Table 1.
Typical parameters of the coronal plasma and slow waves used for the analysis.
| Parameter | Value |
|---|---|
| Temperature, T0 | 0.5–20 MK |
| Number density, n0 | 108–1011 cm−3 |
| Wave periods, τ | 5 min and 15 min |
| Spitzer conductivity, κ |  W m−1 K−1 |
| Adiabatic index, γ | 5/3 |
| Mean particle mass, m | 0.6 × 1.67 × 10−27 kg |
| Specific heat capacity, CV | (γ − 1)−1kB/m J K−1 kg−1 |
Notes. The wave periods τ are shown for propagating waves observed in loops (De Moortel 2009) with τ ≃ 5 min and plumes (Banerjee et al. 2011) with τ ≃ 15 min, and standing SUMER oscillations (Wang 2011; Nakariakov et al. 2019) with τ ≃ 15 min. The constant kB is the Boltzmann constant.
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