概括
一个简单的模型显示了由于磁活动导致的太阳辐射变化. 在太阳最大值期间,太阳的亮度更高,1980年的峰值显示出比以前的周期更明显的亮度.
科学领域:
- 太阳物理 太阳物理
- 恒星辐射的辐射量
- 太空天气空间天气
背景情况:
- 总太阳辐射 (TSI) 呈现缓慢的变化.
- 这些变化与太阳的磁性活动有关,特别是明亮的光圈和黑暗的太阳黑子.
- 以前的卫星测量 (ERB和ACRIM) 提供了1981年至1984年的数据.
研究的目的:
- 通过多个太阳周期的磁性活动模拟和重建太阳辐射调节.
- 为了比较近期太阳周期中辐射亮度增强的幅度.
主要方法:
- 开发了一种简单的模型,该模型基于来自明亮磁的过量辐射和来自暗点的减少辐射.
- 与ERB和ACRIM卫星辐射仪数据同时验证该模型 (1981-1984).
- 将模型扩展到1954年,以分析三个11年的太阳周期.
主要成果:
- 该模型成功匹配了总太阳辐射量的观察到的缓慢变化.
- 该模型预测在活动最大时与最小时相比,太阳辐射总是更高.
- 太阳周期在1980年达到顶峰,显示了0.07%的亮度,比前两个周期更明显.
结论:
- 太阳的磁性活动显著调节了太阳总辐射量.
- 尽管太阳黑子数量较少,但最近的太阳周期 (1980年达到顶峰) 显示出更强烈的辐射亮度.
- 太阳黑子振幅和辐射调制之间的关系在所有太阳周期中可能不是线性的.
相关概念视频
Magnetic Flux
The magnetic flux measures the number of magnetic field lines passing through a given surface area. The SI unit for magnetic flux is the weber (Wb). Magnetic flux is a scalar quantity. It depends on three factors: the strength of the magnetic field B, the area through which the field lines pass, and the relative orientation of the field with the surface area.
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Suppose a surface is divided into elements of area dA. For each element, the component of the magnetic field that is normal to the...
Magnetostatic Boundary Conditions
An electric field suffers a discontinuity at a surface charge. Similarly, a magnetic field is discontinuous at a surface current. The perpendicular component of a magnetic field is continuous across the interface of two magnetic mediums. In contrast, its parallel component, perpendicular to the current, is discontinuous by the amount equal to the product of the vacuum permeability and the surface current. Like the scalar potential in electrostatics, the vector potential is also continuous...
Magnetic Field of a Solenoid
A solenoid is a conducting wire coated with an insulating material, wound tightly in the form of a helical coil. The magnetic field due to a solenoid is the vector sum of the magnetic fields due to its individual turns. Therefore, for an ideal solenoid, the magnetic field within the solenoid is directly proportional to the number of turns per unit length and the current. Conversely, the magnetic field outside the solenoid is zero.
Consider a solenoid with 100 turns wrapped around a cylinder of...
Consider a solenoid with 100 turns wrapped around a cylinder of...
Magnetic Field Lines
The representation of magnetic fields by magnetic field lines is very useful in visualizing the strength and direction of the magnetic field. Each of the magnetic field lines forms a closed loop. The field lines emerge from the north pole (N), loop around to the south pole (S), and continue through the bar magnet back to the north pole.
Magnetic field lines follow several hard-and-fast rules:
Magnetic field lines follow several hard-and-fast rules:
Magnetic Damping
Eddy currents can produce significant drag on motion, called magnetic damping. For instance, when a metallic pendulum bob swings between the poles of a strong magnet, significant drag acts on the bob as it enters and leaves the field, quickly damping the motion.
If, however, the bob is a slotted metal plate, the magnet produces a much smaller effect. When a slotted metal plate enters the field, an emf is induced by the change in flux; however, it is less effective because the slots limit the...
If, however, the bob is a slotted metal plate, the magnet produces a much smaller effect. When a slotted metal plate enters the field, an emf is induced by the change in flux; however, it is less effective because the slots limit the...
Energy In A Magnetic Field
If a magnetic field is sustained, there must be a current in a closed circuit or loop, implying some energy has been spent in creating the field. If this energy is not dissipated via the circuit's resistance, it is stored in the field.
Take an ideal inductor with zero resistance. Although it's practically impossible, assume that the coil's resistance is so small that it is practically negligible. The loss of the field's energy to dissipate thermal energy (or heat) is thus negligible.
The energy...
Take an ideal inductor with zero resistance. Although it's practically impossible, assume that the coil's resistance is so small that it is practically negligible. The loss of the field's energy to dissipate thermal energy (or heat) is thus negligible.
The energy...


