Publications by authors named "Iain Hannah"

We investigate the spatial, temporal, and spectral properties of 10 microflares from AR12721 on 2018 September 9 and 10 observed in X-rays using the Nuclear Spectroscopic Telescope ARray and the Solar Dynamic Observatory's Atmospheric Imaging Assembly and Helioseismic and Magnetic Imager. We find GOES sub-A class equivalent microflare energies of 10-10 erg reaching temperatures up to 10 MK with consistent quiescent or hot active region (AR) core plasma temperatures of 3-4 MK. One microflare (SOL2018-09-09T10:33), with an equivalent GOES class of A0.

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Article Synopsis
  • Solar flares release magnetic energy explosively and Hard X-ray (HXR) emissions provide insights into this energy release, with a new telescope, NuSTAR, offering improved sensitivity in measuring these emissions.* -
  • The study analyzes 11 microflares from specific active regions, revealing they share significant characteristics with larger flares, such as quick time profiles and energy emissions that peak earlier in the HXR spectrum.* -
  • This research is notable for being the first to examine multiple microflares collectively, finding consistent high-energy excess in emissions indicating additional heated plasma, and introducing a correction method for analyzing NuSTAR data.*
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Article Synopsis
  • The study focuses on an extremely weak microflare observed on September 9, 2018, using X-ray imaging spectroscopy tools such as NuSTAR and SDO/AIA.
  • The microflare was found to have an energy level three orders of magnitude lower than typical GOES A class microflares, with a temperature of 6.7 MK and a very low emission measure.
  • Remarkably, this research provides the lowest thermal energy estimate for an active region microflare reported in literature, pushing the boundaries of what qualifies as an X-ray microflare.
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We report the detection of emission from a nonthermal electron distribution in a small solar microflare (GOES class A5.7) observed by the , with supporting observation by the (). The flaring plasma is well accounted for by a thick-target model of accelerated electrons collisionally thermalizing within the loop, akin to the "coronal thick-target" behavior occasionally observed in larger flares.

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Subject-specific musculoskeletal modelling is especially useful in the study of juvenile and pathological subjects. However, such methodologies typically require a human operator to identify key landmarks from medical imaging data and are thus affected by unavoidable variability in the parameters defined and subsequent model predictions. The aim of this study was to thus quantify the inter- and intra-operator repeatability of a subject-specific modelling methodology developed for the analysis of subjects with juvenile idiopathic arthritis.

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A dynamic finite element model of a shod running footstrike was developed and driven with 6 degree of freedom foot segment kinematics determined from a motion capture running trial. Quadratic tetrahedral elements were used to mesh the footwear components with material models determined from appropriate mechanical tests. Model outputs were compared with experimental high-speed video (HSV) footage, vertical ground reaction force (GRF), and center of pressure (COP) excursion to determine whether such an approach is appropriate for the development of athletic footwear.

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Juvenile idiopathic arthritis (JIA) is the leading cause of childhood disability from a musculoskeletal disorder. It generally affects large joints such as the knee and the ankle, often causing structural damage. Different factors contribute to the damage onset, including altered joint loading and other mechanical factors, associated with pain and inflammation.

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We present a new method, fan-beam modulation, for observing weak extended x-ray sources with the Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI). This space-based solar x-ray and gamma-ray telescope has much greater sensitivity than previous experiments in the 3-25 keV range, but is normally not well suited to detecting extended sources since their signal is not modulated by RHESSI's rotating grids. When the spacecraft is offpointed from the target source, however, the fan-beam modulation time-modulates the transmission by shadowing resulting from exploiting the finite thickness of the grids.

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