LOS velocities inferred from: the Si i 10 827 Å full Stokes “standard” inversions (top row), the Si i 10 827 Å “magnetic” inversions (with weights: w_I = 0, w_Q,U = 1.0 and w_V = 0.1) (middle row) and He i 10 830 Å inversions (bottom row) at different times. Note that the color scale is saturated at [−1, 1] and [−2, 2] km s^-1 for silicon and helium respectively. Pixels inside the contours have magnetic field inclinations, with respect to the LOS, between 75° ≤ γ ≤ 105°. In the July 5 maps, the colored contours distinguish between the orphan penumbrae area (green) and the spine region (black). On July 3, only the spine of the filament was seen. Negative velocities (blue) indicate upflows while positive velocities (red) indicate downflows.