Orbit determination and analysis for Cosmos 58 at 15th-order resonance, to evaluate geopotential harmonics of order 15 and 30     

Doreen M. C. Walker 《Planetary and Space Science》1986,34(12):1307-1318

The orbital parameters of Cosmos 58 have been determined at 65 epochs from some 4500 observations, between March 1982 and September 1983, using the RAE orbit refinement program, PROP. During this time, the satellite passed slowly through 15th-order resonance, and the orbital inclination and eccentricity have been analysed. Six lumped 15th-order geopotential harmonic coefficients have been evaluated, with an accuracy equivalent to between 0.8 and 2.0cm in geoid height. Six 30th-order coefficients have also been determined, with accuracies between 2 and 7 cm in geoid height. The coefficients have been compared with those from the GEM 10B and 10C models. There is good agreement for nine of the twelve coefficients.  相似文献   

The distinction between postcranial bones of Bos primigenius Bojanus, 1827 and Bison priscus Bojanus, 1827 from the British pleistocene and the taxonomic status of Bos and Bison     

Henry Gee 《第四纪科学杂志》1993,8(1):79-92

The study of British Pleistocene mammal faunas has been hampered by the difficulty of telling the difference between the postcranial elements of the often abundant remains of the large bovids Bos primigenius Bojanus, 1827 and Bison priscus Bojanus, 1827. Here I present qualitative and morphometric criteria whereby Bos primigenius and Bison priscus radii, metacarpals, tibiae, astragali and metatarsals can be told apart using British Pleistocene material.  相似文献   

HR 7275: A new variable star     

R. E. Fried  Joel A. Eaton  D. S. Hall  G. W. Henry  L. P. Lovell  K. Krisciunas  C. R. Chambliss  P. K. Detterline  H. J. Landis  H. Louth  D. R. Skillman 《Astrophysics and Space Science》1982,83(1-2):181-188

Differential photometry of the KI IV-III RS CVn-type binary HR 7275 in 1978, 1979, and 1980 at nine different observatories shows it definitely to be variable, thus confirming the suspicion of Herbst. The photometric period determined two ways was 27 _. ^d 91 or 27 _. ^d 65, thus about 3% shorter than the spectroscopically determined orbital period of 28 _. ^d 59. The total variation observed during the three years was 0 _. ^m 22 in theV. The light curve was always asymmetrical, with a stillstand on the rising branch in 1978 but on the falling branch in 1980.Kitt Peak National Observatory, operated by the Association of Universities for Research in Astronomy, under contract with the National Science Foundation.Of the AAVSO.  相似文献   

Ionospheric layers of Mars and Earth     

Henry Rishbeth  Michael Mendillo 《Planetary and Space Science》2004,52(9):849-852

We compare the electron densities of two martian ionospheric layers, which we call M1 and M2, measured by Mars Global Surveyor during 9-27 March 1999, with the electron densities of the terrestrial E and F1 layers derived from ionosonde data at six sites. The day-to-day variations are all linked to changes in solar activity, and provide the opportunity of making the first simultaneous study of four photochemical layers in the solar system. The ‘ionospheric layer index’, which we introduce to characterize ionospheric layers in general, varies between layers because different atmospheric chemistry and solar radiations are involved. The M2 and F1 layer peaks occur at similar atmospheric pressure levels, and the same applies to the M1 and E layers.  相似文献   

Hydrogeologic unit flow characterization using transition probability geostatistics   总被引：1，自引：0，他引：1  

Jones NL  Walker JR  Carle SF 《Ground water》2005,43(2):285-289

This paper describes a technique for applying the transition probability geostatistics method for stochastic simulation to a MODFLOW model. Transition probability geostatistics has some advantages over traditional indicator kriging methods including a simpler and more intuitive framework for interpreting geologic relationships and the ability to simulate juxtapositional tendencies such as fining upward sequences. The indicator arrays generated by the transition probability simulation are converted to layer elevation and thickness arrays for use with the new Hydrogeologic Unit Flow package in MODFLOW 2000. This makes it possible to preserve complex heterogeneity while using reasonably sized grids and/or grids with nonuniform cell thicknesses.  相似文献   

Multi-proxy approach to long- and short-term Holocene climate-change: evidence from eastern Lake Ontario     

Melany?A.?McFadden  William?P.?Patterson  Henry?T.?MullinsEmail author  William?T.?Anderson 《Journal of Paleolimnology》2005,33(3):371-391

