Table 1: Coronal magnetic helicity and its variation. The values have been computed using MDI magnetograms at the times shown. This lapse of time includes the three X-ray bursts observed by SXT (see Sect. 2.3). The helicity values are in units of 10³⁹ Mx².
$\alpha$ $H_{\rm cor}$ $H_{\rm cor}$ $\Delta \vert H_{\rm cor}\vert$

Mm^-1 00:03 UT 11:11 UT

-0.08 -5.2 -2.9 -2.3

-0.11 -7.5 -4.2 -3.3

**Table 1:** Coronal magnetic helicity and its variation. The values have been computed using MDI magnetograms at the times shown. This lapse of time includes the three X-ray bursts observed by SXT (see Sect. 2.3). The helicity values are in units of 10³⁹ Mx².
$\alpha$	$H_{\rm cor}$	$H_{\rm cor}$	$\Delta \vert H_{\rm cor}\vert$
Mm^-1	00:03 UT	11:11 UT
-0.08	-5.2	-2.9	-2.3
-0.11	-7.5	-4.2	-3.3

Source LaTeX | All tables | In the text

	1 Introduction
	2 Evolution of the small AR during its full life-time
	3 Physical interpretation of the coronal eruptions
	4 Observational evidence of the interplanetary flux rope
	5 Linking the coronal eruption to the interplanetary MC
	6 Conclusions
	References