Corpus ID: 237605394

Evolution of Kelvin-Helmholtz Instability in the Fan-Spine Topology

@inproceedings{Mishra2021EvolutionOK,
  title={Evolution of Kelvin-Helmholtz Instability in the Fan-Spine Topology},
  author={Sudheer K. Mishra and Balveer Singh and A. K. Srivastava and Pradeep Kayshap and Bhola N. Dwivedi},
  year={2021}
}
We use multiwavelength imaging observations from the Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) to study the evolution of Kelvin-Helmholtz (K-H) instability in a fanspine magnetic field configuration. This magnetic topology exists near an active region AR12297 and is rooted in a nearby sunspot. In this magnetic configuration, two layers of cool plasma flow in parallel and interact with each other inside an elongated spine. The slower plasma flow (5 kms−1) is… Expand

Figures from this paper

References

SHOWING 1-7 OF 7 REFERENCES
Physics of the Solar Corona. An Introduction
Thermal Radiation.- Hydrostatics.- Hydrodynamics.- Magnetic Fields.- Magneto-Hydrodynamics (MHD).- MHD Oscillations.- Propagating MHD Waves.- Coronal Heating.- Magnetic Reconnection.- ParticleExpand
Reviews of Modern Plasma Physics, 2, 1 Hillier, A
  • Physics of Plasmas,
  • 2018
MAGNETIC RECONNECTION
The chapter starts with a discussion about the importance of the concept of magnetic field lines in space plasmas and magnetic reconnection, followed by presentations on: (a) the meaning and validityExpand
The Physics of Fluids and Plasmas
An electrical connector in which two rows of resilient contacts are mounted in a connector housing on opposite sides of a slot which is adapted to receive a printed circuit board or similarExpand
The Astrophysical Journal
  • 2000
The Physics of Fluids and Plasmas: An Introduction for Astrophysicists
This is the only book with which I am familiar that attempts to cover both fluids and plasmas. It is true that these subjects are closely related, but the logic of attempting to survey both fields,Expand
Reviews of Modern Plasma Physics , 2 , 1 Hillier , A . 2019
  • Physics of Plasmas