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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