Vortex structure of neutron stars with CFL quark cores     

D. M. Sedrakian  K. M. Shahabasyan  D. Blaschke  M. K. Shahabasyan 《Astrophysics》2008,51(4):544-558

The Ginzburg-Landau equations are derived for the magnetic and gluomagnetic gauge fields of nonabelian semi-superfluid vortex filaments in color superconducting cores of neutron stars containing a diquark CFL condensate. The interaction of the diquark CFL condensate with the magnetic and gluomagnetic gauge fields is taken into account. The asymptotic values of the energies of these filaments are determined from the quantization conditions. It is shown that a lattice of semi-superfluid vortex filaments with a minimal quantum of circulation develops in the quark superconducting core during rotation of the star. The magnetic field in the core of this vortex is on the order of 10¹⁸ G. A cluster of proton vortices, which develops in the hadron phase surrounding every superfluid neutron vortex owing to an entrainment effect, creates new semi-superfluid vortex filaments with a minimal quantum of circulation in the quark superconducting core. Translated from Astrofizika, Vol. 51, No. 4, pp. 633–646 (November 2008).  相似文献   

Isolated spheroidal geophysical vortices     

A. Viúdez 《地球物理与天体物理流体动力学》2016,110(1):50-77

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Frequency staircases in narrow-gap spherical Couette flow     

Andrew M. Soward  Andrew P. Bassom 《地球物理与天体物理流体动力学》2016,110(2):166-197

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砒砂岩区小流域沟冻融风化侵蚀模型研究   总被引：13，自引：0，他引：13  

杨具瑞  方铎  毕慈芬  乔旺林  李桂芬  李文萍 《中国地质灾害与防治学报》2003,14(2):87-93

文章通过砒砂岩区西召沟小流域冻融风化侵蚀实测资料,分析了冻融风化侵蚀与沟道各变量之间的关系。确定了该流域相同种类支沟上、中、下游的冻融风化坡面侵蚀模数、单位沟沿线沟角线长度和侵蚀量值,不同种类支沟冻融风化坡面蚀模数及单位长度沟沿线沟角线长度和的侵蚀量的比例关系,及上、中、下游冻融风化侵蚀侵蚀量的比例关系。据此建立了小流域单位长度沟沿线沟角线冻融风化侵蚀量比例模型和冻融风化侵蚀模数比例模型。根据西召沟小流域上游20条沟谷的资料,利用两种模型对该流域的冻融风化侵蚀量进行了模拟计算,两种模型的模拟计算结果分别为23757．9t和29165．1t,相差18．5％。  相似文献   

Exposure to extreme climate decreases self-rated health score: Large-scale survey evidence from China     

《Global Environmental Change》2022

High temperature is a growing threat and impacts public health through different exposure mechanisms. Our study constructs a comprehensive exposure measurement based on temperature variability, duration, and effective influence range. We investigate human responses to high temperatures through self-rated health scores based on individual-level data from China Labor-force Dynamic Survey (CLDS). Results show that higher temperature and temperature variability significantly decrease self-rated health scores. Subjective health risk is most significantly related to the cumulative temperature in the previous two weeks. We also find that the exposure effects at night and on weekdays are more severe. Workers who experience greater exposure from commuting and work environments are negatively impacted by high temperatures. In addition, men, the elderly, middle and low education groups, rural residents are more likely to be impacted by high temperatures.  相似文献   

数值模式垂直分辨率对台风大涡模拟的影响          下载免费PDF全文

张威  谈哲敏 《气象科学》2021,41(6):711-719

随着计算能力的提升,台风数值模拟大量采用了大涡尺度模拟,其水平分辨率已达到数10 m的量级,而垂直分辨率提升不大,其问题是数值模式的垂直分辨率对台风大涡模拟的影响如何?因此,本文利用WRF(Weather Research and Forecasting)模式开展理想台风模拟,在不同的模式垂直层次(42,69和90层)情况下,研究并讨论数值模式垂直分辨率对台风大涡模拟的影响。结果表明,42层的垂直分辨率明显不足,而69层和90层的垂直分辨率则都能模拟出细致的台风边界层小尺度结构,龙卷尺度涡旋出现较多。与69层试验相比,90层试验模拟的台风强度要弱、龙卷尺度涡旋数量要少,但模拟的台风强度更稳定,模拟的小尺度涡旋也更精细。  相似文献   

Long‐term evolution of the magnetic field generated by an ensemble of Rossby vortices     

E. Tikhomolov  V. Mordvinov 《Astronomische Nachrichten》2001,322(3):189-195

The evolution of the large‐scale component of the magnetic field generated by an ensemble of Rossby vortices is numerically simulated. The distribution of the Rossby vortices excited at the beginning of each Carrington rotation is determined from the analysis of Kitt Peak synoptic maps. Our model also considers 11‐year hydrodynamic and 22‐year magnetic field oscillations. In the vicinity of the Rossby vortices, the toroidal magnetic field is significantly amplified and the sign of the angle between the rope of the field lines and the equator is in accordance with observations for “normal” sunspots. We also suggest the possibility of the interpretation by our model of “abnormal” sunspot phenomena. We find that an inverse cascade, namely, the merging of Rossby vortices, gives rise to the formation of large‐scale hydrodynamic structures with a life‐time on the order of a solar cycle period. We conclude from this that the formation of such structures can thus explain the appearance of long‐lived, large‐scale component in the distribution of the magnetic field.  相似文献