41 research outputs found

    Verortung des Verstummens und Entstummens traumatischer Erinnerungen bei den Studentenprotesten 2016 in Hyderabad, Indien – eine auto-ethnographische Analyse

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    Psychologists, anthropologists, and historians have researched, revered, and replenished the past. Although the substance of their research is the same, their respective interpretations of the retrieved objects paint a plethora of images. This paper is a peek into the process of silencing and articulating memories. Both silencing and expression of memories are facilitated by temporal and spatial conditionalities, as would be argued here. With the help of an activist petition written by the author during the anti-Caste Discrimination Students’ Movement, known as “Justice for Rohith Vemula”, at the University of Hyderabad (India) in 2016, this study not only delves into the realms of individual memory but also critically evaluates the carrier of the memory undergoing the act of silencing and de-silencing (expression). As the Indian state brutally crushed the protest, the embodied memories carry the mark of the state’s brutality. This paper seeks to ask why and how memories and experiences are silenced, and how those memories find conduits for expression through narratives. How does trauma facilitate the silencing and anticipate the de-silencing of memory? Although the reading of trauma and memory as constitutive of each other helps us to place the narrative within a theoretical debate, the analysis of the author’s petition as an ‘evocative autoethnography’ helps to construct and follow the making and un-making of silence and expression and goes beyond the individual carrier of the traumatic memories. The petition serves as an ‘emotional recall’ and allows the author to enact the felt-emotions that engender the traumatic memory

    Lower Urban Humidity Moderates Outdoor Heat Stress

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    Surface temperature is often used to examine heat exposure in multi-city studies and for informing urban heat mitigation efforts due to scarcity of urban air temperature measurements. Cities also have lower relative humidity, traditionally not accounted for in large-scale observational urban heat risk assessments. Here, using crowdsourced measurements from over 40,000 weather stations in ≈600 urban clusters in Europe, we show the moderating effect of this urbanization-induced humidity reduction on outdoor heat stress during the 2019 heatwave. We demonstrate that daytime differences in heat index between urban clusters and their surroundings are weak, and associations of this urban-rural difference with background climate, generally examined from the surface temperature perspective, are diminished due to moisture feedbacks. We also examine the spatial variability of surface temperature, air temperature, and heat index within these clusters—relevant for detecting hotspots and potential disparities in heat exposure—and find that surface temperature is a poor proxy for the intra-urban distribution of heat index during daytime. Finally, urban vegetation shows much weaker (∼1/6th as strong) associations with heat index than with surface temperature, which has broad implications for optimizing urban heat stress mitigation strategies. These findings are valid for operational metrics of heat stress for shaded conditions (apparent temperature and humidex), thermodynamic proxies (wet-bulb temperature), and empirical heat indices. Based on this large-scale empirical evidence, surface temperature, used due to the lack of better alternatives, may not be suitable for accurately informing heat mitigation strategies within and across cities, necessitating more urban-scale observations and better urban-resolving modelspublishedVersio

    Global 10 m Land Use Land Cover Datasets: A Comparison of Dynamic World, World Cover and Esri Land Cover

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    The European Space Agency’s Sentinel satellites have laid the foundation for global land use land cover (LULC) mapping with unprecedented detail at 10 m resolution. We present a cross-comparison and accuracy assessment of Google’s Dynamic World (DW), ESA’s World Cover (WC) and Esri’s Land Cover (Esri) products for the first time in order to inform the adoption and application of these maps going forward. For the year 2020, the three global LULC maps show strong spatial correspondence (i.e., near-equal area estimates) for water, built area, trees and crop LULC classes. However, relative to one another, WC is biased towards over-estimating grass cover, Esri towards shrub and scrub cover and DW towards snow and ice. Using global ground truth data with a minimum mapping unit of 250 m2 , we found that Esri had the highest overall accuracy (75%) compared to DW (72%) and WC (65%). Across all global maps, water was the most accurately mapped class (92%), followed by built area (83%), tree cover (81%) and crops (78%), particularly in biomes characterized by temperate and boreal forests. The classes with the lowest accuracies, particularly in the tundra biome, included shrub and scrub (47%), grass (34%), bare ground (57%) and flooded vegetation (53%). When using European ground truth data from LUCAS (Land Use/Cover Area Frame Survey) with a minimum mapping unit of <100 m2 , we found that WC had the highest accuracy (71%) compared to DW (66%) and Esri (63%), highlighting the ability of WC to resolve landscape elements with more detail compared to DW and Esri. Although not analyzed in our study, we discuss the relative advantages of DW due to its frequent and near real-time data delivery of both categorical predictions and class probability scores. We recommend that the use of global LULC products should involve critical evaluation of their suitability with respect to the application purpose, such as aggregate changes in ecosystem accounting versus site-specific change detection in monitoring, considering trade-offs between thematic resolution, global versus. local accuracy, class-specific biases and whether change analysis is necessary. We also emphasize the importance of not estimating areas from pixel-counting alone but adopting best practices in design-based inference and area estimation that quantify uncertainty for a given study area. accuracy; deep learning; Earth observation; Sentinel-2; validationpublishedVersio

