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- Mustafa, Nida, et al.
(författare)
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The lived experiences of chronic pain among immigrant Indian-Canadian women : A phenomenological analysis
- 2020
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Ingår i: Canadian Journal of Pain. - : Taylor & Francis. - 2474-0527. ; 4:3, s. 40-50
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Tidskriftsartikel (refereegranskat)abstract
- Background. Chronic pain is a growing public health concern affecting 1.5 million people in Canada. In particular, it is a concern among the expanding immigrant population, as immigrant groups report higher pain intensity than non-immigrants. In 2011, the Indian population became the largest visible minority group, and continues to be the fastest growing. While the prevalence of chronic pain among Canadian-Indians is unknown, research has found a higher prevalence among Indian women than men in India, Malaysia, Singapore and the United Kingdom, with women reporting more severe pain. An understanding of how pain is experienced by this particular group is, therefore, important for providing culturally-sensitive care. Aims. This study explores the lived experiences of chronic pain among immigrant Indian women in Canada. Methods. Thirteen immigrant Indian women participated in a one-on-one interview exploring daily experiences of chronic pain. Results. Using thematic analysis informed by van Manen’s phenomenology of practice, four themes emerged: (1) the body in pain, (2) pain in the context of lived and felt space, (3) pain and relationships and (4) pain and time. Women revealed their experiences were shaped by gender roles and expectations enforced through culture. Specifically, a ‘dual gender-role’ was identified after immigration, in which women had to balance traditional household responsibilities of family labour and care, alongside employment outside the home, exacerbating pain. Conclusions. This research uncovers the multifaceted nature of chronic pain and identifies factors within the socio-cultural context which may place particular groups of women more at risk of living with pain.
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| 2. |
- Verscharen, Daniel, et al.
(författare)
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The angular-momentum flux in the solar wind observed during Solar Orbiter's first orbit
- 2021
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Ingår i: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 656
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Tidskriftsartikel (refereegranskat)abstract
- Aims. We present the first measurements of the angular-momentum flux in the solar wind recorded by the Solar Orbiter spacecraft. Our aim is to validate these measurements to support future studies of the Sun's angular-momentum loss. Methods. We combined 60-min averages of the proton bulk moments and the magnetic field measured by the Solar Wind Analyser and the magnetometer onboard Solar Orbiter. We calculated the angular-momentum flux per solid-angle element using data from the first orbit of the mission's cruise phase in 2020. We separated the contributions from protons and from magnetic stresses to the total angular-momentum flux.Results. The angular-momentum flux varies significantly over time. The particle contribution typically dominates over the magnetic-field contribution during our measurement interval. The total angular-momentum flux shows the largest variation and is typically anti-correlated with the radial solar-wind speed. We identify a compression region, potentially associated with a co-rotating interaction region or a coronal mass ejection, which leads to a significant localised increase in the angular-momentum flux, albeit without a significant increase in the angular momentum per unit mass. We repeated our analysis using the density estimate from the Radio and Plasma Waves instrument. Using this independent method, we find a decrease in the peaks of positive angular-momentum flux, but otherwise, our results remain consistent.Conclusions. Our results largely agree with previous measurements of the solar wind's angular-momentum flux in terms of amplitude, variability, and dependence on radial solar-wind bulk speed. Our analysis highlights the potential for more detailed future studies of the solar wind's angular momentum and its other large-scale properties with data from Solar Orbiter. We emphasise the need for studying the radial evolution and latitudinal dependence of the angular-momentum flux in combination with data from Parker Solar Probe and other assets at heliocentric distances of 1 au and beyond.
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