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

该计划将研究F-日冕尘埃粒子在F-日冕区域以高密度（bbb108质子/cm3）日冕物质抛射的旋转爆发。高自旋速率引起的张力使F-日冕尘埃发生旋转爆裂，其驱动机制有四种。这一提议将从理论上研究四种不同的自旋机制。母粒子及其碎片的反复旋转爆炸将改变尘埃的大小分布，并最终在太阳辐射压力克服太阳引力的作用下，将产生的更小的粒子喷射出太阳系。＃

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. #