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Dataset corresponding to the Stream Interaction Regions (SIRs) observed by the Wind spacecraft during 2007, 2008, 2018, and 2019. The table consists of several columns detailing the solar wind (SW) properties and related parameters. In addition, we show the coronal holes (CHs) locations from which the high-speed streams originate using synoptic maps. CHs can be near the solar equator, at midlatitudes, or as low-latitude extensions of polar CH.
Dataset
Dataset
| selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | 1 | |
| popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network. | Average | |
| influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically). | Average | |
| impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network. | Average |
| views | 10 | |
| downloads | 14 |

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