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Cubespark: A New Satellite-Based 3d Lightning Observing ConceptLegacy and current space-based optical lightning detectors are insensitive to small and dim pulses that make up much of the lightning activity produced by severe storms. Moreover, lightning flashes produced at low altitudes within optically thick clouds are severely under-detected by current optical detectors. Lastly, there is currently no capability to characterize the 3D structure of lightning both day and night at the global scale, yet this information is critical for identifying lightning produced in updraft regions, including lightning occurring in overshooting tops, which is a distinctive signature of severe weather. Global 3D lightning information is also critical for understanding the vertical distribution of NOx production and identifying anomalously electrified storms. Furthermore, the vertical distribution of lightning has implications for how microphysical (e.g., ice-based) and thermodynamical (e.g., latent heat release) processes vary regionally, as well as seasonally – e.g., winter lightning typically occurs at lower altitudes than summer lightning and is often associated with tall, man-made structures. Finally, global-scale 3D lightning observations would directly provide flash type (i.e., CG or IC) information that is very useful in all of the studies mentioned in this paragraph and is fundamental in identifying/documenting deleterious CG-caused impacts (e.g., wildfires, power-outages, crop and property damage, and associated insurance claims).

A new, satellite mission concept called CubeSpark is being designed to address these shortcomings and fill this measurement gap by providing novel 3D observations of total lightning activity. CubeSpark will utilize a constellation of low-Earth orbiting small satellites that make radio frequency (RF) and bi-spectral optical measurements of lightning. Two options for combining these measurements to retrieve the 3D location of lightning are considered with corresponding measurement simulators built to understand the level of detail and viability of each approach. Although the level of detail varies for each combined measurement approach, results indicate that a 3D location accuracy of < 1-2 km in each dimension is feasible across 300-500 km wide swaths, which suggests that CubeSpark can resolve the charge structure of thunderclouds from the tropics to the mid- and high-latitudes.
Document ID
20220019325
Acquisition Source
Marshall Space Flight Center
Document Type
Presentation
Authors
Patrick Gatlin
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Timothy Lang
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Mason Quick
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Jackson Remington
(NPP POST-DOC CONTRACT Redstone Arsenal, Alabama, United States)
Bill Koshak
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Daniel Cecil
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Christopher Schultz
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Sarah Bang
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Sonja Behnke
(Los Alamos National Laboratory Los Alamos, New Mexico, United States)
Harald Edens
(Los Alamos National Laboratory Los Alamos, New Mexico, United States)
Phillip Bitzer
(University of Alabama in Huntsville Huntsville, Alabama, United States)
Sarah Stough
(University of Alabama in Huntsville Huntsville, Alabama, United States)
Date Acquired
January 3, 2023
Subject Category
Meteorology And Climatology
Meeting Information
Meeting: 103rd Annual Meeting of the AMS
Location: Denver, CO
Country: US
Start Date: January 8, 2023
End Date: January 12, 2023
Sponsors: American Meteorological Society
Funding Number(s)
WBS: 387625.02.18.04.01
WBS: 478643.02.13.04.01
CONTRACT_GRANT: 80MSFC22M0004
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
Technical Review
Single Expert
Keywords
lightning
remote sensing
formation flying
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