Conditioning of the solar corona due to large flares

Open Access

Table 3.

Spearman rank correlation of photospheric and coronal quantities prior to major flares.

	ϕ_m	E	E_F	\|H_V\|	\|H_J\|
ϕ_m	1.00	0.94	0.66	0.70	0.52

E		1.00	0.75	0.81	0.62

E_F			1.00	0.90	0.94

\|H_V\|				1.00	0.89

\|H_J\|					1.00



	E_F/E₀	\|H_J\|/\|H_V\|			$\| H_{J} \| / {\tilde{ϕ}}^{2}$ $\|H_{\mathrm{J}}\|/\tilde\phi^2$

E_F/E₀	1.00	0.88			0.90

\|H_J\|/\|H_V\|		1.00			0.82

$\| H_{J} \| / {\tilde{ϕ}}^{2}$ $\|H_{\mathrm{J}}\|/\tilde\phi^2$					1.00

Notes. Mean values are computed from the pre-flare values of C_SR of all flares of sample S_major. The cell colors are indicating the strength of the correlation and refer to a correlation of C_SR ≥ 0.8 (dark red) as “strong”, 0.8 > C_SR ≥ 0.6 (orange) as “moderate”, and C_SR < 0.6 (light red) as “weak”.

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.