Analysis and modelling of recurrent solar flares observed with Hinode/EIS on March 9, 2012

Free Access

Table 3

Maximum Fe xxiii and Fe xvi upflow velocities during the recurrent flares.

Flare	Fe xxiii vel		Fe xvi vel
	(km s^-1)		(km s^-1)


	K1	K2	K1	K2
C2.0	202 ± 14	60 ± 7	76^∗	12 ± 5
C4.7	146 ± 10	110^∗	43 ± 5	39 ± 5


M1.8 (Doschek et al. 2013)	150–170		40–60

Notes. The values followed by an asterisk .

^(∗)

represent the velocity of the most blueshifted component when a double Gaussian fit was performed

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.