Long Term Evolution of Solar Meridional Circulation and Phase Synchronization Viewed Through a Symmetrical Kuramoto Model     

Elena Blanter  Jean-Louis Le Mouël  Mikhail Shnirman  Vincent Courtillot 《Solar physics》2018,293(10):134

The solar-cycle oscillations of the toroidal and poloidal components of the solar magnetic field in the northern solar hemisphere have a persistent phase difference of about \(\pi \). We propose a symmetrical Kuramoto model with three coupled oscillators as a simple way to understand this anti-synchronization. We solve an inverse problem and reconstruct natural frequencies of the top and bottom oscillators under the conditions of a constant coupling strength and a non-delayed coupling. These natural frequencies are associated with angular velocities of the meridional flow circulation near the solar surface and in the deep layer of the solar convection zone. A relationship between our reconstructions of the shallow and the deep meridional flow speed during recent Solar Cycles 21?–?23 is in agreement with estimates obtained in helioseismology and flux-transport dynamo modeling. The reconstructed top oscillator speed presents significant solar-cycle like variations that agree with recent helioseismical reconstructions. The evolution of reconstructed natural frequencies strongly depends on the coupling strength. We find two stable regimes in the case of strong coupling with a change of regime during anomalous solar cycles. We see the onset of a new transition in Solar Cycle 24. We estimate the admitted range of coupling values and find evidence of cross-equatorial coupling between solar hemispheres not accounted for by the model.  相似文献   

High energy phenomena in eta carinae     

Roberto F. Viotti  Lucio Angelo Antonelli  Sonja Rebecchi  Corinne Rossi 《Journal of Astrophysics and Astronomy》2002,23(1-2):19-22

We have investigated with BeppoSAX the long term behaviour of the harder X-ray component of the supposed supermassive binary system η Car along its 5.52 year cycle. We have found that in March 1998 during egress from the last December 1997 eclipse, this component was the same as outside eclipse, but for a large (×3.5) increase of NH _h , that can be attributed to the presence or formation of opaque matter in front of the source near periastron. Unexpectedly, at that time the iron 6.7 keV emission line was 40% stronger. BeppoSAX has for the first time found ahard X-ray tail extending to at least 50 keV, that cannot be adequately fitted with an additional hotter thermal component. The 2–100 keV spectrum of η Car is instead well fitted with an absorbed powerlaw spectrum with photon index 2.53, suggesting non-thermal emission as an alternative model for the core source.  相似文献   

Examples of clustering around high redshift radio-galaxies     

J. M. Deltorn  O. Le Fèvre 《Astrophysics》1995,38(4):379-381

Published in Astrofizika, Vol. 38, No. 4, pp. 677–680, October–December, 1995.  相似文献   

Optical and X-Ray Observations of the Symbiotic System Ag Draconis During Quiescence and Outburst     

Roberto F. Viotti  Rosario González-Riestra  Takashi Iijima  Stefano Bernabei  Riccardo Claudi  Jochen Greiner  Michael Friedjung  Vito Francesco Polcaro  Corinne Rossi 《Astrophysics and Space Science》2005,296(1-4):435-439

We review the main characteristics of the symbiotic system AG Draconis, with special emphasis on its optical and X-ray variations. We also discuss the X-ray to visual energy distribution during quiescence and outburst and describe our spectroscopic and X-ray observations during the 2003 outburst. Based on X-ray observations collected with the XMM–Newton Observatory, on INES data from the IUE satellite, and on optical spectra collected with the Asiago–Cima Ekar, Bologna–Loiano and La Palma–Galileo Italian telescopes.  相似文献   

Large-scale structure in the ELAIS S1 Survey     

E. A. Gonzalez-Solares  S. Oliver  C. Gruppioni  F. Pozzi  C. Lari  M. Rowan-Robinson  S. Serjeant  F. La Franca  M. Vaccari 《Monthly notices of the Royal Astronomical Society》2004,352(1):44-48

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摩擦作用对西南低涡扰动的影响     

卢敬华  李双林 《成都信息工程学院学报》1990,(4)

西南低涡是对流层下层的中尺度扰动。本文在零级近似条件下,采用p坐标系的基本方程组,在边界层内设计两层模式。通过一定的简化方程组后,得到:当Z≤1/2[kL~2/(μ~2Knu~*)] 时,摩擦效应具有二重性,一方面使扰动减弱;另一方面使扰动增强,而前者的影响略大于后者,最终使扰动消失。频率随高度Z的降低而增加。当Z>1/2[kL~2/(μ~2Knμ~*)]时,摩擦作用甚微,几乎可以忽略不计。频率虽然有两个值,但随高度Z的增加,他们趋于一个常值。  相似文献   

