Temporal comparison of nonthermal flare emission and magnetic-flux change rates

Free Access

Table 2:

Information on the used data sets. For each event we list the instrument, wavelength, cadence, and pixel scale of the image time series. A ``yes'' in the Saturation-column indicates that the observations were saturated during the impulsive phase of the event. The last two columns give the used instrument and energy band of the observed nonthermal HXR emission.
	Image time series					HXRs
[-1.2ex]Date	Instrument	Wavelength	Cadence [s]	$^{\prime\prime}$ /pixel	Saturation	Instrument	Energy [keV]
2003 Oct. 28	Meudon Obs.	H $\alpha$ blue wing	$\sim$ 60	1.9	no	INTEGRAL/SPI	>150
2003 Nov. 18	TRACE	1600 Å	$\sim$ 23	0.5	no	RHESSI	20-60
2005 Jan. 15	TRACE	1600 Å	$\sim$ 10	0.5	no	RHESSI	30-100
	BBSO	H $\alpha$ line center	$\sim$ 60	1.05	yes		and 100-300
2006 Jul. 06	Hvar Obs.	H $\alpha$ line center	$\sim$ 4	0.3	yes	RHESSI	20-50
2007 May 19	KSO	H $\alpha$ line center	$\sim$ 60	2.2	yes	RHESSI	15-50

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.