Coronal Mass Ejections and the Rotational Bursting of F-Coronal Dust

该计划将研究F- 日冕尘埃粒子达到高密度（>108质子/立方厘米） F-日冕区域的物质抛射。 F-的旋转爆发 日冕尘埃的发生是由于高自旋造成的张力 速率，可以由四个自旋机制驱动。 将研究四种不同的自旋机制 从理论上讲，这一建议。 从母粒子和它的 碎片会改变尘埃的大小分布， 最终导致将所得的较小颗粒从 太阳系受到太阳辐射压力的作用 克服太阳的引力 #

The program will investigate the rotational bursting of F- Coronal dust particles to high density (>108 protons/cm3) Coronal Mass Ejections in the F-Coronal region. Rotational bursting of F- Coronal dust make take place due to the tension caused by high spin rate, which can be driven by four spin mechanisms. Four different spin mechanisms will be investigated theoretically by this proposal. Repeated rotational bursting from the parent particle and its fragments will alter the size distribution of the dust, and ultimately result in ejecting the resulting smaller particles from the solar system by the action of solar radiation pressure overcoming the gravitational attraction of the Sun. #