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  energy region
     Calculation and Analysis of ~(58)Ni(p,x) Reaction in Energy Region E_p≤200 MeV
     E_p≤200 MeV能区p+~(58)Ni反应的计算与分析
短句来源
     Measurement of cross sections for ~(58)Ni(n,p)~(58m+g)Co reaction induced by neutrons of 14 MeV energy region
     14 MeV能区中子引起的~(58)Ni(n,p)~(58m+g)Co反应截面测量
短句来源
     The determination of the absolute efficiency of a coaxial Ge(Li) detector in the energy region from 0.3MeV to 10MeV
     在0.3~10MeV能区内Ge(Li)探测器效率的绝对刻度
短句来源
     ANALYSIS ON COSMIC RAY MULTI-μ PHENOMENA IN ENERGY REGION 10~(14)-10~(16) eV
     对10~(14)—10~(16)eV能区宇宙线多μ现象的分析
短句来源
     The suppression coefficients are 2.8, 4.2 and 5.3 in the energy region of 100-500, 500-700 and 700-900 keV respectively for 60Co γ-rays.
     测试结果表明,对~(60)Coγ射线源,它的抑制系数在100—500、500—700、700—900keV能区范围内分别为2.8、4.2和5.3。
短句来源
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  energy range
     Measurement of differential cross sections and cross sections of the ~6Li(n,t)~4He reaction in the 1―2MeV energy range
     1―2MeV能区~6Li(n,t)~4He反应微分截面与截面的实验测量
短句来源
     The neutron capture cross sections of 93Nb, 169Tm, 181Ta, Ag, Hf and W were measured with respect to that of 197Au in the energy range from 10 to 100 keV using the time-of-flight method.
     以~(197)Au为标准,用飞行时间方法,测量了10—100keV能区,~3Nb、~(169)Tm、~1Ta、Ag、Hf和W的中子俘获截面.
短句来源
     Measurement of neutron capture cross section of ~(75)As in the energy range from 29 to 1100 keV
     29—1100keV能区~(75)As中子俘获截面测量
短句来源
     Functional fitting to the efficiency curves of coaxial Ge(Li) and HpGe detectors in the energy range of 122- 1400keV
     122—1400keV能区同轴Ge(Li)和HpGe探测器效率曲线的函数拟合
短句来源
     X-RAY ATTENUATION COEFFICIENTS AND PHOTOELECTRIC CROSS SECTIONS OF Sn FOR THE ENERGY RANGE 3.3 keV TO 29.1 keV
     3.3keV—29.1keV能区Sn的X—射线衰减系数和光电截面(英文)
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  energy regions
     The neutron total cross section of natural copper was evaluated in the energy region from 1keV to 20 MeV, using all experimental data available up to 1979. The data were recommended in three energy regions: from 1keV to 100 keV,in which there are lots of resonance structures,J.
     编评了天然铜元素从1keV到20MeV能区的中子全截面实验测量工作,收集评价了1979年以前各家的实验测量。 全能区分三个能段择优推荐:1keV到100keV系共振结构绸密区,推荐J.
短句来源
     In the ISR and SpS energy regions, when 2×10 -3 ≤ x T(A) <1, K factors decrease markedly as x T(A) becomes smaller, but after x T(A) <2×10 -3 , Their values increase rapidly as x T(A) further decrease.
