Computational parameter estimation for a maize crop     

Adrie F. G. Jacobs  John H. Van Boxel 《Boundary-Layer Meteorology》1988,42(3):265-279

During a whole growing season, the evolution of the displacement height, d, and roughness length, z ₀, of a maize crop has been estimated by a measurement programme. The results have been used to check different types of existing models to calculate these parameters from canopy characteristics only; a simple geometric model and two matching models have been investigated. A geometric model is based on geometric features of the surface only. After a simple modification, the geometric model gives good results for the displacement height as well as for the roughness length.A matching model, based on gradient-diffusion theory, yields good results for the displacement height. The roughness parameter, however, is overestimated by 17%. By a simple modification, the model results could be improved considerably.A matching model, based on a second-order closure procedure, yields excellent results for the displacement height and good results for the roughness length. But it appears that, when applying this model, the plant density index and plant area density distribution as a function of height must be well known.  相似文献   

The ‘MESOGERS 84’ experiment: A report     

A. Weill  C. Mazaudier  F. Baudin  C. Klapisz  F. Leca  M. Masmoudi  D. Vidal Madjar  R. Bernard  O. Taconet  B. S. Gera  A. Sauvaget  A. Druilhet  P. Durand  J. Y. Caneil  P. Mery  G. Dubosclard  A. C. M. Beljaars  W. A. A. Monna  J. G. Van Der Vliet  M. Crochet  D. Thomson  T. Carlson 《Boundary-Layer Meteorology》1988,42(3):251-264

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Dynamical stability of convection cells in the upper mantle     

Ludvík Urban  Reviewer J. Vaněk 《Studia Geophysica et Geodaetica》1988,32(2):151-158

Summary A two-dimensional flow model of an incompressible fluid with constant viscosity has been used to study the changes in the large-scale flow pattern (aspect ratio 4). Implications for convection in the Earth's mantle are discussed.

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КРИТИКА     

Milan Burša  Jiří Vaněk  Oldřich Novotný  Ladislav Křivský  Petronela Ochabová  Jan Bednář 《Studia Geophysica et Geodaetica》1988,32(4):416-420

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A Finite-Difference Technique to Incorporate Spatial Variations In Rigidity and Planar Faults Into 3-D Models For Lithospheric Flexure   总被引：1，自引：0，他引：1  

J. D. Van  Wees S. Cloetingh 《Geophysical Journal International》1994,117(1):179-195

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Comment On: 'Early Silurian Palaeolatitude of the Springdale Group Redbeds of Central Newfoundland: A Palaeomagnetic Determination With A Remanence Anisotropy Test For Inclination Error' By J. P. Hodych and K. L. Buchan     

John Stamatakos  Rob Van Der  Voo  Ben Van Der  Pluijm  Stephen Potts  Trond Torsvik 《Geophysical Journal International》1994,119(3):1009-1013

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Reply to Liu and Chao     

T. Soler  B. H. W. Van Gelder 《Geophysical Journal International》1993,113(1):271-271

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Comment On 'The Earth's Equatorial Principal Axes and Moments of Inertia' By H. S. Liu and B. F. Chao     

Tomás Soler  Boudewijn H. W. Van Gelder 《Geophysical Journal International》1993,113(1):268-269

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High-frequency sequences and their stacking patterns: sequence-stratigraphic evidence of high-frequency eustatic cycles   总被引：18，自引：0，他引：18  

Robert M. Mitchum Jr.  John C. Van Wagoner   《Sedimentary Geology》1991,70(2-4):131-147

A hierarchy of interpreted eustatic cyclicity in siliciclastic sedimentary rocks has a pattern of superposed cycles with frequencies in the ranges of 9–10 m.y., 1–2 m.y., 0.1–0.2 m.y., and 0.01–0.02 m.y. (second- through fifth-order cyclicity, respectively). Stratigraphic units displaying this cyclicity include composite sequences, sequences, and parasequences. On the Exxon global cycle chart, fundamental third-order cycles (1–2 m.y. average duration) stack into related groups (second-order cycles: 9–10 m.y. duration). A much larger pattern (about 200 m.y.) is interpreted as tectonically controlled eustasy probably related to sea-floor spreading rates.

One and probably two higher orders of cyclicity (fourth-order: 0.1–0.2 m.y.; and fifth-order: 0.01–0.02 m.y.) are now observed in work with well logs, cores, and outcrops in areas of very rapid deposition. These frequencies are in the range of Milankovitch cycles, and may represent part of the Milankovitch hierarchy which has been widely interpreted for cyclical units in carbonate rocks.

High-frequency (fourth-order) sequences, which form at a 0.1–0.2 m.y. cyclicity, have all the stratal attributes of conventional sequences, including constituent parasequences and systems tracts, and play a dominant role controling reservoir, source, and sealing rock distribution. A consistent hierarchy of stratigraphy is observed. Parasequences (probable fifth-order cyclicity) stack into sets to form systems tracts in fourth-order sequences. Groups (sets) of fourth-order sequences are deposited between major third-order boundaries within third-order composite sequences. Sequences in these sets stack in prograding and backstepping patterns to form third-order lowstand, transgressive, and highstand sequence sets.

Third-order sequence boundaries are marked by greater basinward shifts in facies, by larger more widespread incised valleys, and by more extensive onlap than are fourth-order sequence boundaries. Third-order condensed sections commonly are widespread, faunally rich, and widely correlated biozone and mapping markers. Fourth-order sequence analysis helps to understand reservoir, source, and seal distribution at the play and prospect scale. An example from the Gulf of Mexico is discussed.  相似文献   

An analytical model of seismic travel times for a spherically asymmetric Earth     

Karel Pěč  Zdeněk Martinec  Reviewer J. Vaněk 《Studia Geophysica et Geodaetica》1985,29(3):220-227

Summary A general analytical model for travel times of seismic waves propagating in a radially asymmetric Earth, is suggested. It is represented by a series of irreducible spherical tensor products with bipolar spherical coefficients. The main term of the series describes the travel times in a radially symmetric Earth, the others represent corrections due to the spherical assymmetry. The method of least squares is suggested for determining the bipolar spherical coefficients from observed seismic travel times. Since the proposed theory assumes that the analytical representation is related to the reference earth, the corrections to the non-zero focal depth and non-zero sea-level height of the seismographic station must be introduced.

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