    Isostructural phase transition in Tb2Ti2O7 under pressure and temperature: Insights from synchrotron X-ray diffraction

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    Tb2Ti2O7, a pyrochlore system, has garnered significant interest due to its intriguing structural and physical properties and their dependence on external physical parameters. In this study, utilizing high-brilliance synchrotron X-ray diffraction, we conducted a comprehensive investigation of structural evolution of Tb2Ti2O7 under external pressure and temperature. We have conclusively confirmed the occurrence of an isostructural phase transition beyond the pressure of 10 GPa. The transition exhibits a distinct signature in the variation of lattice parameters under pressure and leads to changes in mechanical properties. The underlying physics driving this transition can be understood in terms of localized rearrangement of atoms while retaining the overall cubic symmetry of the crystal. Notably, the observed transition remains almost independent of temperature. Our findings provide insights into the distinctive behaviour of the isostructural phase transition in Tb2Ti2O7

    Probing magnetic anisotropy and spin-reorientation transition in 3D antiferromagnet, Ho0.5_{0.5}Dy0.5_{0.5}FeO3_{3}\vertPt using spin Hall magnetoresistance

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    Orthoferrites (REREFeO3_{3}) containing rare-earth (RERE) elements are 3D antiferromagnets (AFM) that exhibit characteristic weak ferromagnetism originating due to slight canting of the spin moments and display a rich variety of spin reorientation transitions in the magnetic field (HH)-temperature (TT) parameter space. We present spin Hall magnetoresistance (SMR) studies on a bb-plate (acac-plane) of crystalline Ho0.5_{0.5}Dy0.5_{0.5}FeO3_{3}|Pt (HDFO|Pt) hybrid at various TT in the range, 11 to 300 K. In the room temperature Γ4(Gx,Ay,Fz)\Gamma_4(G_x, A_y, F_z) phase, the switching between two degenerate domains, Γ4(+Gx,+Fz)\Gamma_4(+G_x, +F_z) and Γ4(Gx,Fz)\Gamma_4(-G_x, -F_z) occurs at fields above a critical value, Hc713H_{\text{c}} \approx 713 Oe. Under H>HcH > H_{\text{c}}, the angular dependence of SMR (α\alpha-scan) in the Γ4(Gx,Ay,Fz)\Gamma_4(G_x, A_y, F_z) phase yielded a highly skewed curve with a sharp change (sign-reversal) along with a rotational hysteresis around aa-axis. This hysteresis decreases with an increase in HH. Notably, at H<HcH < H_{\text{c}} , the α\alpha-scan measurements on the single domain, Γ4(±Gx,±Fz)\Gamma_4(\pm G_x, \pm F_z) exhibited an anomalous sinusoidal signal of periodicity 360 deg. Low-TT SMR curves (HH = 2.4 kOe), showed a systematic narrowing of the hysteresis (down to 150 K) and a gradual reduction in the skewness (150 to 52 K), suggesting weakening of the anisotropy possibly due to the TT-evolution of Fe-RERE exchange coupling. Below 25 K, the SMR modulation showed an abrupt change around the cc-axis, marking the presence of Γ2(Fx,Cy,Gz)\Gamma_2(F_x,C_y,G_z) phase. We have employed a simple Hamiltonian and computed SMR to examine the observed skewed SMR modulation. In summary, SMR is found to be an effective tool to probe magnetic anisotropy as well as a spin reorientation in HDFO. Our spin-transport study highlights the potential of HDFO for future AFM spintronic devices.Comment: 12 pages, 7 figure

    Biases in model-simulated surface energy fluxes during the Indian monsoon onset period

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    We use eddy-covariance measurements over a semi-natural grassland in the central Indo-Gangetic Basin to investigate biases in energy fluxes simulated by the Noah land-surface model for two monsoon onset periods: one with rain (2016) and one completely dry (2017). In the preliminary run with default parameters, the offline Noah LSM overestimates the midday (1000–1400 local time) sensible heat flux (H) by 279% (in 2016) and 108% (in 2017) and underestimates the midday latent heat flux (LE) by 56% (in 2016) and 67% (in 2017). These discrepancies in simulated energy fluxes propagate to and are amplified in coupled Weather Research and Forecasting model simulations, as seen from the High Asia Reanalysis dataset. One-dimensional Noah simulations with modified site-specific vegetation parameters not only improve the partitioning of the energy fluxes (Bowen ratio of 0.9 in modified run versus 3.1 in the default run), but also reduce the overestimation of the model-simulated soil and skin temperature. Thus, use of ambient site parameters in future studies is warranted to reduce uncertainties in short-term and long-term simulations over this region. Finally, we examine how biases in the model simulations can be attributed to lack of closure in the measured surface energy budget. The bias is smallest when the sensible heat flux post-closure method is used (5.2 W m −2 for H and 16 W m −2 for LE in 2016; 0.17 W m −2 for H and 2.8 W m −2 for LE in 2017), showing the importance of taking into account the surface energy imbalance at eddy-covariance sites when evaluating land-surface models