     在ISR和Sp pS能区 ,当 2× 10 -3 ≤xT(A) <1时 ,K因子随xT(A) 减小而显著减小 ; 而xT(A) <2× 10 -3 时随xT(A) 继续减小又显著增加 .
短句来源
     The lifetimes of the two complexes SiCO(X()~3∑~-)and SiOC(X()~3∑~-) are longer to be about 2.0×10~(-12) sec and the effective energy regions of the two complex reactions are relatively narrow,i. e. ,E_t≤(37.6560) kJ.
     该两个反应均无阈能,络合物寿命较长,一般在2.0×10-12sec左右,有效络合反应能区较窄(初始相对碰撞平动能Et≤37.6560 kJ.mol-1).
短句来源
     In thetwo energy regions:3.600-4.200MeV and 6.425-6.700MeV,the cross sections exhi-bit a smoothly in creasing variation The measured and calculated cross sectionsshow that in the energy range of 3.60-4.20MeV region,the cross sections are notsignificantly influenced by the scattering angle,but in the energy range of 6.425-6.700MeV region,the cross sections are strongly angle-dependent.
     讨论了对背散射分析感兴趣的窄而孤立的强共振峰4250±10KeV随靶厚、角度的变化关系以及截面变化缓慢的平坦区3.6-4.20MeV,6.425-6.700MeV能区的截面值与背散射角度的关系。
短句来源
     The lifetimes of the two complexes HCO +( X 1Σ +) and COH +( X 1Σ +) are generally short to be about 7.0×10 -12 sec and the effective energy regions for the two complex reactions are relatively narrow.
     该两反应均无阈能 ,络合物寿命较短 ,一般为 7.0× 10 - 12 sec左右 ,有效络合反应能区较窄。
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  “能区”译为未确定词的双语例句
     Measurement of Cross Sections for ~(50)Cr(n,2n)~(49)Cr and ~(52)Cr(n,2n)~(51)Cr Reactions Induced by 13.5—14.6 MeV Neutrons
     13.5—14.6MeV能区中子引起的~(50)Cr(n,2n)~(49)Cr和~(52)Cr(n,2n)~(51)Cr核反应截面的测量(英文)
短句来源
     In the region from thermal energy to 17 MeV, the detectable doseequivalent values range from 10~(-4) to 10~2 mrem·h~(-1) and the neutron doseequivalent sensitivity is approximately 140 cps/mrem·h~(-1) for the counter NR1;
     在热能-17MeV能区,NR 1计数器的剂量探测范围约为10~(-4)—10~2mrem/h,中子剂量灵敏度为140cps/mrem·h~(-1);
短句来源
     ENERGY RESPONSE OF A φ 76mm×100mm BGO SCINTILLATION DETECTOR FOR GAMMA-RAYS BELOW 20 MeV
     φ76mm×100mm BGO闪烁探测器在20 MeV以下能区的能量响应
短句来源
     We report the experimental results of the Stark effect in the vicinity of n = 12, 13, 14 of Na in the field from 0-8kV/cm.
     本文报道钠在主量子数n=12,13,14附近能区的斯塔克(stark)效应,外场从0~8kV/cm.
短句来源
     Measurement of Near-Barrier Fusion Excitation Function of ~6Li+~(208)Pb
     近垒能区~6Li+~(208)Pb熔合激发函数测量
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  energy region
The development of avalanches of relativistic runaway electrons is investigated in an experiment similar to the classical Townsend experiment, but in the relativistic energy region.
      
