Links to some PJ25, part1 renditions:
- http://junocam.pictures/gerald/uploads/20200219/,
- http://junocam.pictures/gerald/uploads/20200219a/,
- http://junocam.pictures/gerald/uploads/20200219b/,
- http://junocam.pictures/gerald/uploads/20200219c/.
Btw, here is a crop #002 to a presumed partial eclipse of one of the moons:
One of the anticyclones between the northern CPCs and the north polar cyclone is well-resolved this time. Here a blink showing its rotation, as well as that of some of the CPCs:
Found the Chalybes Regio plume at top of PJ25-1. Cranked the brightness, found another candidate but not convinced that's what it is.
This is a mosaic of images PJ25_25 and PJ25_27 rendered from Juno's position when it was acquiring image PJ25_27. Approximately true color/contrast and enhanced versions:
Jupiter - Here Be Dragons...
PJ25_24 Eichstadt / Doran
https://flic.kr/p/2ixoaL9
Detail...
https://flic.kr/p/2ixyCGd
For some reason, I'm loving the views of the South Equatorial Belt in this perijove. Nice and clear overview shots with tons of eddies and turbulence. I just wish Juno could get the GRS from this perspective...
https://flic.kr/p/2iya3re
https://flic.kr/p/2iya3re
https://flic.kr/p/2iy3D3h
https://flic.kr/p/2iy3D3h
https://flic.kr/p/2ixEHhU
https://flic.kr/p/2ixEHhU
Beautiful!
Images obtained with JunoCam's methane filter can be used to estimate the relative altitudes of Jupiter's clouds. Features that appear bright in the methane images are high in the atmosphere whereas darker features are located at lower altitudes.This is an experimental anaglyph created by using image PJ25_26 (a methane image) to generate a digital elevation model (DEM) of Jupiter's clouds. A slightly enhanced version of image PJ25_25 (a normal color image) was then draped over the DEM. This turned out way better than I expected. Here it is assumed that the cloud altitudes are a linear function of brightness in the methane image. This assumption is not accurate but is nevertheless good enough to result in a nice DEM and anaglyph. Elevation differences are exaggerated. As expected, the resulting image shows that bright features tend to be higher in the atmosphere than dark features. Red-blue glasses are needed to view this image properly.
I like it- nice job!
John
The long and narrow haze bands often seen at high northern latitudes are especially conspicuous in the PJ25 images. I recently saw a Landsat 8 image that might be of peripheral interest when looking at JunoCam's images of Jupiter's haze bands. I'm attaching a montage showing JunoCam image PJ25_18 at left and the Landsat image at right.
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