Lightning Interferometry, attachment, and wind energy
ORAL · Invited
Abstract
Lightning is the largest operating-environment cause of catastrophic blade
failure, and the number of strikes grows supra-linearly with wind turbine height and
rotor diameter. Despite relatively extensive studies of lightning strikes to tall
towers and aircraft, lightning "attachment" is not well understood. Most lightning
strikes begin with a streamer-leader system descending from a thundercloud.
Electric-field-driven streamers feed into higher-current leaders
and heat air to the point of thermal ionization. Prior to a strike, the high E from an
approaching leader causes structures to emit upward streamers (and radio
pulses). When upward streamers intercept the downward leader, a return stroke
occurs. Engineering models of this dynamic process are limited, and for wind-
turbines include wholly inadequate electrostatic field models to evaluate lightning
protection systems. In lightning rod studies, it was learned that a very sharp
point protects itself by creating a cloud of space charge which suppresses
upward streamer emissions. A moving wind turbine blade can outrun the space
charge (corona discharge) that it produces, making it even more vulnerable to lightning than
an equally tall stationary structure.
The suite of lightning research instrumentation has recently been enhanced by the three-dimensional
lightning interferometer. A lightning interferometer is effectively a small
radio telescope optimized to locate up to a million sources per second. Astronomers
measure right ascension and declination and have to infer range. A 3D-lightning
interferometer gets range intrinsically and can thus produce a full X, Y, Z
moving image of lightning flashes with resolution as high as five meters. We hope to
apply a 3D interferometer combined with high-speed video and current measurements
to gain insight into the process of lightning attachment to wind turbines and
further enable this crucial energy source while illuminating a basic question
of lightning science.
We acknowledge Prof. Ashok Ghosh and Sidharth Arunkumar for work on the attachment
problem in the prototype NM Tech spark lab. We thank Paul Clem of Sandia National Labs for helping
obtain funding for the spark lab.
failure, and the number of strikes grows supra-linearly with wind turbine height and
rotor diameter. Despite relatively extensive studies of lightning strikes to tall
towers and aircraft, lightning "attachment" is not well understood. Most lightning
strikes begin with a streamer-leader system descending from a thundercloud.
Electric-field-driven streamers feed into higher-current leaders
and heat air to the point of thermal ionization. Prior to a strike, the high E from an
approaching leader causes structures to emit upward streamers (and radio
pulses). When upward streamers intercept the downward leader, a return stroke
occurs. Engineering models of this dynamic process are limited, and for wind-
turbines include wholly inadequate electrostatic field models to evaluate lightning
protection systems. In lightning rod studies, it was learned that a very sharp
point protects itself by creating a cloud of space charge which suppresses
upward streamer emissions. A moving wind turbine blade can outrun the space
charge (corona discharge) that it produces, making it even more vulnerable to lightning than
an equally tall stationary structure.
The suite of lightning research instrumentation has recently been enhanced by the three-dimensional
lightning interferometer. A lightning interferometer is effectively a small
radio telescope optimized to locate up to a million sources per second. Astronomers
measure right ascension and declination and have to infer range. A 3D-lightning
interferometer gets range intrinsically and can thus produce a full X, Y, Z
moving image of lightning flashes with resolution as high as five meters. We hope to
apply a 3D interferometer combined with high-speed video and current measurements
to gain insight into the process of lightning attachment to wind turbines and
further enable this crucial energy source while illuminating a basic question
of lightning science.
We acknowledge Prof. Ashok Ghosh and Sidharth Arunkumar for work on the attachment
problem in the prototype NM Tech spark lab. We thank Paul Clem of Sandia National Labs for helping
obtain funding for the spark lab.
*This work is funded in part by NSF grant #AGS-1917069 and the New Mexico Consortium at Los Alamos
–
Publication: 1) Production of runaway electrons and x-rays during streamer inception phase, (submitted to Journal of Physics D, Sept 2022)
2) Jensen, D. P., Sonnenfeld, R. G., Stanley, M. A., Edens, H. E., da Silva, C. L., & Krehbiel, P. R. (2021). Dart-leader
and K-leader velocity from initiation site to termination time-resolved with 3D interferometry. Journal of Geophysical Research: Atmospheres, 126, e2020JD034309. https://doi.org/10.1029/2020JD034309
Presenters
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Richard G Sonnenfeld
- New Mexico Tech and Langmuir Lab
- New Mexico Institute of Mining and Techn