The global electrostatic mode in pair-ion plasmas is discussed for cylindric geometry and for a radially inhomogeneous equilibrium density. In the case of a Gaussian radial density profile, exact analytical eigensolutions are found in terms of the Kummer confluent hypergeometric functions. The mode is identified as a convective cell propagating in the poloidal and axial direction, having at the same time a standing wave structure in the radial direction. © 2008 American Institute of Physics. ͓DOI: 10.1063/1.2907160͔A new research field and a new area of increasing scientific activity have emerged recently after a series of experiments [1][2][3][4] in which a pure pair-ion plasma has been produced; i.e., a plasma without electrons. The two ions, i.e., C 60 Ϯ , are produced in a simultaneous process of impact ionization and electron attachment, and further collected by a magnetic filtering effect; i.e., by a diffusion in the radial direction ͑perpendicular to the magnetic field lines͒. Being separated from electrons, the ions are then collected in a narrow and elongated chamber ͑90 cm long and with a diameter of 8 cm͒. In Refs. 2-4, several types of modes have been reported in such plasmas; viz., the ion plasma wave, the ion acoustic wave ͑IAW͒, and the so-called intermediate frequency wave. The detailed measurements presented in the most recent Refs. 3 and 4, reveal that the IAW actually has two separate branches, and is accompanied by some additional backward propagating mode between these two branches. Some features of the experimentally observed modes still remain unexplained. These experimental works have been followed by numerous studies, 5-14 dealing with various aspects of linear and nonlinear waves and instabilities in pair-ion plasmas. In addition to this, the recent successful production of a pairhydrogen plasma, 4 which is even more attractive because of the small ion mass and the obvious consequences related to this, indicates that the number of experiments and analytical studies in this particular field will grow even further. The topic is interesting also in view of the fact that a similar pair plasma, comprising much lighter particles ͑electrons and positrons͒ in the past years has also been created under laboratory conditions. 15 The knowledge of processes in such plasmas will help us to understand the physics of some pairplasmas in space, comprising electrons and positrons, as in the atmospheres of pulsars and in active galactic nuclei, and even in flares in the lower solar atmosphere.So far, studies dealing with waves and instabilities 5-14 have been carried out mainly in the framework of a local mode analysis and in Cartesian geometry. However, the experimental conditions mentioned above 1-4 are such that, in some domains of frequencies and wavelengths, the proper cylindric geometry is to be used and the effects of the plasma boundary on the modes are to be taken into account. Therefore, in the present work we shall focus on frequencies below the ion gyrofrequency, on the effect of radial densi...