The symmetry energy and incompressibility constrained by the observations of glitching pulsars     

Yan Yan 《天文和天体物理学研究(英文版)》2019,(5):101-112

We investigate the masses of glitching pulsars in order to constrain their equation of state(EOS). The observations of glitches(sudden jumps in rotational frequency) may provide information on the interior physics of neutron stars. With the assumption that glitches are triggered by superfluid neutrons, the masses of glitching neutron stars can be estimated using observations of maximum glitches.Together with the observations of thermal emission from glitching pulsars Vela and J1709–4429, the slope of symmetry energy and incompressibility of nuclear matter at saturation density can be constrained.The slope of symmetry energy L should be larger than 67 MeV while the lower limit of incompressibility for symmetric nuclear matter K_0 is 215 MeV. We also obtain a relationship between L and K_0:6.173 MeV + 0.283 K_0≤ L ≤ 7.729 MeV + 0.291 K_0. The restricted EOSs are consistent with the observations of 2-solar-mass neutron stars and gravitational waves from a binary neutron star inspiral.  相似文献   

Assessing the performance of a large-scale irrigation system by estimations of actual evapotranspiration obtained by Landsat satellite images resampled with cubic convolution     

《International Journal of Applied Earth Observation and Geoinformation》2019

Remote sensing techniques allow monitoring the Earth surface and acquiring worthwhile information that can be used efficiently in agro-hydrological systems. Satellite images associated to computational models represent reliable resources to estimate actual evapotranspiration fluxes, ET_a, based on surface energy balance. The knowledge of ET_a and its spatial distribution is crucial for a broad range of applications at different scales, from fields to large irrigation districts. In single plots and/or in irrigation districts, linking water volumes delivered to the plots with the estimations of remote sensed ET_a can have a great potential to develop new cost-effective indicators of irrigation performance, as well as to increase water use efficiency. With the aim to assess the irrigation system performance and the opportunities to save irrigation water resources at the “SAT Llano Verde” district in Albacete, Castilla-La Mancha (Spain), the Surface Energy Balance Algorithm for Land (SEBAL) was applied on cloud-free Landsat 5 Thematic Mapper (TM) images, processed by cubic convolution resampling method, for three irrigation seasons (May to September 2006, 2007 and 2008). The model allowed quantifying instantaneous, daily, monthly and seasonal ET_a over the irrigation district. The comparison between monthly irrigation volumes distributed by each hydrant and the corresponding spatially averaged ET_a, obtained by assuming an overall efficiency of irrigation network equal to 85%, allowed the assessment of the irrigation system performance for the area served by each hydrant, as well as for the whole irrigation district. It was observed that in all the investigated years, irrigation volumes applied monthly by farmers resulted generally higher than the corresponding evapotranspiration fluxes retrieved by SEBAL, with the exception of May, in which abundant rainfall occurred. When considering the entire irrigation seasons, it was demonstrated that a considerable amount of water could have been saved in the district, respectively equal to 26.2, 28.0 and 16.4% of the total water consumption evaluated in the three years.  相似文献   

Mechanism of sea ice formation based on comprehensive observation data in Liaodong Bay,China     

SHI Yongfang  YANG Yongzeng  TENG Yong  SUN Meng  YUN Shengjun 《海洋湖沼学报（英文）》2019,(6):1846-1856

Sea ice disaster is one of the principal natural hazards that affect some coastal areas of China,and the formation of ice cover in a wave field has important characteristics.However,analysis of the mechanism in which waves affect the thermodynamic process of sea ice is lacking,and the influence of waves is not taken into consideration in numerical models of sea ice,largely because of a lack of simultaneous observations of waves and sea ice.Using observational data of the sea ice cycle in the coastal waters of Liaodong Bay(China),we analyzed the characteristics of hydrology,meteorology,and sea ice thickness during the formation of sea ice,and explored the changes in the interrelationships among heat fluxes,waves,and sea ice under actual sea conditions.The results could provide a decision-making support as a reference to the establishment and improvement of China's early waming system to sea ice disasters,and the protection of ice drilling operations and production platform safety.  相似文献   

亚非副热带西风急流入口区位置及动能异常对中国华北盛夏年代际干旱的影响   总被引：1，自引：0，他引：1  

魏建宁  张杰 《高原气象》2021,40(2):281-291

研究使用了欧洲中期天气预报中心(ECMWF)提供的全球再分析数据,通过局地多尺度能量涡度分析法(MS-EVA)研究7-8月亚非急流入口区域的位置及能量变化对华北地区干旱的影响.结果发现:7月亚非急流入口区域在1997年之后有明显的北抬趋势,使得北大西洋及欧洲辐射的能量更易进入急流;8月亚非急流入口区域在1997年后有东...  相似文献   

