Wavefield extrapolation of body waves for 3-D imaging of earthquake sources     

Wen-Fong Chang  George A. McMechan 《Geophysical Journal International》1991,106(1):85-98

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The 2dF Galaxy Redshift Survey: Wiener reconstruction of the cosmic web     

Pirin Erdo&#;du  Ofer Lahav  Saleem Zaroubi  George Efstathiou  Steve Moody  John A. Peacock  Matthew Colless  Ivan K. Baldry  Carlton M. Baugh  Joss Bland-Hawthorn  Terry Bridges  Russell Cannon  Shaun Cole  Chris Collins  Warrick Couch  Gavin Dalton  Roberto De Propris  Simon P. Driver  Richard S. Ellis  Carlos S. Frenk  Karl Glazebrook  Carole Jackson  Ian Lewis  Stuart Lumsden  Steve Maddox  Darren Madgwick  Peder Norberg  Bruce A. Peterson  Will Sutherland  Keith Taylor 《Monthly notices of the Royal Astronomical Society》2004,352(3):939-960

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The relationship between fish abundance and algal biomass in a seagrass-drift algae community     

George R. Kulczycki  Robert W. Virnstein  Walter G. Nelson 《Estuarine, Coastal and Shelf Science》1981,12(3):341-347

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10 μm polarimetry of ceres     

Paul E. Johnson  James C. Kemp  Marcia J. Lebofsky  George H. Rieke 《Icarus》1983,56(3):381-392

Linear polarimetry of Ceres at 10 μm is presented. These data represent the first published polarization measurements of an asteroid in the thermal infrared. It is found that Ceres is polarized at the 0.2-0.6% level. This data set is compared with theoretical models of the linear polarization of emitted radiation from a spherical plane. These models are used to derive the pole position and thermal inertia of Ceres. Ceres is best fit with a thermal inertia of $\text{0.0010±0.0003}\text{cal}\text{cm}{}^{\mathrm{?2}}\text{°}\text{K}{}^{\mathrm{?1}}\text{sec}{}^{\mathrm{<mtext>1</mtext><mtext>2</mtext>}}$ and a pole orientation of β_p = 36° ± 5°, λ_p = 270° ± 3°. It is concluded that 10μm polarimetry is a potentially powerful technique for remotely sensing the pole orientation and thermal inertia of asteroids.  相似文献   

The global oscillation network group site survey     

Frank Hill  George Fischer  Jennifer Grier  John W. Leibacher  Harrison B. Jones  Patricia P. Jones  Renate Kupke  Robin T. Stebbins 《Solar physics》1994,152(2):351-379

The Global Oscillation Network Group (GONG) Project is planning to place a set of instruments around the world to observe solar oscillations as continuously as possible for at last three years. The Project has now chosen the sites that will comprise the network. This paper describes the methods of data collection and analysis that were used to make this decision.Solar irradiance data were collected with a one-minute cadence at fifteen sites around the world and analyzed to produce statistics of cloud cover, atmospheric extinction, and transparency power spectra at the individual sites. Nearly 200 reasonable six-site networks were assembled from the individual stations, and a set of statistical measures of the performance of the networks was analyzed using a principal component analysis. An accompanying paper presents the results of the survey.  相似文献   

Book reviews     

Kenneth R. Tenore  George R. Helz 《Estuaries and Coasts》1978,1(2):138-138

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Photoelectron thermalization and transport in the ionosphere at low energies     

George P. Mantas 《Planetary and Space Science》1981,29(12):1319-1323

The range of applicability of the transport equation for photoelectrons in the ionosphere (Mantas, 1975), is extended to thermal energies. The extension enables one to calculate the photoelectron distribution in the important low energy region (i.e. < 3 eV), where most of the thermal electron gas heating takes place, and thereby to obtain more accurate excitation rates for the low energy: electronic, vibrational and rotational states of the ionospheric constituents, than was formerly possible.  相似文献   

The maintenance of solar differential rotation by two-dimensional turbulence     

George H. Nickel 《Solar physics》1969,10(2):472-475

A numerical model has been made to test the theory that solar differential rotation is maintained by the Countergradient transport of energy peculiar to two-dimensional turbulence. After a brief discussion of this turbulent process, the numerical methods employed and their application to the sun are reviewed. The results of one problem are presented, indicating that this model can represent the observed large-scale nature of the sun's surface. The reader is referred to the author's dissertation for complete details of the methods and calculations.  相似文献   

Full-wavefield inversion of wide-aperture SH and Love wave data     

Robert Sun  George A. McMechan 《Geophysical Journal International》1991,106(1):67-75

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Big Places,Big Plans by Mark B. Lapping and Owen J. Furuseth,eds.     

George Pomeroy 《The Professional geographer》2007,59(2):270-272

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