  We describe an analysis of the time-resolved measurements of the surface
magnetic field in the roAp star gamma Equ. We have obtained a high-resolution
and high S/N spectroscopic time-series, and the magnetic field was determined
using Zeeman resolved profiles of the Fe II 6149.25 A and Fe I 6173.34 A lines.
Contrary to recent reports we do not find any evidence of magnetic variability
with pulsation phase, and derive an upper limit of 5-10 G for pulsational
modulation of the surface magnetic field in gamma Equ.
