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11.
Using the continuation method we prove that the circular and the elliptic symmetric periodic orbits of the planar rotating
Kepler problem can be continued into periodic orbits of the planar collision restricted 3-body problem. Additionally, we also
continue to this restricted problem the so called “comet orbits”.
An erratum to this article can be found at 相似文献
12.
Xavier Ruiz Laureano Ramírez-Piscina Jaume Casademunt 《Astrophysics and Space Science》2001,276(1):135-140
We study the convective flow induced by residual accelerations in microgravity conditions for different geometric arrangements which are relevant to crystal growth experiments. We consider both constantand oscillating acceleration and focus mostly on the transient relaxation dynamics. Results are relevant to estimate impact of more realistic residual accelerations in crystal growth experiments. 相似文献
13.
This paper investigates the impact of climate change on destination choice decisions in a context of domestic coastal tourism in Spain. Destinations are characterized in terms of travel cost and coastal ‘attractors’, such as temperature and beach-related attributes. By means of a discrete choice model based on the random utility theory, these variables are used to explain the observed pattern of interprovincial domestic trips, showing trade-offs between temperature and attractiveness in the probability of a particular destination being chosen. The model is used to investigate the impact of two climate change scenarios on the allocation of domestic tourism within Spain. The findings show that while Spain’s northern colder provinces would benefit from rising temperatures, provinces in the south would experience a decrease in the frequency of trips. 相似文献
14.
New doubly-symmetric families of comet-like periodic orbits in the spatial restricted (N + 1)-body problem 总被引:1,自引:0,他引:1
For any positive integer N ≥ 2 we prove the existence of a new family of periodic solutions for the spatial restricted (N +1)-body problem. In these solutions the infinitesimal particle is very far from the primaries. They have large inclinations
and some symmetries. In fact we extend results of Howison and Meyer (J. Diff. Equ. 163:174–197, 2000) from N = 2 to any positive integer N ≥ 2.
相似文献
15.
Jaume Giné 《Astrophysics and Space Science》2012,337(1):483-486
In this paper we discuss the recently obtained relation between the Verlinde’s holographic model and the first phenomenological
Modified Newtonian dynamics. This gives also a promising possible explanation to the Pioneer anomaly. 相似文献
16.
Jaume Sanz J. Miguel Juan Adrià Rovira-Garcia Guillermo González-Casado 《GPS Solutions》2017,21(4):1549-1561
17.
18.
Eduard Saura Jean‐Christophe Embry Jaume Vergés David W. Hunt Emilio Casciello Stéphane Homke 《Basin Research》2013,25(2):149-171
The evolution from Late Cretaceous to early Eocene of the well dated Amiran foreland basin in the NW Iranian Zagros Mountains is studied based on the reconstruction of successive thickness, palaeobathymetry and subsidence maps. These maps show the progressive forelandwards migration of the mixed carbonate‐siliciclastic system associated with a decrease in creation of accommodation. Carbonate facies variations across the basin suggest a structural control on the carbonate distribution in the Amiran foreland basin, which has been used as initial constraint to study the control exerted by syndepositional folding in basin architecture and evolution by means of stratigraphic numerical modelling. Modelled results show that shallow bathymetries on top of growing folds enhance carbonate production and basin compartmentalization. As a consequence, coarse clastics become restricted to the internal parts of the basin and only the fine sediments can by‐pass the bathymetric highs generated by folding. Additionally, the development of extensive carbonate platforms on top of the anticlines favours the basinwards migration of the depositional system, which progrades farther with higher fold uplift rates. In this scenario, build‐ups on top of anticlines record its growth and can be used as a dating method. Extrapolation of presented modelling results into the Amiran foreland basin is in agreement with an early folding stage in the SE Lurestan area, between the Khorramabad and Kabir Kuh anticlines. This folding stage would enhance the development of carbonate platforms on top of the anticlines, the south‐westward migration of the system and eventually, the complete filling of the basin north of the Chenareh anticline at the end of the Cuisian. Incremental thickness maps are consistent with a thin (0.4–2 km) ophiolite complex in the source area of the Amiran basin. 相似文献
19.
