Impact of nonthermal electron distributions on the triggering of the ion-ion acoustic instability near the Sun: Kinetic simulations

Open Access

Table 3.

Same as Table 2 but using a single Maxwellian electron distribution with T_e = T_eff instead of a core-strahl distribution.

Name	$\frac{T_{eff}}{T_{c}}$ $\frac{T_{\mathrm{eff}}}{T_{\mathrm{c}}}$	(ω/ω_pc)_Th	(v_res/v_th, c)_Th	(γ/ω_pc)_Th	(γ/ω_pc)_Sim
Case A	7.792	0.268	3.347	0.004	0.00583
Case B	7.989	0.269	3.367	0.0051	0.00679
Case C	8.113	0.270	3.379	0.0057	0.00748
Case D	8.197	0.271	3.387	0.0061	0.00794
Case C′	7.803	0.268	3.349	0.0041	0.00592

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.