Population study on MHD wind-driven disc evolution - Confronting theory and observation

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Table B.2

Characteristics for different strong FUV field populations without EUV radiation shielding.

DW scenario	t_1/2 [Myr]^a)	f_disc,2Myr [%]^b)	f_cavity [%]^c)	[%] ^d)	[%] ^d)	[%] ^d)	[%] ^d)
strong DW + Σ-dep. torque	0.57	9	32	0.3	3.1	86.4	10.2
weak DW + Σ-dep. torque	1.25	36	12	3.3	5.5	87.4	3.9
strong DW + const. torque	0.42	3	34	0.1	2.5	84.6	12.9
weak DW + const. torque	0.88	29	22	5.3	4.4	85.2	5.1

Notes: a) time at which half of the iscs are isperse, b) fraction of iscs remaining at 2 Myr, c) fraction of iscs opening up an inner cavity, d) contribution of the ifferent processes to isc ispersal in terms of mass loss percentage (mean value over all simulations)

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