The Australian National University
Research School of Earth Sciences
SHRIMP

SHRIMP RG

The reverse geometry SHRIMP is based on ion optical designs by Matsuda (1990) to minimize third-order aberrations. The design of the SHRIMP RG yields approximately four times the mass resolution for the same slit sizes compared to SHRIMP II.

SHRIMP RG was completed in 1997 however it was apparent that the instrument was not performing as well as it should. The voltages on the electrostatic quadrupole lenses were very different to the theoretical voltages and good peak shapes could only be obtained by severely limiting the beam divergence. After lengthy examination of the input parameters it was found that the RG electrostatic lenses were clamping the beam too hard and were not consistent with the expectation of Matsuda’s design. Following the re-design of the lenses, the voltages for the quadupole lenses were close to theoretical and high mass resolution could be readily obtained.

 

 

Figures: (upper) the new quadrupole lens structure (right) allows the fringe field of the lenses to expand beyond the physical pole pieces. The old style supports (left) utilized end supports that clamped the electroic field resulting in lenses that were effectively too short. In addition to the lenses, the chambers were also modified with end caps added that increased the distance from the lenses to the chamber walls (below).

 

High resolution scan ranging from mass resolution 5,000 to mass resolution 20,000.

 

Mass scan of mass 207 showing partial resolution of 206PbH from 207Pb at mass resolution 30,000

Mass scan at mass 182 showing separation of the 182W peak from ErO.