太阳极区冕洞内小尺度结构的紫外光谱研究

SOHO/SUMER太阳紫外光谱仪的N Ⅳ谱线观测到太阳南极区冕洞内存在许多小尺度结构,其空间尺度约1～几角秒,寿命尺度约1～几min。小尺度结构沿狭缝方向呈条状,视向多普勒速度可至几十km·s-1。在有的南极区冕洞区域内,小尺度结构的视向多普勒速度呈红、蓝移准周期性交错分布,持续时间长达100 min。部分小尺度结构在同一观测窗口的高温Ne ⅤⅢ谱线还可清晰显现。有的小尺度结构在Ne ⅤⅢ速度演化图的时间和位置与N Ⅳ 谱线速度图基本一致,但它们在Ne ⅤⅢ速度演化图中更延展和弥散。N Ⅳ紫外光谱显示部分小尺度结构谱线呈现非高斯形状,谱线两翼速度可达150 km·s-1,与太阳过渡区爆发事件的光谱特征相似。太阳过渡区爆发事件常出现在宁静区,SOHO/SUMER太阳紫外光谱仪的N Ⅳ谱线显示在南极区冕洞也可产生爆发事件,且具有较强的动力学特征。     

Comparisons of ZnO codoped by group IIIA elements (Al, Ga, In) and N: a first-principle study

The electronic structures and effective masses of the N mono-doped and Al-N,Ga-N,In-N codoped ZnO system have been calculated by a first-principle method,and comparisons among different doping cases are made.According to the results,the impurity states in the codoping cases are more delocalised compared to the N mono-doping case,which means a better conductive behaviour can be obtained by codoping.Besides,compared to the Al-N and Ga-N codoping cases,the hole effective mass of In-N codoped system is much smaller,indicating the p-type conductivity can be more enhanced by In-N codoping.     

交流磁场振幅和频率对J_c不均匀超导体谐波的影响

本文采用Jc不均匀超导体模型来研究多晶超导体的磁性质,运用非线性磁通蠕动模型,通过数值模拟得到交流磁化率基波及谐波随温度的变化关系.系统分析了交流磁场振幅和频率改变对Jc不均匀超导体交流磁化率基波及谐波的影响.结果表明,交流磁场振幅和频率的变化对交流磁化率的影响存在显著差异,并归因为交流磁场振幅和频率的改变引起的磁弛豫时间的改变不同所致.上述结果为分析Jc不均匀超导体交流磁化率的实验现象提供了相关依据.     

Spontaneous U（1） Symmetry Breaking in Coupled Bose System

Adding a U(1) symmetry breaking term V^1/2 a(λ₁a₀+λ*₁a^†₀)+V^1/2(λ₂b₀+λ^*₂b^†₀) to Bogoliubov's truncated Hamiltonian H_B for a weakly interacting coupled Bose system, by using the mean-field approximation rather than the c-number approximation, we find that, via a Feshbach resonance at zero temperature, the states of the coupled Bose system are generalized SU(1,1) × SU(1,1) coherent states. The Bose-Einsteincondensation occurs in response to the spontaneous U(1) symmetry breaking.     

策动力为瞬变力的受迫振动

本文用工程数学中复数积分的方法讨论非周期力的受迫振动。     

La1-xNaxMnO3/YSZ膜的化学溶液法制备及输运性能研究

本文采用化学溶液法在钇稳定的二氧化锆(Y-stabilized ZrO2,YSZ)单晶基板上制备了La1-xNaxMnO3(LNMO)膜并对其输运性能进行了研究.X-射线衍射(XRD)结果表明,所获得的LNMO膜为高度(h00)取向;输运结果表明,所制备的LNMO膜表现为外延膜的性能,且La0.7Na0.3MnO3薄膜在300K、0.5T磁场下可获得～5%磁阻值.     

Comparisons of ZnO codoped by group ⅢA elements （Al,Ga, In） and N： a first-principle study

The electronic structures and effective masses of the N mono-doped and Al N, Ga-N, In-N codoped ZnO system have been calculated by a first-principle method, and comparisons among different doping cases are made. According to the results, the impurity states in the codoping cases are more delocalised compared to the N mono-doping case, which means a better conductive behaviour can be obtained by codoping. Besides, compared to the Al-N and Ga-N codoping cases, the hole effective mass of In-N codoped system is much smaller, indicating the p-type conductivity can be more enhanced by In N codoping     

Ag掺杂熔融织构YBCO峰效应研究

本文对Ag掺杂熔融织构YBCO材料的峰效应进行了研究.磁测量结果表明,Ag掺杂不会影响峰效应的产生,但能显著改变峰效应对温度和磁场的依赖关系;峰效应出现的磁场随Ag掺杂量的增加而增高,且适量的Ag掺杂使得高温下仍能出现峰效应.该研究表明,Ag掺杂可以作为显著提高熔融织构YBCO材料磁场下临界电流密度的有效手段,从而可使其在高场下的性能得以显著改善.     

First-Principle Studies on Conductive Behaviors of P-Type ZnO Codoped by N and B

Using a first-principle method, the electronic structures and the impurity formation energy of ZnO, ZnO （N）, ZnO （N＋B）, and ZnO （2N＋B） have been calculated, based on which the feasibility to obtain p-type ZnO ＆ discussed. According to the results, when ZnO is single doped by N, the acceptor level is deep, and the formation energy is negative, so the ideal p-type ZnO can not be obtained by this way. On the contrary, when 2N＋B are codoped into ZnO, the acceptor level becomes much lower, and the formation energy is positive, so it is a better way to obtain p-type ZnO.     

用偏微分证理想气体内能的性质

本文根据理想气体的状态方程及热力学定律，利用高等数学的偏微分方法证明了理想气体的内能完全决定于气体的热力学温度Ｔ，而与体积Ｖ无关。