Observations and modeling of lightning leaders
By P. Lalande, A. Bondiou-Clergerie, G. Bacchiega, I. Gallimberti. 2002
137 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Computational Mechanics, Global and Planetary Change
View Paper: https://www.semanticscholar.org/paper/e71d9ad5207c70111e978bce05ecfb604309ed93
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In Astronomy and Astrophysics
- Martin A. Uman
- Joseph R. Dwyer
- M. Becerra
- Vernon Cooray
- Earle Williams
- David M. Smith
- V. Pasko
- S. Cummer
In Computational Mechanics
In Global and Planetary Change
Citations in the corpus
- The physics of lightning (2014, background): “, [161,200,208,209]], but are up to two orders of magnitude less than the peak currents (on average 1.”
- Problems in lightning physics—the role of polarity asymmetry (2006, background): “It is interesting to note that during early (∼1996) video camera/ELF comparisons, a substantial fraction (5–10%) of all TLEs without corresponding NLDN-identified positive ground flashes was also tentatively identified as ‘elves’. In retrospect, some of these events could have been haloes instead an”
- A simplified physical model to determine the lightning upward connecting leader inception (2006, methodology): “[18] computed a value of 65 C/m for based on the triggered lightning experiments.”
- A self-consistent upward leader propagation model (2006, methodology): “relaxation time τvt is taken as 100 μs [22] and the value of the constant K is set in such a way that the value of qL computed with (5) is equal to 65 μC m−1 [29] when the leader velocity reaches 2 × 104 m s−1.”