All images are made with a self made CB245 CCD camera, mounted on a 80 mm f/15 refractor. I used oculair projection to enlarge the images. All are processed with unsharp masking. North is on top.
1998
12 Dec 1998
All images have integration times of 0.1 s. The GRS can be seen at the left limb of the planet, as a white spot.
20 Nov 1998
The last image has an integration time of 0.5 s. The other images 0.3 s.
11 Nov 1998
Both images have integration times of 0.2 s. In the first image, you can just see the shadow of the moon Ganymede at the right limb of the planet. At the right of the planet, you can also see Ganymede.
10 Nov 1998
The last image has an integration time of 0.3 s. The other images 0.2 s. You can also see the movement the moon Io.
18 Oct 1998
The second image has an integration time of 0.3 s. The other images 0.2 s. You can clearly see the movement of cloud structures in the atmospheer of Jupiter, caused by it's rotation.
15 Aug 1998
The first image has an integration time of 0.2 s. The other images 0.1 s. In the last image, you can just see the shadow of the moon Io, on the surface of the planet. It's the small dark spot just above the southern belt (a belt is dark and horizontal), at the left side of the planet.
10 Aug 1998
An integration time of 0.2 s was used to make this image. You can just see the GRS (Great Red Spot) at the right limb of the planet. It's a giant storm, as big as the earth, and excists at least for 300 years.
