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Paper detail

First results of the CROME experiment

It is expected that a radio signal in the microwave range is produced in the atmosphere due to molecular bremsstrahlung initiated by extensive air showers. The CROME (Cosmic-Ray Observation via Microwave Emission) experiment was built to search for this microwave signal. Radiation from the atmosphere is monitored in the extended C band (3.4--4.2 GHz) in coincidence with showers detected by the KASCADE-Grande experiment. The detector setup consists of several parabolic antennas and fast read-out electronics. The sensitivity of the detector has been measured with different methods. First results after half a year of data taking are presented.

preprint2011arXivOpen access
R. SmidaH. BluemerR. EngelA. HaungsT. HuegeK. -H. KampertH. KlagesM. KleifgesO. KroemerS. MathysJ. RautenbergM. RiegelM. RothF. SalamidaH. SchielerJ. StasielakM. UngerM. WeberF. WernerH. WilczynskiJ. Wochele
hep-exphysics.ins-detastro-ph.HE
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R. SmidaH. BluemerR. EngelA. HaungsT. HuegeK. -H. KampertH. KlagesM. KleifgesO. KroemerS. MathysJ. RautenbergM. RiegelM. RothF. SalamidaH. SchielerJ. StasielakM. UngerM. WeberF. WernerH. WilczynskiJ. Wochele

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