Modeling of a New Electron Acceleration Mechanism Ahead of Streamers
Metadata Field | Value | Language |
---|---|---|
dc.creator | Ihaddadene, Keven | |
dc.creator | Liu, Ningyu | |
dc.creator | Celestin, Sebastien | |
dc.creator | Shi, Feng | |
dc.creator | Joseph, Dwyer | |
dc.date.accessioned | 2022-11-01T20:44:14Z | |
dc.date.available | 2022-11-01T20:44:14Z | |
dc.date.created | 2019 | |
dc.identifier | 10.1029/2018JA026084 | en_US |
dc.identifier.uri | https://agupubs.onlinelibrary.wiley.com/doi/full/10.1029/2018JA026084 | en_US |
dc.identifier.uri | https://aurora.auburn.edu/handle/11200/50443 | |
dc.identifier.uri | http://dx.doi.org/10.35099/aurora-511 | |
dc.description.abstract | Head-on collisions between negative and positive streamers have been proposed as a mechanism behind X-ray emissions by laboratory spark discharges. Recent simulations using plasma fluid and particle in cell models of a single head-on collision of two streamers of opposite polarities in ground pressure air predicted an insignificant number of thermal runaway electrons >1 keV and hence weak undetectable X-ray emissions. Because the current available models of a single streamer collision failed to explain the observations, we first use a Monte Carlo model coupled with multiple static dielectric ellipsoids immersed in a subbreakdown ambient electric field as a description of multiple streamer environment and we investigate the ability of multiple streamer-streamer head-on collisions to accelerate runaway electrons >1 keV up to energies similar to 200-300 keV instead of just one single head-on collision. The results of simulations show that the streamer head-on collision mechanism fails to accelerate electrons; instead, they decelerate in the positive streamer channel. In a second part, we use a streamer plasma fluid model to simulate a new streamer-electron acceleration mechanism based on a collision of a large negative streamer with a small neutral plasma patch in different Laplacian electric fields vertical bar E-0 vertical bar = (35, 40, 45) kV/cm, respectively. We observe the formation of a secondary short propagating negative streamer with a strong peak electric field >250 up to 378 kV/cm over a time duration of similar to 0.16 ns at the moment of the collision. The mechanism produces up to 10(6) runaway electrons with an upper energy limit of 24 keV. | en_US |
dc.format | en_US | |
dc.publisher | American Geophysical Union | en_US |
dc.relation.ispartof | JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS | en_US |
dc.relation.ispartofseries | 2169-9380 | en_US |
dc.rights | ©American Geophysical Union 2019. This is this the version of record co-published by the American Geophysical Union and John Wiley & Sons, Inc. It is made available under the CC-BY-NC-ND 4.0 license. Item should be cited as: Ihaddadene, K. M., Dwyer, J. R., Liu, N., Celestin, S., & Shi, F. (2019). Modeling of a new electron acceleration mechanism ahead of streamers. Journal of Geophysical Research: Space Physics, 124(8), 7301-7319. | en_US |
dc.title | Modeling of a New Electron Acceleration Mechanism Ahead of Streamers | en_US |
dc.type | Text | en_US |
dc.type.genre | Journal Article, Academic Journal | en_US |
dc.citation.volume | 124 | en_US |
dc.citation.issue | 8 | en_US |
dc.citation.spage | 7301 | en_US |
dc.citation.epage | 7319 | en_US |
dc.description.status | Published | en_US |
dc.description.peerreview | Yes | en_US |
dc.creator.orcid | 0000-0002-2220-3197 | en_US |