太阳表面 - 翻译成英语

sun's surface
the solar surface
太阳 表面

在 中文 中使用 太阳表面 的示例及其翻译为 英语

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我们的最终目标是将我们在模型中看到的影像映射到太阳表面,这样我们就能作出预测。
Our ultimate goal is to map what we're seeing in the model to the sun's surface so that we can then make predictions.”.
如果模型中只有带电粒子,磁场就会卡住,无法在太阳表面之外出现。
With only charged particles in the model, the magnetic fields were stuck, and couldn't rise beyond the sun's surface.
图中,太阳表面正在远离我们的区域以红色表示,正在靠近我们的区域以蓝色表示。
Areas of the solar surface moving away from us are shown in red tones and approaching regions are shown in blue.
年12月,科学家观察到洛夫乔伊彗星成功通过了太阳表面上方516,000英里的强烈加热而幸免于难。
In December 2011, scientist watched as Comet Lovejoy managed to survive the intense heating as it passed 516,000 miles above the solar surface.
上升到太阳表面的磁通量在称为太阳周期的周期中随时间变化。
The amount of magnetic flux that rises up to the Sun's surface varies with time in a cycle called the solar cycle.
太阳表面的黑点和太阳大气中的磁场中断可能导致广泛的技术干扰。
What begins with dark spots on the Sun's surface, and magnetic field disruptions in the Sun's atmosphere, can result in widespread technological disturbance.
这比太阳表面的温度还要热上5倍,太阳表面只有10340华氏度。
That's 5 times hotter than the surface of the sun, which is 10,340 degrees Fahrenheit.
太阳表面的发光比日冕强100万倍,所以要想观测太阳大气需采取一些特殊措施。
The light coming from the surface of the sun is a million times brighter than the corona, requiring special measures to see the solar atmosphere.
太阳表面-我们可以看到的部分-的温度约为5500°C(10000°F)。
The surface of the Sun- the part we can see- is about 10,000 degrees Fahrenheit(5,500 degrees Celsius).
奇怪的是,靠近太阳表面的地方却不存在有组织的风,而在外围的行星之间,却有真正的阵风。
Curiously, there is no organized wind close to the sun's surface, yet out among the planets there blows a veritable gale.
大量物质的温度比太阳表面还高好几倍,将1600千米以内的一切尽数点燃。
Much of the material was many times hotter than the surface of the sun and ignited everything within a thousand miles.
此外,太阳表面覆盖着数以百万计,尺度在50-1,000公里的小磁化区域。
Furthermore, the surface of Sun is covered with millions of small magnetized regions 50- 1,000 km across.
这种太阳风会很狂暴而且太阳表面的大爆发将造成太阳风的大范围扰动。
This solar wind can be very turbulent, and big eruptions on the solar surface will create major perturbations in the wind.
自转常数通过测量多种太阳表面特征(示踪物“tracers”)得到。
The rotation constants have been measured by measuring the motion of various features("tracers") on the solar surface.
太阳表面的重力加速度为地球表面重力加速度的28倍。
At the surface of the Sun, the acceleration of gravity is 28 times that at the surface of the Earth.
它还在太阳表面之下的区域发生着,类似地也在银河系中大多数恒星上存在。
It also takes place in the layers beneath the solar surface, among other places, and similarly in most stars in our galaxy.
帕克距离太阳表面约2400万公里处的等离子体也以比预期快得多的速度绕太阳旋转。
The plasma at Parker's distance of about 24 million kilometers above the solar surface also whips around the sun much faster than expected.
这些方法使用太阳表面的磁场分布,或是太阳日冕中等离子体分布基于物理的反转。
Such methods use either magnetic field distributions on the Sun's surface or physics-based inversions of the plasma distribution in the Sun's corona.
它可以是靠近太阳表面的,也可能埋藏在太阳内部的深处,或是分布在很宽的深度范围内。
It could be close to the solar surface or deep inside the sun- or over a wide range of depths.”.
地球核心处的温度比太阳表面还高,你将会被煮熟。
The centre of the earth is hotter than the surface of the sun, so you would cook.
结果: 154, 时间: 0.0262

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