solar prominence

简明释义

日珥

英英释义

A solar prominence is a large, bright feature extending outward from the Sun's surface, often in the shape of a loop or arch, composed of plasma and magnetic field lines.

太阳突起是从太阳表面向外延伸的大而明亮的特征,通常呈环状或拱形,由等离子体和磁场线组成。

例句

1.The high-resolution images captured by the telescope revealed multiple solar prominences 太阳冠 around the sun.

望远镜捕捉到的高分辨率图像显示了太阳周围多个solar prominences 太阳冠

2.Astronomers often study solar prominences 太阳冠 to understand solar activity and its effects on Earth.

天文学家经常研究solar prominences 太阳冠 以了解太阳活动及其对地球的影响。

3.A solar prominence 太阳冠 can last for several days before it either dissipates or erupts.

一个solar prominence 太阳冠 可以持续几天,然后要么消散,要么爆发。

4.The solar prominences 太阳冠 observed during the solar maximum are often more dramatic and larger.

在太阳活动高峰期观察到的solar prominences 太阳冠 通常更加戏剧性和庞大。

5.During the solar eclipse, we could see a beautiful solar prominence 太阳冠 extending from the sun's surface.

在日食期间,我们可以看到一个美丽的solar prominence 太阳冠 从太阳表面延伸出来。

作文

The sun, a massive ball of gas at the center of our solar system, is not just a source of light and warmth; it is also a dynamic and ever-changing celestial body. One of the most fascinating phenomena associated with the sun is the occurrence of solar prominence, which can be described as large, bright features extending outward from the sun's surface. These structures are composed of plasma and can be seen during solar eclipses or through specialized instruments that can filter out the sun's intense brightness. Understanding solar prominence is crucial for both amateur astronomers and scientists alike, as they offer insights into the complex processes occurring on the sun.Solar prominence typically forms in areas of intense magnetic activity. The sun's magnetic field is incredibly powerful and can create loops of magnetic energy that trap hot plasma in the sun's atmosphere. These loops can rise high above the sun's surface, creating the stunning arcs that we observe as solar prominence. They can last for days or even weeks, but eventually, they may collapse back onto the sun or break away into space, contributing to solar winds and other solar phenomena.The study of solar prominence is essential for understanding the sun's behavior and its impact on the solar system. For instance, when these prominences erupt, they can release massive amounts of energy and charged particles into space. This can lead to solar flares and coronal mass ejections (CMEs), which can have significant effects on Earth. Such events can disrupt satellite communications, power grids, and even pose risks to astronauts in space. Therefore, monitoring solar prominence is vital for space weather forecasting and ensuring the safety of technology that relies on satellite systems.In addition to their scientific importance, solar prominence also captivates the imagination of many. During a total solar eclipse, when the moon completely covers the sun, the corona—the outer atmosphere of the sun—becomes visible, allowing observers to witness the beauty of solar prominence in all its glory. The sight of these fiery arcs against the backdrop of the darkened sky is nothing short of breathtaking, reminding us of the vastness and mystery of our universe.Moreover, the study of solar prominence has implications beyond just solar physics. It helps researchers understand stellar evolution and the life cycles of other stars. By comparing the behavior of solar prominence on our sun with that of other stars, scientists can gain insights into the similarities and differences in stellar activity across the galaxy.In conclusion, solar prominence is a remarkable phenomenon that highlights the sun's dynamic nature and its influence on the solar system. From its role in solar flares and CMEs to its stunning visual displays during eclipses, solar prominence serves as a reminder of the complexity of our nearest star. As we continue to study the sun and its various activities, we deepen our understanding of not only our own solar system but also the broader universe in which we reside.

太阳是我们太阳系中心的一个巨大气体球,不仅是光和热的来源,也是一个动态且不断变化的天体。与太阳相关的最迷人现象之一是发生的太阳突出,可以描述为从太阳表面向外延伸的大而明亮的特征。这些结构由等离子体组成,可以在日食期间或通过能够过滤掉太阳强烈亮度的专用仪器观察到。理解太阳突出对于业余天文学家和科学家来说都至关重要,因为它们提供了对太阳上复杂过程的洞察。太阳突出通常形成于强烈的磁活动区域。太阳的磁场极其强大,可以产生捕捉高温等离子体的磁能环。这些环可以高高升起,形成我们观察到的太阳突出的惊人弧形。它们可以持续数天甚至数周,但最终可能会坍塌回到太阳上,或断裂进入太空,进而影响太阳风和其他太阳现象。研究太阳突出对于理解太阳的行为及其对太阳系的影响至关重要。例如,当这些突出物爆发时,它们可以向太空释放大量能量和带电粒子。这可能导致太阳耀斑和日冕物质抛射(CME),这些事件可能对地球造成重大影响。此类事件可能干扰卫星通信、电网,甚至对宇航员在太空中的安全构成风险。因此,监测太阳突出对空间天气预报至关重要,并确保依赖卫星系统的技术的安全。除了科学重要性,太阳突出也吸引了许多人的想象。在日全食期间,当月球完全遮住太阳时,日冕——太阳的外部大气变得可见,使观察者能够目睹太阳突出的美丽。在黑暗天空背景下,这些火焰弧形的景象令人叹为观止,提醒我们宇宙的浩瀚和神秘。此外,研究太阳突出不仅对太阳物理学有影响。它帮助研究人员理解恒星演化和其他恒星的生命周期。通过比较我们太阳的太阳突出行为与其他恒星的行为,科学家可以获得关于银河系中恒星活动的相似性和差异的洞察。总之,太阳突出是一个显著的现象,突显了太阳的动态特性及其对太阳系的影响。从它在太阳耀斑和CME中的作用,到在日食期间的惊人视觉展示,太阳突出提醒我们我们最近的恒星的复杂性。随着我们继续研究太阳及其各种活动,我们加深了对不仅是我们自己的太阳系,还有我们所居住的更广阔宇宙的理解。

相关单词

solar

solar详解:怎么读、什么意思、用法

prominence

prominence详解:怎么读、什么意思、用法