Continuum Evn and Merlin Observations of Ultra Luminous Infrared Galaxies     

A. G. Polatidis  J. E. Conway  Y. M. Pihlström  R. Parra 《Astrophysics and Space Science》2005,295(1-2):297-302

Radio imaging of ULIR galaxies is ideal to explore the connection between the starburst and the AGN phenomenon since it is unaffected by dust obscuration, and provides the required high angular resolution to distinguish between an AGN and starburst emission. We have made combined 18 cm radio continuum, EVN and MERLIN observations of 13 ULIRGs that have the parsec and deci-parsec scale resolution necessary to distinguish between an AGN and supernovae remnants at the centres of these galaxies, and assess the contribution of each to the total energy distribution. Images of three galaxies are presented here.  相似文献   

An improved algorithm due to laguerre for the solution of Kepler's equation     

Bruce A. Conway 《Celestial Mechanics and Dynamical Astronomy》1986,39(2):199-211

A root-finding method due to Laguerre (1834–1886) is applied to the solution of the Kepler problem. The speed of convergence of this method is compared with that of Newton's method and several higher-order Newton methods for the problem formulated in both conventional and universal variables and for both elliptic and hyperbolic orbits. In many thousands of trials the Laguerre method never failed to converge to the correct solution, even from exceptionally poor starting approximations. The non-local robustness and speed of convergence of the Laguerre method should make it the preferred method for the solution of Kepler's equation.  相似文献   

An instrument for teaching clinometry     

Declan G. De Paor 《Journal of Structural Geology》1984,6(3):335-337

By combining a compass, counterweight and gimbal, an instrument for simultaneous measurement of dip, strike, pitch, plunge and trend data has been constructed. The instrument automatically locates the strike of the surface on which it is placed. It may serve as a useful teaching aid in the structural laboratory.  相似文献   

Ecopolitical battles at the Tarai frontier of Nepal: an emerging human and environmental crisis     

Shrestha NR  Conway D 《International journal of population geography : IJPG》1996,2(4):313-331

"In Nepal, the drama of human and environmental ills is increasingly being played out in the form of peasants' ecopolitical battles over common land access and control, such as in the Tarai frontier, a region bordering the Gangetic Plain of India. This is a complex battle, pitting peasants' day-to-day survival against environmental security on one front, and against the Nepalese State and its dominant class interests on the other. This article critically dissects this raging battle to gain a clear understanding of its complexities as well as its diverse roots."  相似文献   

Some limitations of the R_f/φ technique of strain analysis     

Declan G. De Paor 《Tectonophysics》1980,64(1-2)

Finite strain determined from R_f/φ analysis of deformed ellipse distributions cannot be separated into compactional and tectonic parts on the basis of population asymmetry about the orientational mean, as was originally suggested. Furthermore, where there is a ductility contrast between objects and matrix, R_f/φ analysis yields an invalid estimate of the strain suffered by the objects.  相似文献   

A determination of the CH4, NO x and CO2 emissions from the Prudhoe Bay,Alaska oil development     

D. A. Jaffe  R. E. Honrath  D. Furness  T. J. Conway  E. Dlugokencky  L. P. Steele 《Journal of Atmospheric Chemistry》1995,20(3):213-227

In this paper we quantify the CH₄, CO₂ and NO _x emissions during routine operations at a major oil and gas production facility, Prudhoe Bay, Alaska, using the concentrations of combustion by products measured at the NOAA-CMDL observatory at Barrow, Alaska and fuel consumption data from Prudhoe Bay. During the 1989 and 1990 measurement campaigns, 10 periods (called events) were unambiguously identified where surface winds carry the Prudhoe Bay emissions to Barrow (approximately 300 km). The events ranged in duration from 8–48 h and bring ambient air masses containing substantially elevated concentrations of CH₄, CO₂ and NO _y to Barrow. Using the slope of the observed CH₄ vs CO₂ concentrations during the events and the CO₂ emissions based on reported fuel consumption data, we calculate annual CH₄ emissions of (24+/–8)×10³ metric tons from the facility. In a similar manner, the annual NO _x emissions are calculated to be (12+/–4)×10³ metric tons, which is in agreement with an independently determined value. The calculated CH₄ emissions represent the amount released during routine operations including leakage. However this quantity would not include CH₄ released during non-routine operations, such as from venting or gas flaring.  相似文献   

