1.4k citations
- T. Metcalfe2 profiles70 · h 54
- S. Mathur4 profiles62 · h 64
- S. McIntosh62 · h 47
- J. Christensen-Dalsgaard3 profiles57 · h 85
- W. Chaplin2 profiles57 · h 81
- M. Rempel50 · h 32
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- NSF National Center for Atmospheric ResearchUS515 papers
- Instituto de Astrofísica de CanariasES156 papers
- Max Planck Institute for Solar System ResearchDE123 papers
- Centre National de la Recherche ScientifiqueFR119 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR96 papers
- Universidad de La LagunaES93 papers
- Astrophysique, Instrumentation et ModélisationFR87 papers
- Aarhus UniversityDK85 papers
- Lockheed Martin (United States)US82 papers
- University of BirminghamGB79 papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR75 papers
- University of Colorado BoulderUS72 papers
24 papers · 2 filters
Differential Rotation in Solar Convective Dynamo Simulations
Yuhong Fan, Fang Fang
We carry out a magneto-hydrodynamic (MHD) simulation of convective dynamo in the rotating solar convective envelope driven by the solar radiative diffusive heat flux. The simulatio…
Data-model comparison using FORWARD and CoMP
Sarah Gibson
The FORWARD SolarSoft IDL package is a community resource for model-data comparison, with a particular emphasis on analyzing coronal magnetic fields. FORWARD allows the synthesis o…
Numerical Study on Emergence of Kinked Flux Tube for Understanding of Possible Origin of Delta-spot Regions
Shinsuke Takasao, Yuhong Fan, Mark. C. M. Cheung +1
We carried out a magnetohydrodynamics simulation where a subsurface twisted kink-unstable flux tube emerges from the solar interior to the corona. Unlike the previous expectations…
Numerical simulations of sunspot decay: On the penumbra -- Evershed flow -- moat flow connection
M. Rempel
We present a series of high-resolution sunspot simulations that cover a time span of up to 100 hours. The simulation domain extends about 18 Mm in depth beneath the photosphere and…
Measurements of Photospheric and Chromospheric Magnetic Fields
Andreas Lagg, Bruce Lites, Jack Harvey +2
The Sun is replete with magnetic fields, with sunspots, pores and plage regions being their most prominent representatives on the solar surface. But even far away from these active…
A Center-Median Filtering Method for Detection of Temporal Variation in Coronal Images
Joseph Plowman
Events in the solar corona are often widely separated in their timescales, which can allow them to be identified when they would otherwise be confused with emission from other sour…