Eric Henry Stoneley Burhop, 31 January 1911 - 22 January 1980

1981 ◽  
Vol 27 ◽  
pp. 131-152 ◽  

Eric Henry Stoneley Burhop was born on 31 January 1911 at Hobart, Tasmania, of parents who were Salvation Army officers in poor financial circumstances. Because of the itinerant nature of his parents’ work he often had to change schools. Nevertheless, it soon became apparent that he possessed ability far above the average and his parents were prepared to sacrifice much to give him an opportunity to pursue his education through secondary school and early university until he was able to pay his own way with scholarships. He attended Ballarat and then Melbourne High School before entering Melbourne University as an engineering student in 1928. After one year he changed over to read science, specializing in physics. In 1929 he was awarded an Aitchison Bursary which assisted him financially through the remainder of his undergraduate career. He graduated B.Sc. with first class honours in physics in 1931 and then undertook an M .Sc. course in that subject. At the same time, because of his mathematical ability and interest, he completed the final honours course in mathematics to obtain the B.A. degree in 1932. Professor T . H. Laby, F .R .S., head of the Physics Department at Melbourne University, who took a close interest in promising students, realized that Burhop was exceptional and encouraged him to work towards a scientific career. The research problem for the M .Sc. which Laby proposed was quite a challenging one for the time— the determ ination of the probability of K shell ionization by electron impact, from measurements of the intensity of X -ray emission as a function of electron energy.

2020 ◽  
Author(s):  
Sarah Quais ◽  
Ammar Suhail

Abstract Background: Congenital fused/block vertebrae is an accidental finding in most cases. It remains asymptomatic unless struck by any traumatic event or repetitive event occurs. Symptomatic cases can present with several musculoskeletal impairments including one starting from neck pain. It should be addressed properly to help patients recover the mechanical strains on the structures.Case Presentation: A referred case of a 21-year-old male engineering student who presented with complaints of neck pain (non-radiating) for a week. The intensity of the pain had been intermittently increasing/decreasing for about a year and about 2-3 episodes in a month for approximately one year. He presented with an X-ray which showed C-3/C-4 block vertebrae. The patient was managed using pain education and exercises along with ergonomic advice.Conclusion: Patient-reported pain was decreased significantly from the initial visit. The patient was able to sit for a longer duration and had a considerable improvement in function.


2017 ◽  
Vol 30 (1) ◽  
pp. 63-77 ◽  
Author(s):  
Bruce Allen Stevens ◽  
Rhonda Shaw ◽  
Peter Bewert ◽  
Mavis Salt ◽  
Jennifer Ma

2019 ◽  
Vol 33 (3) ◽  
pp. 299-317
Author(s):  
Andrew Cameron ◽  
Bruce Stevens ◽  
Rhonda Shaw ◽  
Peter Bewert ◽  
Mavis Salt ◽  
...  

A research project by the Schools of Theology and Psychology of Australia’s Charles Sturt University surveyed a large sample of Salvation Army officers. This article considers survey responses to two questions relating to end-of-life care: the use of pain medications that may shorten life, and the cessation of fluid and food intake. The results of the analyses are evaluated in terms of Michael Banner’s proposal that moral theology should more assiduously converse with ‘patient ethnographic study’, which the survey instantiates to some extent. Banner’s proposal and the results of the survey are contrasted to Peter Singer’s analytical moral philosophical dictums on end-of-life care. The results are also compared to a metastudy by Andrea Rodríguez-Prat and Evert van Leeuwen of 14 ethnographic studies of those who wish to hasten death at the end of life. We conclude that respondents exemplify a form of moral reasoning that is embedded within Christian spirituality; counters the assumptions of Singer’s approach; contrasts the diminishment of ‘meaning’ at the end of life, as seen in Rodríguez-Prat and van Leeuwen; and deserves further respectful ethnographic study.


