LUMINOSITY CHARACTERISTICS OF DART LEADERS AND RETURN STROKES IN NATURAL LIGHTNING

Citation
Dm. Jordan et al., LUMINOSITY CHARACTERISTICS OF DART LEADERS AND RETURN STROKES IN NATURAL LIGHTNING, JOURNAL OF GEOPHYSICAL RESEARCH-ATMOSPHERES, 102(D18), 1997, pp. 22025-22032
Citations number
24
Categorie Soggetti
Metereology & Atmospheric Sciences
Volume
102
Issue
D18
Year of publication
1997
Pages
22025 - 22032
Database
ISI
SICI code
Abstract
Streak-camera photographs were obtained in daylight for 23 subsequent strokes in five Florida negative cloud-to-ground flashes. Out of the 2 3 return-stroke streaked images, only 11 were accompanied by leader st reaked images, while all 23 leaders were identified in corresponding e lectric field records. Thus, 12 subsequent leaders (one of which creat ed a new channel to ground) failed to produce luminosity above the day light background level. The brightest three dart-leader/return-stroke sequences from two flashes have been examined for relative light inten sity as a function of time and height. Dart-leader light waveforms app ear as sharp pulses with 20-to-80 % risetimes of about 0.5-1 mu s and widths of 2-6 mu s followed by a more or less constant light level (pl ateau). The plateau continues until it is overridden by the return-str oke light waveform, suggesting that a steady leader current flows thro ugh any channel section behind the downward moving leader tip before t he return-stroke front has passed that channel section. Return-stroke light pulses near ground have 20-to-80 % risetimes of about 1-2 mu s a nd amplitudes a factor of 2 to 3 greater than those of the dart-leader light pulses. As opposed to the return-stroke light pulses that suffe r appreciable degradation during the upward propagation of the return- stroke front, the dart-leader light pulses preserve their shape, and t he pulse amplitude is either more or less constant or increases as the leader approaches ground. The average electric field intensity across the dart-leader front, whose length is inferred from measured light-p ulse risetimes and propagation speed to be of the order of 10 m, shoul d be at least an order of magnitude greater than the average electric field intensity across the return-stroke front, whose length is inferr ed to be of the order of 100 m.