Skip to main navigation
Skip to search
Skip to main content
University of Dundee Discovery Portal Home
Search content at University of Dundee Discovery Portal
Home
Profiles
Research units
Research Outputs
Projects
Datasets
Theses
Activity
Press/Media
Research Facilities
Prizes
Impulsive origin of solar spicule-like jets
A. K. Srivastava (Lead / Corresponding author)
,
Balveer Singh
, K. Murawski
, Y. Chen
, K. Sharma
, D. Yuan
, S. K. Tiwari
, M. Mathioudakis
Mathematics
Research output
:
Contribution to journal
›
Article
›
peer-review
4
Link opens in a new tab
Citations (Scopus)
Overview
Fingerprint
Fingerprint
Dive into the research topics of 'Impulsive origin of solar spicule-like jets'. Together they form a unique fingerprint.
Sort by
Weight
Alphabetically
Keyphrases
Spicules
100%
Solar Spicules
100%
Solar Atmosphere
60%
Synthetic Images
60%
Velocity Enhancement
60%
Non-Gaussian
40%
Interface Region
40%
Imaging Spectrometer
40%
Non-adiabatic
40%
Adiabatic Condition
40%
Kinematics
20%
Two Dimensional Model
20%
Magnetic Field
20%
Transport Energy
20%
Chromosphere
20%
Energy Release
20%
Specific Events
20%
Gaussian Profile
20%
Simulation Data
20%
Jet Plasma
20%
Velocity Fluctuation
20%
Temperature Profile
20%
Transition Region
20%
Line Profiles
20%
Model Atmospheres
20%
Doppler Shift
20%
Line Broadening
20%
Mass Flux
20%
Coronal Holes
20%
Thermal Conduction
20%
Solar Chromosphere
20%
Kinetic Energy Density
20%
Temperature Parameter
20%
Gaussian Line
20%
Model Solar
20%
Conduction Cooling
20%
Transport Mass
20%
Radiative Cooling
20%
Thermal Radiative
20%
Atomic Parameters
20%
Physics
Spicules
100%
Solar Spicules
100%
Solar Atmosphere
60%
Synthetic Image
60%
Blood Plasma
60%
Spectrographs
40%
Gaussian Distribution
40%
Nonadiabatic Condition
40%
Mass Transport
40%
Magnetic Field
20%
Kinetic Energy
20%
Energetics
20%
Flux Density
20%
Doppler Effect
20%
Temperature Profile
20%
Heat Conduction
20%
Solar Chromosphere
20%
Plasma Jet
20%
Cool Cores
20%
Coronal Hole
20%
Earth and Planetary Sciences
Emissions
100%
Solar Atmosphere
100%
Spectrographs
66%
Nonadiabatic Condition
66%
Mass Transport
66%
Flux Density
33%
Kinetic Energy
33%
Data Simulation
33%
Temperature Profile
33%
Coronal Hole
33%
Plasma Jet
33%