Search results for "Solar active regions"

showing 3 items of 3 documents

A space weather tool for identifying eruptive active regions

2019

Funding: UK Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214); UK STFC via the Consolidated Grant SMC1/YST025 and SMC1/YST037 (S.L.Y.); UK STFC and the ERC (SynergyGrant: WHOLE SUN, Grant Agreement No. 810218) for financial support (DHM). One of the main goals of solar physics is the timely identification of eruptive active regions. Space missions such as Solar Orbiter or future Space Weather forecasting missions would largely benefit from this achievement.Our aim is to produce a relatively simple technique that c…

010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsFOS: Physical sciencesSpace weather01 natural sciences3rd-NDASSolar coronal mass ejections0103 physical sciencesRegional sciencemedia_common.cataloged_instanceQB AstronomyEuropean union010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesmedia_commonQBPhysicsHorizon (archaeology)European researchAstronomy and AstrophysicsSolar active region magnetic fieldsSolar active regionsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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On the Coronal Temperature in Solar Microflares

2020

We present a study of solar imaging and spectral observations of a microflare, focusing on the temperature diagnostics provided by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory, and the Extreme-Ultraviolet Imaging Spectrometer (EIS) on board Hinode. Our data analysis, in particular from the emission in the 131 and 94 Å channels, indicates that the heated plasma reaches temperatures of ≿10 MK, at odds with a previous analysis of the same event, and we discuss the reason for the discrepancy. A particularly interesting aspect is the likely presence of the Fe XXIII 263.76 Å line, though weak, in EIS spectra in the early phases of the event, supporting the presen…

PhysicsActive solar coronaSolar active regionsSolar extreme ultraviolet emissionSpace and Planetary ScienceCoronal planeSolar coronaAstronomy and AstrophysicsAstrophysicsSolar coronal heatingSolar coronal loopsThe Astrophysical Journal
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A prospective new diagnostic technique for distinguishing eruptive and noneruptive active regions

2019

This research has received funding from the Science and Technology Facilities Council (UK) through the consolidated grant ST/N000609/1 and the European Research Council (ERC) under the European Union Horizon 2020 research and innovation program (grant agreement No. 647214). This work used the DiRAC@Durham facility managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). The equipment was funded by BEIS capital funding via STFC capital grants ST/P002293/1, ST/R002371/1, and ST/S002502/1, Durham University and STFC operations grant ST/R000832/1. DiRAC is part of the National e-Infrastructure. S.L.Y. would like to acknowledge STFC for sup…

Solar coronal mass ejections (310)010504 meteorology & atmospheric sciencesSpace weatherSolar magnetic fieldsSolar activityT-NDASLibrary scienceFOS: Physical sciencesSpace weather (2037)Solar coronaSolar activity (1475)Solar flares (1496)01 natural sciencesSolar coronal mass ejectionsSolar corona (1483)0103 physical sciencesmedia_common.cataloged_instanceAstrophysics::Solar and Stellar AstrophysicsQB AstronomyEuropean union010303 astronomy & astrophysicsQCSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesmedia_commonQBPhysicsEuropean researchSolar active region magnetic fieldsAstronomy and AstrophysicsSolar active region magnetic fields (1975)Solar magnetic fields (1503)Solar active regionsSolar active regions (1974)QC PhysicsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSolar flaresSpace and Planetary SciencePhysics::Space Physics
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