The resolution of single-and double-stage, homogeneous electric mirror time-of-flight mass spectrometers can be calculated with the derived formulae for detectors located normally to the ion flight direction or parallel to the mirror face. These formulae account for contributions to the peak width from ion initial velocity and position in the source ('turn around' time included), from ion-packet longitudinal and transverse size at the source h a l grid, as well as due to the angular ion spread. Third-order terms are included for beam size, angular aperture and velocity spread, the incidence angle being small. The field-free space needed to obtain energy focusing in time is connected with the length of the accelerating space inside the source.Since the first use of electrostatic mirrors,' their theory has been developed by Gohl et al.,' the resolution of time-of-flight mass spectrometers employing this device being increased to 35Formulae to calculate resolution for single-and double-stage homogeneous electric-field mirror reflectrons have been previously derived in Ref. 4. The second-order components of the detected ion-packet length were accounted for, oblique incidence being assumed. However, flight time inside the ion source and the initial velocity effect (leading to the so-called 'turn around' time) were disregarded. They apply for detectors located parallel to the mirror face.Perturbative effects of the slightly tilted grids or detectors have been simulated by Riggi.' The resolution limitations introduced by wire meshes were calculated in Refs 6 and 7. The results obtained are difficult to include in an analytical resolution formula.The flight time inside the accelerating gap of a singlefield ion source has been given in Ref. 8. Recently, second-order fringing field effects were calculated for single-stage electrostatic mirrors.' A fringing field with plane symmetric structure was assumed, that is unusual for reflectrons.Because in two-stage electrostatic mirror time-offlight mass spectrometers the second-order time aberration coefficient of the energy spread is cancelled, the third-order term becomes relevant. Also cross terms may contribute significantly to the detected packet length.We derive third-order resolution formulae and compare, for various source types and mass spectrometer geometries, the resolution values obtained when thirdorder terms are accounted for and also when they are neglected.
FLIGHT TIMESThe flight time, t, through a homogeneous electric field may be calculated with the formulae of Ref. 10 rewritten in the form: t = (ud-uzi)ml(eE) where m , e, uzi, uZf are respectively the ion mass, its electric charge, the velocity components along the direction of the electric field (E), at the ion entry and exit, h being the distance between the field-limiting planes (Fig. 1). E is positive if ions are accelerated. When E < 0 and uzf= 0, Eqn (1) gives half of the 'turn around' time of ions in that field.We define: (1) the source reference plane, located in the ionization region normal to the ion-...