From the 1 of 4.8k papers with an AI index.
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- Kavli Institute for Theoretical SciencesCN957 papers
- Chinese Academy of SciencesCN830 papers
- Institute of High Energy PhysicsCN528 papers
- State Key Laboratory of Nuclear Physics and Technology525 papers
- Centre National de la Recherche ScientifiqueFR523 papers
- University of Chinese Academy of SciencesCN493 papers
- National Astronomical ObservatoriesCN425 papers
- Joint Institute for Nuclear ResearchRU388 papers
- Collaborative Innovation Center of Quantum MatterCN387 papers
- Carnegie Mellon UniversityUS367 papers
- California Institute of TechnologyUS364 papers
- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di FrascatiIT356 papers
225 papers · 1 filter
Influence of the Lower Atmosphere on Wave Heating and Evaporation in Solar Coronal Loops
Mingzhe Guo, Timothy Duckenfield, Tom Van Doorsselaere +3
We model a coronal loop as a three-dimensional magnetic cylinder in a realistic solar atmosphere that extends from the chromosphere to the corona. Kink oscillations, believed ubiqu…
Why "solar tsunamis" rarely leave their imprints in the chromosphere
Ruisheng Zheng, Yihan Liu, Wenlong Liu +10
Solar coronal waves frequently appear as bright disturbances that propagate globally from the eruption center in the solar atmosphere, just like the tsunamis in the ocean on Earth.…
Statistical Investigation of the Widths of Supra-arcade Downflows Observed During a Solar Flare
Guangyu Tan, Yijun Hou, Hui Tian
Supra-arcade downflows (SADs) are dark voids descending towards the post-reconnection flare loops and exhibit obvious variation in properties like width. However, due to the lack o…
Alfvénic motions arising from asymmetric acoustic wave drivers in solar magnetic structures
Samuel Skirvin, Yuhang Gao, Tom Van Doorsselaere
Alfvénic motions are ubiquitous in the solar atmosphere and their observed properties are closely linked to those of photospheric p-modes. However, it is still unclear how a predom…
Heating of quiescent coronal loops caused by nearby eruptions observed with the Solar Dynamics Observatory and the Solar Upper Transition Region Imager
Leping Li, Hui Tian, Huadong Chen +5
How structures, e.g., magnetic loops, in the upper atmosphere, i.e., the transition region and corona, are heated and sustained is one of the major unresolved issues in solar and s…
Photometric and Spectroscopic monitoring of YSOs in nearby star forming regions. I. Eruptive YSOs
Carlos Contreras Peña, Gregory J. Herczeg, Mizna Ashraf +7
Mid-infrared (mid-IR) variability in young stellar objects (YSOs) is driven by several physical mechanisms, which produce a variety of amplitudes and light curve shapes. One of the…