865 research outputs found
Limnologie et télédétection : situation actuelle et développements futurs
La télédétection satellitaire est un outil employé couramment et avec succès en océanographie. Il n'en va pas de même en limnologie, où les applications sont encore rares.Par le moyen d'une revue bibliographique, nous tentons d'en analyser les raisons. Après une brève description de l'outil et des satellites en service, l'on met en évidence la spécificité des cibles aquatiques, caractérisées par une réflectance basse et une profondeur d'investigation variable. Ces particularités, jointes à la composition complexe des eaux intérieures, rendent impossible l'extension pure et simple, à la limnologie, des algorithmes développés en océanographie.Néanmoins, nous montrons que la télédétection a été utilisée dans l'étude du bassin versant des lacs, ainsi que pour la cartographie de leurs limites, de la végétation aquatique, des courants, de la thermique et de la couleur de l'eau. Des modèles empiriques, exprimant la matière en suspension ou les paramètres de qualité de l'eau, ont été calculés et appliqués avec succès dans certains lacs.On établit ensuite une typologie des difficultés rencontrées dans l'application de la télédétection à la limnologie : intrinsèques (complexité de la composition), technologiques (capteurs actuels non adaptés aux cibles aquatiques) et institutionnels (coûts élevés et manque de professionnels de ta télédétection dans les cercles limnologiques).Finalement, l'on présente quelques propositions pratiques dans la perspective des nouveaux véhicules spatiaux et capteurs des années 90, qui devraient permettre une exploitation de l'énorme potentiel de la télédétection en limnologie.Remote sensing has been used successfully in oceanography for many years, whereas applications in limnology have been comparatively modest. We attempt to discover why from a review of the literature.After a brief description of remote sensing and of satellites in operation, we stress the specificity of inland waters targets compared with "solid" targets : low reflectivity in the visible and near infrared, complex water composition (chlorophyll, mineral suspensoids and gelbstoff which are not covariant) and the variable depth of investigation. Hence, simple chlorophyll and suspended solid retrieval algorithms, developed for type-I waters, cannot be applied to inland waters.Nonetheless, remote sensing may be, and has been applied effectively to the study and management of drainage basins and to the mapping of lake limits, aquatic vegetation, water masses, currents, thermal structures and water colour. Site-specific, regression-type models have been computed to express suspended solid concentration and water quality parameters as functions of radiante. So far, most of the applications have been performed on large lakes (Laurentian Great Lakes, Tahoe, Chad, Biwa, Balaton, Léman), where not only LANDSAT but also CZCS and AVHRR data have been in operation.A typology of present difficulties in applying remote sensing to limnology is proposed : intrinsic (complexity of inland waters), technological (land resource satellite bands not designed for water sensing, revisit time too long) and institutional difficulties (cost of data and equipment, and scarcity of limnologists proficient in remote sensing techniques)
Bridging the Accountability Gap: Rights for New Entities in the Information Society?
Technological developments in the information society bring new challenges, both to the applicability and to the enforceability of the law. One major challenge is posed by new entities such as pseudonyms, avatars, and software agents that operate at an increasing distance from the physical persons "behind" them (the "principal"). In case of accidents or misbehavior, current laws require that the physical or legal principal behind the entity be found so that she can be held to account. This may be problematic if the linkability of the principal and the operating entity is questionable.
In light of the ongoing developments in electronic agents, there is sufficient reason to conduct a review of the literature in order to more closely examine arguments for and against legal personhood for some nonhuman acting entities. This article also includes a discussion of alternative approaches to solving the "accountability gap.
First light of the VLT planet finder SPHERE. I. Detection and characterization of the sub-stellar companion GJ 758 B
GJ758 B is a brown dwarf companion to a nearby (15.76 pc) solar-type,
metal-rich (M/H = +0.2 dex) main-sequence star (G9V) that was discovered with
Subaru/HiCIAO in 2009. From previous studies, it has drawn attention as being
the coldest (~600K) companion ever directly imaged around a neighboring star.
We present new high-contrast data obtained during the commissioning of the
SPHERE instrument at the VLT. The data was obtained in Y-, J-, H-, and Ks-bands
with the dual-band imaging (DBI) mode of IRDIS, providing a broad coverage of
the full near-infrared (near-IR) range at higher contrast and better spectral
sampling than previously reported. In this new set of high-quality data, we
report the re-detection of the companion, as well as the first detection of a
new candidate closer-in to the star. We use the new 8 photometric points for an
extended comparison of GJ758 B with empirical objects and 4 families of
atmospheric models. From comparison to empirical object, we estimate a T8
spectral type, but none of the comparison object can accurately represent the
observed near-IR fluxes of GJ758 B. From comparison to atmospheric models, we
attribute a Teff = 600K 100K, but we find that no atmospheric model can
adequately fit all the fluxes of GJ758 B. The photometry of the new candidate
companion is broadly consistent with L-type objects, but a second epoch with
improved photometry is necessary to clarify its status. The new astrometry of
GJ758 B shows a significant proper motion since the last epoch. We use this
result to improve the determination of the orbital characteristics using two
fitting approaches, Least-Square Monte Carlo and Markov Chain Monte Carlo.
