Inspirational Teaching: Beyond Excellence and Towards Collaboration for Learning with Sustained Impact

Within higher education, there is a continued focus on teaching quality, with teaching excellence often linked to the idea of engaging and motivating students. This article examines the concept of ‘inspirational’ teaching, going beyond notions of excellent teaching, and proposes that inspirational teaching is defined by being transformational in the sense that it has a sustained positive impact on student learning. By exploring current literature on inspirational teaching, including some literature on teaching excellence, four overarching themes are identified as constituents of inspirational teaching: knowledge and passion for the subject, understanding learning and knowledge, constructive and challenging learning environment and students as individuals, partners and colleagues. The practices of the inspirational teachers presented are characterised by their focus on student learning rather than teacher performance and so indicate that inspirational teaching is an outcome that cannot be reduced to a set of characteristics or practices. Finally, we conclude that collaborative and scholarly relationships between students and teachers underpin these four themes and are central to creating inspirational learning experiences

Investigating Peer Tutoring for Academic Writing Support in a UK University

This project outlines the rationale, design, and findings of a peer tutoring project in a UK teaching-led university. Three students received training and tutored their peers in academic writing. Qualitative data was collected from both peer tutors and tutees; quantitative data was collected through a questionnaire administered by the institution’s Careers department. Findings include a positive effect on the tutors’ self-perception of their own employability and understanding of the conventions of academic writing, along with positive feedback from students who received tuition

The use of non-surgical interventions in patients with periimplantitis; a systematic review and meta-analysis

Objectives: To systematically assess the efficacy of different non‐surgical treatment methods to manage peri‐implantitis reported to date in the literature, together with its correlation with time following therapy. Materials and Methods: A systematic literature review was undertaken to identify randomised control trials of the non‐surgical management of peri‐implantitis published up to November 2019. The search was limited to English language human studies containing follow‐up periods of ≥3 months and for sample size of 10 or more patients. A meta‐analysis was implemented for the following clinical parameters: Peri‐implant pocket depth (PPD), bleeding on probing (BOP), clinical attachment level (CAL), radiographic bone loss (RBL) and mucosal recession (MR). Results: Twelve articles met the inclusion criteria. Two principal treatment modalities were identified; mechanical debridement and laser therapy, with two adjunctive therapies antimicrobial and antiseptic agents. Non‐surgical interventions (ultrasonic scalers, Er:YAG laser and powdered air‐abrasive devices) showed significant clinical improvement in the short term (<3 months). Clinical benefit was demonstrated with the adjunctive use of antimicrobial agents in the short term but diminished with time. Antiseptic agents alone have no significant effect. Non‐surgical therapies applied in these studies failed to arrest mucosal recession, peri‐implant bone loss or reduce the counts of viable pathogens in the long term. Conclusion: The evidence demonstrate that the clinical parameters of peri‐implantitis, i.e. BOP, PPD and CAL may all be improved by simple mechanical debridement, using either ultrasonic instrumentation or Er:YAG laser therapy; adjunctive antimicrobial and antiseptic therapy. Further randomised control trials in this area are, however, required

On-Orbit Results From the NASA Time-Resolved Observations of Precipitation Structure and Storm Intensity With a Constellation of Smallsats (TROPICS) Mission

