Hydro_Analysis.git - [no description]

	Commit message (Collapse)	Author	Age
*	Hydro_Analysis: add parameters to control which interpolator is used in	rhaas	2012-11-29
\| \| \| \| \| \| \|	GRHydro_Separation git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@125 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
*	Hydro_Analysis: add verbosity_level option to control	rhaas	2012-11-27
\| \| \| \| \| \| \| \|	how much data to output to stdout git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@123 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
*	Hydro_Analysis: add option to average the location of	rhaas	2012-11-27
\| \| \| \| \| \| \| \| \| \| \|	multiple identical maxima this is useful for cell centering where intially there might be several points with precisely the same density around the center of a star git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@122 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
*	add distance calculation from Whisky	knarf	2010-01-12
\| \| \| \|	git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@32 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
*	update	knarf	2010-01-12
\| \| \| \|	git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@31 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
*	Implement primitive maximum density search ala Whisky. This should be fine most	knarf	2010-01-12
\| \| \| \| \| \| \| \|	of the time, but might break without notice if unlucky. Ideas of a safer neutron star tracking exist, but are not implemented here. git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@26 b6729ddc-ac74-4bd1-908c-9dc7244c52a1
*	bare Hydro_Analysis thorn	knarf	2010-01-11
	git-svn-id: http://svn.einsteintoolkit.org/cactus/EinsteinAnalysis/Hydro_Analysis/trunk@20 b6729ddc-ac74-4bd1-908c-9dc7244c52a1