DocumentCode :
124794
Title :
Investigation of streamer initiation in sprite-halo events
Author :
Jianqi Qin ; Pasko, Victor P. ; McHarg, Matthew G. ; Stenbaek-Nielsen, Hans C.
Author_Institution :
Commun. & Space Sci. Lab., Penn State Univ., University Park, PA, USA
fYear :
2014
fDate :
8-11 Jan. 2014
Firstpage :
1
Lastpage :
1
Abstract :
Sprites are spectacular optical emissions in the mesosphere induced by transient lightning electric fields above thunderstorms. These luminous gas discharges often exhibit a brief descending high-altitude diffuse glow in the shape of a pancake with diameters up to ~80 km near ~75 km altitude, referred to as a sprite halo, that sometimes is accompanied by development of fine-structured filaments with diameters up to several hundred meters in the altitude range of ~40 to ~90 km, commonly referred to as sprite streamers. Since the first video documentation [Franz et al., Science, 249, 48, 1990], sprites have attracted extensive research interest in the last two decades, primarily due to their potential as natural resources for the study of streamer physics, their potential impact on the chemistry in the upper atmosphere, and their ability to perturb the subionospheric radio signals [Qin J., PhD Dissertation, Penn State, 2013, and references therein]. However, up to date, how these filamentary plasmas are initiated in the lower ionosphere remains a subject of active research and existing theories differ fundamentally from each other [Luque and Ebert, Nature Geoscience, 2, 757, 2009; Qin et al., JGR, 116, A06305, 2011]. To better understand the initiation mechanism of sprite streamers, in the present work, a plasma fluid model developed previously by Qin et al. [JGR, 118, 2623, 2013] is used to investigate the initiation of sprite streamers during the development of a sprite halo. High-speed video observations of sprites are also studied in a comparison manner. The reported results suggest that the presence of plasma inhomogeneities in the lower ionosphere is a necessary condition to initiation sprite streamers, in agreement with the recently proposed sprite theory of Qin et al. [2011]. The polarization of the plasma inhomogeneities produces strong space charge field in a localized region, which greatly facilitates the initiation of sprite streamers. The presented resul- s once again reiterate the idea that the strength of the lightning induced electric field produced by a relatively large charge moment change is a necessary but not sufficient factor for initiation of sprite streamers [Lang et al., JGR, 116, A10306, 2011] and the presence of inhomogeneities is an important factor, especially for low charge moment changes.
Keywords :
atmospheric chemistry; ionosphere; ionospheric electromagnetic wave propagation; lightning; mesosphere; sprites; thunderstorms; brief descending high-altitude diffuse glow; filamentary plasma; fine-structured filament; high-speed video observation; large charge moment change; lightning induced electric field; localized region; lower ionosphere; luminous gas discharge; mesosphere; optical emissions; plasma inhomogeneity polarization; sprite halo development; sprite streamer initiation mechanism; sprite-halo events; streamer physics; strong space charge field; subionospheric radio signals; thunderstorms; transient lightning electric field; upper atmosphere chemistry; Educational institutions; Ionosphere; Lightning; Nonhomogeneous media; Plasmas; Sprites (computer);
fLanguage :
English
Publisher :
ieee
Conference_Titel :
Radio Science Meeting (USNC-URSI NRSM), 2014 United States National Committee of URSI National
Conference_Location :
Boulder, CO
Print_ISBN :
978-1-4799-3119-4
Type :
conf
DOI :
10.1109/USNC-URSI-NRSM.2014.6928011
Filename :
6928011
Link To Document :
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