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Return-current-driven instabilities of propagating electron beams

Technical Report ·
OSTI ID:7057468
A stability analysis is performed for the first nine transverse modes (azimuthal mode number plus radial mode number < or = 3) of a self-pinched relativistic electron beam propagating in a collisional plasma. Only frequencies omega in the range omega tau sub d << 1 are considered, where tau sub d is the dipole magnetic decay length. For such modes, the presence of plasma return current is the only destabilizing mechanism. Paraxial flow, space charge neutrality, and a flat radial profile of beam density are also assumed. Within these limitations an exact analysis of the linearized Vlasov stability problem is carried out in closed form. For each mode, the instability threshold, growth rate, and conditions for oscillatory vs. pure growth are determined. For beams with a moderate return current fraction, the hose, sausage and axial hollowing modes appear to be particularly dangerous.
Research Organization:
Naval Research Lab., Washington, DC (USA)
OSTI ID:
7057468
Report Number(s):
AD-A-111911/4; NRL-MR-4767
Country of Publication:
United States
Language:
English