Predicting the time variation of radio emission from MHD simulations of a flaring T-Tauri star (2020)
Attributed to:
Reconnection-driven waves and oscillations in the flaring solar corona
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/staa1681
Publication URI: http://dx.doi.org/10.1093/mnras/staa1681
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3