弱地形上内潮生成问题——Ⅱ.粗糙地形情况下水深对内潮能通量的影响     

戴德君  乔方利  袁业立 《海洋科学进展》2007,25(3):247-256

前人在讨论水深对内潮能通量影响的时候得出结论:有限深海洋中海面对内潮的反射使得正压潮向内潮的能量转化相比较无限深海的情况显著降低,对于选定的地形,在无限深海假定下得到的能通量是该地形上内潮能通量的上限。鉴于前人所研究的基本上都是平滑的地形,而实际的海洋地形总是比较粗糙的,本文探讨了粗糙地形上内潮能通量随水深的变化。选取了弦函数地形、随机白噪声地形、弦函数地形叠加在高斯地形之上、随机白噪声地形叠加在高斯地形之上和随机白噪声地形与弦函数地形同时叠加在高斯地形之上5种情况进行了研究,发现对于这5种情况,都存在海洋有限深时的能通量大于无限深假定时的能通量,这说明前人得出的"有限深海洋中海面对内潮的反射使得正压潮向内潮的能量转化相比较无限深海的情况显著降低"的结论对于粗糙地形并不适用。  相似文献   

青藏高原东部暴雨的中尺度有效位能收支分析          下载免费PDF全文

Kuo Zhou  Lingkun Ran  Yi Liu  Xiuxia Tian 《大气和海洋科学快报》2021,14(2):53-59

针对2018年7月10-11日青藏高原东部一次暴雨过程,利用模式模拟资料分析了有效位能分布特征,成因及其对降水发展演变的影响.结果表明,有效位能主要分布在对流层低层4km以下和高层8-14km,高层有效位能和降水有更好的对应性西北冷平流和降水粒子下落的蒸发作用是低层有效位能高值中心的主要成因,而降水过程释放潜热带来的热...  相似文献   

珠峰和曲宗站2005年4,5月近地辐射能收支初步分析   总被引：10，自引：10，他引：0  

李茂善  马耀明  仲雷  吕世华 《高原气象》2006,25(6):1008-1013

利用中国科学院又一次珠穆朗玛峰地区科学考察(2005年4,5月)期间获得的辐射资料分析该地区地表辐射能的日变化,以及不同海拔高度、不同下垫面辐射各分量的异同,同时分析了不同海拔高度地表反照率在4月和5月的月变化和日变化。  相似文献   

河西走廊风速变化及风能资源研究   总被引：24，自引：9，他引：15  

王毅荣  张存杰 《高原气象》2006,25(6):1196-1202

利用河西走廊地区25年风速气候资料和风塔周年资料,研究了该区域近地面风速及风能的演变和分布。结果表明:河西走廊绿洲内风速下降十分明显,而其它高山站风速比较稳定,没有明显的减少趋势;风速变化具有周期振荡特点;垂直风速差由近地面向上减小,高层风速极大(小)值滞后于低层;风速随高度按自然对数规律增大,风能距地面8 m层内随高度变化迅速;该地区4~12 m/s风居多,是风能的主要贡献者;2~4月风速最大,1,5月最小;该地区风能丰富,10~70 m层内年风能储量在2200 khW/m2以上。  相似文献   

太原冬季采暖期气温变化特征与节能效应分析     

李瑞萍  李鸽 《气象科技》2008,36(6):776-778

采用太原市1951～2003年冬季采暖期逐日气温资料,应用气候方法分析了采暖期平均气温以及与能耗相关的采暖初日、终日、采暖度日等要素的变化特征.结果表明:采暖期气温存在明显升高趋势.而且在20世纪80年代末发生跃变;采暖初日在逐年推后,采暖终日的年代际变化振荡较大,90年代以来有明显提前趋势,采暖期在逐年缩短;采暖度日存在明显减少趋势.结合供暖指标,分别从平均气温升高、采暖期缩短及采暖度日减少等方面进行节能效应分析,指出有必要改变传统的采暖模式.城市采暖具有很大的节能潜力.  相似文献   

On the total kinetic energy of our galaxy     

S. Ninkovi&#x; 《Astronomische Nachrichten》1992,313(2):83-89

The total kinetic energy of the Galaxy is estimated from the potential energy by applying the virial theorem. The limits of the potential energy depend strongly on the value of the local escape velocity. They are estimated to be between −7. 10¹⁶ M_Ȯ km²s⁻² and −1. 10¹⁶ M_Ȯ km²s⁻² (escape velocity approximately between 450 km s⁻¹ and 600 km s⁻¹). The specific kinetic energy of the Galaxy as a whole is most likely about 21 000 km²s⁻², being equally distributed among the subsystems if the local escape velocity is near its lower limit; the higher the local escape velocity is, the higher is the specific kinetic energy of the Galaxy due to the influence of the dark corona. The specific kinetic energy of the dark corona tends to become equal to that of the Galaxy as a whole for very high values of the local escape velocity. For the purpose of estimating the totl potential energy of the Galaxy, inter alia, a new model of the Milky Way is developed, which yields both the potential and the density analytically so that it is suitale for calculating the galactocentric orbits.  相似文献