The distance that a station could transmit depended on the size of the shutters and the power of the telescope being used to observe them. The smallest object visible to the human eye is one that subtends an angle of 40 seconds of arc, but Edelcrantz used a figure of 4 minutes of arc to account for atmospheric disturbances and imperfections of the telescope. On that basis, and with a 32X telescope, Edelcrantz specified shutter sizes ranging from 9 inches () for a distance of 0.5 Swedish miles () to 54 inches () for 3 Swedish miles (). These figures were for the original design with square shutters. The open design of 1809 had long oblong shutters which Edelcrantz thought was more visible. Distances much further than these would require impractically high towers to overcome the curvature of the Earth as well as large shutters. Edelcrantz kept the distance between stations under 2 Swedish miles () except where large bodies of water made it unavoidable.