Work-in-Progress–Design and Evaluation of 360 VR Immersive Interactions in Nursing Education

Nurses need to be adequately prepared to practise competently in increasingly ethnically diverse communities. This study explored nurse educators' views regarding the extent and nature of pre-registration nursing education intended to prepare students for multi-ethnic practice in Wales. A qualitative approach was taken with a purposive sample of programme directors ( n = 6), branch leaders and lecturers ( n = 25) and practice mentors ( n = 35). Data were collected through focus groups, interviews, questionnaire and documentary review. Qualitative data were analysed using thematic analysis and three themes were identified: curriculum design and content, a theory–practice gap and personnel and material resources. Findings indicated that knowledge of the most effective way to prepare pre-registration nursing students for practice in multi-ethnic communities is ‘work in progress’ in Wales. Our findings raise questions about the extent to which the curriculum prepares students to engage with the Welsh social justice agenda. Improved clarity regarding what constitutes an adequate curriculum and improved preparation of nurse educators and mentors to competently and confidently prepare students for working within ethnically diverse communities is required.

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Meridional Circulation, Turbulence, and Diffusion Processes in Stars

International Astronomical Union Colloquium ◽

10.1017/s0252921100080477 ◽

1976 ◽

Vol 32 ◽

pp. 109-116 ◽

Cited By ~ 1

Author(s):

S. Vauclair

Keyword(s):

Convection Zone ◽

Diffusion Processes ◽

Meridional Circulation ◽

Diffusion Time ◽

Work In Progress ◽

First Results ◽

Stellar Envelopes ◽

And Diffusion ◽

Turbulence And Diffusion ◽

Hr Diagram

This paper gives the first results of a work in progress, in collaboration with G. Michaud and G. Vauclair. It is a first attempt to compute the effects of meridional circulation and turbulence on diffusion processes in stellar envelopes. Computations have been made for a 2 Mʘstar, which lies in the Am - δ Scuti region of the HR diagram.Let us recall that in Am stars diffusion cannot occur between the two outer convection zones, contrary to what was assumed by Watson (1970, 1971) and Smith (1971), since they are linked by overshooting (Latour, 1972; Toomre et al., 1975). But diffusion may occur at the bottom of the second convection zone. According to Vauclair et al. (1974), the second convection zone, due to He II ionization, disappears after a time equal to the helium diffusion time, and then diffusion may happen at the bottom of the first convection zone, so that the arguments by Watson and Smith are preserved.

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