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首页> 外文期刊>The Astrophysical journal >Eruption of a Multiple-Turn Helical Magnetic Flux Tube in a Large Flare: Evidence for External and Internal Reconnection That Fits the Breakout Model of Solar Magnetic Eruptions
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Eruption of a Multiple-Turn Helical Magnetic Flux Tube in a Large Flare: Evidence for External and Internal Reconnection That Fits the Breakout Model of Solar Magnetic Eruptions

机译:大火炬中的多匝螺旋磁通管的喷发:外部和内部重新连接的证据符合太阳电磁喷发的爆发模型

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We present observations and an interpretation of a unique multiple-turn spiral flux tube eruption from active region 10030 on 2002 July 15. The TRACE C IV observations clearly show a flux tube that is helical and erupting from within a sheared magnetic field. These observations are interpreted in the context of the breakout model for magnetic field explosions. The initiation of the helix eruption, as determined by a linear backward extrapolation, starts 25 s after the peak of the flare's strongest impulsive spike of microwave gyrosynchrotron radiation early in the flare's explosive phase, implying that the sheared core field is not the site of the initial reconnection. Within the quadrupolar configuration of the active region, the external and internal reconnection sites are identified in each of two consecutive eruptive flares that produce a double coronal mass ejection (CME). The first external breakout reconnection apparently releases an underlying sheared core field and allows it to erupt, leading to internal reconnection in the wake of the erupting helix. This internal reconnection releases the helix and heats the two-ribbon flare. These events lead to the first CME and are followed by a second breakout that initiates a second and larger halo CME. The strong magnetic shear in the region is compatible with the observed rapid proper motion and evolution of the active region. The multiple-turn helix originates from above a sheared-field magnetic inversion line within a filament channel, and starts to erupt only after fast breakout reconnection has started. These observations are counter to the standard flare model and support the breakout model for eruptive flare initiation.
机译:我们介绍了观测结果,并解释了2002年7月15日从活动区域10030发生的独特的多匝螺旋磁通量管喷发。TRACEC IV观测结果清楚地显示了在剪切磁场内呈螺旋状喷发的磁通量管。这些观察结果是在磁场爆炸的突破模型的背景下解释的。由线性向后外推法确定的螺旋爆发的爆发是在火炬爆炸阶段的火炬微波回旋加速器辐射的最强脉冲尖峰峰值之后25 s开始的,这表明剪切的核心场不是火星爆发的地点。初始重新连接。在活动区域​​的四极配置中,外部和内部重新连接位置在两个连续的喷发耀斑中均被识别出,产生两个日冕物质抛射(CME)。第一次外部突破重新连接显然释放了一个潜在的剪切核心场,并使其爆发,从而在螺旋线爆发后导致内部重新连接。内部重新连接释放了螺旋并加热了两个色带的火炬。这些事件导致了第一个CME,随后是第二次突破,引发了第二个更大的光环CME。该区域中的强磁剪切力与观测到的活动区域的快速适当运动和演化相适应。多匝螺旋线起源于细丝通道内的剪切场磁反转线的上方,并且仅在快速中断重新连接开始后才开始爆发。这些观察结果与标准火炬模型相反,并支持爆发性火炬爆发的突破模型。

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