuan</creator><creator>An, MinJie</creator><creator>Tao, HongJiang</creator><creator>Li, XianSheng</creator><creator>Chen, Zhe</creator><creator>Liu, Qiang</creator><creator>Mei, Gui</creator><creator>Yang, Liang</creator><creator>Zhang, Wei</creator><creator>Cheng, WeiQiang</creator><creator>Chen, JianXin</creator><creator>Chen, ChangYa</creator><creator>Gu, Qiang</creator><creator>Huang, QingLong</creator><creator>Liu, MingXing</creator><creator>Han, ChengShan</creator><creator>Xin, HongWei</creator><creator>Chen, ChangZheng</creator><creator>Ni, YiWei</creator><creator>Wang, WenBo</creator><creator>Rao, ShiHao</creator><creator>Li, HaiTang</creator><creator>Lu, Xi</creator><creator>Wang, Wei</creator><creator>Lin, Jun</creator><creator>Jiang, YiXian</creator><creator>Meng, LingJie</creator><creator>Zhao, Jian</creator><general>Science China Press</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>P5Z</scope><scope>P62</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PTHSS</scope></search><sort><creationdate>20220801</creationdate><title>The Chinese Hα Solar Explorer (CHASE) mission: An overview</title><author>Li, Chuan ; Fang, Cheng ; Li, Zhen ; Ding, MingDe ; Chen, PengFei ; Qiu, Ye ; You, Wei ; Yuan, Yuan ; An, MinJie ; Tao, HongJiang ; Li, XianSheng ; Chen, Zhe ; Liu, Qiang ; Mei, Gui ; Yang, Liang ; Zhang, Wei ; Cheng, WeiQiang ; Chen, JianXin ; Chen, ChangYa ; Gu, Qiang ; Huang, QingLong ; Liu, MingXing ; Han, ChengShan ; Xin, HongWei ; Chen, ChangZheng ; Ni, YiWei ; Wang, WenBo ; Rao, ShiHao ; Li, HaiTang ; Lu, Xi ; Wang, Wei ; Lin, Jun ; Jiang, YiXian ; Meng, LingJie ; Zhao, Jian</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c359t-106ff0d945ff738c66a3a6ab1e2dbdcc2a21f8784dc77a150becdac6f7e4c7af3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Astronomy</topic><topic>Chinese space program</topic><topic>Chromosphere</topic><topic>Classical and Continuum Physics</topic><topic>H alpha line</topic><topic>Imaging</topic><topic>Observations and Techniques</topic><topic>Photosphere</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Raster</topic><topic>Raster scanning</topic><topic>Solar activity</topic><topic>Space missions</topic><topic>Spectral resolution</topic><topic>Temporal resolution</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Li, Chuan</creatorcontrib><creatorcontrib>Fang, Cheng</creatorcontrib><creatorcontrib>Li, Zhen</creatorcontrib><creatorcontrib>Ding, MingDe</creatorcontrib><creatorcontrib>Chen, PengFei</creatorcontrib><creatorcontrib>Qiu, Ye</creatorcontrib><creatorcontrib>You, Wei</creatorcontrib><creatorcontrib>Yuan, Yuan</creatorcontrib><creatorcontrib>An, MinJie</creatorcontrib><creatorcontrib>Tao, HongJiang</creatorcontrib><creatorcontrib>Li, XianSheng</creatorcontrib><creatorcontrib>Chen, Zhe</creatorcontrib><creatorcontrib>Liu, Qiang</creatorcontrib><creatorcontrib>Mei, Gui</creatorcontrib><creatorcontrib>Yang, Liang</creatorcontrib><creatorcontrib>Zhang, Wei</creatorcontrib><creatorcontrib>Cheng, WeiQiang</creatorcontrib><creatorcontrib>Chen, JianXin</creatorcontrib><creatorcontrib>Chen, ChangYa</creatorcontrib><creatorcontrib>Gu, Qiang</creatorcontrib><creatorcontrib>Huang, QingLong</creatorcontrib><creatorcontrib>Liu, MingXing</creatorcontrib><creatorcontrib>Han, ChengShan</creatorcontrib><creatorcontrib>Xin, HongWei</creatorcontrib><creatorcontrib>Chen, ChangZheng</creatorcontrib><creatorcontrib>Ni, YiWei</creatorcontrib><creatorcontrib>Wang, WenBo</creatorcontrib><creatorcontrib>Rao, ShiHao</creatorcontrib><creatorcontrib>Li, HaiTang</creatorcontrib><creatorcontrib>Lu, Xi</creatorcontrib><creatorcontrib>Wang, Wei</creatorcontrib><creatorcontrib>Lin, Jun</creatorcontrib><creatorcontrib>Jiang, YiXian</creatorcontrib><creatorcontrib>Meng, LingJie</creatorcontrib><creatorcontrib>Zhao, Jian</creatorcontrib><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest