  The 2dF Galaxy Redshift Survey is the first to measure more than 100,000
redshifts. This allows precise measurements of many of the key statistical
measures of galaxy clustering, in particular redshift-space distortions and the
large-scale power spectrum. This paper presents the current 2dFGRS results in
these areas. Redshift-space distortions are detected with a high degree of
significance, confirming the detailed Kaiser distortion from large-scale infall
velocities, and measuring the distortion parameter beta = 0.43 +/- 0.07. The
power spectrum is measured to < 10% accuracy for k > 0.02 h Mpc^-1, and is well
fitted by a CDM model with Omega_m h = 0.20 +/- 0.03 and a baryon fraction of
0.15 +/- 0.07.
