We have studied the isothermal, magnetic field (H parallel to c) depen
dent rf power P(H) dissipation (H(rf)parallel to a) in the superconduc
ting state of Bi2Sr2CaCu2O8 single crystals prior to and after irradia
tion with 250 MeV Ag-107(17+) ions. In the pristine state, P(H) shows
an initial decrease with increase in field, reaches a minimum at H-M(T
) and increases monotonically for H>H-M(T). This behavior arises when
the electromagnetic coupling between the pancake vortices in adjacent
CuO layers becomes dominant on increasing the field and minimizes the
distortions of the flux lines by confining the 2D vortices. In the pos
t irradiated state, such an initial decrease and the minimum in P(H) i
s not observed but only a much reduced rf dissipation that monotonical
ly increases with held from H=0 onwards is seen. We attribute this dif
ference to the strong enhancement of the tilt modulus C-44 Of the flux
lines on irradiation when the pancake vortices in adjacent CuO bilaye
rs are pinned along the track forming a well-stacked flux line in the
field direction (parallel to c) We have also observed that the rf diss
ipation disappears at a certain temperature T-sf, at which the normal
core of the flux line becomes commensurate with the columnar track dia
meter. (C) 1998 American Institute of Physics.