A customer operates a rooftop ground station for S-band LEO downlinks in the 2200–2290 MHz space-operations band. The reflector is a KTI/SAMI SI 10: a 10 ft (3.05 m) aluminium mesh dish from Judsonia, Arkansas, built in the US home-satellite era. The original installation manual came with it: prime focus, focal length 45 5/8 in (1159 mm), f/D 0.38. It was built for C-band TV at 4 GHz, so the mesh is a solid reflector at 2.2 GHz. The dish sits on an az/el rotator and follows LEO passes.


The task was the feed. The IceConeFeed is designed for 2.4 GHz and an offset dish; for this installation we built a customised unit tuned to 2200 MHz (IceConeFeed Customized, 2200–2500 MHz on request), with the turn count chosen to illuminate a deep prime-focus reflector: at f/D 0.38 the rim sits 67° off axis seen from the feed. Measured before shipping: SWR < 1.1 at 2200 MHz.

Mechanically the feed drops into the original SAMI feed plate. A 3D-printed adapter plate (PETG) carries the IceConeFeed base and bolts to the four SAMI studs; the N connector faces the rear of the plate, where a short pigtail runs into the black cylinder behind the feed. That cylinder is a radome housing the LNA and band filters right at the feed, so the noise figure is set before the long coax down the mount.




The dish slewing in elevation on its az/el mount:
If you have an old C-band mesh dish and want to use it for S-band or L-band satellite work: the geometry is the same problem, and we tune the feed to your frequency. Get in touch.
