The nuclei Sn-106 and Sn-108 have been populated using the Fe-54(Ni-58
,alpha 2p) and Fe-54(Ni-58,4p) reactions, respectively, at a beam ener
gy of 243 MeV and the gamma rays have been detected using the Gammasph
ere array. Two ''rotation-like'' structures consisting of magnetic dip
ole transitions have been observed in each of the nuclei. The bands ca
n be interpreted, using the Tilted Axis Cranking model, as examples of
magnetic rotation. The calculations show excellent agreement with the
data for Sn-108. However, for the lighter isotope, Sn-106, the model
is unable to reproduce the experimental B(M1)/B(E2) ratios. Reasons fo
r this discrepancy are discussed. (C) 1998 Elsevier Science B.V. All r
ights reserved.