78,718 research outputs found
Numerical simulation of the world ocean circulation
A multi-level model, based on the primitive equations, is developed for simulating the temperature and velocity fields produced in the world ocean by differential heating and surface wind stress. The model ocean has constant depth, free slip at the lower boundary, and neglects momentum advection; so that there is no energy exchange between the barotropic and baroclinic components of the motion, although the former influences the latter through temperature advection. The ocean model was designed to be coupled to the UCLA atmospheric general circulation model, for the study of the dynamics of climate and climate changes. But here, the model is tested by prescribing the observed seasonally varying surface wind stress and the incident solar radiation, the surface air temperature and humidity, cloudiness and the surface wind speed, which, together with the predicted ocean surface temperature, determine the surface flux of radiant energy, sensible heat and latent heat
Supersolid and charge density-wave states from anisotropic interaction in an optical lattice
We show anisotropy of the dipole interaction between magnetic atoms or polar
molecules can stabilize new quantum phases in an optical lattice. Using a well
controlled numerical method based on the tensor network algorithm, we calculate
phase diagram of the resultant effective Hamiltonian in a two-dimensional
square lattice - an anisotropic Hubbard model of hard-core bosons with
attractive interaction in one direction and repulsive interaction in the other
direction. Besides the conventional superfluid and the Mott insulator states,
we find the striped and the checkerboard charge density wave states and the
supersolid phase that interconnect the superfluid and the striped solid states.
The transition to the supersolid phase has a mechanism different from the case
of the soft-core Bose Hubbard model.Comment: 5 pages, 5 figures
Discovery of a new supernova remnant G150.3+4.5
Large-scale radio continuum surveys have good potential for discovering new
Galactic supernova remnants (SNRs). Surveys of the Galactic plane are often
limited in the Galactic latitude of |b| ~ 5 degree. SNRs at high latitudes,
such as the Cygnus Loop or CTA~1, cannot be detected by surveys in such limited
latitudes. Using the available Urumqi 6 cm Galactic plane survey data, together
with the maps from the extended ongoing 6 cm medium latitude survey, we wish to
discover new SNRs in a large sky area. We searched for shell-like structures
and calculated radio spectra using the Urumqi 6 cm, Effelsberg 11 cm, and 21 cm
survey data. Radio polarized emission and evidence in other wavelengths are
also examined for the characteristics of SNRs. We discover an enclosed
oval-shaped object G150.3+4.5 in the 6 cm survey map. It is about 2.5 degree
wide and 3 degree high. Parts of the shell structures can be identified well in
the 11 cm, 21 cm, and 73.5 cm observations. The Effelsberg 21 cm total
intensity image resembles most of the structures of G150.3+4.5 seen at 6 cm,
but the loop is not closed in the northwest. High resolution images at 21 cm
and 73.5 cm from the Canadian Galactic Plane Survey confirm the extended
emission from the eastern and western shells of G150.3+4.5. We calculated the
radio continuum spectral indices of the eastern and western shells, which are
and between 6 cm and 21 cm, respectively.
The shell-like structures and their non-thermal nature strongly suggest that
G150.3+4.5 is a shell-type SNR. For other objects in the field of view,
G151.4+3.0 and G151.2+2.6, we confirm that the shell-like structure G151.4+3.0
very likely has a SNR origin, while the circular-shaped G151.2+2.6 is an HII
region with a flat radio spectrum, associated with optical filamentary
structure, H, and infrared emission.Comment: 5 pages, 3 figures, accepted for publication of Astronomy and
Astrophysic
Collision-free trajectory planning algorthm for manipulators
Collision-free trajectory planning for robotic manipulators is investigated. The task of the manipulator is to move its end-effector from one point to another point in an environment with polyhedral obstacles. An on-line algorithm is developed based on finding the required joint angles of the manipulator, according to goals with different priorities. The highest priority is to avoid collisions, the second priority is to plan the shortest path for the end effector, and the lowest priority is to minimize the joint velocity for smooth motion. The pseudo-inverse of the Jacobian matrix is applied for inverse kinematics. When a possible collision is detected, a constrained inverse kinematic problem is solved such that the collision is avoided. This algorithm can also be applied to a time-variant environment
Augmenting bug localization with part-of-speech and invocation
Bug localization represents one of the most expensive, as well as time-consuming, activities during software maintenance and evolution. To alleviate the workload of developers, numerous methods have been proposed to automate this process and narrow down the scope of reviewing buggy files. In this paper, we present a novel buggy source-file localization approach, using the information from both the bug reports and the source files. We leverage the part-of-speech features of bug reports and the invocation relationship among source files. We also integrate an adaptive technique to further optimize the performance of the approach. The adaptive technique discriminates Top 1 and Top N recommendations for a given bug report and consists of two modules. One module is to maximize the accuracy of the first recommended file, and the other one aims at improving the accuracy of the fixed defect file list. We evaluate our approach on six large-scale open source projects, i.e. ASpectJ, Eclipse, SWT, Zxing, Birt and Tomcat. Compared to the previous work, empirical results show that our approach can improve the overall prediction performance in all of these cases. Particularly, in terms of the Top 1 recommendation accuracy, our approach achieves an enhancement from 22.73% to 39.86% for ASpectJ, from 24.36% to 30.76% for Eclipse, from 31.63% to 46.94% for SWT, from 40% to 55% for ZXing, from 7.97% to 21.99% for Birt, and from 33.37% to 38.90% for Tomcat
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