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Prospective White-light Imaging and In Situ Measurements of Quiescent Large-scale Solar-wind Streams from the Parker Solar Probe and Solar Orbiter
文献类型：期刊论文
| 作者 | Xiong, Ming; Davies, Jackie A.; Feng, Xueshang; Li, Bo; Yang, Liping; Xia, Lidong; Harrison, Richard A.; Hayashi, Keiji; Li, Huichao; Zhou, Yufen |
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2018 |
| 卷号 | 868期号:2页码:137 |
| 关键词 | magnetohydrodynamics (MHD) methods: numerical solar wind Sun: corona Sun: heliosphere |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/aae978 |
| 英文摘要 | Deep-space exploration of the inner heliosphere is in an unprecedented golden age, with the recent and forthcoming launches of the Parker Solar Probe (PSP) and Solar Orbiter (SolO) missions, respectively. In order to both predict and understand the prospective observations by PSP and SolO, we perform forward MHD modeling of the 3D inner heliosphere at solar minimum, and synthesize the white-light (WL) emission that would result from Thomson scattering of sunlight from the coronal and heliospheric plasmas. Both solar rotation and spacecraft trajectory should be considered when reconstructing quiescent large-scale solar-wind streams from PSP and SolO WL observations. When transformed from a static coordinate system into a corotating one, the elliptical orbit of PSP becomes a multiwinding spiral. The innermost spiral winding of this corotating PSP orbit takes the form of a closed "heart shape" within around 80 R-circle dot of the Sun. PSP, when traveling along this "heart-shaped" trajectory, can cross a single corotating interaction region (CIR) twice. This enables in situ measurements of the same CIR to be made in both the corona and heliosphere. As PSP approaches perihelion, the WL radiance from the corona increases. Polarization can be used to localize the main WL scattering region in the corona. Large-scale structures around PSP can be further resolved in the longitudinal dimension, using additional WL imagery from the out-of-ecliptic perspective of SolO. Coordinated observations between PSP and SolO are very promising in the quest to differentiate background CIRs from transient ejecta. |
| 语种 | 英语 |
| 源URL | [http://ir.nssc.ac.cn/handle/122/6607]  |
| 专题 | 国家空间科学中心_空间科学部 |
| 推荐引用方式 GB/T 7714 | Xiong, Ming,Davies, Jackie A.,Feng, Xueshang,et al. Prospective White-light Imaging and In Situ Measurements of Quiescent Large-scale Solar-wind Streams from the Parker Solar Probe and Solar Orbiter[J]. ASTROPHYSICAL JOURNAL,2018,868(2):137. |
| APA | Xiong, Ming.,Davies, Jackie A..,Feng, Xueshang.,Li, Bo.,Yang, Liping.,...&Zhou, Yufen.(2018).Prospective White-light Imaging and In Situ Measurements of Quiescent Large-scale Solar-wind Streams from the Parker Solar Probe and Solar Orbiter.ASTROPHYSICAL JOURNAL,868(2),137. |
| MLA | Xiong, Ming,et al."Prospective White-light Imaging and In Situ Measurements of Quiescent Large-scale Solar-wind Streams from the Parker Solar Probe and Solar Orbiter".ASTROPHYSICAL JOURNAL 868.2(2018):137. |
入库方式： OAI收割
来源：国家空间科学中心
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