Image Details
Caption: Figure 2.
In the two pairs of rows, the lower set of panels (with tick marks) are ALMA 1.3 mm continuum images of Juno in equatorial offset coordinates referenced to the phase tracking center corresponding to the JPL ephemeris, but with the centroid shifted by the values in columns 4 and 5 in Table 2. In each frame, the cross marks the position of the peak intensity. The position angle of the Sun was +101.°5 east of north in equatorial coordinates, as indicated by the arrow. The beam size is indicated by the circle in the lower right-hand corner. The ﹩3\sigma ﹩ position uncertainty of the JPL ephemeris in each axis is indicated by the cross in the lower left-hand corner. The rotational phase values (﹩{\phi }_{1}﹩) are from Table 1. The faceted images are DAMIT sky projection models (with artificial lighting) computed for the corresponding mean epoch of each image and are shown on the same angular scale (the models have a 12% uncertainty in scale).
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