Employing a magnetic field to limit the divergence of ion trajectories
in isochronous time-of-flight spectrometers can improve the detection
s efficiency and thereby reduce the background if compared to the alre
ady realized instrument CYLMAS. The time-of-flight section can be comb
ined with a toroidal entrance system and sectorized pixel array detect
ors to yield a 360-degrees field-of-view spectrometer. The sectorizati
on of such an instrument to be flown on a spinning spacecraft allows a
complete mapping of the velocity distribution of the investigated par
ticles and it leads to a further reduction of the counting background
and a significant improvement of the mass resolution.