排序方式： 共有35条查询结果，搜索用时 218 毫秒
1.
2.
Sadiye Cakmak Jameel-Un Nabi Tahsin Babacan Cevad Selam 《Astrophysics and Space Science》2014,352(2):645-663
The Gamow–Teller (GT) transition is inarguably one of the most important nuclear weak transitions of the spin-isospin στ type. It has many applications in nuclear and astrophysics. These include, but are not limited to, r-process β-decays, stellar electron captures, neutrino cooling rates, neutrino absorption and inelastic scattering on nuclei. The quasiparticle random phase approximation (QRPA) is an efficient way to generate GT strength distribution. In order to better understand both theoretical systematics and uncertainties, we compare the GT strength distributions, centroid and width calculations for \({^{40\mbox{--}60}\mathrm{Ti}}\) isotopes, using the pn-QRPA, Pyatov method (PM) and the Schematic model (SM). The pn-QRPA and SM are further sub-divided into three categories in order to highlight the role of particle-particle (pp) force and deformation of the nucleus in the GT strength calculations. In PM, we study only the influence of the pp force in the calculation. We also compare with experimental results and other calculations where available. We found that the inclusion of pp force and deformation significantly improves the performance of SM and pn-QRPA models. Incorporation of pp force leads to pinning down the centroid value in the PM. The calculated GT strength functions using the pn-QRPA (C) and SM (C) models are in reasonable agreement with measured data. 相似文献
3.
4.
基于植被状态指数的全国干旱遥感监测试验研究(Ⅰ)--资料分析与处理部分 总被引：10，自引：0，他引：10
在收集处理了了1981～1994年连续504旬的由NOAA AVHRR第1、2通道的反射率计算得的NDVI时间系列数据,以及1980～1994年全国102个固定农气观测站的旬土壤湿度资料(-20cm)和相应测站的田间持水量资料基础上,分析了全国NDVI及植被状态指数VCI的时空变化特征,发现NDVI值随季节(旬)分别表现为“双峰型”和“单峰型”的变化,在第17～27旬之间达到极大值,并与作物生长有关,VCI的变化与NDVI的变化呈相反趋势;对资料因站点的分布和密度以及时序位相等差异可能影响资料代表性的探讨认为：因旱情发展有一个过程,故NDVI、SHI的时空特性应该不会影响其分析结果的代表性。综合分析了资料的时空代表性,为干旱遥感监测模型的建立作准备。 相似文献
5.
6.
Marine protected areas (MPAs) are among the most widely accepted methods of marine management. MPAs are not, however, always placed such that they can maximize impact on conservation and livelihoods. Current MPA guidelines fall short in focusing primarily on biophysical criteria, overlooking interrelated socioeconomic factors. We identified 32 socioeconomic factors that influence whether MPA placement has an impact on biodiversity and/or livelihoods and weighted the quality of evidence using a novel “Evidence for Impact” Score. Results suggest that stakeholder engagement, poverty, population density, and strong leadership have most potential to positively impact biodiversity and/or livelihoods, but the direction of impact (i.e., positive or negative) can be context-dependent. We found a generally poor evidence base for impact evaluation of socioeconomic factors: though some factors were highly cited, few studies actually evaluate impact. Results indicate the need for a more interdisciplinary approach to MPA placement and more empirical studies that assess impact. 相似文献
7.
List of forthcoming papers 相似文献
8.
S. O. Selam E. M. Esmer H. V. Şenavcı E. Bahar O. Yörükoğlu M. Yılmaz Ö. Baştürk 《Astrophysics and Space Science》2018,363(2):34
In this study, we have performed simultaneous solutions of light and radial velocity curves of two eclipsing binary systems, V566 Oph and V972 Her. We observed both systems spectroscopically with a very recently installed spectrograph on the 40 cm telescope, T40, located in Ankara University Kreiken Observatory (AUKR), for the first time. We made use of the photometric data from the Hipparcos satellite for V972 Her, while we obtained the photometric observations of V566 Oph by using the 35 cm telescope, T35, located also in our observatory campus. We derived the absolute parameters for both systems and discussed their evolutionary states. In addition to the simultaneous analysis, we have also analyzed the change in mid-eclipse times for V566 Oph, and found cyclic variations, for which we have discussed light-time effect and magnetic activity as their potential origin, superimposed on a secular change due to a mass transfer between the components of the binary. 相似文献
9.
B. Albayrak G. Djurašević S. Selam M. Yilmaz S. Erkapić O. Aksu T. Tanriverdi 《Astrophysics and Space Science》2005,296(1-4):293-296
BVR light curves of the recently discovered eclipsing binary V351 Peg were studied to derive the preliminary physical parameters
of the system. The light curves were obtained at the TüBİTAK* – Turkish National Observatory (TUG) during three nights in
August, 2003. The solutions were made using Djurašević’s inverse problem method. V351 Peg is a system in an overcontact configuration
(f
over∼ 21 %) with a relatively small temperature difference between the components ΔT ≈ 20 K. The results suggest a significant mass and energy transfer from the more massive primary onto the less massive secondary.
The hot area on the less massive star, near the neck region, can be considered as a consequence of this mass and energy exchange
between the components through the connecting neck of the common envelope.
TüBİTAK: The Scientific and Technical Research Council of Turkey. 相似文献
10.
IntroductionSeismologistsinChinahaveestablishedmanyseismologicalmethodsandearthquakepredic-tionfactorsintheearthquakeforecastpracticesinthelastthirtyyears.Atpresent,morethanonehundredseismometricfactorsareusedinthemedium-termandmedium-short-termearthquakepredictions,suchastheb-valuetomirrorthestressstateandthedistributiondegreeofthemedium,themf-valuetoexpressiftheseismicactivityisincreasedornot(WANG,etal,1994),thequanti-tativeparameterA(b)todescribetheseismicactivitiesinadistrict(WU,CAO,19… 相似文献