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Radio detection of air showers in the current era has progressed immensely toeffectively extract the properties of these air showers. Primary cosmic rayswith energies of hundreds of PeV have been successfully measured with themethod of radio detection. There are also attempts to observe high-energyneutrinos with this technique. Current radio experiments measuring cosmic-rayair showers mostly operate in the frequency range of 30-80 MHz. An optimizationof the frequency band of operation can be done for maximizing thesignal-to-noise ratio that can be achieved by an array of radio antennas at theSouth Pole, operated along with IceTop. Such an array can improve thereconstruction of air showers performed with IceTop. The prospect of using suchan optimized radio array for measuring gamma rays of PeV energies from theGalactic Center is discussed.

A Surface Radio Array for the Enhancement of IceTop and its Science Prospects