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The Crab pulsar experienced a major flare in 2010 as observed by Fermi LAT.Observations by the Hubble Space Telescope indicate that the flare wasaccompanied by a structural change in the anvil region of the Crab Nebula. Inthe framework of a photometric analysis we reconstruct the energetics of thisevent. Reconnection zones near the light cylinder are expected to releaseenergy by accelerating beams of electrons, leading to flares of varyingamplitude. In this case the major flare would have reduced the magnetic energystored in the reconnection zones, and would thus have had an impact on theproperties of the giant radio flares presumably originating from these regions.We test this scenario by observing giant radio pulses with the WesterborkSynthesis Radio Telescope.

A new interpretation of Giant radio pulses from the Crab pulsar