Keyphrases
Pseudostreamers
72%
Magnetic Field
66%
Heliosphere
63%
Reconnection
59%
Streamer
54%
Coronal Holes
50%
Helicity
44%
Ribbon
36%
Interchange Reconnection
29%
Slow Solar Wind
24%
Solar Corona
23%
Tears
23%
Magnetic Reconnection
23%
Corona
22%
Hole Boundary
22%
Dynamic Formation
22%
Plasma Loop
22%
Proton
22%
Coronal Heating
22%
Dynamic Structure
22%
Vortex
22%
Electron Beam
22%
Current Sheet
22%
Solar Coronal Loops
22%
Force-free Field
22%
Self-generated
22%
Line Broadening
22%
Turbulence
22%
Topological Constraints
22%
Proton Beam
22%
Dynamic Coupling
22%
Energization
22%
Solar Coronal Jets
22%
Non-Gaussian
22%
Boundary Dynamics
22%
Simulated Sunlight
22%
Coronal Loops
22%
Spatially Separated
22%
Magnetohydrodynamic Simulation
18%
Field Lines
15%
Flux Rope
15%
Interface Region
14%
Astrophysical Plasmas
14%
Imaging Spectrometer
14%
Thermal Broadening
14%
Separatrix
14%
Particle Acceleration
14%
Active Regions
14%
High-resolution
14%
Coronal Jets
14%
Magnetic Field Lines
14%
Helmet
14%
Photosphere
12%
Vortex Reconnection
11%
Low Latitude
11%
Magnetic Flux
9%
Null Point
9%
Solar Surface
8%
Wave-like
8%
Parker Solar Probe
8%
Photospheric Magnetic Field
8%
Solar Orbiter
8%
Three-dimensional (3D)
7%
Particle Approach
7%
Nested Loops
7%
Dissipation Mechanism
7%
Tangential Magnetic Field
7%
Effective Dissipation
7%
Spatial Offset
7%
Coordinated Campaigns
7%
Parallel Loops
7%
Plasma Heating
7%
Thermal Width
7%
Line Intensities
7%
In Situ Observation
7%
Bursty
7%
Observational Signatures
7%
Line Profiles
7%
Magnetohydrodynamic Model
7%
Lower Boundary
7%
Plasma Parameters
7%
Velocity Fluctuation
7%
Solar Atmosphere
7%
Magnetic Energy
7%
Magnetic null Points
7%
Two-band
7%
Arcade
7%
3D Model
7%
Current Observations
7%
Emission Lines
7%
Solar Photosphere
7%
Intermittency
7%
Electromagnetic Field
7%
Heating Process
7%
Small Perturbation
7%
Computational Approach
7%
Nanoflares
7%
Heliospheric Current Sheet
7%
Major Contributor
7%
Impulsive Phase
7%
Extreme Ultraviolet
7%
Energy Dissipation
7%
Particle Deposition
7%
Vorticity
7%
Tearing Instability
5%
Barotropic Fluid
5%
Enstrophy
5%
Inverse Cascade
5%
Topology Change
5%
Low Altitude
5%
Vorticity Field
5%
Kinetic Energy
5%
High Reynolds number
5%
Corrugation
5%
Asymptotic Behavior
5%
Numerical Experiments
5%
Separator
5%
Large Region
5%
Magnetohydrodynamics
5%
Rotating Flows
5%
Current Layer
5%
Physics
Magnetic Field
100%
Heliosphere
91%
Coronal Hole
73%
Blood Plasma
52%
Solar Wind
46%
Current Sheet
44%
Coronal Loops
36%
Vorticity
33%
Solar Corona
33%
Magnetohydrodynamic Simulation
32%
Magnetohydrodynamic Generator
22%
Proton Beams
22%
Particle Acceleration
22%
Fine Structure
22%
Gaussian Distribution
22%
Solar Coronal Loops
22%
Solar Probe
18%
Photosphere
18%
High Resolution
14%
Spectrographs
14%
Magnetic Flux
14%
Magnetohydrodynamics
14%
Solar Surface
11%
Plasma Physics
11%
Coronagraphs
11%
Solar Photosphere
11%
Solar Atmosphere
11%
Stellar Jets
11%
Dense Plasmas
11%
Electric Field
11%
Interplanetary Magnetic Field
11%
Astrophysical Plasma
8%
Spacecraft Orbit
7%
Convective Flow
7%
Reynolds Number
7%
Plasma Heating
7%
Line Intensity
7%
Space Weather
7%
Field of View
7%
Kinetic Energy
7%