2,119 research outputs found

    Solar Protons and Magnetic Storms in July 1961

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    Injun i satellite observations of solar protons and magnetic storm

    Prediction and explanation in the multiverse

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    Probabilities in the multiverse can be calculated by assuming that we are typical representatives in a given reference class. But is this class well defined? What should be included in the ensemble in which we are supposed to be typical? There is a widespread belief that this question is inherently vague, and that there are various possible choices for the types of reference objects which should be counted in. Here we argue that the ``ideal'' reference class (for the purpose of making predictions) can be defined unambiguously in a rather precise way, as the set of all observers with identical information content. When the observers in a given class perform an experiment, the class branches into subclasses who learn different information from the outcome of that experiment. The probabilities for the different outcomes are defined as the relative numbers of observers in each subclass. For practical purposes, wider reference classes can be used, where we trace over all information which is uncorrelated to the outcome of the experiment, or whose correlation with it is beyond our current understanding. We argue that, once we have gathered all practically available evidence, the optimal strategy for making predictions is to consider ourselves typical in any reference class we belong to, unless we have evidence to the contrary. In the latter case, the class must be correspondingly narrowed.Comment: Minor clarifications adde

    Characterization of iodine particles with Volatilization-Humidification Tandem Differential Mobility Analyser (VH-TDMA), Raman and SEM techniques

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    Particles formed upon photo-oxidation of CH2I2 and particles of I2O5 and HIO3 have been studied using a Volatilisation and Humidification Tandem Differential Mobility Analyser (VH-TDMA) system. Volatilization and hygroscopic behaviour have been investigated as function of temperature (from 25 to 400 degrees Celsius), humidity (RH from 80 to 98%), initial aerosol sizes (from 27 to 100 nm mobility diameter) and in nitrogen or air as the sheath gasses. The volatility behaviour of particles formed upon photo-oxidation of CH2I2 is more similar to that of HIO3 particles in a filtered sheath air than in nitrogen, with the particle shrinkage occurring at 190 degrees Celsius and accompanied by hygroscopic growth. Despite its high solubility, HIO3 was found not to be hygroscopic at room temperature with no significant growth displayed until the thermodenuder temperature reached 200 degrees Celsius or above when the particles have transformed into I2O5. Diiodopentaoxide (I2O5) particles exhibit relatively low hygroscopic growth factors of 1.2-2 in the humidity range investigated. Scanning Electron Microscopy (SEM) of particles formed upon photo-oxidation of CH2I2 shows that their primary elemental components were iodine and oxygen in a stoichiometric ratio of approximately 1:2 with 10% error. Both Raman spectra and SEM show poor crystallinity for all the aerosols produced

    Relativistic Disk Reflection in the Neutron Star X-ray Binary XTE J1709-267 with NuSTAR

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    We perform the first reflection study of the soft X-ray transient and Type 1 burst source XTE J1709-267 using NuSTAR observations during its 2016 June outburst. There was an increase in flux near the end of the observations, which corresponds to an increase from \sim0.04 LEdd_{\mathrm{Edd}} to \sim0.06 LEdd_{\mathrm{Edd}} assuming a distance of 8.5 kpc. We have separately examined spectra from the low and high flux intervals, which were soft and show evidence of a broad Fe K line. Fits to these intervals with relativistic disk reflection models have revealed an inner disk radius of 13.81.8+3.0 Rg13.8_{-1.8}^{+3.0}\ R_{g} (where Rg=GM/c2R_{g} = GM/c^{2}) for the low flux spectrum and 23.45.4+15.6 Rg23.4_{-5.4}^{+15.6}\ R_{g} for the high flux spectrum at the 90\% confidence level. The disk is likely truncated by a boundary layer surrounding the neutron star or the magnetosphere. Based on the measured luminosity and using the accretion efficiency for a disk around a neutron star, we estimate that the theoretically expected size for the boundary layer would be 0.91.1 Rg\sim0.9-1.1 \ R_{g} from the neutron star's surface, which can be increased by spin or viscosity effects. Another plausible scenario is that the disk could be truncated by the magnetosphere. We place a conservative upper limit on the strength of the magnetic field at the poles, assuming a=0a_{*}=0 and MNS=1.4 MM_{NS}=1.4\ M_{\odot}, of B0.753.70×109B\leq0.75-3.70\times10^{9} G, though X-ray pulsations have not been detected from this source.Comment: Accepted for publication in ApJ, 5 pages, 4 figures, 1 table. arXiv admin note: text overlap with arXiv:1701.0177

    The Rights and Wrongs of Wrongful Birth and Wrongful Life: A Jurisprudential Analysis of Birth Related Torts

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    The advent and increasing sophistication of medical technology, which allows the detection of birth defects in utero, has resulted in recognition of two tort claims unknown at common law: wrongful birth and wrongful life. There is an emerging trend in state legislatures and courts toward rejection of wrongful birth and wrongful life causes of action. This article provides a critical analysis of the legal, medical and ethical issues raised by wrongful birth/life causes of action. The authors utilize Hohfeldian analysis to determine the exact nature of the legal rights essential to a wrongful birth/life cause of action. The authors then turn to a utilitarian analysis to weigh the various interests involved in wrongful birth/life claims. The authors argue that a jurisprudential analysis of birth related torts demonstrates that wrongful birth and wrongful life causes of action are a radical departure from existing law, and require the recognition of new legal theories not recognized in common law or constitutional law
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