This paper presents the results of JET experiments aimed at the study of the operational space of plasmas with a Type III ELMy edge, in terms of both local and global plasma parameters. In JET, the Type III ELMy regime has a wide operational space in the pedestal ne-Te diagram, and Type III ELMs are observed in standard ELMy H-modes as well as in plasmas with an Internal Transport Barrier (ITB). The transition from an H-mode with Type III ELMs to a steady state Type I ELMy H-modes requires a minimum loss power, PTypeI•PTypeI decreases with increasing plasma triangularity. In the pedestal ne-Te diagram, the critical pedestal temperature for the transition to Type I ELMs is found to be inversely proportional to the pedestal density (Tcrit ∝ 1/n) at low density. In contrast, at high density Tcrit does not depend strongly on density. In the density range where Tcrit ∝ 1/n, the critical power required for the transition to Type I ELMs decreases with increasing density. Experimental results are presented suggesting a common mechanism for Type III ELMs at low and high collisionality. A single model for the critical temperature for the transition from Type III to Type I ELMs, based on the resistive interchange instability with magnetic flutter, fit well the density and toroidal field dependence of the JET experimental data. On the other hand, this model fails to describe the variation of the Type III ne-Te operational space with isotopic mass and q95. Other results are instead suggestive of a different physic for Type III ELMs. At low collisionality, plasma current ramp experiments indicate a role of the edge current in determining the transition from Type III to Type I ELMs while at high collisionality, a model based on resistive ballooning instability well reproduces, in term of a critical density, the experimentally observed q95 dependence of the transition from Type I to Type III ELMs. Experimental evidence common to Type III ELMs in standard ELMy H-modes and in plasma with ITB indicates that they are driven by the same instability.