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SOHO OBSERVATIONS OF A CME-DRIVEN SHOCK AND EIT WAVES

机译:CME驱动的冲击波和EIT波的SOHO观察

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We report on observations of a CME-driven shock wave on March 5 2000 from different instruments (EIT, LASCO and UVCS) on board the Solar and Heliospheric Observatory (SOHO). The CME lift-off took place at about 16:12 UT and reached the LASCO/C2 field of view (FOV) at 17:06 UT with a speed (projected in the plane of sky) of about 860 km s-1.On-disk waves are also observed in the EIT difference images. Moreover, enhancement in intensities and widths of the Osignatures of plasma heating are also observed based on the UVCS data suggesting the presence of a driven shock wave propagating in front of the CME. Interestingly, visual evidence for the shock wave is shown based on the propagation of the kink along a streamer where no CME material is present to cause such an effect. The preliminary results on the relationship of different phenomena observed by the different instruments on SOHO are presented.
机译:我们报告了2000年3月5日来自太阳和日球天文台(SOHO)上不同仪器(EIT,LASCO和UVCS)对CME驱动的冲击波的观测结果。 CME升空发生在大约16:12 UT,并于UT 17:06到达LASCO / C2视场(FOV),速度约为860 km s-1。在EIT差异图像中也观察到了-盘波。此外,基于UVCS数据还观察到等离子体加热的信号强度和宽度的增强,表明存在在CME前方传播的驱动冲击波。有趣的是,基于扭结沿着拖缆的传播来显示冲击波的视觉证据,其中不存在CME材料会引起这种影响。给出了用不同仪器对SOHO观测到的不同现象之间的关系的初步结果。

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