Abstract-The origin of ultrahigh-energy cosmic rays (UHECRs)(E ≥ 10 17 eV) is a fundamental question of astroparticle physics. The induced shower of secondary particles in the atmosphere of the Earth provides essential information on the cosmic ray itself: arrival direction, primary energy, and mass. In the air shower many electrons and positrons form a pancakeshaped particle front with a typical thickness less than 1 m close to the shower axis to more than 10 m far from the shower axis The geomagnetic field induces a drift velocity in these particles which is perpendicular to the direction of the initial cosmic ray. The generated current is a source of coherent emission of electromagnetic waves at wavelengths larger than the size of the dimension of the charge cloud i.e., for radio frequencies in the range of 30-300 MHz.The radio technique allows a detail study of the electromagnetic part of an air shower in the atmosphere and provide information complementary to that obtained by surface detectors water Cherenkov tanks, which are predominantly sensitive to the muonic content of an air shower at the ground. One of the promising attempts to observe UHECRs by the detection of their coherent radio emission is a wavelet trigger based on a FPGA.The paper presents first laboratory results from the twodimensional wavelet trigger, implemented into the prototype Front-End Board developed for the Auger surface detector based on the Cyclone R V FPGA 5CEFA9F31I7. The wavelet trigger investigates a distribution of partial power contributions for two Fourier indices, simultaneously in time and frequency domains. Preliminary results are very promising and show that the wavelet trigger could improve a radio detection system