2018•2018 2nd URSI Atlantic Radio Science Meeting (AT-RASC)Requires access
The First Observations of Type I and III Radio Bursts with LOFAR Station in Bałdy
Bartosz Da̧browski, D. E. Morosan, R. A. Fallows, Leszek Błaszkiewicz, Andrzej Krankowski, Jasmina Magdalenić, C. Vocks, G. Mann, Pietro Zucca, Tomasz Sidorowicz, Kacper Kotulak, Adam Froń, Karolina Śniadkowska
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Abstract
The LOw-Frequency ARray (LOFAR) telescope is a radio interferometer, arranged in 51 stations across Europe. The LOFAR maximum baseline in the N - S direction is 1294 km (between the Onsala - Nançay stations) and in the E - W is 1887 km (between the Bałdy - Birr stations). The telescope operates in the frequency range 10 to 240 MHz. Each station consists of two antenna fields: (i) LBA (Low Band Antennas) antennas, operating in frequency range of 10-90 MHz and (ii) HBA (High Band Antennas) antennas operating in frequency range of 110-250 MHz. Details about construction and operating the LOFAR telescope can be found in [2].