Juno perijove 7: GRS images, July 11, 2017 |
Juno perijove 7: GRS images, July 11, 2017 |
Jun 30 2017, 12:38 PM
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Senior Member Group: Members Posts: 2346 Joined: 7-December 12 Member No.: 6780 |
There are another three days left over to vote for Perijove-07 points of interest (POI).
This time, all eyes will be on the Great Red Spot (GRS). Provided everything works as scheduled, one RGB image will be made almost above the center of the GRS. I'd think, that this RGB image will be complemented by a methane image. Since this time, we won't have contact with Earth during the flyby, the amount of data to be collected is rather constraint. Therefore, only a small number of images of the polar region is scheduled, just enough for a long-term observation. Storage will be sufficient for imaging several POIs to be voted for, but we may not get a full latitudinal coverage. In order to obtain a full latitudinal coverage of the GRS and adjacent regions, we should take at least one image near the northern and one image near the southern edge of the GRS, better a set of five RGB images. We would see the GRS from different angles, and we would be able to study the turbulence north and south of the GRS. I'd also expect, that only images from north and south of the GRS will be able to cover most of its longitudinal extent. In addition, a sequence of images near the GRS would provide the raw material for a great and unprecedented fly-over movie. That said, there are several other interesting or potentially interesting targets to consider. Besides for an adjacent region of the GRS, I voted for the two polar-most POIs, since I hope, that we'll get some additional polar and subpolar images for a long-term study, and more close-ups of those incredibly turbulent FFR zones near the poles. |
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Jul 13 2017, 12:41 PM
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Senior Member Group: Members Posts: 2346 Joined: 7-December 12 Member No.: 6780 |
A cylindrical projection of #60 looks like this:
The panorama images I'm usually creating, are projected to spherical coordinates from the perspective of the camera near the time of the exposure, with latitudes of the frame as horizontal axis, and the equator a vertical axis in the horizontal center. This ensures, that the images are about the same resolution as the raws, or some almost constant factor of the raw resolution. Any significant deviation from this projection distorts, enlarges, or reduces the size of the pixels in the raws, resulting in a considerable loss of information, or in excessive supersampling, both in the same image. The horizontal fov of the above spherical projections is 60 degrees. Ther vertical fov is up to 180 degrees. JunoCam looks from horizon to horizon, from only a small altitude compared to Jupiter's diameter. |
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