Tunka-Rex - the Tunka Radio Extension
The Tunka Radio Extension (Tunka-Rex) is a 1 km² digital antenna array at the Tunka-133 experiment. While Tunka-133 measures the Cherenkov light of air showers in the energy range up to 1 EeV, Tunka-Rex measures the radio emission of the same air showers. Tunka-Rex started operation on 8 October 2012 with 18 antennas, was extended to 25 antennas in 2013, to 44 antennas in 2014, and has been densified to a total number of 63 antennas in summer 2016. Since 2015 the antennas are triggered additionally by scintillation detectors measuring secondary particles of the air showers on ground. In 2018 data taking for the current science goals has been completed. In 2019, most antennas were dismantaled leaving a few antenna stations for educational as well as R&D purpose. Moreover, the data analysis is expected to continue until at least 2021.
Tunka still a world-wide unique place for performing Cherenkov-Radio hybrid measurements of ultra-high energy cosmic rays. Meanwhile further instruments have been deployed all together forming the Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy (TAIGA). Also in future this site will be available for further developments of the radio technique for cosmic particles.
The original goals of Tunka-Rex have already been fulfilled:
- A cross-calibration of the radio and the Cherenkov signal emitted by air showers. This allows to determine which precision radio measurements have for the energy and mass of the primary cosmic ray particles. A first analysis obtained a reconstruction precision of 15 % for the energy (20 % absolute scale uncertainty) and about 40 g/cm² for the position of the shower maximum. Meanwhile, the precision could be improved to 30 g/cm² by using more sophisticated techniques for data analysis. Consequently, the radio measurements feature approximately the same accuracy as the traditional Cherenkov-light technique.
- Demonstrating that radio antenna arrays allow to cover relatively large areas with a cost-effective and efficient technology for ultra-high energy cosmic rays: Against earlier doubts, the economic construction with SALLA antennas on wooden poles is completely sufficient to achieve the precision mentioned above.
- Enhancing the duty cycle of Tunka by an order of magnitude, since radio measurements are possible during almost any weather conditions, while Cherenkov light measurements of air showers can only be performed during clear and moonless nights: Since end of 2015, day-time operation is achieved by triggering Tunka-Rex with the Tunka extension of scintillators detecting the secondary air-shower particle on ground.
New analysis goal of Tunka-Rex
- Use the increased statistics provided by the joint measurements with the Tunka-Grande scintillators to study the mass composition of cosmic-rays in the energy range above 0.1 EeV. This is crucial to understand the transition from the highest-energy galactic to ultra-high-energy extragalactic cosmic rays.
Tunka-Rex is foreseen to keep its pioneering role in the radio techniques for air showers by developing new analysis methods. Methods for the accurate determination of the cosmic-ray flux and the measurement of the energy spectrum shall be developed. A particular focus will be on a better understanding of the effiency of the radio measurements.
Semi-blind analysis (referring to our paper JCAP 01 (2016) 052)
At the International Cosmic Ray Conference (ICRC 2015) in The Hague, we presented results of the first measurement season (2012/13) on the reconstruction of the energy and the shower maximum. Moreover, we made a prediction of energy and shower maximum for the second season (2013/14) based on the Tunka-Rex radio measurements, while the Tunka-133 air-Cherenkov values still were blinded. The prediction was published in encrypted form before unblinding on the following webpage: http://reco.tunkarex.info/
Copies of the encrypted event lists can be downloaded here for the first season (tuning season) and the second season (prediction season). The password will be published soon in the first paper on these results.
Tunka-Rex antenna station in winter; further Tunka detectors in background: PMT, housing for local data acquisition, and housing for scintillator detectors.