Chromospheric condensations and magnetic field in a C3.6-class flare studied via He I D3 spectro-polarimetry

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Table B.1

Parameter values for the series of test inversions.

	B_max [G]
0	2500
0	1250
0.001	2500
0.01	2500
0.1	2500
0.1	1250
0.5	2500
0.5	1250

Notes. We tested all of these cases both for a model using one slab and a model using two slabs. The values in boldface corresponds to the test cases that are shown in Figs. B.1 and B.2.

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