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Minimum charge moment change in positive and negative cloud to ground lightning discharges producing sprites

机译:正负云对地雷放电的最小充电矩变化,产生精灵

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Sprites with extensive vertical streamer structures are usually produced by the most intense (i.e., large peak current) positive cloud-to-ground lightning discharges (+CGs) in thunderstorms [e.g., Lyons, JGR, 101, 29641, 1996]. In the conventional breakdown theory of sprites, a large charge moment change of ∼1000 C km, for which the electric field can exceed the conventional breakdown field Ek (∼30 kV/cm at ground level) at mesospheric/lower ionospheric altitudes, is usually assumed to be necessary for sprite production [e.g., Pasko et al., JGR, 102, 4529, 1997]. However, measurements indicate that surprisingly small charge moment changes of ∼200 C km in positive cloud-to-ground lightning discharges (+CGs) can initiate middle atmospheric gas discharges termed sprites [e.g., Hu et al., GRL, 29, 1279, 2002]. In the present work a plasma fluid model is used to study the necessary conditions for a lightning discharge associated with such a small charge moment change to produce sprites. It is demonstrate that for spherically symmetric initial electron density in-homogeneities, the initiation of sprites by such small charge moment changes is only possible when the ionospheric D-region electron density profile is characterized by a reference altitude h′ greater than 90 km. Vertically elongated inhomogeneities are found to be more favorable for sprite initiation consistent with recently published studies of Kosar et al. [JGR, 117, A08328, 2012]. It is calculated that for the same ionospheric conditions (i.e., inhomogeneities and h′ values) that lead to initiation of sprites by +CGs associated with ∼200 C km charge moment changes, the minimum charge moment change required for initiation of sprites by -CGs is 300 C km. We suggest that the intersection of the rarity of QhQ≃300 C km and h′≳88 km leads to the fact that the occurrence of negative sprites are rare, although -CGs associat- d with QhQ≃300 C km are not so rare.
机译:通常在雷暴天气中,最强烈的(即大峰值电流)正对地雷电放电(+ CGs)会产生具有广泛垂直流光结构的子画面[例如,Lyons,JGR,101,29641,1996]。在传统的breakdown子击穿理论中,大的荷电矩变化约为1000 C km,为此,电场可以超过传统的击穿场E k (地平面约30 kV / cm)。通常假定中层/较低的电离层高度是生成子画面所必需的(例如,Pasko等,JGR,102,4529,1997)。但是,测量结果表明,在正向云对地雷电放电(+ CGs)中,约200 C km的微小充电矩变化令人惊讶,可以启动被称为子画面的中等大气气体放电[例如,Hu et al。,GRL,29,1279, 2002]。在本工作中,使用等离子流体模型来研究与如此小的电荷矩变化相关联的雷电放电产生sp的必要条件。已经证明,对于球形对称的初始电子密度不均匀性,只有当电离层D区域电子密度分布的特征是参考高度h'大于90 km时,才能通过如此小的电荷矩变化来引发子画面。与Kosar等人最近发表的研究一致,发现垂直拉长的不均匀性更有利于子图形的激发。 [JGR,117,A08328,2012]。计算得出,对于相同的电离层条件(即不均匀性和h'值),导致+ CG引发约40 C km电荷矩变化的子图形,-CG引发子图形所需的最小电荷矩变化是300 C公里。我们认为Qh Q ≃300C km和h'≳88km的稀有度的交集导致这样的事实,尽管-CGs与Qh < inf> Q ≃C300 km并不罕见。

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