Solar mass

The influence of the variation of solar mass on the orbital elements of asteroids

太阳质量变化对小行星轨道根数的影响

The evolutionary track in the H-R diagram of model stars of 1.2 solar mass

1.2太阳质量的模型恒星在赫-罗图上的演化程

From observations of molecular clouds , astronomers estimate a typical Jeans value of roughly one solar mass .

从分子云的观测上，天文学家推估出典型的金斯质量数值约为一个太阳质量左右。

The Schwarzschild radius of a solar mass black hole is about3km .

太阳质量的黑洞的史瓦西半径约为3公里。

Astronomers tried to estimate what solar mass could produce the required luminosity to explain liquid water on these planets .

天文学家试图去推测是太阳质量是多少才能产生需要的发光度来解释这两个星球上的液体水。

The Gaussian constant is based on solar mass , so the Au was inextricably tied to the mass of the sun .

高斯常数是基于太阳质量的，因此，天文单位与太阳的质量是密不可分的了。

Thickness of Neutron-skin in ~ ( 208 ) Pb and Radius of a 1.4 Solar Mass Neutron Star

中子皮厚度与中子星半径

The influence of the variation of solar mass on the orbital elements of Asteroids is studied by using the method of Celestial Mechanics with variable mass .

利用变质量天体力学方法研究了太阳质量变化对小行星轨道根数的影响。

All the mass measurements that have been done to date of these neutron stars where you see the pulsations * all of them are very close to1.4 solar mass .

对于这些中子星的，质量测量，你看到脉冲，所有的都很接近于。，1。4倍的太阳质量，对此有个很好的解释。

By adding isospin dependent high order correction terms to existing relativistic mean field models , the thickness of neutron-skin in ~ ( 208 ) Pb and the radius of 1.4 solar mass neutron star are studied .

在相对论平均场理论框架下在拉氏量密度中引入同位旋相关的高阶修正项，研究了中子皮厚度和中子星半径的关系。

With the decrease of the solar mass , namely , with the decrease of the solar gravitational field , the orbital scope of the planet extends , and the form of the elliptic orbit may become flatter .

随着太阳质量变小，即随着太阳引力场变弱，行星椭圆轨道变大，轨道形状变得越来越扁平。

Progress in the Study on the Solar Coronal Mass Ejection

日冕物质抛射研究进展

Speed dependence of solar wind mass flux in the ascending phase of solar activity

太阳活动上升期源表面太阳风质量流量的速度关系分析

Fuzzy Classification of Solar Coronal Mass Ejection Properties

太阳日冕物质抛射特性的模糊分类研究

Solar coronal mass ejections in space weather

日冕物质抛射&空间天气的扰动源

The hydromagnetic nature of solar coronal mass ejections

太阳日冕物质抛射的磁流体力学性质

I 've been stunned to learn about the sheer volume of wind , solar , mass transit , nuclear and more efficient coal-burning projects that have sprouted in China in just the last year .

仅仅在去年一年里，中国各地出现的风能、太阳能、大规模运输、核能和高效的燃煤项目数量之巨，已经让我目瞪口呆了。

99.8 % of the Solar System 's mass is in the Sun , but only 1 % angular momentum in it . This special distribution is closely related with the special formation of the Solar System inevitably .

在太阳系中占质量99.8%的太阳，其角动量却只占太阳系总角动量的1%，这一特殊分布必然与太阳系特殊形成密切相关。

Magnetic reconnection plays a very important role in solar flares , corona mass ejections ( CME ), and other solar activities .

在太阳耀斑、日冕物质抛射（CME）和其他太阳活动现象中，磁重联一直都扮演着至关重要的作用。

Some typical example of the largest magnetic storms , the largest radio burst resulting magnetic storms , the most severe short wave communication disturbance in ionosphere and magnetic storms resulted by the large solar flare with bright mass ejection and two-ribbon flares are also given .

进一步分析了21周最大磁暴、最大射电爆发引起的磁暴，最严重的电离层短波通讯干扰及有明亮物质抛射的大耀斑、双带大耀斑引起的磁暴等典型例子。