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51.
Prof. Dr. Leon N. Carapiperis 《Pure and Applied Geophysics》1956,35(1):143-148
Summary This note deals with the great and abrupt falls of air temperature in Athens which occur especially during the cold season of the year. The frequency of these falls, the greatest falls noted per month and the weather situations associated with these falls are examined separately. It was found that the weather situations which cause the great falls of air temperature in Greece can be classified in four categories:A, B, C andD. In theA belong the anticyclones of N and NW Europe both moving and not. TheB comprises the extensions of the anticyclone of the Azorez over Europe. In theC belong the extension of the Russian anticyclones and theD comprises the cold fronts of depressions moving from W to E. 相似文献
52.
Dr. D. J. Clarke 《Ocean Dynamics》1974,27(1):1-8
Summary The existence of long edge waves over a continental shelf is examined for a representative collection of shelf profiles. The frequencies of both trapped and leaky modes are found, when they exist, in terms of the shelf parameters. Certain theoretical trapped waves over a semi-infinite shelf are shown not to exist in the real ocean.A typical shelf profile on the east coast of Australia is modelled in four different ways from the above collection. The amplification of the leaky mode at the shoreline is found in terms of frequency for each model. Comparison of the results illustrates the severe errors introduced by crude approximations to the profile both at the shoreline and at the shelf cut-off region.
Lange Randwellen über einem Festlandsockel
Zusammenfassung Die Existenz von langen Randwellen über einem Festlandsockel wird untersucht für eine repräsentative Sammlung von Schelfprofilen. Die Frequenzen sowohl der trapped (geführten) als auch der leaky (energieoder impulsabgebenden) Eigenfunktionsformen werden — wenn sie existieren — ermittelt, ausgedrückt in Schelf-Parametern. Es wird gezeigt, daß gewisse, trapped waves (geführte Wellen) über einem semi-unendlichen Schelf im wirklichen Ozean nicht existieren.Mit Hilfe der obigen Sammlung hat man ein typisches Schelfprofil von der Ostküste Australiens in vier verschiedenen Arten modelliert. Die Verstärkung des leaky mode an der Küstenlinie wird für jedes Modell gefunden in Termen der Frequenz. Der Vergleich der Ergebnisse verdeutlicht die schweren Fehler, die durch grobe Näherungen an das Profil entstehen, sowohl an der Küstenlinie als auch in dem Gebiet des Übergangs vom Schelf in die Tiefsee.
Ondes transversales à longues crêtes au-dessus d'un plateua continental
Résumé On examine l'existence d'ondes transversales à longues crêtes au-dessus d'un plateau continental, afin de constituer une collection représentative des profils du plateau. On a trouvé les fréquences du «trapped mode» (mode captif) et du «leaky mode» (mode de transfert d'énergie et du moment) — quand ils existent — et cela en fonction des paramètres du plateau. On montre qu'il n'y a pas, dans l'océan réel, certaines ondes captées théoriques qui existeraient au-dessus d'un plateau semi-infini.Grâce à la collection dont il est parlé ci-dessus, on a modelé de quatre façons différentes un profil typique de la côte Est de l'Australie. Pour chaque modèle on a trouvé l'amplification du «leaky mode» sur la ligne de côte en fonction de la fréquence. La comparaison des résultats montre les erreurs importantes introduites par des approximations sommaires du profil, à la fois près de la ligne de côte et dans la région de transition du plateau continental en mer abyssale.相似文献
53.
Joseph Bonaparte Gulf is a large embayment on the northwestern continental margin of Australia. It is approximately 300 km east‐west and 120 km north‐south with a broad continental shelf to seaward. Maximum width from the southernmost shore of Joseph Bonaparte Gulf to the edge of the continental shelf is 560 km. Several large rivers enter the gulf along its shores. The climate is monsoonal, sub‐humid, and cyclone‐prone during the December‐March wet season. A bedrock high (Sahul Rise) rims the shelf margin. The sediments within the gulf are carbonates to seaward, grading into clastics inshore. A seaward‐thinning wedge of highstand muds dominates the sediments of the inner shelf of Joseph Bonaparte Gulf. Mud banks up to 15m thick have developed inshore. Coarse‐grained sand ridges up to 15 m high are found off the mouth of the Ord River. These overlie an Upper Pleistocene transgressive lag of mixed carbonate and gravelly siliciclastic sand. Four drowned strandlines are present on the inner shelf at depths of 20, 25, 28 and 30 m below datum. These are interpreted as having formed during stillstands in the Late Pleistocene transgression. Older strandlines at great depths are inferred as having formed during the fall in sea‐level following the last highstand. For the most part the Upper Pleistocene‐Holocene marine sediments overlie an erosion surface cut into older Pleistocene sediments. Incised valleys cut into this erosion surface are up to 5 km wide and have a relief of at least 20 m. The largest valley is that cut by the Ord River. Upper Pleistocene sediments deposited in the incised valleys include interpreted lowstand fluvial gravels, early transgressive channel sands and floodplain silts, and late transgressive estuarine sands and gravels. Older Pleistocene sediments are inferred to have been deposited before and during the 120 ka highstand (isotope stage 5). They consist of sandy calcarenites deposited in high‐energy tide‐dominated shelf environments. Still older shelf and valley‐fill sediments underlie these. The contrast between the Holocene muddy clastic sediments and the sandy carbonates deposited by the 120 ka highstand suggests that either the climate was more arid in the past, with less fluvial transport, or that mud was more effectively trapped in estuaries, allowing development of carbonate depositional environments inshore. 相似文献
54.
