28,984 research outputs found
Image enhancement from a stabilised video sequence
The aim of video stabilisation is to create a new video sequence where the motions (i.e. rotations, translations) and scale differences between frames (or parts of a frame) have effectively been removed. These stabilisation effects can be obtained via digital video processing techniques which use the information extracted from the video sequence itself, with no need for additional hardware or knowledge about camera physical motion.
A video sequence usually contains a large overlap between successive frames, and regions of the same scene are sampled at different positions. In this paper, this multiple sampling is combined to achieve images with a higher spatial resolution. Higher resolution imagery play an important role in assisting in the identification of people, vehicles, structures or objects of interest captured by surveillance cameras or by video cameras used in face recognition, traffic monitoring, traffic law reinforcement, driver assistance and automatic vehicle guidance systems
Searching for unknown open clusters in the Tycho-2 catalog
We present 11 new open cluster candidates found in a systematic search for
unknown star clusters using the astrometric and photometric data included in
the Tycho2 catalog. The possible existence of these stellar aggregates is
supported by the analysis of proper motions, color-magnitude diagrams, stellar
density distributions, and by the visual inspection of the Digitized Sky Survey
(DSS) plates. With these tools we were able to determine mean absolute proper
motions as well as preliminary reddenings, distances and ages for the majority
of the candidates. We found that most of them are possibly nearby (closer than
about 600 pc) open clusters never studied before.Comment: 14 pages, 6 figures. Accepted by A&
The ACS Survey of Galactic Globular Clusters. III. The Double Subgiant Branch of NGC 1851
Photometry with HST's ACS reveals that the subgiant branch (SGB) of the
globular cluster NGC 1851 splits into two well-defined branches. If the split
is due only to an age effect, the two SGBs would imply two star formation
episodes separated by 1 Gyr. We discuss other anomalies in NGC 1851
which could be interpreted in terms of a double stellar population. Finally, we
compare the case of NGC 1851 with the other two globulars known to host
multiple stellar populations, and show that all three clusters differ in
several important respects.Comment: 22 pages, 7 figures, accepted for pubblication on Ap
Magnetic-Visual Sensor Fusion-based Dense 3D Reconstruction and Localization for Endoscopic Capsule Robots
Reliable and real-time 3D reconstruction and localization functionality is a
crucial prerequisite for the navigation of actively controlled capsule
endoscopic robots as an emerging, minimally invasive diagnostic and therapeutic
technology for use in the gastrointestinal (GI) tract. In this study, we
propose a fully dense, non-rigidly deformable, strictly real-time,
intraoperative map fusion approach for actively controlled endoscopic capsule
robot applications which combines magnetic and vision-based localization, with
non-rigid deformations based frame-to-model map fusion. The performance of the
proposed method is demonstrated using four different ex-vivo porcine stomach
models. Across different trajectories of varying speed and complexity, and four
different endoscopic cameras, the root mean square surface reconstruction
errors 1.58 to 2.17 cm.Comment: submitted to IROS 201
Characteristics of polar coronal hole jets
High spatial- and temporal-resolution images of coronal hole regions show a
dynamical environment where mass flows and jets are frequently observed. These
jets are believed to be important for the coronal heating and the acceleration
of the fast solar wind. We studied the dynamics of two jets seen in a polar
coronal hole with a combination of imaging from EIS and XRT onboard Hinode. We
observed drift motions related to the evolution and formation of these
small-scale jets, which we tried to model as well. We found observational
evidence that supports the idea that polar jets are very likely produced by
multiple small-scale reconnections occurring at different times in different
locations. These eject plasma blobs that flow up and down with a motion very
similar to a simple ballistic motion. The associated drift speed of the first
jet is estimated to be 27 km s. The average outward speed of
the first jet is km s, well below the escape speed, hence
if simple ballistic motion is considered, the plasma will not escape the Sun.
The second jet was observed in the south polar coronal hole with three XRT
filters, namely, Cpoly, Alpoly, and Almesh filters. We
observed that the second jet drifted at all altitudes along the jet with the
same drift speed of 7 km s. The enhancement in the light curves
of low-temperature EIS lines in the later phase of the jet lifetime and the
shape of the jet's stack plots suggests that the jet material is falls back,
and most likely cools down. To support this conclusion, the observed drifts
were interpreted within a scenario where reconnection progressively shifts
along a magnetic structure, leading to the sequential appearance of jets of
about the same size and physical characteristics. On this basis, we also
propose a simple qualitative model that mimics the observations.Comment: Accepted Astronomy and Astrophysic
Prevalence of Small-scale Jets from the Networks of the Solar Transition Region and Chromosphere
As the interface between the Sun's photosphere and corona, the chromosphere
and transition region play a key role in the formation and acceleration of the
solar wind. Observations from the Interface Region Imaging Spectrograph reveal
the prevalence of intermittent small-scale jets with speeds of 80-250 km/s from
the narrow bright network lanes of this interface region. These jets have
lifetimes of 20-80 seconds and widths of 300 km or less. They originate from
small-scale bright regions, often preceded by footpoint brightenings and
accompanied by transverse waves with ~20 km/s amplitudes. Many jets reach
temperatures of at least ~100000 K and constitute an important element of the
transition region structures. They are likely an intermittent but persistent
source of mass and energy for the solar wind.Comment: Figs 1-4 & S1-S5; Movies S1-S8; published in Science, including the
main text and supplementary materials. Reference: H. Tian, E. E. DeLuca, S.
R. Cranmer, et al., Science 346, 1255711 (2014
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