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Table 1.
Fitted parameters of the inversion for the emission and absorption cluster.
| Cluster | Npars | Fitted parameters | Constants |
|---|---|---|---|
| Emission | 14 | B1, θB, 1, χB, 1, τ1, νDop,1, νmac,1, β1 | h = 2″, a = 10−4 |
| B2, θB, 2, χB, 2, τ2, νDop,2, νmac,2, β2 | |||
| Absorption | 7 | B, θB, χBa, τ, νDop, νmac, β | h = 10″, a = 10−4 |
Notes.
(a)
The magnetic field azimuth has been inverted only with one Levenberg-Marquardt cycle, not applying the DIRECT algorithm. The input values for the Levenberg-Marquardt were calculated via loop orientation measurement, see Sect. 3.2.2.
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