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Table 1.

Input parameters (and their uncertainties) of 2D models providing the best fit to the observed Hα profiles from the areas f1–f6.

Position
Vertical size Gas
Area Solar X Solar Y of the slab (Z) Temperature pressure vMT vLOS
[arcsec] [arcsec] [km] [K] [dyn cm−2] [km s−1] [km s−1]
f1 −408 −101 33 000 ± 12% 10 000 ± 10% 0.28 ± 43% 9.33 ± 45% −6.02 ± 7%
f2 −404 −98 38 000 ± 10% 9000 ± 11% 0.20 ± 50% 4.30 ± 93% −6.87 ± 5%
f3 −398 −90 37 500 ± 60% 6000 ± 17% 0.42 ± 67% 8.03 ± 20% −7.35 ± 10%
f4 −392 −88 22 500 ± 15% 12 000 ± 8% 0.15 ± 40% 6.30 ± 82% −1.31 ± 83%
f5 −398 −83 32 000 ± 22% 11 000 ± 9% 0.16 ± 56% 4.87 ± 88% −2.53 ± 37%
f6 −379 −79 37 500 ± 4% 14 000 ± 7% 0.16 ± 56% 4.21 ± 43% −0.10 ± 502%

Notes. The table lists: vertical dimension of the slab (the slab Z-axis), temperature, gas pressure, microturbulence velocity and the LOS component of the plasma-flow velocity. Positive value of the LOS velocity corresponds to flow towards an observer.

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