Table B.1.
Number of major solar wind plasma types and the fraction of each type in anticorrelated structures in different groups.
 |
One | Two | Three | Four | |
|---|---|---|---|---|---|
 |
5 (4)b | 8 (8) | 3 (4) | 0 (0) | |
 |
32 (30) | 35 (32) | 19 (24) | 1 (1) | |
 |
19 (19) | 29 (24) | 15 (19) | 0 (1) | |
 |
18 (15) | 14 (16) | 7 (9) | 1 (0) | |
| Nmajor plasma type = 1 | streamer-belt-origin | coronal-hole-origin | sector-reversal-region | ejecta | |
 |
0 (0) | 0 (0) | 0 (0) | 5 (4) | |
 |
19 (20) | 10 (8) | 2 (1) | 1 (1) | |
 |
10 (11) | 6 (6) | 2 (1) | 1 (1) | |
 |
9 (9) | 4 (2) | 0 (0) | 5 (4) | |
| Nmajor plasma type > 2c | streamer-belt-origin | coronal-hole-origin | sector-reversal-region | ejecta | Number of cases |
 |
36.8% (30.4%) | 3.6% (6.0%) | 12.4% (14.0%) | 47.2% (49.7%) | 3(4) |
 |
34.8% (35.4%) | 14.5% (13.4%) | 14.8% (17.3%) | 35.9% (33.8%) | 20(25) |
 |
32.8% (34.79%) | 13.1% (13.5%) | 14.0% (13.7%) | 38.1% (25.2%) | 15(20) |
 |
39.3% (34.7%) | 13.1% (9.9%) | 15.3% (24.0%) | 32.2% (31.4%) | 8(9) |
| non-ICME&Fe-up | 32.8%(34.0%) | 13.1%(13.6%) | 14.0%(14.4%) | 40.2%(38.0%) | 15(19) |
| non-ICME&Fe-down | 40.8%(39.8%) | 18.8%(12.8%) | 17.1%(26.7%) | 23.2%(20.7%) | 5(6) |
| ICMEs in 2001d | 17.0% | 6.5% | 21.4% | 55.1% | - |
| Solar wind in 2001e | 49.5% | 15.8% | 20.6% | 14.1% | - |
| Solar wind in 2007e | 35.8% | 26.3% | 34.4% | 3.5% | - |
a If the proportion of one solar wind type is over 10%, it is considered as a major type. Solar wind types are based on the four-plasma categorization scheme from Xu & Borovsky (2015).
b The values outside the brackets are based on Sstrong (corresponding to solid markers), and the values within the brackets are based on Sweak (corresponding to empty markers).
c A relatively remarkable mixture of plasma from different origins is very likely.
d ICMEs from Cane & Richardson (2003), calculations are based on 12-min averaged solar wind plasma data.
e Based on 12-min averaged solar wind plasma data, ICMEs excluded.
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