Samenvatting
Energetic cosmic rays impinging on the atmosphere create a particle
avalanche called an extensive air shower. In the leading plasma of this
shower electric currents are induced that generate coherent radio wave
emission that has been detected with LOFAR, a large and dense array of
simple radio antennas primarily developed for radio-astronomy
observations. Our measurements are performed in the 30-80 MHz frequency
band. For fair weather conditions the observations are in excellent
agreement with model calculations. However, for air showers measured
under thunderstorm conditions we observe large differences in the
intensity and polarization patterns from the predictions of fair weather
models. We will show that the linear as well as the circular
polarization of the radio waves carry clear information on the magnitude
and orientation of the electric fields at different heights in the
thunderstorm clouds. We will show that from the measured data at LOFAR
the thunderstorm electric fields can be reconstructed. We thus have
established the measurement of radio emission from extensive air showers
induced by cosmic rays as a new tool to probe the atmospheric electric
fields present in thunderclouds in a non-intrusive way. In part this
presentation is based on the work: P. Schellart et al., Phys. Rev. Lett.
114, 165001 (2015).
Originele taal-2 | English |
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Tijdschrift | EGU General Assembly |
Volume | 18 |
Status | Published - 1-apr.-2016 |
Evenement | EGU General Assembly 2016 - Vienna, Austria Duur: 17-apr.-2016 → 22-apr.-2016 http://www.egu2016.eu |