T. N. G. Trinh, O. Scholten, R. van Loon, B. M. Hare, J. D. Assink, S. Bouma, S. Buitink, A. Corstanje, S. Cummer, M. Desmet, J. Dwyer, H. Falcke, J. R. Hörandel, T. Huege, N. Karastathis, G. K. Krampah, P. Laub, N. Liu, M. Lourens, K. Mulrey, A. Nelles, H. Pandya, C. Sterpka, K. Terveer, S. Thoudam, P. Turekova, S. ter Veen
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引用次数: 0
Abstract
The LOw Frequency ARray (LOFAR) radio telescope possesses the unique capability to measure ultra-high energy cosmic rays as well as image lightning discharges. This study presents a comparison between the inferred thunderstorm charge structures derived from cosmic-ray measurements and from lightning flashes. Our results show a basic triple-layered distribution: a positive upper layer, a main negative layer, and a positive lower layer. However, our cosmic-ray measurement shows a bottom-heavy structure, where the charge in the upper positively charged layer is smaller than that in the lower one. This is consistent with practically all lightning observations with LOFAR, showing well-developed negative leader structures at altitudes below those where positive leaders are seen. This is very different from the vast majority of thundercloud charge structures seen around the world.
期刊介绍:
Geophysical Research Letters (GRL) publishes high-impact, innovative, and timely research on major scientific advances in all the major geoscience disciplines. Papers are communications-length articles and should have broad and immediate implications in their discipline or across the geosciences. GRLmaintains the fastest turn-around of all high-impact publications in the geosciences and works closely with authors to ensure broad visibility of top papers.