Light-curve classification in massive variability surveys – I. Microlensing     

Vasily Belokurov  N. Wyn Evans  Yann Le Du 《Monthly notices of the Royal Astronomical Society》2003,341(4):1373-1384

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Invariance and scaling properties in the distributions of contributing area and energy in drainage basins     

P. La Barbera  G. Roth 《水文研究》1994,8(2):125-135

The cumulative probability distributions for stream order, stream length, contributing area, and energy dissipation per unit length of channel are derived, for an ordered drainage system, from Horton's laws of network composition. It is shown how these distributions can be related to the fractal nature of single rivers and river networks. Finally, it is shown that the structure proposed here for these probability distributions is able to fit the observed frequency distributions, and their deviations from straight lines in a log-log plot.  相似文献   

1990-2020年间念青唐古拉山中段北坡边坝地区冰川变化及气候响应     

张威  李亚鹏  柴乐  唐倩玉  葛润泽  麻浩男 《地理科学进展》2021,40(12):2073-2085

念青唐古拉山作为青藏高原东南缘重要山古冰川分布区,受季风影响,各区域冰川变化特征差异明显。论文通过Landsat TM/ETM+/OLI资料、ASRTMGDEM与气象数据,采用比值—阈值法、目视解译和VOLTA模型,结合实地考察,对1990—2020年间念青唐古拉山中段北坡边坝地区现代冰川进退状况、面积变化、冰储量变化以及冰川变化对气候变化响应特征进行研究。结果表明：① 1990—2020年5条冰川(玉贡拉冰川、玛拉波冰川、祥格拉冰川、孔嘎冰川、贡日—庚东冰川)末端高程逐渐升高,面积和冰储量分别减少30.38 km²和4.64 km³,总体缩减并呈现加速趋势。② 冰川冰储量减少0.14~1.92 km³,总体变化率为0.40%·a^-1。2020年上述5条冰川储量占1990年冰川储量的比例分别为0.70、0.99、0.98、0.91和0.82,显示出冰川规模越大,在短时间尺度的变化量越小。③ 气象数据分析显示,1990—2020年研究区冰川变化受气温升高主导,平均气温变化率为0.51 ℃。水热组合呈现温度升高—降水减少,且在最后10 a日益显著,预测未来冰川变化仍受气温控制并呈加速退缩趋势。④ 区域对比研究表明,念青唐古拉山冰川面积变化总体呈退缩状态,但各区域冰川变化特征差异明显。同时,不同研究方法对同一冰川区冰储量模拟结果相差较大,相对误差范围为34.45%~115.49%,精确的冰储量可对比研究方法仍有待进一步研究。  相似文献   

居住区典型地物热环境的日变化及其相互影响分析     

孙杰  毛智慧  王乐  邓磊 《地球信息科学学报》2020,22(2):279-289

居住区热环境状况是影响局地微气候变化的重要因素,研究居住区地物的热环境特征,对于了解和改善微气候具有重要意义。为了更好地揭示居住区热环境特征,本研究使用热红外成像仪对北京市某校园居住区进行观测,获取了夏季不同天气状况下（晴天、阴天、多云）的24 h热红外影像数据。依据各天气数据和地物属性,系统分析了各地物日变化规律,并通过垂线法判定邻近地物的温度边界范围,进而揭示出地物间温度交互特征。结果如下：① 太阳辐射是影响地物白天温度变化的主要因素,与地物温度呈正相关性;在多云天气下,地物的最高温度滞后至16:00出现,且地物温度曲线呈现连续的“锯齿状”升降趋势,云层的大量运动是导致多云天气下的地物温度波动变化的关键因素;沥青道路在夜间的温度均高于其他地物,并且夜间持续放热,提生周围环境温度;阴影能够有效减少地物吸收的太阳辐射量,降低地物表面温度;植被的冠层厚度与地物温度呈负相关性,因此增加居住区内绿植的冠层厚度,增大区域阴影面积有助于改善局地微气候;② 树木和裸土在06:00和14:00的温度交互作用强烈,表明在地物交界处,全天持续发生显著的热量交换;而夜间至凌晨,草坪与人行道持续进行热量交换,帮助降低路面温度,缓解周围高温状况。  相似文献