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Detecting and Measuring Reconnection Outflows in the Hinode Era

机译：检测和测量Hinode时代中的重新连接越野

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Our aim has been to provide direct quantitative measurements of reconnection signatures during solar flaring events in order to constrain the properties of flare energetics. Reconnection outflows are observed as sunward-flowing voids during long-duration flares, consistent with 3D reconnection mod-els. Through the use of our automatic detection software, we have obtained trajectories, velocities, sizes, and magnetic flux information for outflows in sev-eral flares from various instruments. Several limitations have been encountered with instruments prior to the availability of Hinode, and it is the purpose of this work to show the progress we have made in detecting reconnection signatures in the form of supra-arcade downflows (SADs) and to emphasize the potential of making better detections and measurements with Hinode's X-ray Telescope (XRT).
机译：我们的目标是在太阳辐射事件期间提供重新连接的直接定量测量，以限制耀斑能量学的性质。在长持续时间耀斑期间观察到重新连接的流出作为向后流动的空隙，与3D重新连接Mod-ELS一致。通过使用我们的自动检测软件，我们已经获得了来自各种仪器的Sev-Erares的流出的轨迹，速度，尺寸和磁通量信息。在Hinode可用性之前，仪器遇到了几个限制，这是本工作的目的，以展示我们在检测Supra-arcade下流（SADS）的形式中检测重新连接的进展，并强调潜力通过Hinode的X射线望远镜（XRT）更好地检测和测量。

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