Makoto Adachi (Drawing: 310mm Newtonian)
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≪滋賀県 大津市 安達 誠≫
Dr. P. Clay Sherrod (410mm SC : ToUcam PRO)
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A couple of images from March 29, the earlier one showing the GRS exiting the pr. limb
but lots of interesting activity; I am noting an increased separation of the two major
delineations of the SEB at this time, particularly noted beginning about 20 degrees behind
the activity of the GRS; the most turbulent area by far seen in these two images is that
associated with the current of the NEBsouth, the EZnorth and perhaps within the North
Equatorial Belt ZONE itself.
Note the great predominance of reddish features: the n. component of the SEB is strongly
defined in red for many degrees fol. the GRS, as is the curving s. component of this belt;
both subside some distance from the GRS active area. In addition, note the very strong
segemented portion of the NEBs, the segmentation appearing to be the result of perhaps
higher or more dominant brighter features than the belt itself. The reddish features are
best defined in the blue image of each of these two images, showing about 20 degrees of
rotation....
[Dr. P. Clay Sherrod Arkansas State U.S.A]
Christopher Go (Celestron C8:Toucam webcam)
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Here's my latest image of Jupiter with the GRS transiting. Seeing was around 7/10 with transparency at around 3/5. I had to image through mist. I just have one request, can someone send me the System II Longitude of the GRS? The time I am using is mid time of my exposure. If you want more accurate timing please let me know so I can send this to you. These are 130sec exposures so if you want shorter exposure, I can process these for you.
[Christopher Go : Cebu Philippines]
Ferruccio Zanotti ( 450mm Newtonian : webcam Philips ToUcam pro)
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