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At the GOL-3 facility, experiments on the interaction of powerful hot electron streams with various materials have been performed. For energy densities of the hot electron stream above 10 MJ/m2 an explosive-like erosion was observed, which at energy densities of 30 MJ/m2 reaches 500 mu m for fine grain graphite and 200 mu m for tungsten. Under these conditions, the corona of the carbon vapour cloud has temperatures below 1.2 eV and densities up to 1017 cm-3. It propagates along the magnetic field lines with maximum velocities of 2.1*106 cm/s. The longitudinal and transverse (along and across magnetic field lines) vapour velocities of the colder bulk plasma are about 106 cm/s. A model for explosive-like erosion was developed and tested against the GOL-3 results. For graphite the destruction threshold is 10 kJ/g. This value is considerably lower than the vaporization enthalpy of 20.5 kJ/g for three atomic vaporization. The validated model was applied to a numerical analysis of the occurrence of explosive-like erosion for ITER disruptions and runaway electrons. If the energy density of the runaways remains below 30 MJ/m2, explosive-like erosion of graphite occurs for electron energies below 20 MeV. For the energetic tail of Maxwellian plasma electrons with temperatures up to 20 keV and power densities of 10 MW/cm2 without any angular spread, explosive-like erasion becomes comparable to erosion by vaporization

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