Tharu Barghar-Mukhiya Indigenous Model: A Case Study of Tharu Community of Nepal

This research explores the indigenous conflict resolution processes practiced by the Tharu community living in Nepal’s Bara, Dang and Bardiya districts, the role of Tharu traditions and customs, and the function of the Barghar-Mukhiya. Due to geographic and monetary challenges experienced by the Tharu accessing Nepal’s formal justice system, they continue to serve as a viable and vibrant vehicle for resolving minor and major conflicts at the community level and form the basis of researcher’s Barghar-Mukhiya model. Shaped by Tharu collectivist culture and traditions, it supports the social fabric of the community. Utilizing qualitative case study methodology, this research assesses important aspects of the Barghar-Mukhiya model, processes and impact. Primary data sources include individual and focus group interviews, and researcher observations; and, secondary sources include document collections and archival material. Research findings explore six emergent themes: Rituals/Festivals, Inclusion/Dialogue, Identity/Security, Structure/Barghar-Mukhiya, Process/Reconciliation Processes, and Participation/Acceptance. This model is assessed for strengths and challenges. Where it is practiced, it continues to help maintain community harmony and peace. The model’s core of restorative practices, forgiveness, reconciliation, consensus-based decision-making, and use of dialogue circles is instrumental in transforming conflicts. This research contributes to the field of peace and conflict studies, providing analysis of an indigenous model that strives to reach a balance between traditional beliefs and the modern judicial system

BHUTANESE REFUGEES: ON UNDERSTANDING THE LINKS BETWEEN TRAUMA, DISPLACEMENT, AND COMMUNITY RESILIENCE

Through a unique community based participatory action research project with Bhutanese refugees and immigrants in the Triad area of North Carolina (Greensboro, High Point, and Winston-Salem), the authors explore the links between trauma, displacement, and community resilience. The social experience of displacement and relocation create impacts felt in the entire community. How do we understand and map these impacts and use them to transform community ills? While limited understanding of trauma and displacement among both the newly arrived and long-time citizens acts to limit the pro-social opportunities that trauma creates, the lack of mental health services and support for refugees allows post-traumatic growth in refugee communities to atrophy. While reviving trauma may seem counter-intuitive, we argue that the engagement of collective historical memory is a critical necessity for achieving change. As the United States’ largest community of South Asian refugees, the Bhutanese refugee experience, replete with a high rate of suicide, heart disease, and diabetes is a story largely left untold. This article aims to give voice to the experience of Bhutanese refugees so as to co-create community driven solutions to this community’s unique problems

GPS observations of ionospheric TEC variations over Nepal during 22 July 2009 solar eclipse

As the study of ionospheric behavior during various solar activities is an important task, various studies of ionospheric changes during eclipse events have been widely performed in the different regions of the globe. This paper investigates the ionospheric responses to the solar eclipse on 22 July 2009 over Nepal using the total electron content (TEC) measured by dual-frequency Global Positioning System (GPS) receivers. The time-averaged Vertical TEC (vTEC) of ten GPS stations from Nepal is analyzed and it is found that the value of ionospheric TEC decreases due to the reduction of ionizing radiation. In addition, the deviation in the TEC value on eclipse day from the mean vTEC value of the top five quietest days is found to lie in the range ~1–5 TECu at those regions which were associated with the partial eclipse shadow. On the other hand, the region with the total eclipse (BRN2 and RMTE) faced ~6–7 TECu on average reduction in the TEC value. Considering that the eclipse of 22 July 2009 occurred just at sunrise in the Nepalese zone, a maximum reduction of about 5 TECu is very significant. Higher deviation in TEC is therefore linked with the path of totality and the obscuration rate. This study reveals that the ionospheric TEC over Nepal was altered by wave-like energy and momentum transport, as well as obscuration of the solar disc due to the partial and total solar eclipse. Furthermore, the cross-correlation results presented similar type signatures of the eclipse-induced ionospheric modification over Nepal. This research work serves a crucial future reference for the comparative study of change of ionospheric TEC variability over the Nepal region during Eclipse event

Quasar UV/X-ray relation luminosity distances are shorter than reverberation-measured radius-luminosity relation luminosity distances

We use measurements of 59/58 quasars (QSOs), over a redshift range $0.0041\leq z \leq 1.686$, to do a comparative study of the radius--luminosity ($R-L$) and X-ray$-$UV luminosity ($L_X-L_{UV}$) relations and the implication of these relations for cosmological parameter estimation. By simultaneously determining $R-L$ or $L_X-L_{UV}$ relation parameters and cosmological parameters in six different cosmological models, we find that both $R-L$ and $L_X-L_{UV}$ relations are standardizable but provide only weak cosmological parameter constraints, with $L_X-L_{UV}$ relation data favoring larger current non-relativistic matter density parameter $\Omega_{m0}$ values than $R-L$ relation data and most other available data. We derive $L_X-L_{UV}$ and $R-L$ luminosity distances for each of the sources in the six cosmological models and find that $L_X-L_{UV}$ relation luminosity distances are shorter than $R-L$ relation luminosity distances as well as standard flat $\Lambda$CDM model luminosity distances. This explains why $L_X-L_{UV}$ relation QSO data favor larger $\Omega_{m0}$ values than do $R-L$ relation QSO data or most other cosmological measurements. While our sample size is small and only spans a small $z$ range, these results indicate that more work is needed to determine whether the $L_X-L_{UV}$ relation can be used as a cosmological probe.Comment: 20 pages, 10 figures, MNRAS in pres