Towards Remote Lightning Manipulation by Meters-long Plasma Channels Generated by Ultra-Short-Pulse High-Intensity Lasers.


Journal

Scientific reports
ISSN: 2045-2322
Titre abrégé: Sci Rep
Pays: England
ID NLM: 101563288

Informations de publication

Date de publication:
23 Jan 2019
Historique:
received: 31 05 2018
accepted: 20 11 2018
entrez: 25 1 2019
pubmed: 25 1 2019
medline: 25 1 2019
Statut: epublish

Résumé

Remote manipulation (triggering and guiding) of lightning in atmospheric conditions of thunderstorms has been the subject of intense scientific research for decades. High power, ultrashort-pulse lasers are considered attractive in generating plasma channels in air that could serve as conductors/diverters for lightning. However, two fundamental obstacles, namely the limited length and lifetime of such plasma channels prevented their realization to this date. In this paper, we report decisive experimental results of our multi-element broken wire concept that extends the generated plasma channels to the required tens of meters range. We obtain 13-meter-long plasma wire, limited only by our current experimental setup, with plasma conditions that could be sufficient for the leader initiation. This advance, coupled with our demonstrated method of laser heating for long time sustenance of the plasma channel, is a major, significant step towards controlling lightning.

Identifiants

pubmed: 30674944
doi: 10.1038/s41598-018-36643-2
pii: 10.1038/s41598-018-36643-2
pmc: PMC6344589
doi:

Types de publication

Journal Article

Langues

eng

Pagination

407

Références

Opt Lett. 2002 May 1;27(9):772-4
pubmed: 18007928
Phys Rev Lett. 2008 Apr 18;100(15):155003
pubmed: 18518116
Opt Express. 2008 Apr 14;16(8):5757-63
pubmed: 18542684
Opt Express. 2006 Jun 12;14(12):4946-57
pubmed: 19516654
Opt Express. 2007 Mar 19;15(6):2779-84
pubmed: 19532515
Opt Lett. 1995 Jan 1;20(1):73-5
pubmed: 19855801
Opt Express. 2012 Jun 4;20(12):12721-8
pubmed: 22714301
Opt Express. 2013 Nov 4;21(22):26836-45
pubmed: 24216905
Sci Rep. 2017 Jan 05;7:40063
pubmed: 28053312

Auteurs

Jenya Papeer (J)

Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, 91904, Israel. Evgeny.papeer@mail.huji.ac.il.

Indranuj Dey (I)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Moti Botton (M)

Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, 91904, Israel.

Zohar Henis (Z)

Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, 91904, Israel.

Amit D Lad (AD)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Moniruzzaman Shaikh (M)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Deep Sarkar (D)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Kamalesh Jana (K)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Sheroy Tata (S)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Sudipta Lodh Roy (SL)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Yash M Ved (YM)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

G Ravindra Kumar (GR)

Tata Institute of Fundamental Research, 1 Homi Bhabha Road, Colaba, Mumbai, 400005, India.

Arie Zigler (A)

Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem, 91904, Israel.

Classifications MeSH