Probing quiet Sun magnetism using MURaM simulations and Hinode/SP results: support for a local dynamo

S. Danilovic; M. Schüssler; S. K. Solanki

doi:10.1051/0004-6361/200913379

Home

All issues

Volume 513 (April 2010)

A&A, 513 (2010) A1

Full HTML

Free Access

Table 1:

Details of the three Hinode/SP data sets used.
	Date	Time	FOCUS	$\mu$	Size	Exposure	Noise	$\langle B^{\rm T}_{\rm app}\rangle$	$\langle \vert B^{\rm L}_{\rm app}\vert\rangle$	$\langle B^{\rm L}_{\rm app}\rangle$
	[dd/mm/yy]	UT			[arcsec]	time [s]	$10^{-3} I_{\rm c}$	Mx/cm²	Mx/cm²	Mx/cm²
set I	10/09/07	08:00:00	2031	1	$58 \times 164$	9.6	0.8	56.7	9.7	1.6
set II	27/02/07	00:20:09	2048	1	$0.16 \times 164$	67.2	0.25	54.6	11.0	1.7
set III	09/09/07	13:05:05	2029	0.4	$160 \times 32$	9.6	1	53.5	6.8	0.3

Notes. The last three columns, from left to right, give the mean values of the transversal (with respect to the line of sight), unsigned longitudinal, and signed longitudinal magnetic flux density.

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.