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首页> 外文期刊>Solar physics >Post-Eruptive Arcade Formation in the 25 January 2007 CME/Flare Limb Event: Microwave Observations with the RATAN-600 Radio Telescope
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Post-Eruptive Arcade Formation in the 25 January 2007 CME/Flare Limb Event: Microwave Observations with the RATAN-600 Radio Telescope

机译:2007年1月25日CME /火炬肢事件中爆发后的商场形成:用RATAN-600射电望远镜进行微波观测

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摘要

A CME/flare event occurred at the eastern limb on 25 January, 2007. Seven successive multi-wavelength scans in the range 1.8 cm -aEuro parts per thousand 5.0 cm were obtained with the RATAN-600 radio telescope starting just at the beginning of the post-eruptive arcade formation (30 min after a C6.3 flare peak) and lasting for 3.5 hours. The conditions were favorable to study the off-limb microwave radio source associated with the post-eruptive arcade in different phases of its formation. Microwave radio emission of the arcade was rather intense initially and then considerably decreased; its maximum was co-spatial with the 195 Fe xii loop tops. The RATAN-600 total flux spectra of the off-limb radio source were practically flat during the first two hours indicating a predominant contribution of thermal emission. The X-ray spectrum was thermal (according to RHESSI data) at that time. Data available in the meter wavelength range during this phase were indicative of weak non-thermal processes likely due to accelerated particles. However, free -aEuro parts per thousand free emission of an isothermal source dominated in microwaves. This is indicative of the presence of a large amount of plasma in the region of arcade formation at the initial stage of the event. The weak microwave emission during the decay phase might be interpreted as the thermal cyclotron emission of the loops in the arcade.
机译:CME /耀斑事件发生在2007年1月25日的东部地区。使用RATAN-600射电望远镜,从2007年1月25日开始,连续进行了七次连续的多波长扫描,扫描范围为1.8 cm -aEuro千分之5.0 cm。喷发后的街机形成(C6.3耀斑峰值后30分钟),持续3.5小时。这些条件有利于研究与喷发后拱廊在其形成的不同阶段相关的离岸微波无线电源。最初,拱廊的微波无线电发射非常强烈,然后显着下降。它的最大空间与195 Fe xii环顶同空间。头肢无线电源的RATAN-600总通量谱在最初的两个小时内几乎是平坦的,这表明热量的主要贡献。当时的X射线光谱是热的(根据RHESSI数据)。在此阶段,仪表波长范围内的可用数据表明,可能由于加速的粒子而导致的弱非热过程。但是,微波占主导地位的等温源的千分之几的自由排放量为-aEuro份。这指示在事件的初始阶段在拱廊形成区域中存在大量等离子体。衰变阶段中微弱的微波发射可以解释为拱廊中回路的热回旋加速器发射。

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