Is Artificial Intelligence Really the Next Big Thing in Learning and Teaching in Higher Education? A Conceptual Paper

Artificial Intelligence in higher education (AIED) is becoming a more important research area with increasing developments and application of AI within the wider society. However, as yet AI based tools have not been widely adopted in higher education. As a result there is a lack of sound evidence available on the pedagogical impact of AI for learning and teaching. This conceptual paper thus seeks to bridge the gap and addresses the following question: is artificial intelligence really the new big thing that will revolutionise learning and teaching in higher education? Adopting the technological pedagogical content knowledge (TPACK) framework and the Unified Theory of Acceptance and Use of Technology (UTAUT) as the theoretical foundations, we argue that Artificial Intelligence (AI) technologies, at least in their current state of development, do not afford any real new advances for pedagogy in higher education. This is mainly because there does not seem to be valid evidence as to how the use of AI technologies and applications has helped students improve learning, and/or helped tutors make effective pedagogical changes. In addition, the pedagogical affordances of AI have not yet been clearly defined. The challenges that the higher education sector is currently experiencing relating to AI adoption are discussed at three hierarchical levels, namely national, institutional and personal levels. The paper ends with recommendations with regard to accelerating AI use in universities. This includes developing dedicated AI adoption strategies at the institutional level, updating the existing technology infrastructure and up-skilling academic tutors for AI

Perceptions of Chinese top-up students transitioning through a regional UK university: a longitudinal study using portrait methodology

This thesis seeks to gain a good understanding of the academic and social experiences of a group of Chinese top-up students when they are studying their top-up programme in a UK institution. It adopts the U curve model and Bottery’s variation of portrait methodology as the theoretical foundations. Data were collected through semi-structured interviews, which took place three times at the key transition stages of these students during their one-year study period, namely the moving in stage (pre-departure and post arrival), the moving through stage (the start of their top-up programme to the end of the first semester) and the moving out stage (the start of the second semester to the end of their top-up programme). After each interview, written portraits were produced for the participants based on their interview transcripts. The findings of this thesis suggest that firstly this group of Chinese top-up students seemed to have had a really difficult time during their journey in this UK institution. It appears that their perceptions and some aspects of their behaviour (academic) changed while they went through this one-year study abroad journey, however, other aspects of their behaviour (social) appeared to remain largely the same. Additionally, the transition experiences of most Chinese top-up students in this group seemed to have only partially followed the U curve model. In other words, they experienced the honeymoon, the crisis and the recovery stages, but not the readjustment stage. This study makes a contribution to both the U curve and the portrait methodology literature by showing that when studying the transitional experiences of international students, attention needs to be paid to the factors at the institutional and national levels, apart from those at the personal level. In addition, the findings demonstrate that portrait methodology may produce very different insights when it is applied to different groups of people

Perceptions of Chinese Top-Up Students Transitioning through a Regional UK University: A Longitudinal Study Using the U Curve Model

This article argues an urgent need to better understand the personal experiences of Chinese top-up students studying in the UK since the number of Chinese students taking year-long top-up programmes in the UK has risen rapidly in recent years. This lack of knowledge could potentially have implications for the reputation of some UK institutions and also the attractiveness of the UK higher education sector to future international students. This longitudinal study explored the academic and social experiences of 12 Chinese topup students in a UK institution in-depth and revealed that the students felt their experiences were influenced significantly by their surrounding contexts at the macro and meso levels, which, however, have been largely overlooked in existing research. This article suggests the importance of improving the communications between the partner institutions in China and the UK, and also providing sufficient pre-departure and after arrival support to Chinese top-up students at the institutional level

Policy concern about university students’ online professionalism in the post-pandemic era in UK context

The extensive and intensive online teaching and learning during the pandemic has provided good opportunities for academic staff and students to experiment with learning and teaching using synchronous communication technology and learning platforms. This experience is highly valuable for helping higher education institutions move learning and teaching practices forward after the pandemic. Indeed, many universities are considering adopting blended learning in the new era. However, it is worth noting that a number of emerging issues related to student behaviour also appeared during online learning, such as teaching to blank screens, students’ inappropriate use of social media icons, languages and their inappropriate outfits. It appears that these issues have not yet been investigated properly, and are not addressed by the existing codes of conduct, since these have been written mainly for face-to-face teaching. This study offers some important insights into students’ unprofessional online behaviour from tutors’ perspective, and also the experiences of academic tutors in managing such behaviour in formal online learning and teaching environments. It used semi-structured interviews to collect data, and analysed the narratives of 20 academic staff working in UK universities. The findings report and describe students’ unprofessional online behaviours witnessed by academic tutors in different academic disciplines. The findings also suggest that special attention needs to be paid to policymaking regarding online learning, in particular, in the area of students’ online professionalism

Chandra and ROSAT observations of Abell 194: detection of an X-ray cavity and mapping the dynamics of the cluster

