8,520 research outputs found
The answers are within me. An evaluation of a person centred counselling service for men at HMP Doncaster who have had experience of domestic violence 2005-2007
This report is the second year evaluation of the person centred counselling service for male victims and perpetrators of domestic violence at HMP Doncaster in 2006/7. This report follows on from the previous year's evaluation, Raging Anger Within Me, which evaluated this project in 2005/6. Initiated by the Doncaster Rape and Sexual Abuse Counselling Centre (DRSACC), the second year of counselling service delivery was also funded by Lloyds TSB and the Tudor Trust.
The report provides a background to the service offered, details the key factors in the service's success and makes recommendations for the future sustainability of this innovative service. The report also contains a particularly interesting section detailing how the appropriateness of the service is perceived by experienced prison staff
Organic Haze as a Biosignature in Anoxic Earth-like Atmospheres
Early Earth may have hosted a biologically-mediated global organic haze
during the Archean eon (3.8-2.5 billion years ago). This haze would have
significantly impacted multiple aspects of our planet, including its potential
for habitability and its spectral appearance. Here, we model worlds with
Archean-like levels of carbon dioxide orbiting the ancient sun and an M4V dwarf
(GJ 876) and show that organic haze formation requires methane fluxes
consistent with estimated Earth-like biological production rates. On planets
with high fluxes of biogenic organic sulfur gases (CS2, OCS, CH3SH, and
CH3SCH3), photochemistry involving these gases can drive haze formation at
lower CH4/CO2 ratios than methane photochemistry alone. For a planet orbiting
the sun, at 30x the modern organic sulfur gas flux, haze forms at a CH4/CO2
ratio 20% lower than at 1x the modern organic sulfur flux. For a planet
orbiting the M4V star, the impact of organic sulfur gases is more pronounced:
at 1x the modern Earth organic sulfur flux, a substantial haze forms at CH4/CO2
~ 0.2, but at 30x the organic sulfur flux, the CH4/CO2 ratio needed to form
haze decreases by a full order of magnitude. Detection of haze at an
anomalously low CH4/CO2 ratio could suggest the influence of these biogenic
sulfur gases, and therefore imply biological activity on an exoplanet. When
these organic sulfur gases are not readily detectable in the spectrum of an
Earth-like exoplanet, the thick organic haze they can help produce creates a
very strong absorption feature at UV-blue wavelengths detectable in reflected
light at a spectral resolution as low as 10. In direct imaging, constraining
CH4 and CO2 concentrations will require higher spectral resolution, and R > 170
is needed to accurately resolve the structure of the CO2 feature at 1.57
{\mu}m, likely, the most accessible CO2 feature on an Archean-like exoplanet.Comment: accepted for publication in Astrobiolog
European Union - Reforms - Hungarian interests. What kind of European Union would we like?
The lecture deals with broad topics. First, it addresses some questions related to the current state of the EU integration regarding institutions and common policies. Second, it discusses the continued importance, the main results and hindering factors related to the Lisbon Programme, with a special emphasis on the educational system in Europe and Hungary. Third, the lecture deals with some possibilities in changing the EU’s rather limited external relation models to more flexible instruments
A systematic review and economic evaluation of subcutaneous and sublingual allergen immunotherapy in adults and children with seasonal allergic rhinitis
© Queen’s Printer and Controller of HMSO 2013Severe allergic rhinitis uncontrolled by conventional medication can substantially affect quality of life. Immunotherapy involves administering increasing doses of a specific allergen, with the aim of reducing sensitivity and symptomatic reactions. Recent meta-analyses have concluded that both subcutaneous immunotherapy (SCIT) and sublingual immunotherapy (SLIT) are more effective than placebo in reducing symptoms. It is uncertain which route of administration is more effective and whether or not treatment is cost-effective.National Institute for Health Research Health Technology Assessment programm
A Machine-Checked Formalization of the Generic Model and the Random Oracle Model
Most approaches to the formal analyses of cryptographic protocols make the perfect cryptography assumption, i.e. the hypothese that there is no way to obtain knowledge about the plaintext pertaining to a ciphertext without knowing the key. Ideally, one would prefer to rely on a weaker hypothesis on the computational cost of gaining information about the plaintext pertaining to a ciphertext without knowing the key. Such a view is permitted by the Generic Model and the Random Oracle Model which provide non-standard computational models in which one may reason about the computational cost of breaking a cryptographic scheme. Using the proof assistant Coq, we provide a machine-checked account of the Generic Model and the Random Oracle Mode
From Artifacts to Aggregations: Modeling Scientific Life Cycles on the Semantic Web
In the process of scientific research, many information objects are
generated, all of which may remain valuable indefinitely. However, artifacts
such as instrument data and associated calibration information may have little
value in isolation; their meaning is derived from their relationships to each
other. Individual artifacts are best represented as components of a life cycle
that is specific to a scientific research domain or project. Current cataloging
practices do not describe objects at a sufficient level of granularity nor do
they offer the globally persistent identifiers necessary to discover and manage
scholarly products with World Wide Web standards. The Open Archives
Initiative's Object Reuse and Exchange data model (OAI-ORE) meets these
requirements. We demonstrate a conceptual implementation of OAI-ORE to
represent the scientific life cycles of embedded networked sensor applications
in seismology and environmental sciences. By establishing relationships between
publications, data, and contextual research information, we illustrate how to
obtain a richer and more realistic view of scientific practices. That view can
facilitate new forms of scientific research and learning. Our analysis is
framed by studies of scientific practices in a large, multi-disciplinary,
multi-university science and engineering research center, the Center for
Embedded Networked Sensing (CENS).Comment: 28 pages. To appear in the Journal of the American Society for
Information Science and Technology (JASIST
Identifying Planetary Biosignature Impostors: Spectral Features of CO and O4 Resulting from Abiotic O2/O3 Production
O2 and O3 have been long considered the most robust individual biosignature
gases in a planetary atmosphere, yet multiple mechanisms that may produce them
in the absence of life have been described. However, these abiotic planetary
mechanisms modify the environment in potentially identifiable ways. Here we
briefly discuss two of the most detectable spectral discriminants for abiotic
O2/O3: CO and O4. We produce the first explicit self-consistent simulations of
these spectral discriminants as they may be seen by JWST. If JWST-NIRISS and/or
NIRSpec observe CO (2.35, 4.6 um) in conjunction with CO2 (1.6, 2.0, 4.3 um) in
the transmission spectrum of a terrestrial planet it could indicate robust CO2
photolysis and suggest that a future detection of O2 or O3 might not be
biogenic. Strong O4 bands seen in transmission at 1.06 and 1.27 um could be
diagnostic of a post-runaway O2-dominated atmosphere from massive H-escape. We
find that for these false positive scenarios, CO at 2.35 um, CO2 at 2.0 and 4.3
um, and O4 at 1.27 um are all stronger features in transmission than O2/O3 and
could be detected with SNRs 3 for an Earth-size planet orbiting a
nearby M dwarf star with as few as 10 transits, assuming photon-limited noise.
O4 bands could also be sought in UV/VIS/NIR reflected light (at 0.345, 0.36,
0.38, 0.445, 0.475, 0.53, 0.57, 0.63, 1.06, and 1.27 um) by a next generation
direct-imaging telescope such as LUVOIR/HDST or HabEx and would indicate an
oxygen atmosphere too massive to be biologically produced.Comment: 7 pages, 4 figures, accepted to the Astrophysical Journal Letter
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