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The International Space Station Lightning Imaging Sensor: Performance, Applications, and Cross-Platform ScienceThe Lightning Imaging Sensor (LIS), an optically based lightning detector developed at NASA Marshall Space Flight Center, was launched to the International Space Station (ISS) in February 2017, detecting optical signatures of lightning with storm-scale horizontal resolution (4-km) during both day and night. ISS LIS data are available 1 March 2017 to present. Millisecond timing allows detailed intercalibration and validation with other spaceborne and ground-based lightning sensors. Initial comparisons with those other sensors suggest flash detection efficiency around 60% (diurnal variability of 51-75%), false alarm rate under 5%, timing accuracy better than 2 ms, and horizontal location accuracy around 3 km. The spatially uniform flash detection capability of ISS LIS from low-Earth orbit allows assessment of spatially varying flash detection efficiency for other sensors and networks, particularly the Geostationary Lightning Mappers (GLMs). ISS LIS provides research data suitable for investigations of lightning physics, climatology, thunderstorm processes, and atmospheric composition, as well as realtime lightning data for operational forecasting and aviation weather interests. ISS LIS enables enrichment and extension of the long-term global climatology of lightning from space, and is the only recent platform that extends the global record to higher latitudes (± 55°). The global spatial distribution of lightning from ISS LIS is broadly similar to previous datasets, with globally averaged seasonal/annual flash rates (3-year average: ~44 s) about 5-10% lower. This difference is likely due to reduced flash detection efficiency that will be mitigated in future ISS LIS data processing, as well as the shorter ISS LIS period of record. The expected land/ocean contrast in the diurnal variability of global lightning is also observed. The near-realtime ISS LIS data make the instrument important to operational weather forecasting and related applications, including public safety. Finally, ISS LIS is demonstrating utility as part (or potential part) of cross-platform studies examining a diverse array of topics, including lightning physics, thunderstorm processes, convective precipitation, and atmospheric composition.
Document ID
20205010423
Acquisition Source
Marshall Space Flight Center
Document Type
Poster
Authors
Timothy Lang
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
R. Blakeslee
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
D. Buechler
(University of Alabama in Huntsville Huntsville, Alabama, United States)
D. Mach
(Universities Space Research Association Columbia, Maryland, United States)
S. Bang
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
A. Biazar
(University of Alabama in Huntsville Huntsville, Alabama, United States)
T. Berendes
(University of Alabama in Huntsville Huntsville, Alabama, United States)
K. Brunner
(University of Alabama in Huntsville Huntsville, Alabama, United States)
S. Flynn
(University of Alabama in Huntsville Huntsville, Alabama, United States)
P. Gatlin
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
M. Heumesser
(Technical University of Denmark Kongens Lyngby, Hovedstaden, Denmark)
W. Koshak
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
S. Leake
(Western Michigan University Kalamazoo, Michigan, United States)
E. McCaul
(Universities Space Research Association Columbia, Maryland, United States)
C. Schultz
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
S. Stough
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
K. Virts
(University of Alabama in Huntsville Huntsville, Alabama, United States)
Y. Wu
(University of Alabama in Huntsville Huntsville, Alabama, United States)
Date Acquired
November 19, 2020
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: AGU Fall Meeting
Location: Online
Country: US
Start Date: December 1, 2020
End Date: December 17, 2020
Sponsors: American Geophysical Union
Funding Number(s)
WBS: 347284.02.03.01.01
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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