Special Issues at Low Frequencies:
Ionosphere
Gravity effects on observations
Due to first and second derivative of TEC
Very dependent on geometry: maximum when line of sight is
along wave fronts, small when perpendicular to wavefronts, or //B.
Typical image motion +/- 1 arcmin at 169 MHz, typical timescale:
30 mn.
 At least 10x in worst conditions (+ some image distorsion)
10x less at nightime.
Focusing may occur at low frequencies, exceptionnal cases up to
50 MHz at low elevation.