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- W2799049105 abstract "Context . Coronal mass ejections (CMEs) are intense solar explosive eruptions, and they are frequently correlated with prominence eruptions. Previous observations show that about 70% of CMEs are associated with prominence eruptions. However, there are only a handful of reported observations of prominence plasma materials within interplanetary CMEs (ICMEs), which are the interplanetary manifestations of CMEs. Moreover, approximately 4% of ICMEs exhibit the presence of prominence materials, and approximately 12% of magnetic clouds (MCs) contain prominence materials. Aims . We aim to comprehensively search for cold prominence materials in MCs observed by the Advanced Composition Explorer (ACE) spacecraft during 1998–2007. Methods . Using the criteria of unusual O 5+ and (or) Fe 6+ abundances, we examined 76 MCs observed by ACE during 1998–2007 to search for cold prominence materials. Results . Our results revealed that out of the 76 MCs, 27 (36%) events contained prominence material regions with low-charge-state signatures. Conclusions . Although the fraction is still lower than the approximately 70% of CMEs associated with prominence eruptions, it is much higher than 12%. The unusual O 5+ and (or) Fe 6+ abundances may be simple and reliable criteria to investigate prominence materials in the interplanetary medium." @default.
- W2799049105 created "2018-05-07" @default.
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- W2799049105 date "2018-08-01" @default.
- W2799049105 modified "2023-10-01" @default.
- W2799049105 title "Cold prominence materials detected within magnetic clouds during 1998–2007" @default.
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- W2799049105 doi "https://doi.org/10.1051/0004-6361/201731807" @default.
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