Post-traumatic stress, personal risk and post-traumatic growth among UK journalists

Background: Journalists covering traumatic news events can develop symptoms of post-traumatic stress disorder (PTSD). However, they may also experience perceived post-traumatic growth (PTG). The outcome may be affected by whether work-related traumatic stress has a degree of personal risk. Objective: To investigate the relationship between PTSD symptoms and PTG among journalists who experienced work-related trauma and to examine whether positive associations would exist between exposure to personal risk and PTG. Method: A web-based survey measuring post-traumatic stress symptoms and post-traumatic growth was completed by print and broadcast journalists (N = 69) working for UK-based media organizations. An open-ended question asked participants how media organizations can help to promote growth after work-related trauma. Results: The findings show a significant relationship between PTSD symptoms and PTG (p = 0.04). Journalists working in war-zones had significantly more PTSD symptoms (p < .001) and PTG scores (p < .001) than those who did not. Journalists who described their worst, work-related trauma as having a degree of personal, life-threatening risk, also reported higher levels of PTG than those who did not (p < .001). This was consistent across all PTG subscales. Conclusions: This study, the first to examine PTSD symptoms, personal risk and post-traumatic growth within journalists, suggests those working in conflict areas experience significantly higher levels of post-traumatic stress and post-traumatic growth, than those who do not. Those who experience personal risk also had high PTG levels. Media companies can help develop PTG by recognizing when personal risk plays a role in covering demanding assignments. Participants suggested organizations also needed to allow sufficient time for reflection and meaning-making for all those working in hostile environments

Excitation of the W triplet Delta (U), W singlet Delta (U), B prime triplet Sigma (U) (minus), and A prime singlet Epsison (U) (minus) states of N2 by electron impact

Electron energy-loss spectra have been obtained for N2 at 20.6 eV impact energy, and scattering angles of 10-138 deg. The differential cross section for excitation of the W triplet Delta(U) state is the largest triplet-state cross section at all scattering angles, and is the largest inelastic cross section at angles greater than 70 degrees. (Author Modified Abstract

Molecular Hydrogen Optical Depth Templates for FUSE Data Analysis

The calculation and use of molecular hydrogen optical depth templates to quickly identify and model molecular hydrogen absorption features longward of the Lyman edge at 912 Angstroms are described. Such features are commonly encountered in spectra obtained by the Far Ultraviolet Spectroscopic Explorer and also in spectra obtained by the Space Telescope Imaging Spectrograph, albeit less commonly. Individual templates are calculated containing all the Lyman and Werner transitions originating from a single rotational state (J'') of the 0th vibrational level (v'') of the ground electronic state. Templates are provided with 0.01 Angstrom sampling for doppler parameters ranging from 2 <= b <= 20 km s^-1 and rotational states 0 <= J'' <= 15. Optical depth templates for excited vibrational states are also available for select doppler parameters. Each template is calculated for a fiducial column density of log[N(cm^-2)] = 21 and may be scaled to any column less than this value without loss of accuracy. These templates will facilitate the determination of the distribution of molecular hydrogen column density as a function of rotational level. The use of these templates will free the user from the computationally intensive task of calculating profiles for a large number of lines and allow concentration on line profile or curve-of-growth fitting to determine column densities and doppler parameters. The templates may be downloaded freely from http://www.pha.jhu.edu/~stephan/h2ools2.htmlComment: 20 pages, 2 tables, 6 figures, submitted to PASP 02-04-2003 Accepted for publication on 03-05-2003 with revisions, including modified fg1, modifed fg6 to become fg2 to support improved error discussion. To appear in the June 2003 issue of the PAS

The excitation of O2 in auroras

Newly measured electron impact cross sections for excitation of the a 1 Delta g and b 1 Sigma g+ electronic states of O2 were employed to predict the absolute volume emission rates from these states under auroral conditions. A secondary electron electron flux typical of an IBC II nighttime aurora was used and the most important quenching processes were included in the calculations. The new excitation cross sections for the a 1 Delta g and b 1 Sigma g+ states are more than an order of magnitude larger than previous estimates, and lead to correspondingly greater intensities in the atmospheric and IR-atmospheric band systems. The calculated intensity ratios of the volume emission rates of 7621 A and 1.27 microns to that for 3914 A are smaller than obtained from aircraft observations and recent rocket experiments

