Lightning Strikes Up

Démêler les mystères des éclats de foudre “Gigantic Jet” qui atteignent 50 miles dans l’espace

Les télescopes de Maunakea reposent calmement à une altitude d’environ 4200 mètres (13 800 pieds) sous un ciel rempli d’une lumière extraordinaire. Les Cloud Cams nocturnes de Gemini North ont capturé ce phénomène lumineux extraordinaire. La colonne de lumières bleues et rouges entourée d’un flamboiement de lumière blanche apparaît si surnaturelle qu’elle semble être un effet spécial. Cette image à couper le souffle, cependant, est tout à fait réelle. Crédit : Observatoire international Gemini/NOIRLab/NSF/AURA/A. Forgeron

De nouvelles informations sur un phénomène atmosphérique insaisissable connu sous le nom de jets gigantesques ont été découvertes par une étude 3D détaillée d’une décharge électrique massive qui s’est élevée à 50 miles dans l’espace au-dessus d’un orage de l’Oklahoma. En tant que jet gigantesque le plus puissant étudié à ce jour, la décharge de l’Oklahoma transportait 100 fois plus de charge électrique qu’un éclair d’orage typique.

Formation d'un gigantesque jet au-dessus de l'Oklahoma

Cette série d’images, tirée d’une vidéo, montre la formation d’un gigantesque jet au-dessus de l’Oklahoma en mai 2018. Crédit : Chris Holmes

Le jet gigantesque a déplacé environ 300 coulombs de charge électrique de l’orage dans l’ionosphère – le bord inférieur de l’espace. Les éclairs typiques transportent moins de cinq coulombs entre le nuage et le sol ou à l’intérieur des nuages. La décharge vers le haut inclus relativement frais (environ 400 degrés

Fahrenheit
L’échelle Fahrenheit est une échelle de température, nommée d’après le physicien allemand Daniel Gabriel Fahrenheit et basée sur celle qu’il a proposée en 1724. Dans l’échelle de température Fahrenheit, le point de congélation de l’eau gèle est de 32 °F et l’eau bout à 212 °F, un Séparation de 180 °F, telle que définie au niveau de la mer et à la pression atmosphérique standard.

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Radio Mapping Sources Extending Up From Convective Structure of Storm

Radio mapping sources extending up from the convective structure of the storm. The gray plane represents the storm top. Credit: Georgia Tech Research Institute

Steve Cummer, professor of electrical and computer engineering at Duke, uses the electromagnetic waves that lightning emits to study the powerful phenomenon. He operates a research site where sensors resembling conventional antennas are arrayed in an otherwise empty field, waiting to pick up signals from locally occurring storms.

“The VHF and optical signals definitively confirmed what researchers had suspected but not yet proven: that the VHF radio from lightning is emitted by small structures called streamers that are at the very tip of the developing lightning, while the strongest electric current flows significantly behind this tip in an electrically conducting channel called a leader,” Cummer said.

Doug Mach, a co-author of the paper at the Universities Space Research Association (USRA), said the study was unique in determining that the 3D locations for the lightning’s optical emissions were well above the cloud tops.

“The fact that the gigantic jet was detected by several systems, including the Lightning Mapping Array and two geostationary optical lightning instruments, was a unique event and gives us a lot more information on gigantic jets,” Mach said. “More importantly, this is probably the first time that a gigantic jet has been three-dimensionally mapped above the clouds with the Geostationary Lightning Mapper (GLM) instrument set.”

Levi Boggs

GTRI researcher Levi Boggs is shown with a schematic showing the structure of a gigantic jet. Credit: Georgia Tech Research Institute

Gigantic jets have been observed and studied over the past two decades. However, because there’s no specific observing system to look for them, detections have been rare. Boggs learned about the Oklahoma event from a colleague, who told him about a gigantic jet that had been photographed by a citizen-scientist who had a low-light camera in operation on May 14, 2018.

Fortuitously, the event took place in a location with a nearby VHF lightning mapping system, within range of two Next Generation Weather Radar (NEXRAD) locations and accessible to instruments on satellites from NOAA’s Geostationary Operational Environmental Satellite (GOES) network. Boggs determined that the data from those systems were available and worked with colleagues to bring it together for analysis.

“The detailed data showed that those cold streamers start their propagation right above the cloud top,” Boggs explained. “They propagate all the way to the lower ionosphere to an altitude of 50-60 miles, making a direct electrical connection between the cloud top and the lower ionosphere, which is the lower edge of space.”

That connection transfers thousands of amperes of current in about a second. The upward discharge transferred negative charge from the cloud to the ionosphere, typical of gigantic jets.

The data showed that as the discharge ascended from the cloud top, VHF radio sources were detected at altitudes of 22 to 45 kilometers (13 to 28 miles), while optical emissions from the lightning leaders remained near the cloud top at an altitude of 15 to 20 kilometers (9 to 12 miles). The simultaneous 3D radio and optical data indicate that VHF lightning networks detect emissions from streamer corona rather than the leader channel, which has broad implications to lightning physics beyond that of gigantic jets.

Why do the gigantic jets shoot charge into space? Researchers speculate that something may be blocking the flow of charge downward – or toward other clouds. Records of the Oklahoma event show little lightning activity from the storm before it fired the record gigantic jet.

“For whatever reason, there is usually a suppression of cloud-to-ground discharges,” Boggs said. “There is a buildup of negative charge, and then we think that the conditions in the storm top weaken the uppermost charge layer, which is usually positive. In the absence of the lightning discharges we normally see, the gigantic jet may relieve the buildup of excess negative charge in the cloud.”

For now, there are many unanswered questions about gigantic jets, which are part of a class of mysterious transient luminous events. That’s because observations of them are rare and happen by chance – from pilots or aircraft passengers happening to see them or ground observers operating night-scanning cameras.

Estimates for the frequency of gigantic jets range from 1,000 per year up to 50,000 per year. They’ve been reported more often in tropical regions of the globe. However, the Oklahoma gigantic jet – which was twice as powerful as the next strongest one – wasn’t part of a tropical storm system.

Beyond their novelty, gigantic jets could have an impact on the operation of satellites in low-earth orbit, Boggs said. As more of those space vehicles are launched, signal degradation and performance issues could become more significant. The gigantic jets could also affect technologies such as over-the-horizon radars that bounce radio waves off the ionosphere.

Reference: “Upward propagation of gigantic jets revealed by 3D radio and optical mapping” by Levi D. Boggs, Doug Mach, Eric Bruning, Ningyu Liu, Oscar A. van der Velde, Joan Montanyá, Steve Cummer, Kevin Palivec, Vanna Chmielewski, Don MacGorman and Michael Peterson, 3 August 2022, Science Advances.
DOI: 10.1126/sciadv.abl8731

Boggs is affiliated with the Severe Storms Research Center, which was established at GTRI to develop improved technologies for warning of severe storms, such as tornadoes, that are common in Georgia. The work on gigantic jets and other atmospheric phenomena is part of that effort.



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