首页> 外文期刊>The Astrophysical journal >DISSOCIATIVE CHARGE EXCHANGE AND IONIZATION OF O_2 BY FAST H~+ AND O~+ IONS: ENERGETIC ION INTERACTIONS IN EUROPA'S OXYGEN ATMOSPHERE AND NEUTRAL TORUS
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DISSOCIATIVE CHARGE EXCHANGE AND IONIZATION OF O_2 BY FAST H~+ AND O~+ IONS: ENERGETIC ION INTERACTIONS IN EUROPA'S OXYGEN ATMOSPHERE AND NEUTRAL TORUS

机译:快速H〜+和O〜+离子的解离电荷交换和O_2的电离:欧洲氧气氛和中性环中的能量离子相互作用

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摘要

Measurements of electron capture and ionization of O_2 molecules in collisions with H~+ AND O~+ ions have been made over an energy range 10-100 keV. Cross sections for dissociative and nondissociative interactions have been separately determined using coincidence techniques. Nondissociative channels leading to O_2~+ product formation are shown to be dominant for both the H~+ and the O~+ projectiles in the capture collisions and only for the H~+ projectiles in the ionization collisions. Dissociative channels are dominant for ionizing collisions involving O~+ projectiles. The energy distributions of the O~+ fragment products from collisions involving H~+ AND O~+ have also been measured for the first time using time-of-flight methods, and the results are compared with those from other related studies. These measurements have been used to describe the interaction of the energetic ions trapped in Jupiter's magnetosphere with the very thin oxygen atmosphere of the icy satellite Europa. It is shown that the ionization of oxygen molecules is dominated by charge exchange plus ion impact ionization processes rather than photoionization. In addition, dissociation is predominately induced through excitation of electrons into high-lying repulsive energy states (electronically) rather than arising from momentum transfer from knock-on collisions between colliding nuclei, which are the only processes included in current models. Future modeling will need to include both these processes.
机译:在10-100 keV的能量范围内,已经测量了与H〜+和O〜+离子碰撞时O_2分子的电子俘获和电离。用于分离和非分离相互作用的横截面已使用巧合技术分别确定。结果表明,在捕获碰撞中,导致H_2 +和O〜+射弹的非离解通道均占主导地位,而在电离碰撞中,仅导致H〜+射弹的非离解通道占主导地位。离解通道在涉及O〜+射弹的电离碰撞中占主导地位。还使用飞行时间方法首次测量了由涉及H〜+和O〜+的碰撞产生的O〜+碎片产物的能量分布,并将其结果与其他相关研究的结果进行了比较。这些测量已被用来描述木星磁层中捕获的高能离子与冰卫星欧罗巴的非常薄的氧气气氛的相互作用。结果表明,氧分子的电离主要由电荷交换加离子碰撞电离过程而不是光电离来控制。此外,离解主要是通过电子激发成高阶排斥能态(电子方式)引起的,而不是由碰撞核之间的碰撞碰撞所产生的动量传递引起的,这是当前模型中唯一的过程。未来的建模将需要包括这两个过程。

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