The first application of the SHETRAN basin‐scale, landslide erosion and sediment yield model is carried out for a major landsliding event in the upper 505 km2 of the Llobregat basin, in the eastern Spanish Pyrenees, in November 1982. The model simulates the spatial distribution of shallow landslides and their sediment yield. Acknowledging uncertainty in the model parameter evaluation, the aim of the application was not to reproduce the observed occurrence of landslides as accurately as possible with one simulation, but to bracket the observed pattern with several simulations representing uncertainty in the key input conditions. Bounds on the landslide simulations were thus determined as a function of uncertainty in the vegetation root cohesion (used in the model factor of safety calculations). The resulting upper bound considerably overestimates the observed pattern (17 000 landslides compared with an observation of around 700), but it reproduces several of the principal clusters in the observed pattern. The lower bound contains around 500 landslides. The sediment yield estimates (2670–14 630 t km?2) are comparable to measurements elsewhere in the Pyrenees for extreme events. The results demonstrate an ability to simulate the basin‐scale landslide response to a rainfall event and the resulting sediment yield. They also highlight the need for further research in setting the uncertainty bounds and in avoiding large overestimates of landslide occurrence arising in part from a current inability to model small‐scale controls for a basin of the given size. Copyright © 2006 John Wiley & Sons, Ltd. 相似文献
55.
56.
Shude Mao Hans J. Witt Leon V. E. Koopmans 《Monthly notices of the Royal Astronomical Society》2001,323(2):301-307
Recent observations indicate that many if not all galaxies host massive central black holes. In this paper we explore the influence of black holes on the lensing properties. We model the lens as an isothermal ellipsoid with a finite core radius plus a central black hole. We show that the presence of the black hole substantially changes the critical curves and caustics. If the black hole mass is above a critical value, then it will completely suppress the central images for all source positions. Realistic central black holes are likely to have masses below this critical value. Even in such subcritical cases, the black hole can suppress the central image when the source is inside a zone of influence, which depends on the core radius and black hole mass. In the subcritical cases, an additional image may be created by the black hole in some regions, which for some radio lenses may be detectable with high-resolution and large dynamic range VLBI maps. The presence of central black holes should also be taken into account when one constrains the core radius from the lack of central images in gravitational lenses. 相似文献
57.
Multipath error is considered one of the major errors affecting GPS observations. One can benefit from the repetition of satellite
geometry approximately every sidereal day, and apply filtering to help minimize this error. For GPS data at 1 s interval processed
using a double-difference strategy, using the day-to-day coordinate or carrier-phase residual autocorrelation determined with
a 10-h window leads to the steadiest estimates of the error-repeat lag, although a window as short as 2 h can produce an acceptable
value with > 97% of the optimal lag’s correlation. We conclude that although the lag may vary with time, such variation is
marginal and there is little advantage in using a satellite-specific or other time-varying lag in double-difference processing.
We filter the GPS data either by stacking a number of days of processed coordinate residuals using the optimum “sidereal”
lag (23 h 55 m 54 s), and removing these stacked residuals from the day in question (coordinate space), or by a similar method
using double-difference carrier-phase residuals (observational space). Either method results in more consistent and homogeneous
set of coordinates throughout the dataset compared with unfiltered processing. Coordinate stacking reduces geometry-related
repeating errors (mainly multipath) better than carrier-phase residual stacking, although the latter takes less processing
time to achieve final filtered coordinates. Thus, the optimal stacking method will depend on whether coordinate precision
or computational time is the over-riding criterion. 相似文献
58.
Mesozooplankton samples were collected between March 2005 and November 2008 in St Lucia, the largest estuarine lake system in South Africa. St Lucia experienced an extended period of drought before and during the present study. This drought led to natural closing of the estuary mouth as a result of flood-tide marine sediment deposition in 2002. In March 2007 the mouth was washed open by exceptionally high tidal and wave conditions. This resulted in an influx of a large volume of seawater. The mouth closed again in August 2007. Before opening of the mouth salinities in the Estuary were below 10 and large parts of North Lake dried up while South Lake retained a relatively stable waterbody with salinities between 10 and 30. When the mouth opened seawater flooded the system and salinities changed to about 35. After the mouth had closed again in August 2007 salinities increased in the lakes and decreased in the Estuary. The mesozooplankton community was dominated by copepods during all sampling sessions, especially by the estuarine calanoids Pseudodiaptomus stuhlmanni and Acartia natalensis. Mean mesozooplankton densities were significantly higher in South Lake before the mouth opened in March 2007. While zooplankton density decreased when the mouth opened species richness increased with the influx of coastal marine species, especially in the Estuary. Overall zooplankton densities declined progressively as salinity increased to hypersaline levels after mouth closure. Multivariate analyses supported significant differences between the lakes and the Estuary in terms of mesozooplankton community composition. Taxa mostly responsible for the similarities within and dissimilarity between sections of the system were the copepods P. stuhlmanni and A. natalensis with the meroplankton, crab zoeae and mollusc larvae, also contributing significantly after the mouth-opening event. 相似文献
59.
60.
Michael D. West Jonathan D.A. Clarke Matilda Thomas Malcolm R. Walter 《Planetary and Space Science》2010,58(4):447-458
Australia has numerous landforms and features, some unique, that provide a useful reference for interpreting the results of spacecraft orbiting Mars and exploring the martian surface. Examples of desert landforms, impact structures, relief inversion, long-term landscape evolution and hydrothermal systems that are relevant to Mars are outlined and the relevant literature reviewed. The Mars analogue value of Australia's acid lakes, hypersaline embayments and mound spring complexes is highlighted along with the Pilbara region, where the oldest convincing evidence of life guides exploration for early life on Mars. The distinctive characteristics of the Arkaroola Mars Analogue Region are also assessed and opportunities for future work in Australia are outlined. 相似文献