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lNJECTION OF ≥ 10 MeV PROTONS IN ASSOCIATION WITH A CORONAL MORETON WAVE

机译:与冠状莫顿波相关的≥10 MeV质子的注入

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We report extreme-UV observations of the coronal Moreton wave and concurrcnt observations of ~ l0-l00 MeV protons. Observations are carried out with the Extreme-UV Imaging Telescope and the Energetic and Relativistic Nuclei and Electron instrument on board the SOHO spacecraft. We study the proton events associated with coronal mass ejections (CMEs) centered near the central meridian. Observations reveal the initial injection of ≥ l0 MeV protons during the period when the coronal Moreton wave was traversing the western hemisphere of the Sun, this being an early signature of the CME launch. Acceleration of the CME-associated protons starts during the CME liftoff. while the main proton Production occurs several hours later,when the CME expands in the interplanetary medium. Between the first proton production and the maximum intensity time. a spectral softening is observed. We analyze in detail the l997 September 24 event. Development of the event indicates that the spectral softening may be due to a change in thc acceleration regime. so the proton production starts with the less inten- sivc but hard-spectrum injection and then moves to the more intensive but soft-spectrum injection farther from the Sun.
机译:我们报告了冠状莫顿波的极端紫外线观测结果,以及〜10-100 MeV质子的同时观测结果。用SOHO航天器上的极紫外成像望远镜和高能相对论核与电子仪器进行观测。我们研究与中心子午线附近的冠状物质抛射(CME)相关的质子事件。观测表明,在冠状莫顿波横越太阳的西半球期间,最初注入了≥10 MeV质子,这是CME发射的早期标志。在CME升空期间,与CME相关的质子开始加速。当主要的质子产生发生在几个小时后,当CME在行星际介质中膨胀时。在第一次质子产生和最大强度时间之间。观察到光谱软化。我们将详细分析l997年9月24日的活动。事件的发展表明频谱软化可能是由于加速机制的变化所致。因此质子的产生从强度较低但光谱较硬的注入开始,然后转移到距离太阳较远的强度较高但光谱较软的注入。

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