Results 131 to 140 of about 232,020 (293)
High-spatial-resolution microwave and related observations as diagnostics of coronal loops [PDF]
High spatial resolution microwave observations of coronal loops, together with theoretical models for the loop emission, can provide detailed information about the temperature, density, and magnetic field within the loop, as well as the environment ...
Holman, Gordon D.
core
Seismology of transversely oscillating coronal loops with siphon flows
There are ubiquitous flows observed in the solar atmosphere of sub-Alfvénic speeds; however, after flaring and coronal mass ejection events flows can become Alfvénic.
Arregui, Inigo +7 more
core +1 more source
Show Me the Brain!!: A modern approach to neuroanatomy education
Abstract Show Me the Brain!! (SMtB) is a digital system for interactive graphics that is designed to support instruction in neuroanatomy and neuroscience. It will soon be made open‐source and freely available. SMtB bridges medical and traditional neuroanatomy instruction with the computational systems and representational conventions common in ...
Nicholas C. Hindy +3 more
wiley +1 more source
Coronal heating by waves [PDF]
Alfven waves or Alfvenic surface waves carry enough energy into the corona to provide the coronal energy requirements. Coronal loop resonances are an appealing means by which large energy fluxes enter active region loops.
Hollweg, J. V.
core
Abstract Mixed reality (MR) using head‐mounted displays provides three‐dimensional visualizations that have been suggested to enhance learning when used alongside conventional anatomy teaching in medical education. This study explored student perceptions of the integration of MR and traditional cadaveric learning, and their optimal delivery to support ...
Harpreet Kasbia +12 more
wiley +1 more source
Magnetohydrodynamic waves in coronal loops provide key seismological diagnostics through their characteristic time signatures. While fast and slow magnetoacoustic modes are routinely exploited, the entropy mode, despite being another eigenmode of the ...
Dmitrii Kolotkov +2 more
doaj +1 more source
Magnetic structure of coronal dark halos
Context. At low coronal temperatures around or below 1 MK distinct areas in the surroundings of active regions (ARs) show emission at a level significantly below the emission coming from the quiet Sun (QS). These areas are referred to as dark halos, dark
Nölke J. D. +7 more
doaj +1 more source
Heating and Cooling of Coronal Loops with Turbulent Suppression of Parallel Heat Conduction. [PDF]
Bian N, Emslie AG, Horne D, Kontar EP.
europepmc +1 more source
Damped transverse oscillations of interacting coronal loops
Damped transverse oscillations of magnetic loops are routinely observed in the solar corona. This phenomenon is interpreted as standing kink magnetohydrodynamic waves, which are damped by resonant absorption owing to plasma ...
Roberto Soler, Manuel Luna
core +1 more source
Feedback strategies: Applying theory to practice
Abstract Feedback is a cornerstone of the learning process, as evidenced by extensive educational research on enhancing its process and impact. However, learners consistently rate the quality of feedback lower compared to other aspects of teaching. Over the past decade, feedback models have shifted from a traditional, one‐way transmission from educator
Jenny Clancy +2 more
wiley +1 more source

