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题名: PRESSURE PULSES AT VOYAGER 2: DRIVERS OF INTERSTELLAR TRANSIENTS?
作者: Richardson, J. D.; Wang, C.; Liu, Y. D.; Safrankova, J.; Nemecek, Z.; Kurth, W. S.
作者部门: 空间科学部
通讯作者: Richardson, JD (reprint author), MIT, Kavli Ctr Astrophys & Space Sci, 77 Massachusetts Ave, Cambridge, MA 02139 USA.
关键词: ISM: kinematics and dynamics ; solar wind ; Sun: coronal mass ejections (CMEs) ; Sun: heliosphere
刊名: ASTROPHYSICAL JOURNAL
ISSN号: 0004-637X
出版日期: 2017
卷号: 834, 期号:2, 页码:190
收录类别: SCI
项目资助者: International Space Science Institute for the team "Facing the Most Pressing Challenges to Our Understanding of the Heliosheath and Its Outer Boundaries" ; NASA from the Jet Propulsion Laboratory [959203] ; Czech Ministry of Education [LH15136] ; NASA [1279980]
英文摘要: Voyager 1 (V1) crossed the heliopause into the local interstellar medium (LISM) in 2012. The LISM is a dynamic region periodically disturbed by solar transients with outward-propagating shocks, cosmic-ray intensity changes and anisotropies, and plasma wave oscillations. Voyager 2 (V2) trails V1 and thus may observe the solar transients that are later observed at V1. V2 crossed the termination shock in 2007 and is now in the heliosheath. Starting in 2012, when solar maximum conditions reached V2, five possible merged interaction regions (MIRs) have been observed by V2 in the heliosheath. The timing is consistent with these MIRs driving the transients observed by V1 in the LISM. The largest heliosheath MIR was observed by V2 in late 2015 and should reach V1 in 2018.
语种: 英语
内容类型: 期刊论文
URI标识: http://ir.nssc.ac.cn/handle/122/5848
Appears in Collections:空间科学部_期刊论文

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