The table below shows the most common keywords used by the author. The letters in brackets after some keywords denote if the keyword corresponds to Solar Physics (S) or Heliospheric Physics (H).
| Keyword
| Occurrences
|
|---|
| Instrumentation: Adaptive Optics
| 12
|
| Techniques: Image Processing
| 8
|
| Atmospheric Effects
| 7
|
| Sun: Photosphere [S]
| 7
|
| Techniques: High Angular Resolution
| 5
|
| Sunspots [S]
| 5
|
| Astrophysics - Solar And Stellar Astrophysics [S]
| 4
|
| Sun: Filaments [S]
| 4
|
| Instrumentation: High Angular Resolution
| 4
|
| Sun: Activity
| 4
|
| Telescopes
| 4
|
| Methods: Observational
| 3
|
| Astrophysics - Instrumentation And Methods For Astrophysics
| 3
|
| Instrumentation And Data Management
| 3
|
| Methods: Data Analysis
| 3
|
| Active
| 2
|
| Optical Transfer Function
| 2
|
| Sun: Flares [S]
| 2
|
| Chromosphere
| 2
|
| Sun: General
| 2
|
| Far-field Intensity
| 2
|
| Atmospheric Coherent Length
| 2
|
| Flares
| 2
|
| Piston Error
| 2
|
| Sun: Granulation [S]
| 2
|
| Sparse-optical-synthetic-aperture
| 2
|
| Sun: Corona [S]
| 2
|
| Sun: Magnetic Fields
| 2
|
| Solar Active Regions [S]
| 2
|
| Contrast
| 2
|
| Parallel Computing
| 1
|
| Other
| 1
|
| Optical Testing Techniques
| 1
|
| Models
| 1
|
| Model Comparison
| 1
|
| Methods: Numerical
| 1
|
| Mathematical Model
| 1
|
| Lensless Imaging
| 1
|
| Image Restoration
| 1
|
| Heat-stop
| 1
|
| Ground Telescopes
| 1
|
| Graphics Processing Unit
| 1
|
| Granulation
| 1
|
| Geometry Learning
| 1
|
| Geodetic Coordinates
| 1
|
| Extended Object
| 1
|
| Extended Depth-of-field
| 1
|
| Experiment Validation
| 1
|
| End-to-end
| 1
|
| ELT Astronomy With AO
| 1
|
| Dynamics
| 1
|
| Deconvolution
| 1
|
| Cross
| 1
|
| Correlation Coefficient
| 1
|
| Computer-generated Holograms
| 1
|
| Computer Graphics
| 1
|
| Chinese Large Solar Telescope
| 1
|
| Astronomy Image Processing
| 1
|
| Astronomy Data Analysis
| 1
|
| Astronomical Techniques
| 1
|
| Algorithms
| 1
|
| Adaptive Optics
| 1
|
| 2π Ambiguity
| 1
|
| Wavefront Aberration
| 1
|
| Wave Fronts And Ray Tracing
| 1
|
| Umbra
| 1
|
| Turbulence
| 1
|
| Three-dimension Shape Representation
| 1
|
| Three-dimension Reconstruction
| 1
|
| Thermal Control
| 1
|
| Techniques: Imaging Spectroscopy
| 1
|
| Target
| 1
|
| Sun: Evolution
| 1
|
| Sun: Chromosphere [S]
| 1
|
| Structure Learning
| 1
|
| Spectrum
| 1
|
| Solar Telescopes
| 1
|
| Solar Telescope
| 1
|
| SOLAR SURFACE GRANULATION
| 1
|
| Solar Observatories
| 1
|
| Solar Magnetic Reconnection
| 1
|
| Solar Magnetic Bright Points
| 1
|
| Solar Instruments
| 1
|
| Solar Activity
| 1
|
| Solar Active Region Magnetic Fields [S]
| 1
|
| Satellite
| 1
|
| Redundant Data
| 1
|
| Radiative Transfer [S]
| 1
|
| Pupil Function
| 1
|
| Point Spread Function
| 1
|
| Phase Mask
| 1
|
| Phase Diversity
| 1
|
| Absolute Difference Algorithm
| 1
|
| Aberrations
| 1
|
| 42.87.-d
| 1
|
| 42.40.MY
| 1
|
| 42.40.Jv
| 1
|
| 42.30.RX
| 1
|
| 42.15.Fr
| 1
|
| 42.15.Dp
| 1
|
| Wavefront Sensing
| 1
|