Observation of, and temporal variations in, solar p-mode multiplet frequency asymmetries at  ℓ= 2      

W. J. Chaplin  Y. Elsworth  G. R. Isaak  B. A. Miller  R. New  S. Thiery  P. Boumier  A. H. Gabriel 《Monthly notices of the Royal Astronomical Society》2003,343(1):343-352

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Galaxy voids in cold dark matter universes     

A. J. Benson  Fiona Hoyle  Fernando Torres  Michael S. Vogeley 《Monthly notices of the Royal Astronomical Society》2003,340(1):160-174

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Some statistical aspects of estimating the local red clump absolute magnitude     

Chris Koen  Fred Lombard 《Monthly notices of the Royal Astronomical Society》2003,343(1):241-248

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Impersonal parameters from Hertzsprung–Russell diagrams     

R. E. Wilson  Jarrod R. Hurley 《Monthly notices of the Royal Astronomical Society》2003,344(4):1175-1186

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A Bayesian approach to discrete object detection in astronomical data sets     

M. P. Hobson  C. McLachlan 《Monthly notices of the Royal Astronomical Society》2003,338(3):765-784

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A Faraday rotation template for the Galactic sky     

Patrick Dineen  Peter Coles 《Monthly notices of the Royal Astronomical Society》2005,362(2):403-410

Using a set of compilations of measurements for extragalactic radio sources, we construct all-sky maps of the Faraday rotation produced by the Galactic magnetic field. In order to generate the maps, we treat the radio source positions as a kind of 'mask' and construct combinations of spherical harmonic modes that are orthogonal on the masked sky. As long as relatively small multipoles are used, the resulting maps are quite stable to changes in the selection criteria for the sources, and show clearly the structure of the local Galactic magnetic field. We also suggest the use of these maps as templates for cosmic microwave background (CMB) foreground analysis, illustrating the idea with a cross-correlation analysis between the Wilkinson Microwave Anisotropy Probe ( WMAP ) data and our maps. We find a significant cross-correlation, indicating the presence of a significant residual contamination.  相似文献   

REVIEWS OF GEOGRAPHIC SOFTWARE     

《The Professional geographer》1987,39(1):85-94

Reviews of geographic software in this article: DEMO-GRAPHICS: WORLD POPULATIONS AND PROJECTIONS. ESP GAUSS. CEMODEL S. Damus LIMDEP. William H. Greene MICROSTAT 4.1 OTIS PCIPS. (Personal Computer Image Processing System) . H.J. Meyers and R. Bernstein. REGRESSION ANALYSIS OF TIME SERIES (RATS) SPSS/PC+ URBAN DATA MANAGEMENT SOFTWARE (UDMS)  相似文献   

Extracting star formation histories from medium-resolution galaxy spectra     

H. Mathis  S. Charlot  J. Brinchmann 《Monthly notices of the Royal Astronomical Society》2006,365(2):385-400

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球状星团的天体测量(英)     

王家骥 《天文学进展》1997,(2)

球状星团是银河系中最年老的天体之一，是储存着银河系早期演化珍贵信息的“化石”．球状星团的天体测量，主要包括球状星因天区内恒星相对自行的测定，并由这些相对自行数据采用适当方法定出星团的绝对自行，或者直接测定绝对自行．利用这些自行数据，或者进一步与测光和视向速度数据结合，可以开展与球状星团的距离、运动、动力学状况、质量、年龄、演化等等以及银河系的结构和演化等有关的一系列重要的研究．在本文中对本世纪70年代中期以来在球状星团相对自行测定和成员概率估计、内部运动检测、绝对自行测定和空间运动研究这三方面取得的成果和进展以及存在的问题作了评述．  相似文献   

Implications of low-pass filtering on power spectra and autocorrelation functions of turbulent velocity signals     

《Mathematical Geology》1997,29(5):653-668

Filtering either through the electronics of an instrument or through digital procedure is performed routinely on geophysical data. When velocity fluctuations are measured in turbulent flows using electromagnetic current meters (ECMs), a builtin lowpass Butterworth filter of order n usually attenuates fluctuations at high frequencies. However, the effects of this filter may not be acknowledged in turbulence studies, thus impeding comparisons between data collected with different ECMs. This paper explores the implications of the filters on the characteristics of velocity signals, mainly on variance, power spectra, and correlation analyses. Variance losses resulting from filtering can be important but will vary with the order n of the Butterworth filter, decreasing as n increases. Knowing the filter response, it is possible to reconstruct the original signal spectrum to evaluate the effect of filtering on variance and to allow comparisons between data collected with different instruments. The autocorrelation function also is affected by filtering which increases the value of the coefficients in the first lags, resulting in an overestimation of the integral length scale of coherent structures. These important effects add to those related to size and shape differences in ECM sensors and must be taken into account in comparative studies.  相似文献