From the 1 of 10 linked papers with an AI index.
10 papers
High-Frequency Magnetohydrodynamic Waves with Substantial Energy in the Solar Polar Corona
Yuhang Gao, Hui Tian, Richard Morton +5
Using high‑cadence EUV images from Solar Orbiter, the authors detect a previously hidden population of high‑frequency kink MHD waves in solar polar coronal plumes, many with period…
Rankine-Hugoniot conditions in Q-variables: a wave-aligned formulation of MHD discontinuities
Anna Krupka, Tijs Van Hoof, Tom Van Doorsselaere
The recently developed Q-variable formalism generalises the Elsässer representation by providing a wave-aligned representation applicable to a broad class of magnetohydrodynamic di…
Imaging magnetically driven astrospheres: a forward modelling approach
Ziqi Wu, Tom Van Doorsselaere, Jiansen He +5
An astrosphere is a vast, tailed bubble-like volume around a star, formed through the interaction between the stellar magnetic field, the stellar wind, and the interstellar medium…
Chromospheric turbulence as a regulator of stellar wind mass flux
Munehito Shoda, Tom Van Doorsselaere, Allan Sacha Brun
The mass flux of solar and stellar winds is a key quantity for stellar evolution and space weather, yet its physical regulation mechanism remains an unsolved problem. In particular…
Propagating Kink Waves in Chromospheric Jet-like Structures and Coronal Plumelets
Youqian Qi, Mingzhe Guo, Zhenghua Huang +5
Coronal plumes and chromospheric jet-like structures are believed to be highly dynamic. We report the first direct observations of a propagating kink wave in a chromospheric jet-li…
Probing spectral line asymmetries due to the propagating transverse waves in the solar corona
Ambika Saxena, Vaibhav Pant, Tom Van Doorsselaere +1
Decades-long studies of asymmetric spectral lines in the solar corona suggest mass and energy transport from lower atmospheric layers to the corona. While slow magnetoacoustic wave…