论文标题
剂量旋转如何效应对流标准和太阳颗粒尺寸
How Dose Rotation Effect Convection Criterion and Solar Granule Size
论文作者
论文摘要
颗粒的旋转显示与分子的热运动相似，这会影响对流标准和太阳颗粒的大小。颗粒旋转产生旋转的额外压力，并在球形对称的旋转旋转温度中产生旋转的旋转速度和旋转速度的旋转速度等于旋转的旋转尺寸的旋转温度等于旋转的温度，这是旋转速度的等值。对流标准由颗粒的尺寸，温度梯度和旋转速度梯度共同确定。在大多数太阳对流区域中，对流是由温度梯度驱动的，并由旋转速度梯度抑制，太阳速度梯度。在太阳安静区域，颗粒尺寸较大，比对流较大，而自然尺寸较大，而较大的小granuul较大，而较大的granuul尺寸较大，而较大的granuul shiles则是较大的，而较大的granuul尺寸在较大的地方，而较大的尺寸则在在强迫对流中。在太阳活跃区域，旋转速度越大，临界尺寸和温度越小。SOSOSSPOTES具有较小的颗粒和较低的温度。
The rotation of granules shows thermal properties similar to the thermal motion of molecules, which effects convection criterion and solar granule size.The granular rotation generates the rotational additional pressure and corresponding rotational equivalent temperature in the spherically symmetric expansion of the granule.The rotation equivalent temperature represented by the rotational speed and the granular size is combined with the Schwarzschild criterion to obtain a new convection criterion determined jointly by the granular size, temperature gradient, and rotational speed gradient.In most of the solar convection zone, the convection is driven by the temperature gradient and suppressed by the rotational speed gradient.In the solar quiet region, the larger the granular size, the weaker the convection.The small granules with the sizes smaller than the critical size are in natural convection, while the large granules with the sizes larger than the critical size are in forced convection.In the solar active region, the larger the rotational speed, the smaller the critical size and the temperature.So sunspots have smaller granules and lower temperatures.
