Inside a radiofrequency cavity, the electric field accelerates electrons (produced by field emission, photo-emission, residual gas ionization, etc) towards the system's chamber wall. Depending on the wall's surface properties and on the electron impacting energy, these primary electrons produce secondary electrons when they hit the chamber wall, which in turn are accelerated if the electric field is at the correct phase. This bouncing back and forth between surfaces is called the electron multipacting, or multipactoring, effect. It was first described by Farnsworth in the 1930's [1]. The name is derived from the term "multiple electron impacts". If the number of emitted electrons per impinging electron, given by the Secondary Electron Yield (SEY) of the wall surface, is greater than unity, the electron density inside the vacuum chamber increases exponentially creating a so-called electron cloud. This usually ends in catastrophic drop in system performance. Depending on the multipacting scenario, the exponential growth is finally limited by the available power and/or space-charge effects. Inside an accelerator's vacuum chamber, or beam pipe, the radiofrequency electric field is provided by the beam, and the effect is often referred to as Beam Induced Multipacting (BIM). In this case, the electron cloud is defined as an accumulation of electrons inside the beam pipe which, if sufficiently strong, can affect the machine performance by increasing the vacuum pressure, producing beam instabilities, causing beam loss and/or interference in beam diagnostics [2]. The proton storage ring of the Budker Institute of Nuclear Physics (BINP, Novosibirsk) in 1965 [3] and the Ion Storage Ring at CERN in 1972 [4] are perhaps the first machines to suffer from electron clouds. In the 1990's, electron clouds were observed in many accelerators with positively charged particles (the PSR at LANL, the PF at KEK, the PEP-II at SLAC, the SPS at CERN, etc), often acting as a fundamental limit to machine performance resulting from the aforementioned effects. These limitations led accelerator scientists to develop complex computer simulation codes that model the circumstances in which the build up of an electron cloud occurs [5]. The phenomenon is quite sensitive to a host of accelerator parameters including beam bunch intensity, beam bunch spacing, beam dimensions, chamber geometry, and properties of the chamber surface material. If a given threshold is crossed, an electron cloud quickly develops or disappears. The least well known property is the SEY dependence on electron energy, especially for low energy electrons [6]. It plays a crucial role because it determines the number of surviving electrons when the electric field is absent, a condition that occurs regularly during the gap between the passage of two consecutive beam bunches. In 2001, after one year of operation, the first attempts to fill the Relativistic Heavy Ion Collider (RHIC) at BNL with intense ion beams resulted in intolerable pressure rises inside the vacuum chamber. These ...