238 citations · 1.2k across the 20 of their papers we have counts for
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Solar differential rotation driven by baroclinic forcing
L. S. Menicucci, G. Guerrero, M. Dikpati +3
A combination of recent observations and numerical simulations has called into question whether Sun's interior is characterized by strong turbulent convection, a problem known as c…
Eruption of EUV Hot-Channel near Solar Limb and Associated Moving Type-IV Radio Burst
P. Vemareddy, P. Démoulin, K. Sasikumar Raja +3
Using the observations from Solar Dynamics Observatory, we study an eruption of a hot-channel flux rope (FR) near the solar-limb on February 9, 2015. The pre-eruptive structure is…
When do solar erupting hot magnetic flux ropes form?
A. Nindos, S. Patsourakos, A. Vourlidas +2
We investigate the formation times of eruptive magnetic flux ropes relative to the onset of solar eruptions, which is important for constraining models of coronal mass ejection (CM…
The Structure of Solar Coronal Mass Ejections in the Extreme-Ultraviolet Passbands
H. Q. Song, J. Zhang, L. P. Li +5
So far most studies on the structure of coronal mass ejections (CMEs) are conducted through white-light coronagraphs, which demonstrate about one third of CMEs exhibit the typical…
The Origin of Solar Filament Plasma Inferred from in situ Observations of Elemental Abundances
Hongqiang Song, Yao Chen, Bo Li +6
Solar filaments/prominences are one of the most common features in the corona, which may lead to energetic coronal mass ejections (CMEs) and flares when they erupt. Filaments are a…
Observation of Magnetic reconnection at a 3D null point associated with a solar eruption
J. Q. Sun, J. Zhang, K. Yang +2
Magnetic null has long been recognized as a special structure serving as a preferential site for magnetic reconnection (MR). However, the direct observational study of MR at null-p…