A precise rime-of-flight method previously developed is used to investigate
the average kinetic energy of an N+ ion cloud. From values obtained for di
fferent points in the Mathieu stability diagram, variation of the kinetic e
nergy versus the corresponding experimental parameters is estimated. It is
observed that the magnitude depends essentially on the smallest two-dimensi
onal component of the three-dimensional potential well. Measurements at dif
ferent radiofrequencies (0.5, 1, and 1.5 MHz) show that the kinetic energy
does not increase with the rf frequency. From the observed temporal variati
on of the kinetic energy, collisional cooling is evidenced. (Int J Mass Spe
ctrom 190/191 (1999) 37-45) (C) 1999 Elsevier Science B.V.