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2021 ◽  
Vol 9 ◽  
Author(s):  
Wang Yanhui ◽  
Fan Xiangpeng ◽  
Wang Tuo ◽  
Min Yingchang ◽  
Liu Yali ◽  
...  

In this work, we studied the waveforms of all lightning discharges from about 15 min. Eighty-three percent of all lightning discharges contain particular waveforms called regular pulse bursts (RPBs), which have regular microsecond-scale electric or magnetic field pulses. Maximum proportion of RPBs occur in middle or rear of lightning discharges. Prior to or after RPBs, there is always a chaotic pulse period. The analysis indicated that RPBs are caused by a secondary discharge in the fractured old breakdown channel, likeness to dart-stepped leader occuring in negative cloud-to-ground discharge (-CG). Four types of RPBs, namely, category of normal RPBs, category of back RPBs, category of symmetric RPBs, and category of reversal RPBs, were sorted in the light of the evolution of the pulse amplitude, interval between neighboring pulses and pulse polarity. In addition, the difference between normal RPBs and back RPBs was considered to be caused by the distance between neighboring charge pockets and the magnitude of the charge in every charge pocket. The symmetric RPBs were considered to be caused by a discharge channel with a large central charge area. Reversal RPBs were considered to be caused by a bending channel or superposition of two or more RPBs. We located some RPBs in a typical intra-cloud flash (IC) in three-dimensional. The analysis showed that the developing velocity of RPBs ranged from approximately 1.2 × 106 m/s to 3.0 × 106 m/s, which slower less than both of the dart leader or dart-stepped leader process from previous studies. And we found it is several meters to dozens of meters that the lengths range of discharge step which between two adjacent pulses.


2021 ◽  
Vol 19 (1) ◽  
pp. 102-103
Author(s):  
M. Weinberg

The authors report a peculiar disease, hitherto not described in the literature, observed in one asylum of r. Mlheimer'a. in Germany. The disease was clinically expressed by nausea, vomiting, dizziness, ptosis, diplopia, absence of pupil response to light and their dilation, Babinski's symptom, paraesthesias, nasal speech, difficulty in swallowing, cyanosis, Cheyne-Stokes breathing with good, regular pulse and normal temperature.


2020 ◽  
Vol 17 (3) ◽  
pp. 2516-2529
Author(s):  
Juan Palomares-Ruiz ◽  
◽  
Efrén Ruelas ◽  
Flavio Muñoz ◽  
José Castro ◽  
...  
Keyword(s):  

Atmosphere ◽  
2019 ◽  
Vol 10 (3) ◽  
pp. 141
Author(s):  
Sankha Nanayakkara ◽  
Mahendra Fernando ◽  
Vernon Cooray

General characteristics of K-changes, including their duration and probability of occurrence associated with ground flashes in Sri Lanka in the tropics, together with their fine structure, are presented. In 98 ground flashes where the small step changes associated with K-changes are clearly visible, there were about two K-changes per flash on average. The mean K-change time duration observed in this study is 0.38 ms. In 53 of the ground flashes, there were 120 consecutive K-changes. In these cases, the geometric mean of the time interval between K-changes was 12 ms. Analysis of the fine structure of the K-changes reveals the K-changes are always associated with either a chaotic pulse train or a combination of chaotic and regular pulse trains. The results suggest that the small step-like static electric fields identified in the literature as K-changes are the step-like static fields associated with the processes that generate chaotic or a combination of chaotic and regular pulse trains. Thus, at larger distances where the static fields are negligible, K-changes may appear as a chaotic pulse train or a combination of chaotic and regular pulse trains.


Author(s):  
Sankha Nanayakkara ◽  
Mahendra Fernando ◽  
Vernon Cooray

General characteristics of K changes together with their fine structure associated with ground flashes in Sri Lanka in the tropics are presented. It is found that on average there are about 2 K changes associated with each return stroke. Analysis of the fine structure of the K changes shows that the K change is a chaotic pulse burst. Some of these chaotic pulse bursts start and the others end as a regular pulse bursts. Sometimes the chaotic part occurs in between two regular pulse bursts. This is in agreement with the recent published results that claim that chaotic pulse bursts are a random superposition of regular pulse bursts. The results show that the small step fields identified in the literature as K changes are the static fields associated with these pulse bursts.


2016 ◽  
Vol 24 (6) ◽  
pp. 431-432 ◽  
Author(s):  
B. Bellmann ◽  
C. Gemein ◽  
P. Schauerte
Keyword(s):  

2016 ◽  
Vol 24 (6) ◽  
pp. 435-437
Author(s):  
B. Bellmann ◽  
C. Gemein ◽  
P. Schauerte
Keyword(s):  

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