EVA: GPS-based extended velocity and acceleration determination 总被引:1,自引:0,他引:1
Dagoberto Salazar Manuel Hernandez-Pajares Jose Miguel Juan-Zornoza Jaume Sanz-Subirana Angela Aragon-Angel 《Journal of Geodesy》2011,85(6):329-340
In this work, a new GPS carrier phase-based velocity and acceleration determination method is presented that extends the effective
range of previous techniques. The method is named ‘EVA’, and may find applications in fields such as airborne gravimetry when
rough terrain or water bodies make difficult or impractical to set up nearby GPS reference receivers. The EVA method is similar
to methods such as Kennedy (Precise acceleration determination from carrier phase measurements. In: Proceedings of the 15th
international technical meeting of the satellite division of the Institute of Navigation. ION GPS 2002, Portland pp 962–972,
2002b) since it uses L1 carrier phase observables for velocity and acceleration determination. However, it introduces a wide network
of stations and it is independent of precise clock information because it estimates satellite clock drifts and drift rates
‘on-the-fly’, requiring only orbit data of sufficient quality. Moreover, with EVA the solution rate is only limited by data
rate, and not by the available precise satellite clocks data rate. The results obtained are more robust for long baselines
than the results obtained with the reference Kennedy method. An advantage of being independent of precise clock information
is that, beside IGS Final products, also the Rapid, Ultra-Rapid (observed) and Ultra-Rapid (predicted) products may be used.
Moreover, the EVA technique may also use the undifferenced ionosphere-free carrier phase combination (LC), overcoming baseline
limitations in cases where ionosphere gradients may be an issue and very low biases are required. During the development of
this work, some problems were found in the velocity estimation process of the Kennedy method. The sources of the problems
were identified, and an improved version of the Kennedy method was used for this research work. An experiment was performed
using a light aircraft flying over the Pyrenees, showing that both EVA and the improved Kennedy methods are able to cope with
the dynamics of mountainous flight. A RTK-derived solution was also generated, and when comparing the three methods to a known
zero-velocity reference the results yielded similar performance. The EVA and the improved-Kennedy methods outperformed the
RTK solutions, and the EVA method provided the best results in this experiment. Finally, both the improved version of the
Kennedy method and the EVA method were applied to a network in equatorial South America with baselines of more than 1,770 km,
and during local noon. Under this tough scenario, the EVA method showed a clear advantage for all components of velocity and
acceleration, yielding better and more robust results. 相似文献
20.
The ionosphere: effects,GPS modeling and the benefits for space geodetic techniques 总被引:12,自引:8,他引:4
Manuel Hernández-Pajares J. Miguel Juan Jaume Sanz Àngela Aragón-Àngel Alberto García-Rigo Dagoberto Salazar Miquel Escudero 《Journal of Geodesy》2011,85(12):887-907
The main goal of this paper is to provide a summary of our current knowledge of the ionosphere as it relates to space geodetic
techniques, especially the most informative technology, global navigation satellite systems (GNSS), specifically the fully
deployed and operational global positioning system (GPS). As such, the main relevant modeling points are discussed, and the
corresponding results of ionospheric monitoring are related, which were mostly computed using GPS data and based on the direct
experience of the authors. We address various phenomena such as horizontal and vertical ionospheric morphology in quiet conditions,
traveling ionospheric disturbances, solar flares, ionospheric storms and scintillation. Finally, we also tackle the question
of how improved knowledge of ionospheric conditions, especially in terms of an accurate understanding of the distribution
of free electrons, can improve space geodetic techniques at different levels, such as higher-order ionospheric effects, precise
GNSS navigation, single-antenna GNSS orientation and real-time GNSS meteorology. 相似文献