Abstract
We report on an investigation of the atmospheric electric field during
thunder storm conditions over the core of LOFAR, the Low-Frequency
Array, for 11 events in the period of December 2011 till September 2014
using a non-intrusive detection method based on the detection of radio
emission from cosmic-ray air showers. LOFAR is a software radio
telescope primarily used for astronomy and build from a large number of
simple dipole antennas. The core of LOFAR, where the antenna density is
highest, lies in the northern part of The Netherlands. Energetic cosmic
rays penetrating the atmosphere create a particle avalanche. The
atmospheric electric fields induce electric currents in the plasma at
the front of this avalanche. These currents emit radio waves since their
strength varies as function of distance to the ground. The atmospheric
electric fields can be deduced from the polarization and intensity
pattern of the emitted radio waves in the frequency band of 30-80 MHz as
measured for each cosmic-ray event at LOFAR. Here we report on the
analysis of several events. Most of the events we measure are consistent
with the lower positive charge regions occurring near the 0 isotherm as
determined from GDAS data. We have observed rather large horizontal
component of the electric fields. In some cases where there is clear
triple layered structure while there are also some where only two charge
layers are detected. T.N.G. Trinh, et al., Phys. Rev. D 95, 083004
(2017); arXiv:1703.06008
Original language | English |
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Title of host publication | 20th EGU General Assembly, EGU2018, Proceedings from the conference |
Pages | 9937-9937 |
Number of pages | 1 |
Publication status | Published - 1-Apr-2018 |
Event | 20th EGU General Assembly, EGU 2018 - Vienna, Austria Duration: 4-Apr-2018 → 13-Apr-2018 |
Conference
Conference | 20th EGU General Assembly, EGU 2018 |
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Country/Territory | Austria |
City | Vienna |
Period | 04/04/2018 → 13/04/2018 |