Can the Solar p-modes Contribute to the High-frequency Transverse Oscillations of Spicules? (2024)
Attributed to:
Revealing the Pattern of Solar Alfvénic Waves - RiPSAW
funded by
FLF
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ad1038
Publication URI: http://dx.doi.org/10.3847/1538-4357/ad1038
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2