We use a multi-proxy (n = 11) paleolimnological approach on deep-water sediment from eastern Lake Ontario to characterize both long- and short-term regional climate change over the past ~10,000 calendar years. Proxies included % total organic matter, % total carbonate, magnetic susceptibility, C/N ratios, % organic carbon, % total nitrogen, % biogenic silica and ¹⁸O and ¹³C of carbonate, as well as ¹³C and ¹⁵N of bulk organic matter. There is a marked shift in most proxies at ~9.4 ka which defines the start of Holocene warmth in this region. Prior to this, the area was influenced by the post-Younger Dryas cold/wet interval, controlled by a southward displacement of the polar front jet stream, when many proxies were at their minimum. The Hypsithermal interval (~9.4–5.3 ka) was the warmest and wettest of the Holocene due to a long-term increase in summer insolation. The Hypsithermal, however, was interrupted by two cold climates; the 8.2 ka event (~8.4–8.0 ka) and the Nipissing Rise (~6.8–5.0 ka), both of which are linked to a reduction in thermohaline circulation and northward oceanic heat transport. The Neoglacial interval (~5.3 ka to ~1850 AD), driven by a long-term decrease in summer insolation, was cooler and dryer, but more stable, than the Hypsithermal. The short Historic interval (post ~1850 AD) was characterized by some of the largest amplitude and most abrupt anomalies of the past 10,000 years, due to intense anthropogenic activity, when a number of proxies reached unprecedented values.  相似文献   

Relationships between photosynthetically active radiation and clearness index at Bloemfontein, South Africa   总被引：1，自引：0，他引：1  

M. Tsubo  S. Walker 《Theoretical and Applied Climatology》2005,80(1):17-25

Summary Relationships between photosynthetically active radiation (PAR) and solar radiation (SR) and between diffuse radiation and global radiation at Bloemfontein, South Africa were investigated. The ratio of PAR to SR (PAR/SR) has been reported from many places in the northern hemisphere, but there were not many PAR/SR measurements documented from the southern hemisphere, including the study region. Based on the present observations, mean PAR/SR in the region (0.48) was not exceptionally different from other reported data (0.45–0.50). The effects of sky condition on PAR/SR were also investigated and confirmed the previous findings. PAR/SR increased as the clearness index (K_T=ratio of global to extraterrestrial SR) decreased, as sky conditions varied from clear to cloudy. Thus, PAR/SR can be a simple function of the clearness index (the global PAR model). In this study, PAR/SR was explained by a quadratic function of K_T. For the relationship between diffuse and global radiation, a simple linear threshold diffuse PAR model, as a linear function of K_T, was proposed for the study region using long-term data of diffuse and global SR. Using the previous findings on the relationship between the ratio of diffuse to global SR (K_SR) and the ratio of diffuse to global PAR (K_PAR), at high K_T, K_PAR can be estimated as 30% higher than K_SR, while at low K_TK_PAR is equivalent to K_SR.  相似文献   

The change in satellite orbital inclination caused by a rotating atmosphere with day-to-night density variation     

D. G. King-Hele  Doreen M. C. Walker 《Celestial Mechanics and Dynamical Astronomy》1972,5(1):41-54

The theory specifying the change i in a satellite's orbital inclination due to atmospheric rotation, in terms of the decrease in orbital period T, has been extended to an atmosphere with sinusoidal variation of density between day and night. It is found that with certain special sets of values for the orbital parameters, the day-to-night variation in the Earth's atmosphere can alter the equation for i/T by as much as 25% though only for a few days. Appreciable changes in i/T persisting for several months can only occur for certain resonant orbits: the maximum change is then about 8%. Near-resonance is very unlikely, but the resonance conditions are derived so that orbits can be recognised and avoided.  相似文献   

Track view of the regolithic elephant     

G. Crozaz  R. M. Walker 《Earth, Moon, and Planets》1975,13(1-3):229-234

Information gained from track studies in lunar soils is reviewed; soil maturity indices are compared and briefly discussed; track methods to establish the layering chronology of lunar cores are also treated.  相似文献   

Radar studies of magnetosphere dynamics     

A. D. M. Walker 《Astrophysics and Space Science》1995,230(1-2):415-430

Ionospheric radars are an important tool for studying magnetospheric dynamics. The nature of such instruments is described and their application to a number of important problems is discussed, emphasizing South African work. A study of the theory of reflection from irregularities is discussed. The nature of ULF pulsations of more than one type has been elucidated by radar studies. An improvement of the understanding of magnetospheric convection has been achieved. A new HF radar experiment being developed for operation at SANAE, Antarctica, is described. An HF radar will be operated at SANAE in conjunction with the British radar at Halley to provide vector information about magnetospheric convection within that part of the magnetosphere which maps to a large portion of the Antarctic continent. The radar will be part of the SuperDARN international network of radars.  相似文献