Finally, we analyze the sensitivity of our data to additional closer-in
companions and reject the possibility of other massive brown dwarf companions
down to 4-5 AU. [abridged]Comment: 20 pages, 15 figures. Accepted for publication in A&
First light of the VLT planet finder SPHERE. II. The physical properties and the architecture of the young systems PZ Tel and HD 1160 revisited
[Abridged] Context. The young systems PZ Tel and HD 1160, hosting known
low-mass companions, were observed during the commissioning of the new planet
finder SPHERE with several imaging and spectroscopic modes. Aims. We aim to
refine the physical properties and architecture of both systems. Methods. We
use SPHERE commissioning data and REM observations, as well as literature and
unpublished data from VLT/SINFONI, VLT/NaCo, Gemini/NICI, and Keck/NIRC2.
Results. We derive new photometry and confirm the nearly daily photometric
variability of PZ Tel A. Using literature data spanning 38 yr, we show that the
star also exhibits a long-term variability trend. The 0.63-3.8 mic SED of PZ
Tel B allows us to revise its properties: spectral type M7+/-1, Teff=2700+/-100
K, log(g)<4.5 dex, log(L/L_Sun)=-2.51+/-0.10 dex, and mass 38-72 MJ. The 1-3.8
mic SED of HD 1160 B suggests a massive brown dwarf or a low-mass star with
spectral type M5.5-7.0, Teff=3000+/-100 K, [M/H]=-0.5-0.0 dex,
log(L/L_Sun)=-2.81+/-0.10 dex, and mass 39-168 MJ. We confirm the deceleration
and high eccentricity (e>0.66) of PZ Tel B. For e<0.9, the inclination,
longitude of the ascending node, and time of periastron passage are well
constrained. The system is seen close to an edge-on geometry. We reject other
brown dwarf candidates outside 0.25" for both systems, and massive giant
planets (>4 MJ) outside 0.5" for the PZ Tel system. We also show that K1-K2
color can be used with YJH low-resolution spectra to identify young L-type
companions, provided high photometric accuracy (<0.05 mag) is achieved.
Conclusions. SPHERE opens new horizons in the study of young brown dwarfs and
giant exoplanets thanks to high-contrast imaging capabilities at optical and
near-infrared wavelengths, as well as high signal-to-noise spectroscopy in the
near-infrared from low (R~30-50) to medium resolutions (R~350).Comment: 25 pages, 23 figures, accepted for publication in A&A on Oct. 13th,
2015; version including language editing. Typo on co-author name on astroph
page corrected, manuscript unchange
Investigation of Effects of Geometric Dihedral on Low-speed Static Stability and Yawing Characteristics of an Untapered 45 Degree Sweptback-wing Model of Aspect Ratio 2.61
Low-speed Wind-tunnel Investigation of Lateral Control Characteristics of a 60 Degrees Triangular-wing Model Having Half-delta Tip Controls
The ANTARES Optical Beacon System
ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It
consists of a three dimensional array of photomultiplier tubes that can detect
the Cherenkov light induced by charged particles produced in the interactions
of neutrinos with the surrounding medium. High angular resolution can be
achieved, in particular when a muon is produced, provided that the Cherenkov
photons are detected with sufficient timing precision. Considerations of the
intrinsic time uncertainties stemming from the transit time spread in the
photomultiplier tubes and the mechanism of transmission of light in sea water
lead to the conclusion that a relative time accuracy of the order of 0.5 ns is
desirable. Accordingly, different time calibration systems have been developed
for the ANTARES telescope. In this article, a system based on Optical Beacons,
a set of external and well-controlled pulsed light sources located throughout
the detector, is described. This calibration system takes into account the
optical properties of sea water, which is used as the detection volume of the
ANTARES telescope. The design, tests, construction and first results of the two
types of beacons, LED and laser-based, are presented.Comment: 21 pages, 18 figures, submitted to Nucl. Instr. and Meth. Phys. Res.
Reactive oxygen-related diseases: therapeutic targets and emerging clinical indications
SIGNIFICANCE
Enhanced levels of reactive oxygen species (ROS) have been associated with different disease states. Most attempts to validate and exploit these associations by chronic antioxidant therapies have provided disappointing results. Hence, the clinical relevance of ROS is still largely unclear.
RECENT ADVANCES
We are now beginning to understand the reasons for these failures, which reside in the many important physiological roles of ROS in cell signaling. To exploit ROS therapeutically, it would be essential to define and treat the disease-relevant ROS at the right moment and leave physiological ROS formation intact. This breakthrough seems now within reach.
CRITICAL ISSUES
Rather than antioxidants, a new generation of protein targets for classical pharmacological agents includes ROS-forming or toxifying enzymes or proteins that are oxidatively damaged and can be functionally repaired.
FUTURE DIRECTIONS
Linking these target proteins in future to specific disease states and providing in each case proof of principle will be essential for translating the oxidative stress concept into the clinic. Antioxid. Redox Signal. 23, 1171-1185
Molecular excitation in the Interstellar Medium: recent advances in collisional, radiative and chemical processes
We review the different excitation processes in the interstellar mediumComment: Accepted in Chem. Re
- …
