Abstract
Possible persistent ionization caused by giant blue jets
Department of Electrical Engineering, Stanford University, Stanford, California, USA
Department of Electrical Engineering, Stanford University, Stanford, California, USA
We consider the possible production of persistent ionization at low altitudes (h ≤ 70 km) by giant blue jets (GBJ), using a new five constituent model of stratospheric/lower-ionospheric chemistry. Results
indicate substantial ionization at h < 50 km, which exhibits an initially rapid (few seconds) recovery due to electron attachment, followed by a long enduring
recovery (>10 minutes) determined by the time scale of mutual neutralization of negative and positive ions. Such recovery
signatures may be observable in subionospheric VLF data in the form of Early/fast events with long lasting recoveries. Analysis
also indicates that electrons may sometimes be quickly (
1 ms) removed by the dissociative attachment mechanism in the presence of a high electric field, while the negative and positive
ions remain and persist for extended periods of time. In such cases, the initial rapid recovery may not be observable in VLF
data due to its typical time resolution of ∼10 to 20 ms. In stratosphere (h
50 km) the ionization recovery is found to not be accurately described by a four-constituent model proposed by
Received 13 December 2006; accepted 26 February 2007; published 18 April 2007.
Citation: (2007), Possible persistent ionization caused by giant blue jets, Geophys. Res. Lett., 34, L08804, doi:10.1029/2006GL029051.
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