Guan Yunong, Lü Weitao, Qi Qi, et al. Difference between 2D and 3D development characteristics of an upward lightning leader. J Appl Meteor Sci, 2023, 34(5): 598-607. DOI:  10.11898/1001-7313.20230508.
Citation: Guan Yunong, Lü Weitao, Qi Qi, et al. Difference between 2D and 3D development characteristics of an upward lightning leader. J Appl Meteor Sci, 2023, 34(5): 598-607. DOI:  10.11898/1001-7313.20230508.

Difference Between 2D and 3D Development Characteristics of an Upward Lightning Leader

DOI: 10.11898/1001-7313.20230508
  • Received Date: 2023-02-08
  • Rev Recd Date: 2023-05-25
  • Publish Date: 2023-09-30
  • Tall object not only has a high probability of being struck by downward lightning, but also is easy to trigger upward lightning. Comparing with 2D optical observation, reconstructed 3D observation by dual-station optical observation can better reflect the real characteristics of the lightning channel. Based on the synchronous dual-station optical observations from the Tall-Object Lightning Observatory in Guangzhou (TOLOG), an upward lightning triggered by a nearby positive cloud-to-ground (CG) flash at Guangzhou Tower is investigated, and 2D and 3D development characteristics of the upward leader are compared.The result shows that the length of 3D channel is 5.4 km, which is 1.5 times of 2D channel. 3D channel is developed at a height of more than 4.6 km in the vertical direction and about 800 m in the horizontal direction. 2D speed ranges from 1.8×104 to 4.5×105 m·s-1, with an average of 1.8×105 m·s-1. 3D speed ranges from 3.8×104 to 7.2×105 m·s-1, with an average value of 2.8×105 m·s-1. Within 10 ms after the leader initiation, 3D and 2D speeds show roughly the same trend. After 10 ms, 2D rate decreases significantly and changes little over time, while 3D speed shows an obvious irregular fluctuation with time. The ratio of 3D speed and 2D speed ranges from 1 to 4.7, with an average of 1.5. The ratio remains stable at 1-2 for the first 10 ms after leader initiation and then shows irregular fluctuations with time. In fact, due to the change of horizontal development direction of the channel 10 ms after the leader initiation, the distance between the channel and the station-1 increases rapidly, leading to increasing speed difference between 3D and 2D observations. The cause for the fluctuation of 3D speed and 2D speed ratio is that the angle between the development direction of the channel and the sight direction of the observation station changes greatly. The results of 2D and 3D vary greatly at a certain stage of upward leader development, which further proves the importance of analyzing 3D development characteristics of lightning.
  • Fig. 1  Waveforms of changes in fast electric field(a) and image brightness(b)

    Fig. 2  Positions of Canton Tower relative to ground termination points of positive cloud-to-ground flash, station-1 and station-2

    Fig. 3  2D leader speed change with time(a) and change with height(b) of FA19014

    Fig. 4  Upward lightning images captured by HC-1 at station-1(a) and LCI-03 at station-2(b)

    (images are inverted and pixel values of lightning channel in images are enhanced for better display)

    Fig. 5  reconstruction channel of FA19014 and projection view on X-Y plane(a),X-Z plane(b) and Y-Z plane(c)

    Fig. 6  3D speed changes with time(a) and with height(b) of FA19014

    Fig. 7  3D speed,2D speed and their ratio change with time of FA19014

    Fig. 8  Differences in velocity between 3D and 2D

    (a)actual ratio of 3D speed and 2D speed versus theoretical values of ratio, (b)changes of actual and theoretical ratio with time, (c)relative position of 3D reconstruction channel and station-1 in space (grey channel denotes huge difference between 3D and 2D speed), (d)changes of d1 and φ with ime

    Table  1  Details of optical observation instruments in the study

    设备编号 观测站点 帧率/s-1 空间分辨率 记录时长/ms 预触发时长/ms 焦距/mm
    HC-1 观测点1 20000 1024 × 1024 50 25 14
    HC-3 观测点1 1000 1024 × 1024 1650 150 8
    LCI-03 观测点2 50 780 × 582 5
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    • Received : 2023-02-08
    • Accepted : 2023-05-25
    • Published : 2023-09-30

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