From the 1 of 7 linked papers with an AI index.
7 papers
A self-consistent solar coronal heating model by Alfvenic waves
Hidetaka Kuniyoshi, Richard J. Morton
Alfvenic waves are prevalent throughout the solar atmosphere and are believed to play an essential role in coronal heating, classified as alternating current (AC) heating in contra…
Synthetic Fe XIII 1074.7 nm Observations of Torsional Alfvén Waves in Coronal Waveguides
Samuel Skirvin, Richard Morton, Thomas Schad
Torsional Alfvén waves are a promising mechanism for transporting energy through the solar atmosphere, with implications for coronal heating and solar wind acceleration. Recently,…
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…
Spatially Coherent and Intermittent Alfvénic Fluctuations in Solar Polar Spicules
Edris Tajfirouze, Christopher H. K. Chen, Richard J. Morton +1
Alfvénic fluctuations are considered a key mechanism for transporting energy from the lower solar atmosphere into the corona, with spicules acting as dynamic conduits for this tra…
A Robust Deep Learning Framework for Prominence Detection through Composite Feature Representations
Harry Birch, Stéphane Régnier, Richard Morton
Solar prominences are dynamic structures suspended within the solar corona and are manifestation of solar activity. Their evolution includes eruptions linked to coronal mass ejecti…
High-frequency coronal Alfvénic waves observed with DKIST/Cryo-NIRSP
Richard J. Morton, Momchil Molnar, Steven R. Cranmer +1
The presence and nature of low-frequency (0.1-10~mHz) Alfvénic waves in the corona has been established over the last decade, with many of these results coming from coronagraphic…