active sunspot prominence

简明释义

活动黑子日珥;

英英释义

例句

1.The latest solar activity report highlighted the emergence of new active sunspot prominences on the Sun's surface.

最新的太阳活动报告强调了新的活跃的太阳黑子突出层在太阳表面的出现。

2.Astronomers use specialized equipment to track active sunspot prominences and predict solar flares.

天文学家使用专业设备跟踪活跃的太阳黑子突出层并预测太阳耀斑。

3.The telescope captured a stunning image of an active sunspot prominence, which is a large and bright feature extending outward from the Sun's surface.

望远镜捕捉到一幅惊人的图像，显示了一个活跃的太阳黑子突出层，这是一个从太阳表面向外延伸的大而明亮的特征。

4.Scientists are studying the effects of active sunspot prominence on solar radiation and its impact on Earth's climate.

科学家们正在研究活跃的太阳黑子突出层对太阳辐射的影响及其对地球气候的影响。

5.During the solar storm, we observed several active sunspot prominences that released massive amounts of energy.

在太阳风暴期间，我们观察到了几个活跃的太阳黑子突出层，它们释放了大量的能量。

作文

The sun, our closest star, is a magnificent source of energy and light. It plays a crucial role in sustaining life on Earth. However, the sun is not just a static ball of fire; it is an active celestial body that undergoes various dynamic processes. One of these processes is the occurrence of sunspots and their associated phenomena, such as the active sunspot prominence. Understanding this term requires delving into the intricate workings of solar activity.Sunspots are temporary phenomena on the sun's photosphere that appear as spots darker than the surrounding areas. They are caused by the sun's magnetic field, which inhibits convection and reduces the surface temperature in those regions. Sunspots can vary in size and number, and they often occur in cycles, known as the solar cycle, which lasts about 11 years. During periods of high solar activity, numerous sunspots can be observed, leading to heightened solar phenomena.An active sunspot prominence refers specifically to a type of solar prominence that is associated with these sunspots. Solar prominences are large, bright features extending outward from the sun's surface, often in loop shapes. They are composed of plasma, a hot ionized gas, and can reach heights of several hundred thousand kilometers. Active prominences are particularly dynamic and are linked to regions of strong magnetic activity, which often coincide with sunspots.These active sunspot prominences can have significant implications for space weather and, consequently, for Earth. When they erupt, they can release vast amounts of energy and charged particles into space, a phenomenon known as a coronal mass ejection (CME). CMEs can disrupt satellite communications, navigation systems, and even power grids on Earth. Therefore, understanding the behavior of active sunspot prominences is essential for predicting space weather and mitigating its effects on modern technology.In addition to their practical implications, active sunspot prominences also offer a glimpse into the fundamental processes of astrophysics. Studying these phenomena helps scientists understand the sun's magnetic field and how it influences solar activity. Observations of active sunspot prominences contribute to our knowledge of stellar dynamics and the interactions between magnetic fields and plasma.Moreover, the beauty of active sunspot prominences cannot be overlooked. When viewed through specialized telescopes or instruments, they present a stunning visual display against the backdrop of the sun. The colors and shapes of these prominences can change rapidly, making them a fascinating subject for both amateur and professional astronomers.In conclusion, the term active sunspot prominence encapsulates a dynamic aspect of solar activity that has far-reaching implications for our understanding of the sun and its effects on Earth. By studying these phenomena, we gain insights into the complex interactions of magnetic fields and plasma, while also enhancing our ability to predict and prepare for space weather events. As we continue to explore the mysteries of the sun, active sunspot prominences will undoubtedly remain a key area of interest for scientists and enthusiasts alike.

太阳是我们最近的恒星，是能量和光的宏伟来源。它在维持地球生命方面发挥着至关重要的作用。然而，太阳并不是一个静态的火球；它是一个活跃的天体，经历各种动态过程。其中一个过程就是太阳黑子及其相关现象的出现，例如活跃的太阳黑子突出。理解这个术语需要深入研究太阳活动的复杂运作。太阳黑子是在太阳光球上出现的暂时现象，它们看起来比周围区域暗。它们是由太阳的磁场引起的，抑制了对流并降低了这些区域的表面温度。太阳黑子的大小和数量可以变化，通常以周期性方式发生，被称为太阳周期，约为11年。在高太阳活动时期，可以观察到大量的太阳黑子，导致太阳现象的增强。活跃的太阳黑子突出特指与这些太阳黑子相关的一种太阳突出。太阳突出是从太阳表面向外延伸的大而明亮的特征，通常呈环形。它们由等离子体组成，即一种高温电离气体，可以达到数十万公里的高度。活跃的突出特别动态，通常与强磁活动区域相关，这些区域通常与太阳黑子重叠。这些活跃的太阳黑子突出可能对太空天气产生重大影响，因此对地球产生影响。当它们爆发时，可能会释放出大量的能量和带电粒子进入太空，这一现象被称为日冕物质抛射（CME）。CME可能会干扰卫星通信、导航系统，甚至对地球的电网造成破坏。因此，理解活跃的太阳黑子突出的行为对于预测太空天气和减轻其对现代技术的影响至关重要。除了实际影响之外，活跃的太阳黑子突出还提供了对天体物理基本过程的洞察。研究这些现象有助于科学家了解太阳的磁场以及它如何影响太阳活动。对活跃的太阳黑子突出的观察有助于我们了解恒星动力学以及磁场与等离子体之间的相互作用。此外，活跃的太阳黑子突出的美丽也不容忽视。当通过专门的望远镜或仪器观察时，它们在太阳的背景下呈现出惊人的视觉展示。这些突出物的颜色和形状可以迅速变化，使它们成为业余和专业天文学家都感兴趣的迷人主题。总之，术语活跃的太阳黑子突出概括了太阳活动的一个动态方面，这对我们理解太阳及其对地球的影响具有深远的意义。通过研究这些现象，我们获得了对磁场和等离子体复杂相互作用的深入见解，同时也增强了我们预测和准备太空天气事件的能力。随着我们继续探索太阳的奥秘，活跃的太阳黑子突出无疑将继续成为科学家和爱好者关注的关键领域。