Case	Heliocentric	Af$\rho$	Dust	Nucleus	MHD Mean	Additional
Name	Distance		Distribution	Density	Ion Mass	Description
	AU	cm	r=10$^\mathrm{-7}$...10$^{-2}$ m	kg/m$^{3}$	amu
CG_1.3_au_00	1.3	100 to 500	-4	300	17	Perihelion: Original ISSI Case
CG_1.3_au_01	1.3		x	300	17	min perihelion Case
CG_1.3_au_02	1.3		x	300	17	max perihelion Case
CG_2.0_au_00	2.0	40 to 300	-4	300	17	Original ISSI Case
CG_2.0_au_01	2.0		-3.5	300	17	Detailed Chemistry
CG_2.0_au_02	2.0		x	300	17	Min Case
CG_2.0_au_03	2.0	40 to 300	x	300	17	Max Case
CG_2.7_au_00	2.7	25 to 250	-4	300	17	Original ISSI Case
CG_2.7_au_01	2.7	20	-4	300	17	H2O Driven
CG_2.7_au_02	2.7	10	-4	300	17	H2O Driven
CG_2.7_au_03	2.7	250	Knee*	300	35	CO/CO2 Driven
CG_2.7_au_04	2.7	25	Knee*	300	35	CO/CO2 Driven
CG_2.7_au_05	2.7	20	-4	300	17	H2O Driven/Jet
CG_2.7_au_06	2.7	250	Knee*	300	35	CO/CO2 Driven/Jet
CG_3.0_au_01	3.0	10	-4	300	17	H2O Driven
CG_3.0_au_02	3.0	5	-4	300	17	H2O Driven
CG_3.0_au_03	3.0	200	Knee*	300	35	CO/CO2 Driven
CG_3.0_au_04	3.0	20	Knee	300	35	CO/CO2 Driven
CG_3.0_au_05	3.0	10	-4	300	17	H2O Driven/Jet
CG_3.0_au_06	3.0	200	Knee*	300	35	CO/CO2 Driven/Jet
CG_3.0_au_07	3.0		-3.5	300	17	H2O Driven
CG_3.0_au_08	3.0		-3.5	300	17	CO Driven
CG_3.0_au_09	3.0		-3.5	300	17	CG_3.0_au_07 with Q +20%
CG_3.0_au_10	3.0		-3.5	300	17	CG_3.0_au_07 with Q -20%
CG_3.0_au_11	3.0		-3.5	300	17	CG_3.0_au_07 with Q +50%
CG_3.0_au_12	3.0		-3.5	300	17	CG_3.0_au_07 with Q -50%
CG_3.0_au_13	3.0		-3.5	300	17	CG_3.0_au_07 with Knudsen layer temperature +20 K
CG_3.0_au_14	3.0		-3.5	300	17	CG_3.0_au_07 with Knudsen layer temperature -20 K
CG_3.0_au_15	3.0		x	300	17	Min Case
CG_3.0_au_16	3.0		x	300	17	Max Case
CG_3.3_au_00	3.3	5 to 150	-4	300	17	Rendezvous: Original ISSI Case
CG_3.5_au_01	3.5	5 to 150	-3.5	300	17	Nominal Case
CG_3.5_au_02	3.5	5 to 150	-3.5	300	17	CO/CO2 Driven
CG_3.5_au_03	3.5	5 to 150	-3.5	300	17	H2O Driven,Low production rates

