NAMMA Lightning ZEUS Data Table of Contents
The NAMMA Lightning ZEUS data are provided by World-ZEUS Long Range Lightning Monitoring Network. The NASA Science Mission Directorate funded the Zeus network to provide lightning detection and location observations in the African continental and maritime region during the NAMMA experiment. This network has been funded by the National Science Foundation (Water Cycle Program), with joint support by the Hellenic General Secretariat for Research and Development, Univeristy of Nevada, State University of Ceara, University of Sao Paulo and Companhia de Energia Eletrica do Estado do Ceara. Lightning data is obtained from "sferics" (Very low frequency radio receivers), located at thirteen ground stations spread across the European and African continents and Brazil. Lightning activity occurring over a large part of the globe is continuously monitored at varying spatial accuracy (e.g. 10-20 km within and >50 km outside the network periphery) and high temporal resolution (1 msec). Time is determined by the Arrival Time Difference (ATD) between the time series from pairs of the receivers. CampaignThese data files were generated during support of the NASA African Monsoon Multidisciplinary Analyses (NAMMA) campaign, a field research investigation sponsored by the Science Mission Directorate of the National Aeronautics and Space Administration (NASA). This mission was based in the Cape Verde Islands, 350 miles off the coast of Senegal in west Africa. Commencing in August 2006, NASA scientists employed surface observation networks and aircraft to characterize the evolution and structure of African Easterly Waves (AEWs) and Mesoscale Convective Systems over continental western Africa, and their associated impacts on regional water and energy budgets. For more information about the NAMMA Campaign, go to the NAMMA web site: http://namma.nsstc.nasa.gov/ Network DescriptionZeus long-range lightning detection system is based on detection of sferics - the impulsive radio noise emitted by a lightning strike - in the Very Low Frequency (VLF) spectrum between 7 and 15 kHz. In the VLF portion of the radio spectrum sferics propagate thousands of kilometers through the earth-ionosphere waveguide. This lightning detection system, built by Resolution Displays, Inc., consists of a network of thirteen Very Low Frequency (7-15 kHz) radio receivers spread over the European and African continents. Each receiver reports the vertical electric field as a time series which represents the sferic's waveform, and includes a time stamp synchronized by the Global Positioning System (GPS) clock. The Arrival Time Difference (ATD) between the time series from pairs of receivers is extracted by time correlation. Each ATD yields an elliptic locus-of-points on the earth's surface for the lightning location, and the intersection of several ellipses from a sferics candidate defines a ''fix'' location. The European receivers are situated in Birmingham (UK), Roskilde (Denmark), Iasi (Romania), Larnaka (Cyprus), and Evora (Portugal), and the African receivers are in Addis Ababa (Ethiopia), Dar es Salaam (Tanzania), Bethlehem (South Africa), Osun state (Nigeria), Dakar (Senegal), Guadeloupe, Fortaleza (Brazil) and Sao Paulo (Brazil) . Additional information about the ZEUS network can be found here. Each file represents a 15 minute timeframe of lightning data, with the time embedded in the file name as the starting time. The files are distributed as tar compressed files named as
Thes files uncompress and contain multiple files named according to the example shown below:
where, yyyy is the year, mm is the month, dd is the day, and tttt is the starting time. Data Format and ContentThe data were reprocessed in October 2009 and an adiitional field was added. The file format is shown below. The PI documentation also contains the data format adn additionally hte Fortran format to read the data and coordination infomation for rx locations. These data are arranged in ASCII data files, space delimited, and each file supplies data for a 15 minute period of time. Below is the a line of a data file shown as an example.
Where each column of the ZEUS data file is defined below: Contact Information Questions related to these data should be directed to the data provider listed below:
To order these data or for further information, please contact:
|
||