T Felipe,H Socas-Navarro,E Khomenko
T Felipe
Spectropolarimetric temporal series from Fe i λ6301.5 Å and Ca ii infrared triplet lines are obtained by applying the Stokes synthesis code NICOLE to a numerical simulation of wave propagation in a sunspot umbra from MANCHA code. The anal...
EVALUATION OF THE CAPABILITY OF LOCAL HELIOSEISMOLOGY TO DISCERN BETWEEN MONOLITHIC AND SPAGHETTI SUNSPOT MODELS [0.03%]
局部日震学在区分整体太阳黑子模型和意大利面太阳黑子模型能力的评估
T Felipe,A D Crouch,A C Birch
T Felipe
The helioseismic properties of the wave scattering generated by monolithic and spaghetti sunspots are analyzed by means of numerical simulations. In these computations, an incident f- or p1-mode travels through the sunspot model, which prod...
CONSTRAINING RELATIVISTIC BOW SHOCK PROPERTIES IN ROTATION-POWERED MILLISECOND PULSAR BINARIES [0.03%]
限制旋转驱动毫秒脉冲星双星系统中的相对论激波性质
Zorawar Wadiasingh,Alice K Harding,Christo Venter et al.
Zorawar Wadiasingh et al.
Multiwavelength followup of unidentified Fermi sources has vastly expanded the number of known galactic-field "black widow" and "redback" millisecond pulsar binaries. Focusing on their rotation-powered state, we interpret the radio to X-ray...
SUN-TO-EARTH MHD SIMULATION OF THE 14 JULY 2000 "BASTILLE DAY" ERUPTION [0.03%]
2000年7月14日“ Bastille 日”爆发事件的太阳系内模拟计算研究
Tibor Török,Cooper Downs,Jon A Linker et al.
Tibor Török et al.
Solar eruptions are the main driver of space-weather disturbances at the Earth. Extreme events are of particular interest, not only because of the scientific challenges they pose, but also because of their possible societal consequences. He...
STRUCTURE IN THE 3D GALAXY DISTRIBUTION: III. FOURIER TRANSFORMING THE UNIVERSE: PHASE AND POWER SPECTRA [0.03%]
三维星系分布中的结构：第三部分：傅立叶变换宇宙：相位和功率谱
Jeffrey D Scargle,M J Way,P R Gazis
Jeffrey D Scargle
We demonstrate the effectiveness of a relatively straightforward analysis of the complex 3D Fourier transform of galaxy coordinates derived from redshift surveys. Numerical demonstrations of this approach are carried out on a volume-limited...
POLYCYCLIC AROMATIC HYDROCARBONS WITH STRAIGHT EDGES AND THE 7.6/6.2 AND 8.6/6.2 INTENSITY RATIOS IN REFLECTION NEBULAE [0.03%]
具直线边缘的多环芳香烃以及反射星云中的7.6/6.2和8.6/6.2强度比
Alessandra Ricca,Charles W Bauschlicher Jr,Joseph E Roser et al.
Alessandra Ricca et al.
We have investigated the mid-infrared spectral characteristics of a series of polycyclic aromatic hydrocarbons (PAHs) with straight edges and containing an even or odd number of carbons using density functional theory (DFT). For several eve...
Modifying the Standard Disk Model for the Ultraviolet Spectral Analysis of Disk-dominated Cataclysmic Variables. I. The Novalikes MV Lyrae, BZ Camelopardalis, and V592 Cassiopeiae [0.03%]
修改标准盘模型用于类新星MV天龙座，BZ骆驼座和V592 Cassiopeiae 盘主导型密近双星的紫外光谱分析
Patrick Godon,Edward M Sion,Şölen Balman et al.
Patrick Godon et al.
The standard disk is often inadequate to model disk-dominated cataclysmic variables (CVs) and generates a spectrum that is bluer than the observed UV spectra. X-ray observations of these systems reveal an optically thin boundary layer (BL) ...
Heating and Cooling of Coronal Loops with Turbulent Suppression of Parallel Heat Conduction [0.03%]
湍流抑制平行热传导的冕环加热和冷却
Nicolas Bian,A Gordon Emslie,Duncan Horne et al.
Nicolas Bian et al.
Using the "enthalpy-based thermal evolution of loops" (EBTEL) model, we investigate the hydrodynamics of the plasma in a flaring coronal loop in which heat conduction is limited by turbulent scattering of the electrons that transport the th...
Reconnection-Driven Magnetohydrodynamic Turbulence in a Simulated Coronal-Hole Jet [0.03%]
模拟冠洞喷流中的重联驱动磁流体动力学湍流
Vadim M Uritsky,Merrill A Roberts,C Richard DeVore et al.
Vadim M Uritsky et al.
Extreme-ultraviolet and X-ray jets occur frequently in magnetically open coronal holes on the Sun, especially at high solar latitudes. Some of these jets are observed by white-light coronagraphs as they propagate through the outer corona to...
DETECTING EXOMOONS AROUND SELF-LUMINOUS GIANT EXOPLANETS THROUGH POLARIZATION [0.03%]
通过偏振检测自身发光的巨行星周围的系外卫星
Sujan Sengupta,Mark S Marley
Sujan Sengupta
Many of the directly imaged self-luminous gas giant exoplanets have been found to have cloudy atmospheres. Scattering of the emergent thermal radiation from these planets by the dust grains in their atmospheres should locally give rise to s...