大质量光子对分裂过程中日冕的加热机制
Mechanism of heating the Solar Corona in the splitting of Massive Photon Pairs
摘要：
在INTERBALL-Tail Probe（1995-2000年）和RHESSI（从2002年至今）项目框架内获得的数据显示，在太阳平静期间，在2-15千电子伏光子能量范围内，日冕X射线强度存在变化。以前，有人提出一种假设，认为这种现象可能与日冕加热的影响有关。本文根据实验数据和宇宙膨胀过程中真空产生的光子对的量子理论，提出了一种新的日冕等离子体加热机制。基于行星际和星系际空间光子对分裂的类似机制也被提出来解释观测到的微波背景辐射。
英文摘要：
Data obtained in the framework of the INTERBALL-Tail Probe (1995-2000) and RHESSI (from 2002 to the present) projects have revealed variations in the X-ray intensity of the solar corona in the photon energy range of 2-15 keV during the period of the quiet Sun. Previously, a hypothesis was proposed that this phenomenon could be associated with the effect of coronal heating. In the present study, a new mechanism of coronal plasma heating is proposed on the basis of the experimental data and the quantum theory of photon pairs that are produced from vacuum in the course of the Universe's expansion. A similar mechanism based on the splitting of photon pairs in the interplanetary and intergalactic space is also proposed to explain the observed microwave background radiation.
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