Evidence for magnetic flux cancelation leading to an ejective solar eruption observed by Hinode, TRACE, STEREO, and SoHO/MDI

Free Access

Table 2:

Log averaged densities (cm^-3) over box locations within eruption region.
Location	Mg VII	Mg VII Spike	Fe XIII	Fe XIII Spike	Fe XIV	Fe XIV Spike
Box 1	$9.9 \pm 0.3$	No^*	$9.65 \pm 0.10$	9.78	$9.31 \pm 0.06$	9.43
Box 2	$9.7 \pm 0.5$	No	$9.37 \pm 0.05$	9.63	$9.13 \pm 0.07$	9.42
Box 3	$9.8 \pm 0.6$	No?	$9.68 \pm 0.08$	No	$9.25 \pm 0.10$	No

Notes. Columns 2, 4, and 6 are densities averaged over boxes of Fig. 11, and over time outside of enhanced density (``spike'') times. Columns 3, 5, and 7 are densities averaged over boxes of Fig. 11 during times of enhanced-density spikes.
^(*) ``No'' means no spike apparent within the scatter of the data.

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.