The NASA TROPICS Earth Venture (EVI-3) CubeSat constellation mission will provide nearly all-weather observations of 3-D temperature and humidity, as well as cloud ice and precipitation horizontal structure, at high temporal resolution to conduct high-value science investigations of tropical cyclones. TROPICS will provide rapid-refresh microwave measurements (median refresh rate better than 60 minutes for the baseline mission) over the tropics that can be used to observe the thermodynamics of the troposphere and precipitation structure for storm systems at the mesoscale and synoptic scale over the entire storm lifecycle. The TROPICS constellation mission comprises four 3UCubeSats (5.4 kg each) in two low-Earth orbital planes. Each CubeSat contains a Blue Canyon Technologies bus and a high-performance radiometer payload to provide temperature profiles using seven channels near the 118.75 GHz oxygen absorption line, water vapor profiles using three channels near the 183 GHz water vapor absorption line, imagery in a single channel near 90 GHz for precipitation measurements (when combined with higher resolution water vapor channels), and a single channel at 205 GHz that is more sensitive to precipitation-sized ice particles. TROPICS spatial resolution and measurement sensitivity is comparable with current state-of-the-art observing platforms. Two dedicated launches (two spacecraft per launch) for the TROPICS constellation mission on Rocket Lab Electron vehicles occurred in 2023 (May 8 and May 26) to place the spacecraft in 32.75-degree inclined orbits at 550 km altitude. Data will be downlinked to the ground via the KSAT-Lite ground network. NASA\u27s Earth System Science Pathfinder (ESSP) Program Office approved the separate TROPICS Pathfinder mission, which launched on June 30, 2021, in advance of the TROPICS constellation mission as a technology demonstration and risk reduction effort. The TROPICS Pathfinder mission has provided an opportunity to checkout and optimize all mission elements prior to the primary constellation mission and is still operating nominally

TXS 0506+056 with Updated IceCube Data

Past results from the IceCube Collaboration have suggested that the blazar TXS 0506+056 is a potential source of astrophysical neutrinos. However, in the years since there have been numerous updates to event processing and reconstruction, as well as improvements to the statistical methods used to search for astrophysical neutrino sources. These improvements in combination with additional years of data have resulted in the identification of NGC 1068 as a second neutrino source candidate. This talk will re-examine time-dependent neutrino emission from TXS 0506+056 using the most recent northern-sky data sample that was used in the analysis of NGC 1068. The results of using this updated data sample to obtain a significance and flux fit for the 2014 TXS 0506+056 "untriggered" neutrino flare are reported

Galactic Core-Collapse Supernovae at IceCube: “Fire Drill” Data Challenges and follow-up

The next Galactic core-collapse supernova (CCSN) presents a once-in-a-lifetime opportunity to make astrophysical measurements using neutrinos, gravitational waves, and electromagnetic radiation. CCSNe local to the Milky Way are extremely rare, so it is paramount that detectors are prepared to observe the signal when it arrives. The IceCube Neutrino Observatory, a gigaton water Cherenkov detector below the South Pole, is sensitive to the burst of neutrinos released by a Galactic CCSN at a level >10σ. This burst of neutrinos precedes optical emission by hours to days, enabling neutrinos to serve as an early warning for follow-up observation. IceCube\u27s detection capabilities make it a cornerstone of the global network of neutrino detectors monitoring for Galactic CCSNe, the SuperNova Early Warning System (SNEWS 2.0). In this contribution, we describe IceCube\u27s sensitivity to Galactic CCSNe and strategies for operational readiness, including "fire drill" data challenges. We also discuss coordination with SNEWS 2.0

All-Energy Search for Solar Atmospheric Neutrinos with IceCube

The interaction of cosmic rays with the solar atmosphere generates a secondary flux of mesons that decay into photons and neutrinos – the so-called solar atmospheric flux. Although the gamma-ray component of this flux has been observed in Fermi-LAT and HAWC Observatory data, the neutrino component remains undetected. The energy distribution of those neutrinos follows a soft spectrum that extends from the GeV to the multi-TeV range, making large Cherenkov neutrino telescopes a suitable for probing this flux. In this contribution, we will discuss current progress of a search for the solar neutrino flux by the IceCube Neutrino Observatory using all available data since 2011. Compared to the previous analysis which considered only high-energy muon neutrino tracks, we will additionally consider events produced by all flavors of neutrinos down to GeV-scale energies. These new events should improve our analysis sensitivity since the flux falls quickly with energy. Determining the magnitude of the neutrino flux is essential, since it is an irreducible background to indirect solar dark matter searches