Truly transdisciplinary approaches are needed to tackle the complex problems that the Arctic is facing at the moment. Collaboration between Indigenous rights holders and researchers through co-creative research approaches can result in high-quality research outcomes, but crucially also address colonial legacies and power imbalances, enhance mutual trust, and respect the rights of Indigenous Peoples. However, to be successful, collaborative research projects have specific requirements regarding research designs, timeframes, and dissemination of results, which often do not fit into the frameworks of academic calendars and funding guidelines. Funding agencies in particular play an important role in enabling (or disabling) meaningful collaboration between Indigenous rights holders and researchers. There is an urgent need to re-think existing funding-structures. This article will propose a new paradigm for the financing of Arctic research, which centres around the inclusion of Indigenous partners, researchers, and institutions from the initial planning stages of funding programmes to the final stages of research projects. These findings and recommendations have been contextualized based on critical reflections of the co-authors, a group of Indigenous and non-Indigenous partners, who have practiced their own collaborative work process, the challenges encountered, and lessons learned.
Aims. This paper investigates how the far-IR water ice features can be used to infer properties of disks around T Tauri stars and the water ice thermal history. We explore the power of future observations with SOFIA/HIRMES and SPICA's proposed far-IR instrument SAFARI. Methods. A series of detailed radiative transfer disk models around a representative T Tauri star are used to investigate how the far-IR water ice features at 45 and 63 µm change with key disk properties: disk size, grain sizes, disk dust mass, dust settling, and ice thickness. In addition, a series of models is devised to calculate the water ice emission features from warmup, direct deposit and cooldown scenarios of the water ice in disks. Results. Photodesorption from icy grains in disk surfaces weakens the mid-IR water ice features by factors 4-5. The far-IR water ice emission features originate from small grains at the surface snow line in disks at distance of 10-100 au. Unless this reservoir is missing in disks (e.g. transitional disks with large cavities), the feature strength is not changing. Grains larger than 10 µm do not contribute to the features. Grain settling (using turbulent description) is affecting the strength of the ice features by at most 15%. The strength of the ice feature scales with the disk dust mass and water ice fraction on the grains, but saturates for dust masses larger than 10 −4 M and for ice mantles that increase the dust mass by more than 50%. The various thermal histories of water ice leave an imprint on the shape of the features (crystalline/amorphous) as well as on the peak strength and position of the 45 µm feature. SOFIA/HIRMES can only detect crystalline ice features much stronger than simulated in our standard T Tauri disk model in deep exposures (1 hr). SPICA/SAFARI can detect the typical ice features in our standard T Tauri disk model in short exposures (10 min).Conclusions. The sensitivity of SPICA/SAFARI will allow the detailed study of the 45 and 63 µm water ice feature in unbiased surveys of T Tauri stars in nearby star forming regions and an estimate of the mass of their ice reservoir. The water ice emission features carry an imprint of the thermal history of the ice and thus can distinguish between various formation and transport scenarios. Amorphous ice at 45 µm that has a much broader and flatter peak could be detected in deep surveys if the underlying continuum can be well characterized and the baseline stability of SAFARI is better than a few percent.
In the Netherlands in the last decade, the number of pupils with Down's Syndrome integrated into regular schools has been growing. Previously such pupils were referred to special schools, and this research, undertaken by Annette Scheepstra, Sip Jan Pijl, and Professor Han Nakken from the University of Groningen, describes the steps taken by parents to apply for regular education placements; the decision‐making of the school teams; and the differences between these parents and other parents with pupils in regular education.
This perspective presents a statement of the 10th International Congress of Arctic Social Sciences Indigenous Knowledge and knowledge co-production panel and discussion group, 20 July 2021. The statement is designed to serve as a characterization of the state-of-the-art and guidance for further advancement of Indigenous Knowledge and knowledge co-production in the Arctic. It identifies existing challenges and provides specific recommendations for researchers, Indigenous communities, and funding agencies on meaningful recognition and engagement of Indigenous Knowledge systems.
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