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DOI | 10.1029/2019GL082126 |
Interplanetary Shock Parameters Near Jupiter's Orbit | |
Echer, E. | |
2019-06-16 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS
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ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2019 |
卷号 | 46期号:11页码:5681-5688 |
文章类型 | Article |
语种 | 英语 |
国家 | Brazil |
英文摘要 | Fast interplanetary shocks occurrence, their parameters, and drivers near Jupiter's orbit are determined in this paper. It was found that 70% of the fast shocks are forward (FS) and 30% are reverse (RS). Interplanetary coronal mass ejection-driven FS occur more frequently in all solar cycle phases except in the declining phase, when corotating interaction region-driven shocks predominate. Most of the shocks were quasi-perpendicularly (65 degrees to 70 degrees) propagating relative to the ambient interplanetary magnetic field. The average shock magnetosonic Mach number is slightly higher for FS (2.6) than for RS (2.4), which in turn are stronger than shocks near 1 and 10 AU reported in previous works. This occurs because of the full development of corotating interaction region shocks and higher occurrence of strong interplanetary coronal mass ejections near 5 AU and that the magnetosonic speed at 5 AU has only 60% of its value at 1 AU. |
英文关键词 | solar wind interplanetary shocks Jupiter' s magnetosphere |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000477616200006 |
WOS关键词 | SOLAR-WIND ; ULYSSES OBSERVATIONS ; EVOLUTION ; DRIVERS ; STORMS ; WAVES ; EARTH |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/184070 |
专题 | 气候变化 |
作者单位 | INPE, Sao Jose Dos Campos, Brazil |
推荐引用方式 GB/T 7714 | Echer, E.. Interplanetary Shock Parameters Near Jupiter's Orbit[J]. GEOPHYSICAL RESEARCH LETTERS,2019,46(11):5681-5688. |
APA | Echer, E..(2019).Interplanetary Shock Parameters Near Jupiter's Orbit.GEOPHYSICAL RESEARCH LETTERS,46(11),5681-5688. |
MLA | Echer, E.."Interplanetary Shock Parameters Near Jupiter's Orbit".GEOPHYSICAL RESEARCH LETTERS 46.11(2019):5681-5688. |
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