Energy and density of ions in vacuum arcs between axial and radial magnetic field contacts

In vacuum circuit breakers, two different contact types are used to overcom e the consequences of arc constriction, which sets in when currents of seve ral kiloamperes are exceeded. Radial magnetic fields (RMF) force the constr icted arc to rotate and distribute its power more evenly on the contact sur face. Axial magnetic field (AMF) contacts prevent the arc from becoming con stricted up to higher thresholds. To improve the interruption capability of vacuum circuit breakers of both types, it is essential to know about the p rocesses and properties of the vacuum plasma ("vacuum arc") around current zero, such as plasma density and its decay and the energy of the plasma spe cies. In this work, the energy distribution of ions in the vacuum arc plasm a during the last 3 ms before current zero has been investigated by means o f a retarding field analyzer up to arc currents of approximate to 9 kA RMS, and significant differences could be observed between RMF and AMF contacts . For currents above 5 kA the distribution in both cases resembles a Maxwel lian distribution, characteristic for a collision-determined plasma. On low er currents, i.e., when current zero is approached, RMF arrangements show i ons with strongly directed motion, while the energy distribution for AMF co ntacts seems to be more influenced by collisions. There are also indication s of the v x B ion rotation in the AMF field. Furthermore, the post-arc cha rge as an indication of the plasma density and its free decay after current zero has been investigated. With AMF contacts, the initial density at curr ent zero lies higher, especially on lower arc currents. The first decay tim e constant grows slightly with the arc current, and lies higher for larger shield diameter, i.e., higher ratio between plasma volume and shield surfac e for recombination.