“…In 1966, Chendzey and Hurle grew Te-doped InSb in a horizontal magnetic field and observed that as the field strength was increased, temperature fluctuations in the melt changed from chaotic to periodic variations, and then to stable and steady values [34]. In 1970, Witt and coworkers [35] applied a horizontal (transverse) magnetic field to Czochralski growth of Te-doped InSb. In addition to near elimination of the socalled non-rotational striations that are associated with turbulent melt convection, they observed an amplification of periodic striations caused by rotation of the crystal in an asymmetric thermal field.…”