    Detailed study of the ELAIS N1 field with the uGMRT - I. Characterizing the 325 MHz foreground for redshifted 21 cm observations

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    In this first paper of the series, we present initial results of newly upgraded Giant Meterwave Radio Telescope (uGMRT) observation of European Large-Area ISO Survey-North 1 (ELAIS-N1) at 325 MHz with 32 MHz bandwidth. Precise measurement of fluctuations in Galactic and extragalactic foreground emission as a function of frequency as well as angular scale is necessary for detecting redshifted 21-cm signal of neutral hydrogen from Cosmic Dawn, Epoch of Reionization (EoR) and post-reionization epoch. Here, for the first time we have statistically quantified the Galactic and extragalactic foreground sources in the ELAIS-N1 field in the form of angular power spectrum using the newly developed Tapered Gridded Estimator (TGE). We have calibrated the data with and without direction-dependent calibration techniques. We have demonstrated the effectiveness of TGE against the direction dependent effects by using higher tapering of field of view (FoV). We have found that diffuse Galactic synchrotron emission (DGSE) dominates the sky, after point source subtraction, across the angular multipole range 11155083 1115 \leqslant \mathcal{\ell} \leqslant 5083 and 15654754 1565 \leqslant \mathcal{\ell} \leqslant 4754 for direction-dependent and -independent calibrated visibilities respectively. The statistical fluctuations in DGSE has been quantified as a power law of the form C=Aβ\mathcal{C}_{\mathcal{\ell}}= A \mathcal{\ell}^{-\beta} . The best fitted values of (A, β\beta) are (62±6 62 \pm 6 mK2mK^{2}, 2.55±0.32.55 \pm 0.3 ) and (48±4 48 \pm 4 mK2mK^{2}, 2.28±0.42.28 \pm 0.4 ) for the two different calibration approaches. For both the cases, the power law index is consistent with the previous measurements of DGSE in other parts of sky.Comment: 13 pages, 5figures, 4 tables; accepted for publication in MNRA

    Three-dimensional quasi-quantized Hall insulator phase in SrSi2

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    In insulators, the longitudinal resistivity becomes infinitely large at zero temperature. For classic insulators, the Hall conductivity becomes zero at the same time. However, there are special systems, such as two-dimensional quantum Hall isolators, in which a more complex scenario is observed at high magnetic fields. Here, we report experimental evidence for a quasi-quantized Hall insulator in the quantum limit of the three-dimensional semimetal SrSi2. Our measurements reveal a magnetic field-range, in which the longitudinal resistivity diverges with decreasing temperature, while the Hall conductivity approaches a quasi-quantized value that is given only by the conductance quantum and the Fermi wave vector in the field-direction. The quasi-quantized Hall insulator appears in a magnetic-field induced insulating ground state of three-dimensional materials and is deeply rooted in quantum Hall physics.Comment: 29 pages including SI, 3 main figures and 6 SI figure

    Cosmic-ray soil water monitoring: the development, status & potential of the COSMOS-India network

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    Soil moisture (SM) plays a central role in the hydrological cycle and surface energy balance and represents an important control on a range of land surface processes. Knowledge of the spatial and temporal dynamics of SM is important for applications ranging from numerical weather and climate predictions, the calibration and validation of remotely sensed data products, as well as water resources, flood and drought forecasting, agronomy and predictions of greenhouse gas fluxes. Since 2015, the Centre for Ecology and Ecology has been working in partnership with several Indian Research Institutes to develop COSMOS-India, a new network of SM monitoring stations that employ cosmic-ray soil moisture sensors (CRS) to deliver high temporal frequency, near-real time observations of SM at field scale. CRS provide continuous observations of near-surface (top 0.1 to 0.2 m) soil volumetric water content (VWC; m3 m-3) that are representative of a large footprint area (approximately 200 m in radius). To date, seven COSMOS-India sites have been installed and are operational at a range of locations that are characterised by differences in climate, soil type and land management. In this presentation, the development, current status and future potential of the COSMOS-India network will be discussed. Key results from the COSMOS-India network will be presented and analysed
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