Abstract:Terrestrial gamma ray flashes (TGFs) (Fishman et al., 1994) represent a spectacular naturally occurring high energy phenomenon in the Earth's atmosphere. These events contain photons with several tens of mega electron-volt energies and likely involve large quantities of energetic electrons, sharing the same physical origin as X-rays generated by laboratory sparks (Stankevich & Kalinin, 1967) or originating from stepping lightning leaders (Moore et al., 2001). Dwyer et al. (2012) provide a review of principal p… Show more
“…Their initial energy is 1 MeV. These seed electrons can be thought of as produced by cosmic ray secondaries (e.g., Chilingarian et al, 2021), thermal runaway electrons injected by a lightning leader (e.g., Celestin et al, 2015) or relativisticfeedback-produced electrons (e.g., Dwyer, 2003;Pasko et al, 2023). The injection rate is a variable parameter between the different simulations.…”
Terrestrial gamma ray flashes (TGFs) are short bursts of gamma rays occurring during thunderstorms. They are believed to be produced by relativistic runaway electron avalanches (RREAs). It is usually admitted that the number of high‐energy electrons produced in the brightest TGFs remains mostly confined within a range from 1017 to 1019. To understand the constraints in the development of RREAs, we perform self‐consistent simulations using a newly developed model with a finite acceleration region and various injection rates. We find that RREAs should naturally self‐quench for a fixed total number of runaway electrons, and hence a fixed number of bremsstrahlung photons. From the idea that TGF sources quench themselves, we derive a simple equation controlling the total number of runaway electrons. In this framework, the existence of a saturation in the electron density discovered in a previous work places a lower limit on TGF durations.
“…Their initial energy is 1 MeV. These seed electrons can be thought of as produced by cosmic ray secondaries (e.g., Chilingarian et al, 2021), thermal runaway electrons injected by a lightning leader (e.g., Celestin et al, 2015) or relativisticfeedback-produced electrons (e.g., Dwyer, 2003;Pasko et al, 2023). The injection rate is a variable parameter between the different simulations.…”
Terrestrial gamma ray flashes (TGFs) are short bursts of gamma rays occurring during thunderstorms. They are believed to be produced by relativistic runaway electron avalanches (RREAs). It is usually admitted that the number of high‐energy electrons produced in the brightest TGFs remains mostly confined within a range from 1017 to 1019. To understand the constraints in the development of RREAs, we perform self‐consistent simulations using a newly developed model with a finite acceleration region and various injection rates. We find that RREAs should naturally self‐quench for a fixed total number of runaway electrons, and hence a fixed number of bremsstrahlung photons. From the idea that TGF sources quench themselves, we derive a simple equation controlling the total number of runaway electrons. In this framework, the existence of a saturation in the electron density discovered in a previous work places a lower limit on TGF durations.
“…Because of the short duration of NBEs, the assumed length of the discharge channel is several hundred meters or less (Watson & Marshall, 2007; Dwyer & Uman, 2014; Rison et al., 2016). It has been suggested recently that relativistic runaway discharges driven by photoelectric feedback can be sources of NBEs on these compact scales (Pasko et al., 2023). Significantly longer channel lengths were estimated in (Eack, 2004; da Silva & Pasko, 2015).…”
In this work the electric field of narrow bipolar events (NBEs) measured at a remote location is used to extract the current waveform of the source discharge. All calculations correspond to a vertical linear current source above a perfectly conducting ground plane. The current study uses the well established formulation of electromagnetic fields in the frequency domain, and develops a deconvolution based technique to obtain exact reconstruction of the source current, improving upon previous modeling of NBEs, which often require tuning several inter‐dependent parameters to determine the current that best reproduces the observed electric field. Our proposed solution, although readily available in standard electromagnetic textbooks, has never been employed in the context of lightning related discharges, and offers a simple and efficient alternative to previous conventional time domain calculations.
“…In works [99,100], attention was focused on the study of RAEs in TOKAMAK-type installations and devices for their diagnostics in these conditions. Works [101][102][103][104][105] studied RAEs registered in atmospheric discharges, and work [106] investigated the application of RAE discharges for materials processing.…”
Runaway electron (RAE) generation in high-pressure gases is an important physical phenomenon that significantly influences discharge shapes and properties of initiated plasma. The diffuse discharges formed due to RAEs in the air and other gases at atmospheric pressure find wide applications. In the present review, theoretical and experimental results that explain the reason for RAE occurrence at high pressures are analyzed, and recommendations are given for the implementation of conditions under which the runaway electron beam (RAEB) with the highest current can be obtained at atmospheric pressure. The experimental results were obtained using subnanosecond, nanosecond, and submicrosecond generators, including those specially developed for runaway electron generation. The RAEBs were recorded using oscilloscopes and collectors with picosecond time resolution. To theoretically describe the phenomenon of continuous electron acceleration, the method of physical kinetics was used based on the Boltzmann kinetic equation that takes into account the minimum but sufficient number of elementary processes, including shock gas ionization and elastic electron scattering. The results of modeling allowed the main factors to be established that control the RAE appearance, the most important of which is electron scattering on neutral atoms and/or molecules. Theoretical modeling has allowed the influence of various parameters (including the voltage, pressure, gas type, and geometrical characteristics of the discharge gap) to be taken into account. The results of the research presented here allow RAE accelerators with desirable parameters to be developed and the possibility of obtaining diffuse discharges to be accessed under various conditions. The review consists of the Introduction, five sections, the Conclusion, and the References.
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