174 citations · 261 across the 11 of their papers we have counts for
12 papers
Polarization of decayless kink oscillations in a 3D MHD coronal loop model
Sudip Mandal, Cosima Breu, Hardi Peter
Decayless kink oscillations are frequently observed in solar coronal loops and are considered potential contributors to coronal heating. Despite the ubiquity of this wave phenomeno…
A self-consistent 3D MHD model producing a solar blowout jet
Yajie Chen, Hardi Peter, Damien Przybylski +2
Context. Solar blowout jets are a distinct subclass of ubiquitous extreme-ultraviolet (EUV) and X-ray coronal jets. Aims. Most existing models of blowout jets prescribe an initial…
Magnetic reconnection sustains the mass budget of the solar wind
Yajie Chen, Hardi Peter, Damien Przybylski +2
The solar wind originates from regions of open magnetic fields on the Sun, but the relevant processes remain unsolved. We present a self-consistent numerical model of the source re…
Three dimensional magnetic reconnection mediated with plasmoids and the resulted multi-thermal emissions in the cool atmosphere of the Sun
Guanchong Cheng, Lei Ni, Robert Cameron +3
Flux emergence is ubiquitous in the Sun's lower atmosphere, where the emerging magnetic flux can reconnect with the pre-existing magnetic field. We investigate plasmoid formation a…
Investigating explosive events in a 3D quiet-Sun model: Transition region and coronal response
Yajie Chen, Hardi Peter, Damien Przybylski
Transition region explosive events are characterized by non-Gaussian profiles of the emission lines formed at transition region temperatures, and they are believed to be manifestat…
Bidirectional propagating brightenings in arch filament systems observed by Solar Orbiter/EUI
Yajie Chen, Sudip Mandal, Hardi Peter +1
Arch filament systems (AFSs) are chromospheric and coronal manifestations of emerging magnetic flux. Using high spatial resolution observations taken at a high cadence by the Extre…
Eruption of a million-Kelvin warm magnetic flux rope on the Sun
Leping Li, Hongqiang Song, Hardi Peter +4
Solar magnetic flux rope (MFR) plays a central role in the physics of coronal mass ejections (CMEs). It mainly includes a cold filament at typical chromospheric temperatures (10000…
Evolution of dynamic fibrils from the cooler chromosphere to the hotter corona
Sudip Mandal, Hardi Peter, Lakshmi Pradeep Chitta +17
Dynamic fibrils (DFs) are commonly observed chromospheric features in solar active regions. Recent observations from the Extreme Ultraviolet Imager (EUI) aboard the Solar Orbiter h…
Diffuse solar coronal features and their spicular footpoints
Nikolina Milanović, Lakshmi Pradeep Chitta, Hardi Peter
In addition to a component of the emission that originates from clearly distinguishable coronal loops, the solar corona also exhibits extreme-ultraviolet (EUV) and X-ray ambient em…
A Magnetic Reconnection model for Hot Explosions in the Cool Atmosphere of the Sun
Lei Ni, Yajie Chen, Hardi Peter +2
UV bursts and Ellerman bombs are transient brightenings observed in the low solar atmospheres of emerging flux regions. Observations have discovered the cospatial and cotemporal EB…
Observations and modeling of the onset of fast reconnection in the solar transition region
L. -J. Guo, B. De Pontieu, Y. -M. Huang +2
Magnetic reconnection is a fundamental plasma process that plays a critical role not only in energy release in the solar atmosphere, but also in fusion, astrophysical, and other sp…
Generation of Solar Spicules and Subsequent Atmospheric Heating
Tanmoy Samanta, Hui Tian, Vasyl Yurchyshyn +9
Spicules are rapidly evolving fine-scale jets of magnetized plasma in the solar chromosphere. It remains unclear how these prevalent jets originate from the solar surface and what…