發(fā)布時(shí)間：2018-06-12 17:08

  本文選題：等離子體加熱 + 日冕物質(zhì)拋射��； 參考：《科學(xué)通報(bào)》2016年34期

【摘要】：正太陽爆發(fā)活動(dòng)是指太陽大氣中磁場的劇烈變化引起的各類等離子體加熱、加速和輻射增強(qiáng)現(xiàn)象,主要表現(xiàn)形式為日冕物質(zhì)拋射和太陽耀斑,前者可拋射出巨量的磁化等離子體至行星際空間;后者可在短時(shí)間內(nèi)釋放出大量的高能粒子與輻射.它們是導(dǎo)致日地空間災(zāi)害性天氣事件的重要源頭.太陽爆發(fā)的研究涉及到多個(gè)重要的科學(xué)問題,包括磁
[Abstract]:Positive solar burst activity refers to all kinds of plasma heating, acceleration and radiation enhancement caused by dramatic changes in the magnetic field in the solar atmosphere, mainly in the form of coronal mass ejections and solar flares. The former can emit a huge amount of magnetized plasma into interplanetary space, while the latter can release a large number of high energy particles and radiation in a short time. They are an important source of severe weather events in solar-terrestrial space. The study of solar eruptions involves a number of important scientific issues, including magnetism
【作者單位】： 中國天文學(xué)會(huì)太陽與日球?qū)I(yè)委員會(huì)-青年研討會(huì)聯(lián)絡(luò)組;
【分類號(hào)】：P182-2
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本文編號(hào)：2010414