Density-gradient-driven drift-wave turbulence in the solar corona

Open Access

Table 1.

Physical parameter settings and perpendicular domain sizes of non-linear simulations.

Case	β	ω_n	$\hat{s}$ ${\hat {s}}$
1	electrostatic	100	0.25

2	electrostatic	200	0.25
3	electrostatic	50	0.25

4	electrostatic	100	0.5
5	electrostatic	100	1

6	1·10⁻⁴	100	0.25

7	3.5·10⁻⁴	50	0.25
8	3.5·10⁻⁴	150	0.25
9	3.5·10⁻⁴	250	0.25

Notes. Normalised electron pressure β, normalised density gradient ω_n and normalised magnetic shear $\hat{s}$ ${\hat {s}}$ .

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