WWLL Network Global Lightning Locations


World Wide Lightning Location Network (wwlln.net)

wwlln.net/new where you will find amazing an amazing new visualization of global lightning
(which works on modern versions of Firefox, Google Chrome and IE 11 or higher.)

WWLLN backup webserver http://dudwlln.otago.ac.nz/
Global Lightning Climatology with amazing movies!.
Volcano global monitor Explosive Ash Cloud Monitor, updated every minute.
and most importantly: WWLLN Publications: peer reviewed publications.
Google Earth overlay for 1 hour of global data ending 6 hours ago is found HERE .

Contact Prof. Holzworth at bobholz@washington.edu , Director of WWLLN, with any questions you may have.

Americas Lightning

Americas Lightning

Americas Lightning

Americas Lightning

- click on image to get a bigger version -
(Notes: cloud data thanks to National Weather Service/Aviation Weather Center; blue overlay dots are WWLLN Lightning; Red circles are WWLLN receivers; Red line is the terminator)

University of Washington in Seattle operating a network of lightning location sensors at VLF (3-30 kHz). Most ground-based observations in the VLF band are dominated by impulsive signals from lightning discharges called “sferics”. Significant radiated electromagnetic power exists from a few hertz to several hundred megahertz, with the bulk of the energy radiated at VLF.

With our network of sferic sensors we are producing regular maps of lightning activity over the entire Earth. Our map showing the entire world uses coloured spots to indicate lightning strokes (red stars inside an open circle are active WWLLN lightning sensor locations).  Click on the map for explanation.

The WWLLN Management Team, lead by Prof Robert Holzworth of the University of Washington produced these data and images with the cooperation of the universities and institutes which host the stations as listed below.

Wideband VLF spectrograms from all WWLLN stations are available this link or by clicking on the station name below.
We currently have over 50 sensors around the globe to detect sferic activity in the VLF band, listed below in the order of their establishment:

Dunedin and ScottBase

University of Otago/Te Whare Wānanga o Otāgo (New Zealand)


Griffith University, Brisbane


Murdoch University, Perth


National University of Singapore


Ōsaka University


Eotvos Lorand University


University of Washington


Massachusetts Institute of Technology

Durban and Hermanus and SANAE Base

University of KwaZulu-Natal (South Africa)

Sao Paulo

INPE (Brazilian National Institute for Space Research)


University of the South Pacific (Fiji)

Los Alamos

Los Alamos National Laboratory

Mexico City

Universidad Nacional Autonoma de Mexico


Universite de la Polynesie Francaise

Tel Aviv

Tel Aviv University


University of Sheffield


Portugal Meteorological Institute


Instituto Geofisico del Peru

Puerto Rico

University of Puerto Rico, Mayaguez


Universidad Nacional de Cordoba (Argentina)


SodankyaGeophysical Observatory, Sodankyla, Finland


University of Hawaii at Manoa


British Antarctic Survey


Cold and Arid Regions Environmental and Engineering Research Insitute, Chinese Academy of Sciences

Ascension Is.

British Geological Survey and BAS

Kingston and Davis

Australian Antarctic Division


Hermanus Magnetic Observatory and University of KwaZulu-Natal (South Africa)

Boulder and Fairbanks

USGS/Magnetic Observatories (USA)


Dept. of Atmospheric and Oceanic Sciences (USA)

Costa Rica

Center for Geophysical Research (CIGEFI), University of Costa Rica (Costa Rica)



Yu.G. Shafer Institute of Cosmophysical Research and Aeronomy


Beijing and Nanjing

Chinese Academy of Sciences


Scott Base

Antarctica New Zealand, Host: U. Otago, Dunedin, NewZealand



Florida State University, Department of Meteorology 



INPA (Brazilian National Institute for Amazon Research) - LBA Program, Manaus, Brazil 



Universite de la Reunion, La Reunion Island (Indian Ocean), France 



CONICET, RioGallegos, Argentina 



Antarctic station host NCAOR, Goa, India 



Univ. of Electro-Communications, Chofu-city, Tokyo, Japan 



Departamento de Fisica, Universidad Nacional de la Patagonia, Trelew, Argentina 



University Cheikh Anta Diop of Dakar (SENEGAL) 



Ebonyi State University Abakaliki Nigeria 



Michigan Technological University(MTU), Houghton, Michigan 



Laboratório de Análise e Processamento de Imagens de Satélites (LAPIS)  



Institute of Cosmophysical Research and Radio Wave Propagation, Russian Academy of Sciences 



Valparaiso University, Indiana  



Egypt-Japan University of Science and Technology (E-Just), Egypt 



Mullard Space Science Laboratory, Surrey, UK 



University of Valencia, Valencia, Spain






How it works

We welcome offers of hosting a new WWLLN sensor to add to the list above. All hosts receive all the world-wide data for their own research on monthly CDs. In return, each host provides the computer and meets any local expenses like power, Internet, and maintenance.  However, do not think that a sensor on your own campus is going to give you lightning location data on its own. Only the whole network does that.

Each lightning stroke location requires the time of group arrival (TOGA) from a least 5 WWLLN sensors. These sensors may be several thousand km distant from the stroke. The geographical  arrangement  of the sensors is important: a lightning stroke which is enclosed by sensors is much more accurately located than one which is not so enclosed. Clearly a uniform spacing of sensors around the Earth is the ideal. Since the Earth is round, there are no edges: every lightning stroke is surrounded by sensors, but not necessarily by the sensors which sense it. Typically only about 15 to 30% of strokes detected  by one sensor are detected by 5 or more. These strokes are usually the stronger ones. Recent research indicates our detection efficiency for strokes about 30 kA is approximately 30% globally.

To cover the whole world by sensors spaced uniformly about 1000 km apart would require roughly 500 sensors. If spaced 3000 km apart, we would need “only” around 50 to 60 sensors. Presently we have 40 WWLLN sensors, and we are in the process of expanding to 60 sensors within the next year or two.

More information


More information on the World Wide  Lightning Location network (WWLLN) is available from our publication list

WWLLN Data available
WWLLN Monthly CDs containing all stroke locations over the whole world for 1 month. These are mailed to subscribers each month, or they may opt to download the data weekly. Archival data are available for sale from August 15, 2004 to the present. Our site hosts receive a free monthly subscription.

WWLLN Data are available via internet with cadence every 10 minutes for research purposes from the University of Washington, or with a cadence of as fast as every minute (i.e. in realtime) from our commercial reseller. Contact Prof. Holzworth for more info.


for all questions relating to WWLLN:
Prof Robert Holzworth, Earth and Space Sciences,
University of Washington


Webpage maintained by:
Craig J Rodger (
University of Otago)
Robert Holzworth (
University of Washington)

Lightning image thanks to photolib.noaa.gov

link to noaa photo library
Web editing:
Bob Holzworth (bobholz@washington.edu)