Table 1.
Adopted combinations of heating models and shearing motions with their outcomes.
| Heating model | Shearing | Condensation | nmax (×1011 cm−3) | Tmin (K) | ||
|---|---|---|---|---|---|---|
| Exponential | E |  |
+ | Y | 3.84 | 7529 |
| Mixed | M | cBαρβ | ||||
| Magnetic | M0 | cB2 | − | Y | ||
| Quasi-magnetic | M1 | cB2.1ρ−0.1 | + | N | ||
| − | Y | 2.50 | 8503 | |||
| M2 | cB2.2ρ−0.2 | + | N | |||
| − | Y | |||||
| Mok et al. (2008) | M3 | cB2.5ρ−0.5 | − | Y | ||
| Reduced exponential | RE |  |
+ | Y | 3.08 | 9196 |
| Reduced mixed | RM1 | f(u)×cB2.1ρ−0.1 | + | Y | 6.37 | 8551 |
Notes. Each model has an abbreviation for further reference. Shearing and anti-shearing motions are denoted by + and −, respectively. For those simulations that were advanced far into the prominence evolution, physical values are considered at t = 6741 s. Both maximum number density and minimum temperature are assumed to be reached in the prominence core.
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