High-speed video observations of the fine structure of a natural negative stepped leader at close distance

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Abstract

We present new high-speed video observations of a natural downward negative lightning flash that occurred at a close distance of 350 m. The stepped leader of this flash was imaged by three high-speed video cameras operating at framing rates of 1000, 10,000 and 50,000 frames per second, respectively. Synchronized electromagnetic field records were also obtained. Nine pronounced field pulses which we attributed to individual leader steps were recorded. The time intervals between the step pulses ranged from 13.9 to 23.9 μs, with a mean value of 17.4 μs. Further, for the first time, smaller pulses were observed between the pronounced step pulses in the magnetic field derivative records. Time intervals between the smaller pulses (indicative of intermittent processes between steps) ranged from 0.9 to 5.5 μs, with a mean of 2.2 μs and a standard deviation of 0.82 μs. A total of 23 luminous segments, commonly attributed to space stems/leaders, were captured. Their two-dimensional lengths varied from 1 to 13 m, with a mean of 5 m. The distances between the luminous segments and the existing leader channels ranged from 1 to 8 m, with a mean value of 4 m. Three possible scenarios of the evolution of space stems/leaders located beside the leader channel have been inferred: (A) the space stem/leader fails to make connection to the leader channel; (B) the space stem/leader connects to the existing leader channel, but may die off and be followed, tens of microseconds later, by a low luminosity streamer; (C) the space stem/leader connects to the existing channel and launches an upward-propagating luminosity wave. Weakly luminous filamentary structures, which we interpreted as corona streamers, were observed emanating from the leader tip. The stepped leader branches extended downward with speeds ranging from 4.1 × 105 to 14.6 × 105 m s-1.

Figures

  • Table 1 Characteristics of negative stepped leaders that involved space stems/leaders based on high-sp
  • Fig. 1.High-speed video images (HC-1) of the descending negative stepped leader and the return stroke of F1213. Time 0 corresponds to the onset of the return stroke. Frames a and b are consecutive frames that were 120 μs and 20 μs prior to the return stroke onset, respectively. Frame c shows the return stroke channel 780 μs after the beginning of the return stroke. In the FOV of HC-1, the vertical extent of the lightning channel was approximately 170 m. Some of the luminous segments (space stems/leaders) are indicated by arrows.
  • Fig. 2.Variations of the electric field (top andmiddle panels) andmagneticfield (bottompanel), the common time scale. The full time scale is 200 μs. Time 0 corresponds to the onset of the re
  • Fig. 3. (a) Electric field and (b) magnetic field derivative waveforms (with noise reduced using a wavelet transform) showing step pulses P1, P2 and P3 in Fig. 2, displayed on a 40-μs time scale. The smaller pulses occurring between the step pulses are marked with vertical arrows.
  • Fig. 4. (a) Magnetic field derivative waveform of the stepped leader obtained by differentiatin (b) The same magnetic field derivative waveform with noise reduced using a wavelet transfor
  • Fig. 5. Histogram of the time intervals between the peaks of the 52 smaller pulses occurring between the step pulses P1 to P9. The 7 time intervals that cross the step pulses were not included in this histogram.
  • Fig. 6. Intensity-inverted images of the descendingnegative stepped leader that is shown in Fig. in the paper.
  • Fig. 7.High-speed video (HC-2) images (inverted) of the descending negative stepped leader (a to g) and part of the return-stroke channel (h). Images a to g are consecutive frames from −140 μs to−20 μs, and image h shows part of the return-stroke channel, 600 μs after its onset. Six luminous segments are labeled 3 to 8, and three less luminous formations (streamers) that are associated with the space stems/leaders are labeled 1, 2 and 9 (for example, streamer 9 is associated with space stem/leader 3).

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APA

Qi, Q., Lu, W., Ma, Y., Chen, L., Zhang, Y., & Rakov, V. A. (2016). High-speed video observations of the fine structure of a natural negative stepped leader at close distance. Atmospheric Research, 178179, 260–267. https://doi.org/10.1016/j.atmosres.2016.03.027

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