Table 5.
The magnetopause subsolar position and tail radii for each case.
| Case name |
 (R
E) |
 (R
E) |
 (R
E) |
 (R
E) |
 (R
E) |
|---|---|---|---|---|---|
| 1 | 11.0 | 11.2 | 21.5 | 18.2 | 22.1 |
| 2 | 11.0 | 10.8 | 19.9 | 17.2 | 21.3 |
| 3 | 8.7 | 8.8 | 18.5 | 16.5 | 18.5 |
| 4 | 10.2 | 10.9 | 23.6 | 21.0 | 24.6 |
| 5 | 9.6 | 10.3 | 24.0 | 22.3 | 25.2 |
| 6 | 8.2 | 8.0 | 20.6 | 17.6 | 20.4 |
Notes. 
and 
refer to the subsolar position and tail radius at x = −20.0 R
E of the magnetopause which are established according to the magnetopause model of Shue et al. (1997). 
refer to the magnetopause subsolar position, while 
and 
refer to the magnetopause tail radii at x = −20.0 R
E along y-axis and z-axis, respectively. These parameters marked by a superscript star are obtained from our MHD model.
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