Influence of climate on landscape characteristics in safety assessments of repositories for radioactive wastes.

In safety assessments of repositories for radioactive wastes, large spatial and temporal scales have to be considered when developing an approach to risk calculations. A wide range of different types of information may be required. Local to the site of interest, temperature and precipitation data may be used to determine the erosional regime (which may also be conditioned by the vegetation characteristics adopted, based both on climatic and other considerations). However, geomorphological changes may be governed by regional rather than local considerations, e.g. alteration of river base levels, river capture and drainage network reorganisation, or the progression of an ice sheet or valley glacier across the site. The regional climate is in turn governed by the global climate. In this work, a commentary is presented on the types of climate models that can be used to develop projections of climate change for use in post-closure radiological impact assessments of geological repositories for radioactive wastes. These models include both Atmosphere-Ocean General Circulation Models and Earth Models of Intermediate Complexity. The relevant outputs available from these models are identified and consideration is given to how these outputs may be used to inform projections of landscape development. Issues of spatial and temporal downscaling of climate model outputs to meet the requirements of local-scale landscape development modelling are also addressed. An example is given of how climate change and landscape development influence the radiological impact of radionuclides potentially released from the deep geological disposal facility for spent nuclear fuel that SKB (the Swedish Nuclear Fuel and Waste Management Company) proposes to construct at Forsmark, Sweden.

Limits on neutrino emission from gamma-ray bursts with the 40 string IceCube detector.

IceCube has become the first neutrino telescope with a sensitivity below the TeV neutrino flux predicted from gamma-ray bursts if gamma-ray bursts are responsible for the observed cosmic-ray flux above 10(18) eV. Two separate analyses using the half-complete IceCube detector, one a dedicated search for neutrinos from pγ interactions in the prompt phase of the gamma-ray burst fireball and the other a generic search for any neutrino emission from these sources over a wide range of energies and emission times, produced no evidence for neutrino emission, excluding prevailing models at 90% confidence.

Cosmic ray electrons and positrons from supernova explosions of massive stars.

We attribute the recently discovered cosmic ray electron and cosmic ray positron excess components and their cutoffs to the acceleration in the supernova shock in the polar cap of exploding Wolf-Rayet and red supergiant stars. Considering a spherical surface at some radius around such a star, the magnetic field is radial in the polar cap as opposed to most of 4pi (the full solid angle), where the magnetic field is nearly tangential. This difference yields a flatter spectrum, and also an enhanced positron injection for the cosmic rays accelerated in the polar cap. This reasoning naturally explains the observations. Precise spectral measurements will be the test, as this predicts a simple E;{-2} spectrum for the new components in the source, steepened to E;{-3} in observations with an E;{-4} cutoff.

Limits on a muon flux from neutralino annihilations in the sun with the IceCube 22-string detector.

A search for muon neutrinos from neutralino annihilations in the Sun has been performed with the IceCube 22-string neutrino detector using data collected in 104.3 days of live time in 2007. No excess over the expected atmospheric background has been observed. Upper limits have been obtained on the annihilation rate of captured neutralinos in the Sun and converted to limits on the weakly interacting massive particle (WIMP) proton cross sections for WIMP masses in the range 250-5000 GeV. These results are the most stringent limits to date on neutralino annihilation in the Sun.

Extending the search for neutrino point sources with IceCube above the horizon.

Point source searches with the IceCube neutrino telescope have been restricted to one hemisphere, due to the exclusive selection of upward going events as a way of rejecting the atmospheric muon background. We show that the region above the horizon can be included by suppressing the background through energy-sensitive cuts. This improves the sensitivity above PeV energies, previously not accessible for declinations of more than a few degrees below the horizon due to the absorption of neutrinos in Earth. We present results based on data collected with 22 strings of IceCube, extending its field of view and energy reach for point source searches. No significant excess above the atmospheric background is observed in a sky scan and in tests of source candidates. Upper limits are reported, which for the first time cover point sources in the southern sky up to EeV energies.

Observation of pulsed gamma-rays above 25 GeV from the Crab pulsar with MAGIC.

One fundamental question about pulsars concerns the mechanism of their pulsed electromagnetic emission. Measuring the high-end region of a pulsar's spectrum would shed light on this question. By developing a new electronic trigger, we lowered the threshold of the Major Atmospheric gamma-ray Imaging Cherenkov (MAGIC) telescope to 25 giga-electron volts. In this configuration, we detected pulsed gamma-rays from the Crab pulsar that were greater than 25 giga-electron volts, revealing a relatively high cutoff energy in the phase-averaged spectrum. This indicates that the emission occurs far out in the magnetosphere, hence excluding the polar-cap scenario as a possible explanation of our measurement. The high cutoff energy also challenges the slot-gap scenario.

Very-high-energy gamma rays from a distant quasar: how transparent is the universe?

The atmospheric Cherenkov gamma-ray telescope MAGIC, designed for a low-energy threshold, has detected very-high-energy gamma rays from a giant flare of the distant Quasi-Stellar Radio Source (in short: radio quasar) 3C 279, at a distance of more than 5 billion light-years (a redshift of 0.536). No quasar has been observed previously in very-high-energy gamma radiation, and this is also the most distant object detected emitting gamma rays above 50 gigaelectron volts. Because high-energy gamma rays may be stopped by interacting with the diffuse background light in the universe, the observations by MAGIC imply a low amount for such light, consistent with that known from galaxy counts.

Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector.