One Sustainability</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>Natural Science Collection</collection><collection>Earth, Atmospheric & Aquatic Science Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Advanced Technologies & Aerospace Database</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Earth, Atmospheric & Aquatic Science Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>Engineering Collection</collection><jtitle>Science China. Physics, mechanics & astronomy</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Li, Chuan</au><au>Fang, Cheng</au><au>Li, Zhen</au><au>Ding, MingDe</au><au>Chen, PengFei</au><au>Qiu, Ye</au><au>You, Wei</au><au>Yuan, Yuan</au><au>An, MinJie</au><au>Tao, HongJiang</au><au>Li, XianSheng</au><au>Chen, Zhe</au><au>Liu, Qiang</au><au>Mei, Gui</au><au>Yang, Liang</au><au>Zhang, Wei</au><au>Cheng, WeiQiang</au><au>Chen, JianXin</au><au>Chen, ChangYa</au><au>Gu, Qiang</au><au>Huang, QingLong</au><au>Liu, MingXing</au><au>Han, ChengShan</au><au>Xin, HongWei</au><au>Chen, ChangZheng</au><au>Ni, YiWei</au><au>Wang, WenBo</au><au>Rao, ShiHao</au><au>Li, HaiTang</au><au>Lu, Xi</au><au>Wang, Wei</au><au>Lin, Jun</au><au>Jiang, YiXian</au><au>Meng, LingJie</au><au>Zhao, Jian</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The Chinese Hα Solar Explorer (CHASE) mission: An overview</atitle><jtitle>Science China. Physics, mechanics & astronomy</jtitle><stitle>Sci. China Phys. Mech. Astron</stitle><date>2022-08-01</date><risdate>2022</risdate><volume>65</volume><issue>8</issue><spage>289602</spage><pages>289602-</pages><artnum>289602</artnum><issn>1674-7348</issn><eissn>1869-1927</eissn><abstract>The Chinese Hα Solar Explorer (CHASE), dubbed “Xihe”—Goddess of the Sun, was launched on October 14, 2021 as the first solar space mission of China National Space Administration (CNSA). The CHASE mission is designed to test a newly developed satellite platform and to acquire the spectroscopic observations in the Hα waveband. The Hα Imaging Spectrograph (HIS) is the scientific payload of the CHASE satellite. It consists of two observational modes: raster scanning mode and continuum imaging mode. The raster scanning mode obtains full-Sun or region-of-interest spectral images from 6559.7 to 6565.9 Å; and from 6567.8 to 6570.6 Å with 0.024 Å pixel spectral resolution and 1 min temporal resolution. The continuum imaging mode obtains photospheric images in continuum around 6689 Å with the full width at half maximum of 13.4 Å. The CHASE mission will advance our understanding of the dynamics of solar activity in the photosphere and chromosphere. In this paper, we present an overview of the CHASE mission including the scientific objectives, HIS instrument overview, data calibration flow, and first results of on-orbit observations.</abstract><cop>Beijing</cop><pub>Science China Press</pub><doi>10.1007/s11433-022-1893-3</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Astronomy Chinese space program Chromosphere Classical and Continuum Physics H alpha line Imaging Observations and Techniques Photosphere Physics Physics and Astronomy Raster Raster scanning Solar activity Space missions Spectral resolution Temporal resolution |
| title | The Chinese Hα Solar Explorer (CHASE) mission: An overview |
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