Dataset corresponding to the SIRs observed by the Wind spacecraft during 2007, 2008, 2018, and 2019
Authors/Creators
- 1. SCiESMEX/LANCE, Instituto de Geofísica, Universidad Nacional Autónoma de México, México
Description
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.
Files
Table.pdf
Files
(75.3 kB)
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