2014
DOI: 10.1002/2014gl062127
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Burst of intracloud current pulses during the initial continuous current in a rocket‐triggered lightning flash

Abstract: For a rocket-triggered lightning flash on 2 August 2013, the measurement with one pair of broadband low-frequency (20-400 kHz) magnetic induction coils registered a long sequence of over 600 intermittent pulses during the initial continuous current. The timescale of these pulses is about 3-8 μs, and the typical interpulse interval is about 30 μs. The source discharges of these pulses, which are not readily detectable in the frequency range (140-300 MHz) of a short-baseline very high frequency (VHF) lightning i… Show more

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Cited by 29 publications
(35 citation statements)
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“…Though no correlation was observed between the pulses of current and VHF radiation, they presumed a stepwise propagation of the positive leader. Referring to the same event, Lu et al () correlated the azimuthal position of the source of magnetic pulses (time correlated with the measured pulses of current at the beginning of the ICC) with that of the tip of the positive leader, as inferred from the VHF radiation field. Note that no conclusions about stepped propagation could have been derived from the observations of VHF radiation, since both continuous and stepped developing leaders are sources of VHF radiation pulses.…”
Section: Discussion On Specific Features Of Upward Leaders In Naturalmentioning
confidence: 99%
See 1 more Smart Citation
“…Though no correlation was observed between the pulses of current and VHF radiation, they presumed a stepwise propagation of the positive leader. Referring to the same event, Lu et al () correlated the azimuthal position of the source of magnetic pulses (time correlated with the measured pulses of current at the beginning of the ICC) with that of the tip of the positive leader, as inferred from the VHF radiation field. Note that no conclusions about stepped propagation could have been derived from the observations of VHF radiation, since both continuous and stepped developing leaders are sources of VHF radiation pulses.…”
Section: Discussion On Specific Features Of Upward Leaders In Naturalmentioning
confidence: 99%
“…Though no correlation was observed between the pulses of current and VHF radiation, they presumed a stepwise propagation of the positive leader. Referring to the same event, Lu et al (2014) correlated the azimuthal position of the source of magnetic pulses (time correlated with the measured pulses of current at the beginning of the ICC) with that of the tip of the positive leader, as inferred from the VHF radiation field.…”
Section: The Propagation Mode Of Upward Positive Leadersmentioning
confidence: 99%
“…Continuing current (CC) is defined as the relatively low-level current lasting for tens to hundreds of milliseconds that immediately follows a return stroke (RS) in both natural flashes (Kitagawa et al, 1962;Rakov & Uman, 1990) and triggered flashes (W. Lu et al, 2011;Saba et al, 2016). In order to distinguish from CC, the term initial continuous current is used, which follows an upward positive leader that occurred before a RS in the initial stage in both rocket-triggered (Fisher et al, 1993;G. Lu et al, 2015) and object-initiated lightning (Flache et al, 2008;Miki et al, 2005).…”
Section: Introductionmentioning
confidence: 99%
“…Figure shows one example of typical channel‐base current waveform acquired (with a 5 mΩ shunt) for a rocket‐triggered lightning flash (as examined in details by Sun et al [] and Lu et al []) in SHandong Artificially Triggered Lightning Experiment (SHATLE) during the summer campaign in 2013. As shown in the figure, the minimum magnitude of current pulses measured at the channel base is approximately 8 A, and the data are not appropriate for resolving even smaller‐current pulses that have been reported in the literature [e.g., Willett et al ., ; Lalande et al ., , ; Ngin et al ., ].…”
Section: Introductionmentioning
confidence: 99%