Determining atmospheric electric fields through radio emission from air showers

被引：0
|
作者：
Trinh, Gia [1 ]
Scholten, Olaf [1 ,2 ]
Ebert, Ute [3 ,4 ]
Leijnse, Hidde [5 ]
Rutjes, Casper [3 ]
机构：
[1] Univ Groningen, KVI Ctr Adv Radiat Technol, POB 72, NL-9700 AB Groningen, Netherlands
[2] Vrije Univ Brussel, Interuniv Inst High Energy, Pl Laan 2, B-1050 Brussels, Belgium
[3] Ctr Math & Comp Sci CWI, POB 94079, NL-1090 GB Amsterdam, Netherlands
[4] Eindhoven Univ Technol TU E, Dept Appl Phys, POB 513, NL-5600 MB Eindhoven, Netherlands
[5] KNMI, Dutch Meteorol Serv, Utrechtseweg 297, NL-3731 GA De Bilt, Netherlands
来源：
8TH INTERNATIONAL CONFERENCE ON ACOUSTIC AND RADIO EEV NEUTRINO DETECTION ACTIVITIES (ARENA 2018) | 2019年 / 216卷
关键词：
RADIATION;
D O I：
10.1051/epjconf/201921603010
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
During thunderstorm conditions the radio footprint (intensity as well as polarization) of cosmic ray showers deviates strongly from those measured during fair weather. We have been able to interpret this pattern in terms of atmospheric electric fields. We see that even when there is no thunderstorm activity within 100 km distance within an hour of the event, the radio footprint may be strongly affected.
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页数：3
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