2001
DOI: 10.1029/2000ja000160
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Effects of thunderstorm‐driven runaway electrons in the conjugate hemisphere: Purple sprites, ionization enhancements, and gamma rays

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Cited by 56 publications
(66 citation statements)
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“…It is pertinent to note that the characteristics of the terrestrial g ray flashes detected in the near space aboard CGRO [Fishman et al, Table 1. Number, Flux Density, and Fluence of Neutrons at the "Detector Altitude" for Neutron Source Located at "Cloud Altitude" 1994] and RHESSI are explained more or less adequately by bremsstruhlung of ascending relativistic electron avalanches (for instance, [Dwyer and Smith, 2005;Dwyer, 2008;Cummer et al, 2005;Williams et al, 2006;Babich et al, 2007b;2008a, 2008b, 2008c), as in the earlier works, where the CGRO data were analyzed [e.g., Taranenko and Roussel-Dupre, 1996;Roussel-Dupre et al, 1998;Lehtinen et al, 1996Lehtinen et al, , 1999Lehtinen et al, , 2001Gurevich and Zybin, 2001;Babich et al, 2001Babich et al, , 2004b.…”
Section: Discussionmentioning
confidence: 81%
“…It is pertinent to note that the characteristics of the terrestrial g ray flashes detected in the near space aboard CGRO [Fishman et al, Table 1. Number, Flux Density, and Fluence of Neutrons at the "Detector Altitude" for Neutron Source Located at "Cloud Altitude" 1994] and RHESSI are explained more or less adequately by bremsstruhlung of ascending relativistic electron avalanches (for instance, [Dwyer and Smith, 2005;Dwyer, 2008;Cummer et al, 2005;Williams et al, 2006;Babich et al, 2007b;2008a, 2008b, 2008c), as in the earlier works, where the CGRO data were analyzed [e.g., Taranenko and Roussel-Dupre, 1996;Roussel-Dupre et al, 1998;Lehtinen et al, 1996Lehtinen et al, , 1999Lehtinen et al, , 2001Gurevich and Zybin, 2001;Babich et al, 2001Babich et al, , 2004b.…”
Section: Discussionmentioning
confidence: 81%
“…However, even if only ∼3 to 10% of the electrons precipitate on the conjugate atmosphere, they create detectable emissions via interactions with atmospheric species. For 500 C of charge removed from 15 km altitude (M q =7500 C-km), consistent with the largest observed gamma-ray fluxes, the injected beam density is N e =10 5 m −3 , and the predicted emissions should be of a similar magnitude to elves (Lehtinen et al, 2001). While this charge moment is very high compared to observed values (e.g., Cummer and Inan, 2000), it results in a relativistic beam density that is consisted with BATSE gamma-ray flash observations (Lehtinen et al, 2001).…”
Section: Introductionmentioning
confidence: 85%
“…However, the beam may undergo pitch angle scattering and energy degradation during its traverse, through wave-particle resonance interactions, so that only a fraction of electrons remain in the loss cone. In the worst case, when pitch angles are scattered into an isotropic distribution, the number in the loss cone is a function of geomagnetic latitude; at latitudes of 30-40 deg, this number varies from 10 down to 3% (Lehtinen et al, 2001). However, even if only ∼3 to 10% of the electrons precipitate on the conjugate atmosphere, they create detectable emissions via interactions with atmospheric species.…”
Section: Introductionmentioning
confidence: 99%
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“…Some problems arise because the runaway theory predicts that the lightning charge moment change needs to be about 5000 C km to generate the runaway breakdown at the altitude range 30-50 km followed by the TGFs events (Lehtinen et al, 2001). This contradicts with observations since the measured lightning charge moment changes in TGF-associated strokes are 50-500 times smaller than what the runaway theory predicts (Cummer et al, 2005).…”
Section: V Surkov and M Hayakawa: Underlying Mechanisms Of Transmentioning
confidence: 99%