Solar heat is acurately focused at a fixed point fron sunrise to sunset. It is relatively very simple to reproduce and also very easy to operate. For daily tracking of the sun, a very efficient, cheap- inbuilt electronic system has been created that operates at voltages as low as 3V. The seasonal movements of the sun between the tropics has also been perfectly taken care of through a provision for simple manual adjustments. In equatorial regions the model will have two focal points: the north focal point (March to September) and the south focal point (September to March) to increase efficiency with sun`s movements across Equator. For field installations, a survey tool has been designed to facilitate apropriate geographical orientations. All these achievements have been made almost single-h