no code implementations • 24 Feb 2021 • Julia M. Riedl, Caitlin A. Gilchrist-Millar, Tom Van Doorsselaere, David B. Jess, Samuel D. T. Grant
While the analysis of the energy flux for ideal and non-ideal MHD simulations with a plane driver cannot reproduce the observed damping, the numerically predicted damping for a localized driver closely corresponds with the observations.
Solar and Stellar Astrophysics Plasma Physics
no code implementations • 5 Feb 2021 • Konstantinos Karampelas, Tom Van Doorsselaere
This, in addition to the fact that the background flow is constant and not periodic, makes us treat this as a self-oscillating process.
Solar and Stellar Astrophysics
no code implementations • 4 Jan 2021 • Mijie Shi, Tom Van Doorsselaere, Mingzhe Guo, Konstantinos Karampelas, Bo Li, Patrick Antolin
In the quest to solve the long-standing coronal heating problem, it has been suggested half a century ago that coronal loops could be heated by waves.
Solar and Stellar Astrophysics
no code implementations • 2 Dec 2020 • Tom Van Doorsselaere, Abhishek K. Srivastava, Patrick Antolin, Norbert Magyar, Soheil Vasheghani Farahani, Hui Tian, Dmitrii Y. Kolotkov, Leon Ofman, Mingzhe Guo, Iñigo Arregui, Ineke De Moortel, David Pascoe
In this review we focus on recent advances in our understanding of MHD wave heating mechanisms.
Solar and Stellar Astrophysics
