A distinct negative leader propagation mode

Abstract The common phenomenon of lightning still harbors many secrets such as what are the conditions for lightning initiation and what is driving the discharge to propagate over several tens of kilometers through the atmosphere forming conducting ionized channels called leaders. Since lightning is...

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Main Authors: O. Scholten, B. M. Hare, J. Dwyer, N. Liu, C. Sterpka, I. Kolmašová, O. Santolík, R. Lán, L. Uhlíř, S. Buitink, A. Corstanje, H. Falcke, T. Huege, J. R. Hörandel, G. K. Krampah, P. Mitra, K. Mulrey, A. Nelles, H. Pandya, J. P. Rachen, T. N. G. Trinh, S. ter Veen, S. Thoudam, T. Winchen
Format: Article
Language:English
Published: Nature Publishing Group 2021-08-01
Series:Scientific Reports
Online Access:https://doi.org/10.1038/s41598-021-95433-5
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spelling doaj-cf9ed01604704320a54a252ce959fc832021-08-15T11:28:03ZengNature Publishing GroupScientific Reports2045-23222021-08-0111111110.1038/s41598-021-95433-5A distinct negative leader propagation modeO. Scholten0B. M. Hare1J. Dwyer2N. Liu3C. Sterpka4I. Kolmašová5O. Santolík6R. Lán7L. Uhlíř8S. Buitink9A. Corstanje10H. Falcke11T. Huege12J. R. Hörandel13G. K. Krampah14P. Mitra15K. Mulrey16A. Nelles17H. Pandya18J. P. Rachen19T. N. G. Trinh20S. ter Veen21S. Thoudam22T. Winchen23Kapteyn Astronomical Institute, University GroningenKapteyn Astronomical Institute, University GroningenDepartment of Physics and Astronomy, University of New HampshireDepartment of Physics and Astronomy, University of New HampshireDepartment of Physics and Astronomy, University of New HampshireDepartment of Space Physics, Institute of Atmospheric Physics of the Czech Academy of SciencesDepartment of Space Physics, Institute of Atmospheric Physics of the Czech Academy of SciencesDepartment of Space Physics, Institute of Atmospheric Physics of the Czech Academy of SciencesDepartment of Space Physics, Institute of Atmospheric Physics of the Czech Academy of SciencesDepartment of Astrophysics/IMAPP, Radboud University NijmegenDepartment of Astrophysics/IMAPP, Radboud University NijmegenDepartment of Astrophysics/IMAPP, Radboud University NijmegenAstrophysical Institute, Vrije Universiteit BrusselDepartment of Astrophysics/IMAPP, Radboud University NijmegenAstrophysical Institute, Vrije Universiteit BrusselAstrophysical Institute, Vrije Universiteit BrusselAstrophysical Institute, Vrije Universiteit BrusselErlangen Center for Astroparticle Physics, Friedrich-Alexander-Univeristät Erlangen-NürnbergAstrophysical Institute, Vrije Universiteit BrusselAstrophysical Institute, Vrije Universiteit BrusselDepartment of Physics, School of Education, Can Tho UniversityNetherlands Institute for Radio Astronomy (ASTRON)Department of Physics, Khalifa UniversityAstrophysical Institute, Vrije Universiteit BrusselAbstract The common phenomenon of lightning still harbors many secrets such as what are the conditions for lightning initiation and what is driving the discharge to propagate over several tens of kilometers through the atmosphere forming conducting ionized channels called leaders. Since lightning is an electric discharge phenomenon, there are positively and negatively charged leaders. In this work we report on measurements made with the LOFAR radio telescope, an instrument primarily build for radio-astronomy observations. It is observed that a negative leader rather suddenly changes, for a few milliseconds, into a mode where it radiates 100 times more VHF power than typical negative leaders after which it spawns a large number of more typical negative leaders. This mode occurs during the initial stage, soon after initiation, of all lightning flashes we have mapped (about 25). For some flashes this mode occurs also well after initiation and we show one case where it is triggered twice, some 100 ms apart. We postulate that this is indicative of a small (order of 5 km $$^2$$ 2 ) high charge pocket. Lightning thus appears to be initiated exclusively in the vicinity of such a small but dense charge pocket.https://doi.org/10.1038/s41598-021-95433-5
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language English
format Article
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author O. Scholten
B. M. Hare
J. Dwyer
N. Liu
C. Sterpka
I. Kolmašová
O. Santolík
R. Lán
L. Uhlíř
S. Buitink
A. Corstanje
H. Falcke
T. Huege
J. R. Hörandel
G. K. Krampah
P. Mitra
K. Mulrey
A. Nelles
H. Pandya
J. P. Rachen
T. N. G. Trinh
S. ter Veen
S. Thoudam
T. Winchen
spellingShingle O. Scholten
B. M. Hare
J. Dwyer
N. Liu
C. Sterpka
I. Kolmašová
O. Santolík
R. Lán
L. Uhlíř
S. Buitink
A. Corstanje
H. Falcke
T. Huege
J. R. Hörandel
G. K. Krampah
P. Mitra
K. Mulrey
A. Nelles
H. Pandya
J. P. Rachen
T. N. G. Trinh
S. ter Veen
S. Thoudam
T. Winchen
A distinct negative leader propagation mode
Scientific Reports
author_facet O. Scholten
B. M. Hare
J. Dwyer
N. Liu
C. Sterpka
I. Kolmašová
O. Santolík
R. Lán
L. Uhlíř
S. Buitink
A. Corstanje
H. Falcke
T. Huege
J. R. Hörandel
G. K. Krampah
P. Mitra
K. Mulrey
A. Nelles
H. Pandya
J. P. Rachen
T. N. G. Trinh
S. ter Veen
S. Thoudam
T. Winchen
author_sort O. Scholten
title A distinct negative leader propagation mode
title_short A distinct negative leader propagation mode
title_full A distinct negative leader propagation mode
title_fullStr A distinct negative leader propagation mode
title_full_unstemmed A distinct negative leader propagation mode
title_sort distinct negative leader propagation mode
publisher Nature Publishing Group
series Scientific Reports
issn 2045-2322
publishDate 2021-08-01
description Abstract The common phenomenon of lightning still harbors many secrets such as what are the conditions for lightning initiation and what is driving the discharge to propagate over several tens of kilometers through the atmosphere forming conducting ionized channels called leaders. Since lightning is an electric discharge phenomenon, there are positively and negatively charged leaders. In this work we report on measurements made with the LOFAR radio telescope, an instrument primarily build for radio-astronomy observations. It is observed that a negative leader rather suddenly changes, for a few milliseconds, into a mode where it radiates 100 times more VHF power than typical negative leaders after which it spawns a large number of more typical negative leaders. This mode occurs during the initial stage, soon after initiation, of all lightning flashes we have mapped (about 25). For some flashes this mode occurs also well after initiation and we show one case where it is triggered twice, some 100 ms apart. We postulate that this is indicative of a small (order of 5 km $$^2$$ 2 ) high charge pocket. Lightning thus appears to be initiated exclusively in the vicinity of such a small but dense charge pocket.
url https://doi.org/10.1038/s41598-021-95433-5
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