* Knee distribution: -3 for dust particles with radius up to 1mm and -4 beyond

Case	Dimension	Production Rate
Name	DSMC	Total	H$_2$O	CO	CO$_2$	Dust
		molecules/s				kg/s
CG_1.3_au_00	2d	$5\times10^{27}$	$4.76\times10^{27}$	$2.4\times10^{26}$	0	114
CG_1.3_au_01	2d	$4.14\times10^{27}$	$4\times10^{27}$	$4\times10^{25}$	$1\times10^{26}$	0
CG_1.3_au_02	2d	$1.13\times10^{28}$	$1\times10^{28}$	$5\times10^{26}$	$8\times10^{26}$	0
CG_2.0_au_00	2d	$8\times10^{26}$	$7.62\times10^{26}$	$3.8\times10^{25}$	0	23
CG_2.0_au_01	1d	$8.7\times10^{26}$	$7.62\times10^{26}$	$3.8\times10^{25}$	$1.9\times10^{25}$	23
CG_2.0_au_02	2d	$4.14\times10^{26}$	$4\times10^{26}$	$4\times10^{24}$	$1\times10^{25}$	0
CG_2.0_au_03	2d	$2.4\times10^{27}$	$2\times10^{27}$	$2\times10^{26}$	$2\times10^{26}$	0
CG_2.7_au_00	2d	$8\times10^{25}$	$7.62\times10^{25}$	$3.8\times10^{24}$	0	2
CG_2.7_au_01*	2d	$2.4\times10^{26}$	$2\times10^{26}$	$2\times10^{25}$	$2\times10^{25}$	10
CG_2.7_au_02	2d	$2.4\times10^{26}$	$2\times10^{26}$	$2\times10^{25}$	$2\times10^{25}$	5
CG_2.7_au_03	2d	$2.2\times10^{27}$	$2\times10^{26}$	$1\times10^{27}$	$1\times10^{27}$	80
CG_2.7_au_04	2d	$2.2\times10^{27}$	$2\times10^{26}$	$1\times10^{27}$	$1\times10^{27}$	8
CG_2.7_au_05**	2d	$2.4\times10^{26}$	$2\times10^{26}$	$2\times10^{25}$	$2\times10^{25}$	10
CG_2.7_au_06***	2d	$2.98\times10^{27}$	$2\times10^{26}$	$1.39\times10^{27}$	$1.39\times10^{27}$	80
CG_3.0_au_01	2d	$6\times10^{25}$	$5\times10^{25}$	$5\times10^{24}$	$5\times10^{24}$	5
CG_3.0_au_02	2d	$6\times10^{25}$	$5\times10^{25}$	$5\times10^{24}$	$5\times10^{24}$	2
CG_3.0_au_03	2d	$2.1\times10^{27}$	$5\times10^{25}$	$1\times10^{27}$	$1\times10^{27}$	60
CG_3.0_au_04	2d	$2.1\times10^{27}$	$5\times10^{25}$	$1\times10^{27}$	$1\times10^{27}$	6
CG_3.0_au_05**	2d	$6\times10^{25}$	$5\times10^{25}$	$5\times10^{24}$	$5\times10^{24}$	35
CG_3.0_au_06***	2d	$2.98\times10^{27}$	$5\times10^{25}$	$1.47\times10^{27}$	$1.47\times10^{27}$	60
CG_3.0_au_07	1d	$5.5\times10^{25}$	$5\times10^{25}$	$5\times10^{24}$	0	60
CG_3.0_au_08	1d	$1.1\times10^{27}$	$1\times10^{26}$	$1\times10^{27}$	0	60
CG_3.0_au_09	1d	$6.6\times10^{25}$	$6\times10^{25}$	$6\times10^{24}$	0	72
CG_3.0_au_10	1d	$4.4\times10^{25}$	$4\times10^{25}$	$4\times10^{24}$	0	48
CG_3.0_au_11	1d	$8.25\times10^{25}$	$7.5\times10^{25}$	$7.5\times10^{24}$	0	90
CG_3.0_au_12	1d	$2.75\times10^{25}$	$2.5\times10^{25}$	$2.5\times10^{24}$	0	30
CG_3.0_au_13	1d	$5.5\times10^{25}$	$5\times10^{25}$	$5\times10^{24}$	0	60
CG_3.0_au_14	1d	$5.5\times10^{25}$	$5\times10^{25}$	$5\times10^{24}$	0	60
CG_3.0_au_15	2d	$2.08\times10^{24}$	$2\times10^{24}$	$2\times10^{22}$	$6\times10^{22}$	0
CG_3.0_au_16	2d	$3.6\times10^{26}$	$3\times10^{26}$	$3\times10^{25}$	$3\times10^{25}$	0
CG_3.3_au_00	2d	$1\times10^{24}$	$9.52\times10^{23}$	$4.8\times10^{22}$	0	0.03
CG_3.5_au_01	1d	$6\times10^{26}$	$5\times10^{26}$	$5\times10^{25}$	$5\times10^{25}$	21
CG_3.5_au_02	1d	$1.05\times10^{28}$	$5\times10^{26}$	$5\times10^{27}$	$5\times10^{27}$	61
CG_3.5_au_03	1d	$2\times10^{23}$	$1.67\times10^{23}$	$1.67\times10^{22}$	$1.67\times10^{22}$	0.007

* The rest of the total production rate comes from others parent species
** 50% of productions as in the "non-jet" case and the other 50% of productions are due to the jet in an area centered on the sub-solar point which represents 10% of the total surface of the nucleus.
*** The size of the jet is adjusted so that the right dust size is lifted off, that is to say 1 cm particles.