stellar wind

stellar wind的基本解释

-

(恒)星风

与stellar wind相关的网络例句 [注：此内容来源于网络，仅供参考]

For A-early F type MS stars, stellar chromospheric activity decrease with stellar rotation period, but increase with Rossby number; For M type MS stars, stellar chromospheric activity increase with stellar rotation period and Rossby number, and stellar chromospheric activity reach saturation at large color index; For the MS stars between mid-F to M type, stellar chromospheric activity decrease with stellar rotation period and Rossby number.

在第五章中，我们采用不同的磁活动指数研究了晚型恒星磁活动与恒星自转参量(自转周期、Rossby数)、磁活动与恒星色指数以及恒星磁活动指数之间的相关性。大样本分析显示晚型主序恒星的色球活动与恒星自转参量的研究晚型主序恒星的色球活动与恒星自转参量间的关系表现出对恒星光谱型的依赖。

The author discussed the effect of opacity on stellar evolution and concentrated on the mechanism of triggering blue loop by using Padova stellar model. It shows that extended mixing at the bottom of the convective envelope changed the interior hydrogen profile, which triggers or suppresses blue loop. Laboratory astrophysics, which is a cross subject of astrophysics and plasma physics, combines the demand of accurate data of radiative opacity with the latest advances in high intense lasers to devise the third independent method to study the radiative opacity. On the basis of the comparison between stellar material and laser-produced plasma in terrestrial laboratory, the desirable way to study opacity in laboratory and the brief introduction to the experiments relative to opacity are given.

本论文就开展辐射不透明度实验室研究的背景、内容和意义进行了介绍，并在对实验室的激光等离子体和天体环境下的恒星物质两者差异和相关性的认识基础上，论证了开展辐射不透明度实验室研究的可行性，而且对世界上正在开展的类似研究予以简要介绍，期望可以将天体物理领域对辐射不透明度数据可靠程度的质疑以及对其准确数值的广泛要求，与激光等离子体物理实验的最新进展相结合，推进辐射不透明度实验室研究，为辐射不透明度的研究开拓了继天文观测和理论计算的第三种独立的手段。

Their shells, which apart from hydrogen, helium, and carbon also contain portions of the heavy elements formed in the stellar core, are inherently unstable, and their pulsing creates a withering stellar wind a billion times stronger than the solar wind we know today.

它的壳层除了氢层、氦曾和碳层外还有包含一部分产生自恒星核心的重元素，天生的不稳定，它们的脉动产生了一种毁灭性的星风，比我们现在知道的太阳风要强数百万倍。

与stellar wind相关的网络解释 [注：此内容来源于网络，仅供参考]

stellar wind：恒星风

另外四颗则显示物质流出的证据,不是作为恒星风(stellar wind)延伸出来,就是像来自于拱星盘的风. 其中一颗恒星的尘埃区域似乎比预计的更接近这颗恒星. 尘埃如此接近恒星,因此温度可能高得足以让它们蒸发. 但实际情况并不是这样,

stellar wind：星风

恒星风 星风(Stellar Wind)是恒星表面发出的物质流,是恒星质量流失的一种手段. 星风在所有恒星中都普遍存在,但速度和强度有很大差别. 太阳发出的星风通常称为太阳风,速度大约为每小时

stellar wind：[天]恒星风

stellar /星的/似星的/恒星的/主要的/ | stellar wind /[天]恒星风/ | stellarator /[物]彷星器/

normal stellar wind：正常星风

normal steel casting 普通铸钢 | normal stellar wind 正常星风 | normal stochastic process 正态随机过程