| 9 | | 1. Runs and SUS ('''Outline all the proposed computational algorithms and simulations''') |
| | 9 | 1. Runs and SUS ('''Outline all the proposed computational algorithms and simulations''')\\ |
| | 10 | |
| | 11 | 1) Colliding Flows |
| | 12 | |
| | 13 | || Shearing angle($\theta$) || magnetic field($\beta$) || field orientation || SUs || |
| | 14 | || 0 || 1 || 90 || 1,050,000 || |
| | 15 | || 15 || 1 || 90 || 1,050,000 || |
| | 16 | || 30 || 1 || 90 || 1,050,000 || |
| | 17 | || 0 || 10 || 90 || 1,050,000 || |
| | 18 | || 15 || 10 || 90 || 1,050,000 || |
| | 19 | || 30 || 10 || 90 || 1,050,000 || |
| | 20 | || total || || || 6,3000,000 || |
| | 21 | |
| | 22 | 2) Triggering Star Formation |
| | 23 | || Resolution || magnetic field || Rotation || SUs || |
| | 24 | || 1024 || 1, toroidal || Y || 1,150,000 || |
| | 25 | || 1024 || 1, poloidal || Y || 1,150,000 || |
| | 26 | || 1024 || hydro || N || 1,150,000 || |
| | 27 | || 1024 || hydro || Y || 1,150,000 || |
| | 28 | || total || || || 4,600,000 || |
| | 29 | |
| | 30 | |