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radiation pressure相关的网络例句

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

Some interesting phenomena are observed which related to acoustic streaming and acoustic radiation pressure.

这些现象与声流及声辐射压力有关。

Lyman-# radiation pressure can reverse the infall in the polar regions when the protostar grows to 20 30M, but cannot significantly reduce the accretion rate.

当星坯的质量增长至20-30太阳质量的时候,赖曼alpha辐射压可以使极区的气体下落反转,但是不会把吸积率降低太多。

The modified expression of the broad emission-line profiles ire derived for the outflow kinematics model of the BLR driven by the radiation pressure. Taking into account the difference between the two lines HeI λ5876 and Hβ, it is shown the fact that the observed line width of HeIλ 5876 is broader than that of Hβ cannot be explained by the popular outflow BLR model evoked by W. G. Mathews. For comparison, line profiles of the gravitational infall model and orbital disk model are also calculated; the later is in good agreement with the observations Thereupon, conclusion is reached that the gravitational infall is an important process in the real BLR gas motion.

1推导了辐射压加速宽线云团径向外流,以及引力下落和转动等BLR运动学模型的谱线轮廓表达式,并考虑到光致电离计算表明的云团本身对Hβ和HeIλ5876谱线的辐射差异,用数值方法计算了它们的谱线轮廓,发现普遍流行的辐射加速气体外流模型不能解释HeIλ5876线宽大于Hβ线宽的观测事实,而引力下落模型则可以较好地解释观测,因此我们倾向于认为、径向内流运动很可能是BLR内的发射线云团真实运动的一个重要成分。

As a result, parts of the dust cloud have become stratified, pointing toward Merope. The closest particles are the most massive and the least affected by the radiation pressure. A longer-term result will be the general destruction of the dust by the energetic starlight.

因此,部份尘埃云形成指向昴宿五的层状结构,最靠近昴宿五的尘埃粒质量也最大,因为它们受到辐射压的影响最小,更长期的效应是尘埃微粒会被高能量星光给全部破坏。

Rna - Rns, see "Partitioning of net radiation", for multiple plants the fraction of radiation to each plant is calculated in the radiation section, see "Partitioning of radiation between plants", es is the vapour pressure at saturation, ea is the actual vapour pressure,ρa is air density, cp is the specific heat of air at constant pressure, Lν is the latent heat of vaporisation,Δ is the slope of saturated vapour pressure versus temperature curve,γ is the psychrometer "constant", rs is an "effective" surface resistance and ra is the aerodynamic resistance.

潜在蒸腾量 Etp 根据Monteith(1965)给出的彭曼联合方程形式计算:式中: Rn 为对于蒸腾的有效净辐射量(也就是 Rna - Rns ,见"净辐射划分"-Partitioning of net radiation,对于多重植被,每一株植物的辐射比率的计算见辐射一节的"植物间的辐射划分"Partitioning of radiation between plants); es 为饱和水气压;ea 为实际水气压;ρa 为空气密度; cp 为常压下的空气比热;Lν为汽化潜热;Δ为与温度曲线饱和水气压关系曲线斜率;γ为干湿球湿度计"常数";rs 为"有效"表面阻力;ra 为气动阻力。

The dependence of the spontaneous radiation pressure and ultimate temperature on quantum interference, average photon numbers and Rabi frequencies are analyzed.

分析了原子的自发辐射压力和冷却的最终温度与量子相干强度,拉比频率,平均光子数的依赖关系。

It has been found that the spectral energy density and radiation pressure of a Kerr nonlinear blackbody are larger than those of a normal blackbody, and there is a regular variety of the spectral energy density and radiation pressure in a Kerr nonlinear blackbody with the change of temperature and frequency.

通过和普通黑体比较发现,克尔非线性黑体的光谱能量密度和辐射压强都要比普通黑体大,非线性黑体中的热辐射光谱能量密度和辐射压强随着温度和频率的改变有着规律的变化。

However, solar sail cannot realize all formation control because the direction of the solar sail radiation pressure force is restricted to certain range.

由于太阳光压力的方向受到限制,并非所有编队控制都能利用太阳帆。

Rna - Rns, see "Partitioning of net radiation", for multiple plants the fraction of radiation to each plant is calculated in the radiation section, see "Partitioning of radiation between plants", es is the vapour pressure at saturation, ea is the actual vapour pressure,ρa is air density, cp is the specific heat of air at constant pressure, Lν is the latent heat of vaporisation,Δ is the slope of saturated vapour pressure versus temperature curve,γ is the psychrometer "constant", rs is an "effective" surface resistance and ra is the aerodynamic resistance.

潜在蒸腾量 Etp 根据Monteith(1965)给出的彭曼联合方程形式计算:式中: Rn 为对于蒸腾的有效净辐射量(也就是 Rna - Rns ,见&净辐射划分&-Partitioning of net radiation,对于多重植被,每一株植物的辐射比率的计算见辐射一节的&植物间的辐射划分&Partitioning of radiation between plants); es 为饱和水气压;ea 为实际水气压;ρa 为空气密度; cp 为常压下的空气比热;Lν为汽化潜热;Δ为与温度曲线饱和水气压关系曲线斜率;γ为干湿球湿度计&常数&;rs 为&有效&表面阻力;ra 为气动阻力。

This invention relates to a method and device for generating cold atomic beam. Said method includes heating hot atom source in vacuum chamber to form atomic saturated vapor pressure atmosphere, cooling hot atom by three-D MOT to below 200uk and trapped to form cold atomic cloud, by the quarter wave plate reflection mirror in MOT the laser radiation pressure being unbalanced to make cold atom emitting along said direction, four tape arranged straight line set with contrary current direction is set in atom beam emission direction, which makes the atom emitted to forward to obtain cold atom beam with low speed, large flux and small transverse speed, laser beam vertical with atom beam set in the direction of cold atom emitting for atom beam state preparation to realize state concordant emitted cold atom beam.

本发明涉及一种冷原子束产生方法和装置,该方法包括在抽真空的真空室内,加热热原子源,在真空室中形成相应的原子饱和蒸汽压气氛;采用三维MOT对热原子进行冷却,冷却到200μk以下,并被捕获形成冷原子云团;通过三维MOT中开小孔的四分之一波片反射镜,而使得在该方向上激光辐射压力不平衡,使冷原子沿此方向出射;在冷原子束出射方向上,还置有载有彼此电流方向相反的四根成锥形排列的直导线,从而原子出射时将在磁场的作用下,不会沿横向膨胀而向前射出;便得到了出射速度低的、通量较大的、横向速度非常小的连续冷原子束;同时在冷原子束的出射方向上,设置有与原子束垂直的激光束,用于原子束的态制备,实现态一致的出射冷原子束。

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Breath, muscle contraction of the buttocks; arch body, as far as possible to hold his head, right leg straight towards the ceiling (peg-leg knee in order to avoid muscle tension).

呼气,收缩臀部肌肉;拱起身体,尽量抬起头来,右腿伸直朝向天花板(膝微屈,以避免肌肉紧张)。

The cost of moving grain food products was unchanged from May, but year over year are up 8%.

粮食产品的运输费用与5月份相比没有变化,但却比去年同期高8%。

However, to get a true quote, you will need to provide detailed personal and financial information.

然而,要让一个真正的引用,你需要提供详细的个人和财务信息。