Fig. 5.
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Positions of the sensor’s elements, H(r, α), for the LCVR retardances evaluation in Eq. (5). We considered different heliocentric distances, r, from 3.14 R⊙ to 3.63 R⊙ and different polar angles, α. The PILS reference frame position relative to the Sun is shown in blue. In particular, the zPILS axis results were found to be at −45deg from the west solar limb.
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