Forbush decreases and turbulence levels at coronal mass ejection fronts

Free Access

Table 4:

Summary of various observationally derived parameters for the three events we consider, leading to $\sigma ^{2}$ (Eq. (12)) as our final result.
Event	R₀	$V_{\rm exp}$	T	R(T)	$B_{\rm MC}$	Average $\sigma ^{2}$ (Kolmogorov)
	( $R_{\odot}$ )	(km s^-1)	(h)	(AU)	(nT)
2001 April 11	2.84	2411	47.1	0.10	17.8	2%
2003 October 29	5.84	2459	24.8	0.14	44	249%
2003 November 20	6.3	1660	49.4	0.12	50	6%

Source LaTeX | All tables | In the text

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.