All of these images were produced by using viewing geometry information from SPICE kernels to reproject the raw framelets to a simple cylindrical map. SPICE is an acronym that refers to files/kernels containing various information associated with spacecraft observations:

S = Spacecraft ephemeris, P = planet ephemeris, I = instrument description including FOVs, position and orientation on the spacecraft, C = spacecraft and/or instrument dynamic orientation, and E = Event or Experimenter's description of the observation effort.

For the best results, I had to make corrections to the camera pointing. I then used a 3D renderer to create perspective views of an oblate spheroid, using the spacecraft's location and the camera pointing at three different points in time when JunoCam was acquiring the original framelets.

Since JunoCam has a very wide field of view (58°), these images should give a fairly good idea of what a naked eye view from Juno's location would look like. This is different from Voyager, Galileo and Cassini images, where the field of view is less than 0.5°. The images from these spacecraft are therefore more similar to what one would see through a small astronomical telescope from a distance of a few million kilometers from Jupiter.

Juno's altitude above Jupiter was only about 14,500 km when the original images were obtained. Therefore, the area covered by the images isn't particularly big. Below is a quick and dirty context view. It is based on John Rogers' Perijove 4 (PJ4) predictive map that can be seen here.