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We present a multiwavelength study of recurrent surges observed in H{\alpha},UV (SOHO/EIT) and Radio (Learmonth, Australia) from the super-active regionNOAA 10484 on 25 October, 2003. Several bright structures visible in H{\alpha}and UV corresponding to subflares are also observed at the base of each surge.Type III bursts are triggered and RHESSI X-ray sources are evident with surgeactivity. The major surge consists of the bunches of ejective paths forming afan-shape region with an angular size of (\approx 65\degree) during its maximumphase. The ejection speed reaches upto \sim200 km/s. The SOHO/MDI magnetogramsreveal that a large dipole emerges east side of the active region on 18-20October 2003, a few days before the surges. On October 25, 2003, the majorsunspots were surrounded by "moat regions" with moving magnetic features(MMFs). Parasitic fragmented positive polarities were pushed by the ambientdispersion motion of the MMFs and annihilated with negative polarities at theborders of the moat region of the following spot to produce flares and surges.A topology analysis of the global Sun using PFSS shows that the fan structuresvisible in the EIT 171 A images follow magnetic field lines connecting thepresent AR to a preceding AR in the South East. Radio observations of type IIIbursts indicate that they are coincident with the surges, suggesting thatmagnetic reconnection is the driver mechanism. The magnetic energy released byreconnection is transformed into plasma heating and provides the kinetic energyfor the ejections. A lack of a radio signature in the high corona suggests thatthe surges are confined to follow the closed field lines in the fans. Weconclude that these cool surges may have some local heating effects in theclosed loops, but probably play a minor role in global coronal heating and thesurge material does not escape to the solar wind.

Observations of Multiple Surges Associated with Magnetic Activities in AR10484 on 25 October 2003