An Update on the Charaterictics of Positive Flashes Recorded on the Santis Tower

被引:0
|
作者
Azadifar, M. [1 ]
Paolone, M. [2 ]
Pavanello, D. [3 ]
Rachidi, F. [1 ]
Rakov, V. A. [4 ]
Romero, C. [1 ]
Rubinstein, M. [5 ]
机构
[1] Swiss Fed Inst Technol, EMC Lab, CH-1015 Lausanne, Switzerland
[2] Swiss Fed Inst Technol, DESL, CH-1015 Lausanne, Switzerland
[3] Univ Appl Sci Western Switzerland, Sion, Switzerland
[4] Univ Florida, Dept Elect & Comp Engn, Gainesville, FL USA
[5] Univ Appl Sci Western Switzerland, IICT, Yverdon, Switzerland
来源
2014 INTERNATIONAL CONFERENCE ON LIGHTNING PROTECTION (ICLP) | 2014年
关键词
positive lightning; upward flashes; Santis Tower;
D O I
暂无
中图分类号
TM [电工技术]; TN [电子技术、通信技术];
学科分类号
0808 ; 0809 ;
摘要
We present an update on the characteristics of positive flashes recorded on the Santis Tower in Switzerland from May 2010 to January 2013, during which period 38 positive flashes were recorded. Out of the 38 recorded flashes, 1 was identified as a normal downward flash, 5 were classified as type-1 flashes (characterized by a large unipolar impulse) and the rest of the flashes (32) were classified as type-2 flashes (characterized by a slow waveform with superimposed pulse train). We present a summary of the characteristics of the lightning current parameters for type-1 and type-2 flashes separately and for both types combined. We also present a comparison between the present results corresponding to type-1 flashes and Berger et al.'s data for flashes with large impulsive currents. A similar comparison is presented between type-2 flashes in this study and Berger et al.'s data for flashes without large impulsive currents. In the latter comparison, the most significant differences between the two datasets are in the peak current and the amount of transferred charge, both of which are substantially larger in our type-2 flash dataset. We finally present a discussion of the oscillatory pulse trains in type-2 flashes. Our data are found to be, in general, consistent with those observed at the Gaisberg tower. However, the overall leader pulse duration and the individual pulse duration observed at Santis are higher than their counterparts at Gaisberg.
引用
收藏
页码:777 / 781
页数:5
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