Author(s):  
R.F. Egerton

SIGMAL is a short (∼ 100-line) Fortran program designed to rapidly compute cross-sections for L-shell ionization, particularly the partial crosssections required in quantitative electron energy-loss microanalysis. The program is based on a hydrogenic model, the L1 and L23 subshells being represented by scaled Coulombic wave functions, which allows the generalized oscillator strength (GOS) to be expressed analytically. In this basic form, the model predicts too large a cross-section at energies near to the ionization edge (see Fig. 1), due mainly to the fact that the screening effect of the atomic electrons is assumed constant over the L-shell region. This can be remedied by applying an energy-dependent correction to the GOS or to the effective nuclear charge, resulting in much closer agreement with experimental X-ray absorption data and with more sophisticated calculations (see Fig. 1 ).


Materials ◽  
2018 ◽  
Vol 11 (12) ◽  
pp. 2572 ◽  
Author(s):  
Ya-Na Wu ◽  
Dar-Bin Shieh ◽  
Li-Xing Yang ◽  
Hwo-Shuenn Sheu ◽  
Rongkun Thordarson ◽  
...  

Finding a cancer-selective drug that avoids damaging healthy cells and organs is a holy grail in medical research. In our previous studies, gold-coated iron (Fe@Au) nanoparticles showed cancer selective anti-cancer properties in vitro and in vivo but were found to gradually lose that activity with storage or "ageing.” To determine the reasons for this diminished anti-cancer activity, we examined Fe@Au nanoparticles at different preparation and storage stages by means of transmission electron microscopy combined with and energy-dispersive X-ray spectroscopy, along with X-ray diffraction analysis and cell viability tests. We found that dried and reconstituted Fe@Au nanoparticles, or Fe@Au nanoparticles within cells, decompose into irregular fragments of γ-F2O3 and agglomerated gold clumps. These changes cause the loss of the particles’ anti-cancer effects. However, we identified that the anti-cancer properties of Fe@Au nanoparticles can be well preserved under argon or, better still, liquid nitrogen storage for six months and at least one year, respectively.


2018 ◽  
Vol 620 ◽  
pp. L13 ◽  
Author(s):  
A. Rouco Escorial ◽  
J. van den Eijnden ◽  
R. Wijnands

We present our Swift monitoring campaign of the slowly rotating neutron star Be/X-ray transient GX 304–1 (spin period of ∼275 s) when the source was not in outburst. We found that between its type I outbursts, the source recurrently exhibits a slowly decaying low-luminosity state (with luminosities of 1034 − 35 erg s−1). This behaviour is very similar to what has been observed for another slowly rotating system, GRO J1008–57. For that source, this low-luminosity state has been explained in terms of accretion from a non-ionised (“cold”) accretion disc. Because of the many similarities between the two systems, we suggest that GX 304–1 enters a similar accretion regime between its outbursts. The outburst activity of GX 304–1 ceased in 2016. Our continued monitoring campaign shows that the source is in a quasi-stable low-luminosity state (with luminosities a few factors lower than previously seen) for at least one year now. Using our NuSTAR observation in this state, we found pulsations at the spin period, demonstrating that the X-ray emission is due to accretion of matter onto the neutron star surface. If the accretion geometry during this quasi-stable state is the same as during the cold-disc state, then matter indeed reaches the surface (as predicted) during this later state. We discuss our results in the context of the cold-disc accretion model.


1968 ◽  
Vol 1 ◽  
pp. 202-205
Author(s):  
Laurence E. Peterson

In this paper we wish to present briefly the latest results which have been obtained on the hard X-ray spectra of two strong sources in the Northern skies. These observations, which have been discussed in detail previously (Peterson et al., 1967), were made from balloons launched at Palestine, Texas, to 3 gm/cm2 atmospheric depth during September 1966. The Crab Nebula and the Cygnus XR-1 were observed to have a differential number power law spectra with an index of about –2 over the 20–200 keV range. Both sources have the same intensity within about 10%. The Crab Nebula has been observed on two occasions, one year apart, and showed no change in intensity over this range at about a 5% significance level.


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