FORTE CID Peak Current
FORTE Compact Intra-cloud Discharge Detection Parameterized by
Peak Current
M J Heavner,
D. M. Suszcynsky, A. R. Jacobson, B. D. Heavner, and
D A Smith
LAUR-02-5759
Conclusions/Summary
This study was motivated by the VLF NBE amplitude thresholding
in the GPS/LASA lightning observations. We have examined
FORTE/VHF lightning observations and do not find a similar
threshold effect. Any minor threshold effect is probably masked
by other physical effects--possibly non-isotropic CID/NBE
radiation, or a lack of any strong VLF/VHF power relationship.
The large number of VLF NBE events which FORTE/VHF `missed' have
many large amptidue VLF NBE events, indicating that additional
physical insight into the CID process is needed to understand
the discrepency between VLF and VHF observations.
Future Directions
The data set presented here is biased towards Florida thunderstorms.
Efforts towards studying more storm types are underway, including the
recent participation in a Brazilian lightning campaign. This study
began with LASA/VLF NBE observations and looked for matching and
missed FORTE/VHF events. A complimentary study of FORTE/VHF TIPPs
while in view of LASA is currently underway.
Bibliography
[1] K. L. Cummins, et al, NLDN peak current estimates - 1996 update,
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[4] D. A. Smith, et al., The Los
Alamos Sferic Array: Ground truth for the FORTE
satellite, J. Geohpys. Res., 2000.H4
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The Los Alamos Sferic Array: A research tool for lightning
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JGR, 107(D13):10.1029/2001JD000502, 2002.
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Radiation field and current of the lightning stepped leader.
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Acknowledgements
This study was possible due to the hard work of the FORTE team.
This research was supported by the Department of Energy. Ryan
Woodard and Laura Peticolas contributed to software development.
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