They are complex in shape; in particular, an intense Wien emission component is formed in their high-energy region at high accretion rates.
      
Comparison of the nucleon spectrum with the proton spectrum indicates that the contribution of nucleons from nuclei increases toward the 100-TeV energy region compared to the 1-TeV region.
      
It is shown that in the energy region ~1018-1019 eV the spectrum probably coincides with the injection spectrum whose exponent is equal approximately to 3.2-3.3.
      
The flatter component in the energy region (3.2-5.0)×1019 eV is due to braking of extragalactic protons on primordial photons (the cosmic background radiation).
      
更多          
  energy range
We present the results on variations of ion spectra in the energy range from 1 keV to 3 MeV.
      
The theory predicts that in the 1-100 MeV energy range, where the adiabatic cooling of particles is dominant, ν = 1, while we have derived a ν double-peak distribution.
      
Using the data of ground-based and satellite measurements of the CR intensity in the period under study, we have investigated variations of the rigidity spectrum of protons in the energy range from ~15 MeV to tens of GeV.
      
A new method of determining the spectral index for protons in the energy range about 1013 eV
      
Moreover, they will enable us to considerably extend the accessible energy range and to check predictions of various models of the origin of the highest-energy particles in the Universe.
      
更多          
  energy regions
The energy regions below the fission barrier and above 6 MeV have been scanned with pitches of 0.05 and 0.1 MeV, respectively.
      
This decomposition makes it possible to estimate the contributions of various fission components and to calculate the fissilities of 238U in the photon-energy regions under study.
      
The formation of a giant dipole resonance and quasideuteron absorption are considered as two mechanisms that are responsible for the photoexcitation of a nucleus in the energy regions Eγ ? 20 MeV and Eγ ? 40 MeV, respectively.
      
a transition from the local density of states with a smooth behavior in some energy regions to another one without any smooth part.
      
The formation of singly charged ions in these excitation energy regions is caused by direct photoionization from outermost shell electrons in both Kr and Xe.
      
更多          


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这篇总结性文章论述了由π-p,p-p,-p,γ-N作用产生奇异粒子及奇异粒子与核子相互作用实验方面目前的情况。它是上一篇文章“能量在10Bev以下的π-N,p-N和-N相互作用”的继续和补充。本文概括了最新的关于奇异粒子产生及作用的实验结果。并特别着重于讨论π-p作用产生奇异粒子及奇异粒子与核子相互作用的材料。对π-p作用,区分了近阈能区及高能区的现象,讨论了截面与角分布随能量变化的情况及产生过程中的极化现象,进行了振幅分析,同时列出了稀有事例的最新成果。对于实验数据比较少的p-p,-p及γ-N产生奇异粒子的作用作了简单的归纳。对奇异粒子与粒子相互作用,叙述了K-N作用的总截面、弹性散射、非弹性散射及不同的共振态。在弹性散射方面,研究了微分截面的角分布。在非弹性散射方面,我们看了各种非弹性过程及分枝比。对与π的共振态这一极为重要的现象所提出的二种解释作了叙述。最后还提出了一些问题,特别是对KKππ作用的看法,我们认为这也许是奇异粒子产生及作用中主要的过程。

A cloud chamber experiment is described, in which the angular distribution of secondary particles produced in nuclear interaction by high energy cosmic ray particles with paraffin has been studied. Sixty-four ns ≥4 events with average primary energy of 70 BeV have been analysed. The result shows that, in this energy region, the angular distribution in CMS is not isotropic but possesses maxima in the 0° and 180° directions; furthermore, there is already an appreciable fraction ( 20%) of the events with angular...

A cloud chamber experiment is described, in which the angular distribution of secondary particles produced in nuclear interaction by high energy cosmic ray particles with paraffin has been studied. Sixty-four ns ≥4 events with average primary energy of 70 BeV have been analysed. The result shows that, in this energy region, the angular distribution in CMS is not isotropic but possesses maxima in the 0° and 180° directions; furthermore, there is already an appreciable fraction ( 20%) of the events with angular distribution exhibiting the features given by the "fire-ball" model.

本文描述一个利用云室研究高能宇宙线粒子与石蜡的核作用中次级粒子角分布的实验。共分析了64个n_s≥4的事例,其平均初能E_0≈70BeV。结果表明,在此能区,次级粒子在CMS中,角分布不是各向同性,而在0°和180°方向呈现极大,且有相当比例(≥20%)事例的角分布形式显示出火球模型给出图象。

The reactions of Be9(d, p0)Be10(0), Be9(d, p1)Be10(3.368 MeV), Be9(d, t0)Be8(0), Be9(d, α0)Li7(0) and Be9(d, α1) Li7 (0.478 MeV) have been studied at deuteron bombarding energies from 0.1 to 2.5 MeV. The angular distributions of these five groups of outgoing particles have been measured respectively between θL = 10°?and 155°?at eleven bombarding energies of 0.150, 0.220, 0.401, 0.706, 1.005, 1.301, 1.484, 1.750, 2.000, 2.250 and 2.500 MeV. The excitation functions of the Be9 (d,p0) Be10 reaction have been measured...