Based on Chandra and ROSAT observations, we investigated the nearby poor cluster Abell 194, which hosts two luminous radio galaxies, NGC547 (3C 40B) and NGC541 (3C 40A). We demonstrated the presence of a large X-ray cavity (r~34 kpc) formed by the giant southern radio lobe arising from 3C 40B in NGC547. The estimated age of the cavity is t=7.9 x 10^7 years and the total work of the AGN is 3.3 x 10^59 erg, hence the cavity power is P_cav=1.3 x 10^44 erg/s. Furthermore, in the Chandra images of NGC545 and NGC541 we detected sharp surface brightness edges, identified as merger cold fronts, and extended tails. Using the pressure ratios between inside and outside the cold fronts we estimated that the velocities of NGC545 and NGC541 correspond to Mach-numbers of M=1.0^{+0.3}_{-0.5} and M=0.9^{+0.2}_{-0.5}, respectively. The low radial velocities of these galaxies relative to the mean radial velocity of Abell 194 imply that their motion is oriented approximately in the plane of the sky. Based on these and earlier observations, we concluded that NGC545 and NGC541 are falling through the cluster, whose center is NGC547, suggesting that Abell 194 is undergoing a significant cluster merger event. Additionally, we detected 20 bright X-ray sources around NGC547 and NGC541, a surprisingly large number, since the predicted number of resolved LMXBs and CXB sources is 2.2 and 4.1, respectively. To explain the nature of additional sources, different possibilities were considered, none of which are satisfactory. We also studied the origin of X-ray emission in Minkowski's Object, and concluded that it is most likely dominated by the population of HMXBs rather than by hot diffuse ISM. Moreover, in view of the galaxy dynamics in Abell 194, we explored the possibility that the starburst in Minkowski's Object was triggered by its past interaction with NGC541, and concluded that it may be a viable path.Comment: 12 pages, 7 figures, accepted for publication in Ap

Cross-Cultural Integration through the Lens of Loneliness: a Study of Chinese Direct Entry Students in the United Kingdom

This study explores cross-cultural integration of Chinese top-up students in a UK university from the perspective of loneliness. Existing research on integration has underplayed loneliness. This study used semi-structured interviews to collect data at three key transition points during the top-up year. The findings suggest that students experienced loneliness both within and beyond their group, notwithstanding a number of reasons why they might be expected to be less lonely than other international students. Loneliness seemed to have a significant impact on cross-cultural integration, and participants were also unable to form strong bonds within their cohort of Chinese top-up students, and unable to experience healthy solitude. There are implications for the pre-departure preparation of such students, for the institutions hosting such students, and for responses to the social and emotional challenges they experience

Young AGN outburst running over older X-ray cavities

Although the energetic feedback from active galactic nuclei (AGN) is believed to have a profound effect on the evolution of galaxies and clusters of galaxies, details of the AGN heating remain elusive. Here, we study NGC 193 - a nearby lenticular galaxy - based on X-ray (Chandra) and radio (VLA and GMRT) observations. These data reveal the complex AGN outburst history of the galaxy: we detect a pair of inner X-ray cavities, an outer X-ray cavity, a shock front, and radio lobes extending beyond the inner cavities. We suggest that the inner cavities were produced ~78 Myr ago by a weaker AGN outburst, while the outer cavity, the radio lobes, and the shock front are due to a younger (13-26 Myr) and (4-8) times more powerful outburst. Combining this with the observed morphology of NGC 193, we conclude that NGC 193 likely represents the first example of a second, more powerful, AGN outburst overrunning an older, weaker outburst. These results help to understand how the outburst energy is dissipated uniformly in the core of galaxies, and therefore may play a crucial role in resolving how AGN outbursts suppress the formation of large cooling flows at cluster centers.Comment: 6 pages, 3 figures, 1 table, accepted for publication in ApJ

The impact of a new high-resolution ocean model on the Met Office North-West European Shelf forecasting system

The North-West European Shelf ocean forecasting system has been providing oceanographic products for the European continental shelf seas for more than 15 years. In that time, several different configurations have been implemented, updating the model and the data assimilation components. The latest configuration to be put in operation, an eddy-resolving model at 1.5 km (AMM15), replaces the 7 km model (AMM7) that has been used for 8 years to deliver forecast products to the Copernicus Marine Environment Monitoring Service and its precursor projects. This has improved the ability to resolve the mesoscale variability in this area. An overview of this new system and its initial validation is provided in this paper, highlighting the differences with the previous version. Validation of the model with data assimilation is based on the results of 2 years (2016–2017) of trial experiments run with the low- and high-resolution systems in their operational configuration. The 1.5 km system has been validated against observations and the low-resolution system, trying to understand the impact of the high resolution on the quality of the products delivered to the users. Although the number of observations is a limiting factor, especially for the assessment of model variables like currents and salinity, the new system has been proven to be an improvement in resolving fine-scale structures and variability and provides more accurate information on the major physical variables, like temperature, salinity, and horizontal currents. AMM15 improvements are evident from the validation against high-resolution observations, available in some selected areas of the model domain. However, validation at the basin scale and using daily means penalized the high-resolution system and does not reflect its superior performance. This increment in resolution also improves the capabilities to provide marine information closer to the coast even if the coastal processes are not fully resolved by the model

A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole

We present Atacama Large Millimeter/submillimeter Array and Multi-Unit Spectroscopic Explorer observations of the brightest cluster galaxy in Abell 2597, a nearby (z = 0.0821) cool core cluster of galaxies. The data map the kinematics of a three billion solar mass filamentary nebula that spans the innermost 30 kpc of the galaxy's core. Its warm ionized and cold molecular components are both cospatial and comoving, consistent with the hypothesis that the optical nebula traces the warm envelopes of many cold molecular clouds that drift in the velocity field of the hot X-ray atmosphere. The clouds are not in dynamical equilibrium, and instead show evidence for inflow toward the central supermassive black hole, outflow along the jets it launches, and uplift by the buoyant hot bubbles those jets inflate. The entire scenario is therefore consistent with a galaxy-spanning "fountain," wherein cold gas clouds drain into the black hole accretion reservoir, powering jets and bubbles that uplift a cooling plume of low-entropy multiphase gas, which may stimulate additional cooling and accretion as part of a self-regulating feedback loop. All velocities are below the escape speed from the galaxy, and so these clouds should rain back toward the galaxy center from which they came, keeping the fountain long lived. The data are consistent with major predictions of chaotic cold accretion, precipitation, and stimulated feedback models, and may trace processes fundamental to galaxy evolution at effectively all mass scales.</p