A numerical model of the Martian polar cap winds     

Robert M. Haberle  Conway B. Leovy  James B. Pollack 《Icarus》1979,39(2):151-183

An investigation of the Martian polar cap winds and their response to a variety of factors is carried out by a series of numerical experiments based on a zonally symmetric primitive equation model. These factors are the seasonal thermal forcing, mass exchange between polar caps and atmosphere, large-scale topography, and polar cap size. The thermal forcing sets up a circulation whose surface winds adjust to achieve angular momentum balance, with low-latitude easterlies and high-latitude westerlies. The maximum westerlies occur roughly where the horizontal temperature gradients are largest. This pattern changes when cap and atmosphere exchange mass. Corriolis forces acting on the net outflow or inflow produce easterlies at the surface during spring (outflow) and westerlies during winter (inflow). Topography appears to have a small effect, but cap size does play a role, the circulation intensity increasing with cap size. Peak surface winds occur when outflow or inflow is a maximum and are 20 m sec^?1 during spring and 30 m sec^?1 during winter for the northern hemisphere. The model results show that surface winds near the edge of a retreating polar cap are substantially enhanced, a result which is consistent with the Viking observations of local dust storm activity near the edge of the south polar cap during spring. The results also indicate that the surficial wind indicators near the south pole are formed during spring and those near the north pole during winter. The implication is that the high-latitude dune fields in the northern hemisphere are formed at a time when the terrain is being covered with frost. It is therefore suggested that the saltating particles are “snowflakes” which have formed by the mechanism proposed by Pollack etal. The model results for the winter simulation, which have formed by the mechanism transport by large-scale eddies, compare favorably with general circulation model (GCM) calculations. This suggests that the eddy transports may be less important than those associated with the net mass flow, and that 2-D climate modeling may be more succesful for Mars than Earth.  相似文献   

Extended two-body problem for rotating rigid bodies     

Ho  Alex  Wold  Margrethe  Conway  John T.  Poursina  Mohammad 《Celestial Mechanics and Dynamical Astronomy》2021,133(8):1-44

Given the interest in future space missions devoted to the exploration of key moons in the solar system and that may involve libration point orbits, an efficient design strategy for transfers between moons is introduced that leverages the dynamics in these multi-body systems. The moon-to-moon analytical transfer (MMAT) method is introduced, comprised of a general methodology for transfer design between the vicinities of the moons in any given system within the context of the circular restricted three-body problem, useful regardless of the orbital planes in which the moons reside. A simplified model enables analytical constraints to efficiently determine the feasibility of a transfer between two different moons moving in the vicinity of a common planet. In particular, connections between the periodic orbits of such two different moons are achieved. The strategy is applicable for any type of direct transfers that satisfy the analytical constraints. Case studies are presented for the Jovian and Uranian systems. The transition of the transfers into higher-fidelity ephemeris models confirms the validity of the MMAT method as a fast tool to provide possible transfer options between two consecutive moons.

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Lava-ice interaction on a large composite volcano: a case study from Ruapehu,New Zealand     

C. E. Conway  D. B. Townsend  G. S. Leonard  C. J. N. Wilson  A. T. Calvert  J. A. Gamble 《Bulletin of Volcanology》2015,77(3):1-18

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Enhanced runout and erosion by overland flow at low pressure and sub-freezing conditions: Experiments and application to Mars     

Susan J. Conway  Michael P. Lamb  Martin C. Towner  John B. Murray 《Icarus》2011,211(1):443-457

We present the results of laboratory experiments to study the sediment transport and erosional capacity of water at current martian temperature and pressure. We have performed laboratory simulation experiments in which a stream of water flowed over test beds at low temperature (∼−20 °C) and low pressure (∼7 mbar). The slope angle was 14° and three sediment types were tested. We compared the erosive ability, runout and resulting morphologies to experiments performed at ambient terrestrial temperature (∼20 °C) and pressure (∼1000 mbar), and also to experiments performed under low pressure only. We observed that, as expected, water is unstable in the liquid phase at low temperature and low pressure, with boiling and freezing in competition. Despite this, our results show that water at low temperature and low pressure has an equivalent and sometimes greater erosion rate than at terrestrial temperature and pressure. Water flows faster over the sediment body under low temperature and low pressure conditions because the formation of ice below the liquid-sediment contact inhibits infiltration. Flow speed and therefore runout distance are increased. Experiments at low pressure but Earth-ambient temperature suggest that flow speeds are faster under these conditions than under Earth-ambient pressure and temperature. We hypothesise that this is due to gas bubbles, created by the boiling of the water under low atmospheric pressure, impeding liquid infiltration. We have found that both basal freezing and low pressure increase the flow propagation speed - effects not included in current models of fluvial activity on Mars. Any future modelling of water flows on Mars should consider this extra mobility and incorporate the large reduction in fluid loss through infiltration into the substrate.  相似文献