Publications (10)
Evolution of the Magnetic Field Distribution of Active Regions
Sally Dacie, Pascal Démoulin, Lidia van Driel-Gesztelyi +5
Aims. Although the temporal evolution of active regions (ARs) is relatively well understood, the processes involved continue to be the subject of investigation. We study how the ma…
Integrated broadband optical isolator via dynamic rotating destructive interference
Kyunghun Han, Yiliang Bao, Junyeob Song +7
Photonic integrated circuits route and shape light on a chip, but back-reflections feed back into coherent on-chip lasers, destabilizing operation and corrupting signals. Robust op…
Nine Best Practices for Research Software Registries and Repositories: A Concise Guide
Task Force on Best Practices for Software Registries, :, Alain Monteil +30
Scientific software registries and repositories serve various roles in their respective disciplines. These resources improve software discoverability and research transparency, pro…
Understanding the plasma and magnetic field evolution of a filament using observations and Nonlinear force-free field modelling
Stephanie L. Yardley, Antonia Savcheva, Lucie M. Green +4
We present observations and magnetic field models of an intermediate filament present on the Sun in August 2012, associated with a polarity inversion line that extends from AR 1154…
Observations and Interpretation of a Low Coronal Shock Wave Observed in the EUV by the SDO/AIA
Suli Ma, John C. Raymond, Leon Golub +5
Taking advantage of both the high temporal and spatial resolution of the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamics Observatory (SDO), we studied a limb coronal…
Locating Hot Plasma in Small Flares using Spectroscopic Overlappogram Data from the Hinode {\it EUV} Imaging Spectrometer
Louise Harra, Sarah Matthews, David Long +6
One of the key processes associated with the "standard" flare model is chromospheric evaporation, a process where plasma heated to high temperatures by energy deposition at the fla…
Genesis and impulsive evolution of the 2017 September 10 coronal mass ejection
Astrid M. Veronig, Tatiana Podladchikova, Karin Dissauer +7
The X8.2 event of 10 September 2017 provides unique observations to study the genesis, magnetic morphology and impulsive dynamics of a very fast CME. Combining GOES-16/SUVI and SDO…
Sequential eruptions triggered by flux emergence - observations and modeling
Sally Dacie, Tibor Torok, Pascal Demoulin +5
We describe and analyze observations by the Solar Dynamics Observatory of the emergence of a small, bipolar active region within an area of unipolar magnetic flux that was surround…
Non-thermal distributions and energy transport in the solar flares
Sarah Matthews, Guilio del Zanna, Ariadna Calcines +9
Determining the energy transport mechanisms in flares remains a central goal in solar flares physics that is still not adequately answered by the 'standard flare model'. In particu…
The connection between solar coronal abundances and the underlying lower atmospheric properties
Paola Testa, Juan Martinez-Sykora, Bart De Pontieu +4
Elemental abundances in the solar corona and solar wind are often observed to differ from those in the solar photosphere, most commonly showing an enhancement of low first ionizati…