Near threshold response of a wave shifted Cerenkov radiator to heavy ions

The response of Pilot 425 to heavy ions with energies less than 600 MeV/amu beta approximately 0.8 is examined both theoretically and experimentally. Measurements are presented from an experiment which employed a Ne-20 beam at many energies below 575 MeV/amu. The signal is assumed to come from three sources: (1) Cerenkov light from the heavy ion, (2) Cerenkov light from secondary electrons, and (3) scintillation of the radiator. It is found that the effective index of refraction is 1.518 and that scintillation is present at a level of approximately 2.7 percent of the Cerenkov signal for beta = 1 for Ne-20. The first of these values differs from values previously quoted in the literature

High resolution Cerenkov and range detectors for balloon-borne cosmic-ray experiment

A combination of an active Cerenkov detector and passive range detectors is proposed for the high resolution measurement of isotopic composition in the neighborhood of iron in the galactic cosmic rays. A large area (4,300 sq cm) Cerenkov counter and passive range detectors were tested. Tests with heavy ions (2.1 GeV/amu C-12, 289 MeV/amu Ar-40, and 594 MeV/amu Ne-20) revealed the spatial uniformity of response of the Cerenkov counter to be better than 1% peak-to-peak. Light collection efficiency is independent of projectile energy and incidence angle to within at least 0.5%. Passive Lexan track recorders to measure range in the presence of the nuclear interaction background which results from stopping particles through 0.9 interaction lengths of matter were also tested. It was found that nuclear interactions produce an effective range straggling distribution only approximately 75% wider than that expected from range straggling alone. The combination of these tested techniques makes possible high mass resolution in the neighborhood of iron

A Composite Genome Approach to Identify Phylogenetically Informative Data from Next-Generation Sequencing

We have developed a novel method to rapidly obtain homologous genomic data for phylogenetics directly from next-generation sequencing reads without the use of a reference genome. This software, called SISRS, avoids the time consuming steps of de novo whole genome assembly, genome-genome alignment, and annotation. For simulations SISRS is able to identify large numbers of loci containing variable sites with phylogenetic signal. For genomic data from apes, SISRS identified thousands of variable sites, from which we produced an accurate phylogeny. Finally, we used SISRS to identify phylogenetic markers that we used to estimate the phylogeny of placental mammals. We recovered phylogenies from multiple datasets that were consistent with previous conflicting estimates of the relationships among mammals. SISRS is open source and freely available at https://github.com/rachelss/SISRS.Comment: 12 pages plus36 figures, 1 supplementary table, 3 supplementary figure

Hunting Causes and Using Them: Is There No Bridge from Here to There?

Causation is in trouble—at least as it is pictured in current theories in philosophy and in economics as well, where causation is also once again in fashion. In both disciplines the accounts of causality on offer are either modelled too closely on one or another favoured method for hunting causes or on assumptions about the uses to which causal knowledge can be put—generally for predicting the results of our efforts to change the world. The first kind of account supplies no reason to think that causal knowledge, as it is pictured, is of any use; the second supplies no reason to think our best methods will be reliable for establishing causal knowledge. So, if these accounts are all there is to be had, how do we get from method to use? Of what use is knowledge of causal laws that we work so hard to obtain

Quantifying the Human-Nature Relationship: A User\u27s Guide

A growing trend in environmental research is the quantification of the human-nature relationship. This review of human-nature psychometric instruments should be used as a reference for individuals seeking to incorporate these tools into their outdoor and environmental education research. Extensive literature review and autoethnographic techniques were employed to identify and evaluate thirty-four instruments. Instruments were evaluated on structure, ease of use, and concepts represented. Diversity exists amongst the instruments in terms of length, concepts reflected, and structure. The majority of tools reflect environmental attitudes/views (16) or relationship/connection with nature (13). Fewer instruments reflect concern, identity, or environmental behavior. Twenty-eight instruments are deemed easy to use, based on time required to complete and ease of scoring. A timeline outlining the development of the instruments is presented and conclusions and recommendations from original and comparative studies are summarized