The Initial Stage of Cloud Lightning Imaged in High-Resolution

被引:20
|
作者
Scholten, O. [1 ,2 ,3 ]
Hare, B. M. [1 ]
Dwyer, J. [4 ,5 ]
Sterpka, C. [4 ,5 ]
Kolmasova, I. [6 ,7 ]
Santolik, O. [6 ,7 ]
Lan, R. [6 ]
Uhlir, L. [6 ]
Buitink, S. [8 ,9 ]
Corstanje, A. [8 ,9 ]
Falcke, H. [8 ,10 ,11 ,12 ]
Huege, T. [9 ,13 ]
Horandel, J. R. [8 ,9 ,10 ]
Krampah, G. K. [9 ]
Mitra, P. [9 ]
Mulrey, K. [9 ]
Nelles, A. [14 ,15 ]
Pandya, H. [9 ]
Pel, A. [2 ]
Rachen, J. P. [9 ]
Trinh, T. N. G. [16 ]
ter Veen, S. [11 ]
Thoudam, S. [17 ]
Winchen, T. [12 ]
机构
[1] Univ Groningen, Kapteyn Astron Inst, Groningen, Netherlands
[2] Univ Groningen, KVI Ctr Adv Radiat Technol, Groningen, Netherlands
[3] Vrije Univ Brussel, Interuniv Inst High Energy, Brussels, Belgium
[4] Univ New Hampshire, Dept Phys, Durham, NH 03824 USA
[5] Univ New Hampshire, Space Sci Ctr EOS, Durham, NH 03824 USA
[6] Czech Acad Sci, Inst Atmospher Phys, Dept Space Phys, Prague, Czech Republic
[7] Charles Univ Prague, Fac Math & Phys, Prague, Czech Republic
[8] Radboud Univ Nijmegen, Dept Astrophys IMAPP, Nijmegen, Netherlands
[9] Vrije Univ Brussel, Astrophys Inst, Brussels, Belgium
[10] NIKHEF, Sci Pk Amsterdam, Amsterdam, Netherlands
[11] Netherlands Inst Radio Astron ASTRON, Dwingeloo, Netherlands
[12] Max Planck Inst Radioastron, Bonn, Germany
[13] Karlsruhe Inst Technol KIT, Inst Kernphys, Karlsruhe, Germany
[14] Friedrich Alexander Univ Erlangen Nurnberg, Erlangen Ctr Astroparticle Phys, Erlangen, Germany
[15] DESY, Zeuthen, Germany
[16] Can Tho Univ, Sch Educ, Dept Phys, Campus 2, Can Tho City, Vietnam
[17] Khalifa Univ, Dept Phys, Abu Dhabi, U Arab Emirates
基金
欧洲研究理事会;
关键词
INTRACLOUD;
D O I
10.1029/2020JD033126
中图分类号
P4 [大气科学(气象学)];
学科分类号
0706 ; 070601 ;
摘要
With LOFAR we have been able to image the development of lightning flashes with meter-scale accuracy and unprecedented detail. We discuss the primary steps behind our most recent lightning imaging method. To demonstrate the capabilities of our technique we show and interpret images of the first few milliseconds of two intracloud flashes. In all our flashes, the negative leaders propagate in the charge layer below the main negative charge. Among several interesting features we show that in about 2 ms after initiation the primary initial leader triggers the formation of a multitude (>10) negative leaders in a rather confined area of the atmosphere. From these only one or two continue to propagate after about 30 ms to extend over kilometers horizontally while another may propagate back to the initiation point. We also show that normal negative leaders can transition into an initial leader like state, potentially in the presence of strong electric fields. In addition, we show some initial breakdown pulses that occurred during the primary initial leader, and even during two "secondary" initial leaders that developed out of stepped leaders.
引用
收藏
页数:19
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