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Static and dynamic solar coronal loops with cross-sectional area variations
P. J. Cargill, S. J. Bradshaw, J. A. Klimchuk +1
The Enthalpy Based Thermal Evolution of Loops (EBTEL) approximate model for static and dynamic coronal loops is developed to include the effect of a loop cross-sectional area which…
Flows in Enthalpy Based Thermal Evolution of Loops
Abhishek Rajhans, Durgesh Tripathi, Stephen Bradshaw +2
Plasma-filled loop structures are common in the solar corona. Because detailed modeling of the dynamical evolution of these structures is computationally costly, an efficient metho…
Signatures of Type III Solar Radio Bursts from Nanoflares: Modeling
Sherry Chhabra, James A. Klimchuk, Dale E. Gary
There is a wide consensus that the ubiquitous presence of magnetic reconnection events and the associated impulsive heating (nanoflares) is a strong candidate for solving the solar…
The Coronal Veil
A. Malanushenko, M. C. M. Cheung, C. E. DeForest +2
Coronal loops, seen in solar coronal images, are believed to represent emission from magnetic flux tubes with compact cross-sections. We examine the 3D structure of plasma above an…
How Turbulent is the Magnetically Closed Corona?
James A. Klimchuk, Spiro K. Antiochos
We argue that the magnetically closed corona evolves primarily quasi-statically, punctuated by many localized bursts of activity associated with magnetic reconnection at a myriad o…
Non-thermal Velocity in the Transition Region of Active Regions and its Centre-to-Limb Variation
Avyarthana Ghosh, Durgesh Tripathi, James A. Klimchuk
We derive the non-thermal velocities (NTVs) in the transition region of an active region using the \ion{Si}{4}~1393.78~Å line observed by the Interface Region Imaging Spectrograph…