The reactions of Be9(d, p0)Be10(0), Be9(d, p1)Be10(3.368 MeV), Be9(d, t0)Be8(0), Be9(d, α0)Li7(0) and Be9(d, α1) Li7 (0.478 MeV) have been studied at deuteron bombarding energies from 0.1 to 2.5 MeV. The angular distributions of these five groups of outgoing particles have been measured respectively between θL = 10°?and 155°?at eleven bombarding energies of 0.150, 0.220, 0.401, 0.706, 1.005, 1.301, 1.484, 1.750, 2.000, 2.250 and 2.500 MeV. The excitation functions of the Be9 (d,p0) Be10 reaction have been measured at θL = 135°? from Ed = 0.1 to 2.5 MeV, at θL = 95°? from Ed = 0.1 to 2.2 MeV and at θL = 112.5°? from Ed, = 0.5 to 2.5 MeV, respectively. By use of thicker targets (100-300 ?μ/cm2) and at Ed = 1.2 MeV, the absolute cross sections of the Be9(d, p0)Be10 reaction were measured at θL = 135°?and 112.5°;? the results obtained are: σp0(θL = 135°= 1.60 mb/st and σp0(θL = 112.5°=1.55 mb/st. Thus, the behaviours of the cross sections of all these five groups of outgoing particles have been obtained in this energy range. These experimental results are discussed to some extent.

本文在E_d=0.1—2.5MeV能量范围内,研究了Be~9(d,p_0)Be~(10)(0),Be~9(d,p_1)Be~(10)(3.368MeV),Be~9(d,t_0)Be~8(0),Be~9(d,α_0)Li~7(0)及Be~9(d,α_1)Li~7(0.478MeV)诸反应。在E_d=0.150,0.220,0.401,0.706,1.005,1.301,1.484,1.750,2.000,2.250和2.500MeV共十一个能量上分别测量了这五群出射粒子在θ_L=10—155°区间的角分布。在θ_L=135°,E_d=0.1—2.5MeV,在θ_L=95°,E_d=0.1—2.2MeV,和在θ_L=112.5°,E_d=0.5—2.5MeV测量了Be~9(d,p_0)Be~(10)的激发函数。在θ_L=135°和112.5°,E_d=1.2MeV,用较厚靶(100—300μg/cm~2)测量了Be~9(d,p_0)Be~(10)(0)反应的截面绝对值,结果为σ_p_0(θ_L=135°)=1.60mb/sr,σ_p_0(θ_L=112.5°)=1.55mb/sr。这样就得到了在此能区...

本文在E_d=0.1—2.5MeV能量范围内,研究了Be~9(d,p_0)Be~(10)(0),Be~9(d,p_1)Be~(10)(3.368MeV),Be~9(d,t_0)Be~8(0),Be~9(d,α_0)Li~7(0)及Be~9(d,α_1)Li~7(0.478MeV)诸反应。在E_d=0.150,0.220,0.401,0.706,1.005,1.301,1.484,1.750,2.000,2.250和2.500MeV共十一个能量上分别测量了这五群出射粒子在θ_L=10—155°区间的角分布。在θ_L=135°,E_d=0.1—2.5MeV,在θ_L=95°,E_d=0.1—2.2MeV,和在θ_L=112.5°,E_d=0.5—2.5MeV测量了Be~9(d,p_0)Be~(10)的激发函数。在θ_L=135°和112.5°,E_d=1.2MeV,用较厚靶(100—300μg/cm~2)测量了Be~9(d,p_0)Be~(10)(0)反应的截面绝对值,结果为σ_p_0(θ_L=135°)=1.60mb/sr,σ_p_0(θ_L=112.5°)=1.55mb/sr。这样就得到了在此能区内,这五群出射粒子的截面情况。对所得结果进行了一些讨论。

 
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