On 27 December 2004, a giant gamma flare from the Soft Gamma-Ray Repeater 1806-20 saturated many satellite gamma-ray detectors, being the brightest transient event ever observed in the Galaxy. AMANDA-II was used to search for down-going muons indicative of high-energy gammas and/or neutrinos from this object. The data revealed no significant signal, so upper limits (at 90% C.L.) on the normalization constant were set: 0.05(0.5) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the gamma flux and 0.4(6.1) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the high-energy neutrino flux.

Search for extraterrestrial point sources of neutrinos with AMANDA-II.

We present the results of a search for point sources of high-energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several active-galactic-nuclei blazars, microquasars, magnetars, and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

Evaluation of the Neuroscience Nurse Internship Program: the first decade.

This article describes the evaluation of the Neuroscience Nurse Internship Program (NNIP). The NNIP was initiated in 1988 by the National Institutes of Health Clinical Center to meet the demand for highly skilled nurses to care for persons with nervous system disorders. To determine whether the program was meeting its goals, an evaluation component was incorporated into the program. The evaluation process was based on the RSA Model of Continuing Education for nursing. The RSA model consists of four basic components, three of which were included in the assessment of the NNIP--process, content, and outcome. The evaluation revealed that the nurse-interns were satisfied with the lectures and clinical content of the program. Moreover, the nurse-interns improved their knowledge of neuroscience nursing and their confidence in performing neuroscience nursing skills. Information from the evaluation was used to modify the structure of the program and to refine lecture content and clinical requirements.

The Neuroscience Nurse Internship Program: the description.

This article describes the Neuroscience Nurse Internship Program (NNIP) and its implementation at the National Institutes of Health (NIH) Clinical Center in Bethesda, MD. The program, developed in 1988, is designed to prepare nurses to deliver care to persons with nervous system disorders. The program comprises 6 months of lecture and clinical instruction in the country's most well-known biomedical research center. In order to complete the program, nurse-interns must receive a passing grade of 90% or higher on all written tests and achieve satisfactory completion of all clinical assignments. NNIP is cosponsored by the NIH Clinical Center Nursing Department and the National Institute of Neurological Disorders and Stroke (NINDS). Nurses interested in NNIP may apply by submitting an application and a letter of interest to the Clinical Center Human Resources Department. Evaluation of the program is conducted on a regular basis and consists of both process and outcome assessments.

Differential diagnosis of malignant melanoma.

The incidence of malignant melanoma is rising. Early recognition and surgical treatment give the best chance for a cure. Since a variety of skin tumors and conditions may resemble melanoma, knowledge of the differential diagnosis and a systematic approach to the evaluation of a suspicious lesion are essential.

Production and reversal of the neuromuscular pathology and related signs of zinc deficiency in guinea pigs.

The purposes of this study were to use vocalization and posture as indices of the neuromuscular pathology that develops in zinc-deficient guinea pigs and to determine the rate of depletion before and of repletion after intraperitoneal (IP) zinc therapy. When severe signs of deficiency developed, tissues were analyzed for their zinc content to assess sites of depletable and mobilizable zinc stores. Weanling guinea pigs were fed low (less than 1 mg/kg) and adequate (100 mg/kg) zinc diets based on isolated soybean protein or autoclaved egg white. The first signs (stage 1) of vocalization due to handling, abnormal posture and skin lesions developed after approximately 4 wk. Severe (stage 3) signs followed after 5-6 wk. A single IP dose of ZnSO4 (50 mumol/kg) caused remission of signs within 4-5 d following which all signs regressed to stage 3 within 7 d. Analysis of 15 tissues from severely deficient guinea pigs showed that only plasma and bone had significantly lower zinc concentrations than tissues from comparable age-related controls fed a zinc-adequate diet. It seems unlikely that major soft tissues, such as muscle, brain, liver and skin, serve as mobilizable stores of zinc for other critical metabolic functions. Bone zinc is slowly mobilized but at a rate insufficient to maintain health or even life.

High affinity, calcium-stimulated adenosine triphosphatase activity in the particulate fraction of rat pancreatic acini.

Adenosine triphosphatase activity which is Mg2+-dependent and stimulated by submicromolar concentrations of Ca2+ (as Ca . ATP) was identified in the total particulate fraction of rat pancreatic acini. Half-maximal activity (V0.5) is obtained at 100.1 +/- 6 nM Ca . ATP with a Hill coefficient of 2.2 +/- 0.1 (mean +/- S.E.; n = 4). Maximal activity was 75 +/- 19 pmol of Pi released from ATP minute-1 microgram of membrane protein-1 (mean +/- S.E.; n = 7). High affinity Ca2+-ATPase activity was unaffected by ouabain, Na+, K+, La3+, and added calmodulin. Activity was slightly reduced by ruthenium red (0.1 mM) and by oligomycin (80 micrograms/ml) but was reduced almost 50% by the phenothiazine derivative fluphenazine in a dose-related and Ca2+-dependent manner. Hydrolysis of p-nitrophenyl phosphate was 9% of the rate of ATP hydrolysis and was independent of Ca2+ concentration. However, ADP, GTP, UTP, and ITP were hydrolyzed at 76-93% the rate that ATP was hydrolyzed with V0.5 values and Hill coefficients similar to those of Ca . ATP. We conclude that rat pancreatic acini contain an enzyme for active Ca2+ translocation: ATPase activity that is Mg2+-dependent and stimulated by submicromolar concentrations of Ca . ATP. Substrate hydrolysis appears to involve positive cooperative interactions of multiple ligand-binding sites and may be regulated in part by calmodulin.