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This paper presents multiwavelength observations of a flare-generated type IIradio burst. The kinematics of the shock derived from the type II closely matcha fast EUV wave seen propagating through coronal arcade loops. The EUV wave wasclosely associated with an impulsive M1.0 flare without a related coronal massejection, and was triggered at one of the footpoints of the arcade loops inactive region NOAA 12035. It was initially observed in the AIA 335 \AA\ imageswith a speed of ~800 km/s and accelerated to ~1490 km/s after passing throughthe arcade loops. A fan-spine magnetic topology was revealed at the flare site.A small, confined filament eruption (~340 km/s) was also observed moving in theopposite direction to the EUV wave. We suggest that breakout reconnection inthe fan-spine topology triggered the flare and associated EUV wave thatpropagated as a fast shock through the arcade loops.

Flare Generated Shock Wave Propagation Through Solar Coronal Arcade Loops and Associated Type II Radio Burst