The authors study the radiation intensity produced by a monoenergetic electron in circular motion as a function of the distance to the orbit. The analysis is carried out along two directions, namely in the radial direction, and along the tangent to the orbit. They find that, near the orbit, the intensity of radiation in the radial direction differs significantly from the value given in Schott's (1912) formula. Together with an increase of the radiation intensity as one moves closer to the orbit, the angular spread of the radiation decreases. As a result, a focusing effect of the radiation in the orbit plane is obtained. In particular, when radiation is detected almost touching the electron orbit, all the electron radiation tends to be concentrated into a line, giving rise to a very high density of energy per unit area. Except for points very close to the tangential point, they show that the intensity of radiation in the forward direction is given by Schwinger's (1949) formula, independent of the distance to the tangential point.