Table A.1
Summarising information for the streams used in this study including dates and number of switchbacks, with the results only shown for those streams where the analysis in Sect. 2 was successful.
| ID | Start | End | Number | Source | R (AU) |  |
 |
R2 | W (km) | Aspect ratio |
|---|---|---|---|---|---|---|---|---|---|---|
| E1S1 | 31/10/2018 01:20 | 01/11/2018 10:53 | 239 | CH | 0.24 | –8 | 0 | 0.94 | 89 000 | 59 |
| E1S2 | 01/11/2018 16:56 | 02/11/2018 11:28 | 114 | CH | 0.22 | – | – | – | – | – |
| E1S3 | 02/11/2018 11:35 | 03/11/2018 19:37 | 245 | CH | 0.2 | – | – | – | – | – |
| E1S4 | 03/11/2018 20:13 | 04/11/2018 18:35 | 283 | CH | 0.18 | – | – | – | – | – |
| E1S5 | 05/11/2018 00:48 | 05/11/2018 20:30 | 223 | CH | 0.17 | –7 | 2 | 0.96 | 33 000 | 28 |
| E1S6 | 05/11/2018 22:28 | 07/11/2018 09:30 | 510 | CH | 0.17 | –6 | 3 | 0.87 | 55 000 | 15 |
| E1S7 | 07/11/2018 09:54 | 08/11/2018 08:00 | 375 | CH | 0.18 | – | – | – | – | – |
| E1S8 | 08/11/2018 17:50 | 09/11/2018 06:19 | 178 | CH | 0.19 | – | – | – | – | – |
| E1S9 | 09/11/2018 14:23 | 10/11/2018 12:30 | 330 | CH | 0.21 | – | – | – | – | – |
| E1S10 | 15/11/2018 17:23 | 19/11/2018 10:39 | 1054 | CH | 0.38 | – | – | – | – | – |
| E2S1 | 30/03/2019 00:52 | 30/03/2019 18:36 | 214 | NA | 0.25 | – | – | – | – | – |
| E2S2 | 30/03/2019 21:24 | 01/04/2019 08:30 | 295 | NA | 0.22 | – | – | – | – | – |
| E2S3 | 01/04/2019 09:30 | 03/04/2019 08:00 | 285 | Inside | 0.19 | –3 | 0 | 0.92 | 94 000 | 23 |
| E2S4 | 03/04/2019 08:52 | 06/04/2019 11:49 | 435 | Outside | 0.17 | –15 | 0 | 0.96 | 20 000 | 34 |
| E2S5 | 06/04/2019 22:00 | 07/04/2019 18:19 | 198 | Outside | 0.19 | – | – | – | – | – |
| E2S6 | 08/04/2019 03:50 | 09/04/2019 19:09 | 396 | Inside | 0.21 | –7 | –15 | 0.95 | 43 000 | 11 |
Notes. A graphical representation of these streams can be seen in Fig. 1. The radial distance (R) is the mean distance from the Sun within each stream. The source region is shown, with CH standing for coronal hole and Inside and Outside refer to the streamer belt.
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